diff --git a/Version b/Version index 09fdf9d4..033b3a7c 100644 --- a/Version +++ b/Version @@ -1,2 +1,2 @@ # Do not edit this document -3.82 +3.83 diff --git a/doc/TeX/Makefile b/doc/TeX/Makefile index 361fd195..cb3f6d6d 100644 --- a/doc/TeX/Makefile +++ b/doc/TeX/Makefile @@ -1,8 +1,9 @@ # -*- Makefile -*- # for a better html result, do 'make pdf' right before 'make html' (so that the aux file of the former can be used by the latter) -TEX := latex -DVIPS := dvips -PDFTEX := pdflatex +#TEX := latex +#DVIPS := dvips +PDFTEX := /usr/local/texlive/2018/bin/x86_64-darwin/pdflatex +#PDFTEX := /usr/local/texlive/2024/bin/universal-darwin/pdflatex TEXFLAGS := DVIFLAGS := PDFFLAGS := @@ -39,6 +40,7 @@ SHORTEN := ./shorten_section_tag.sh INSERTFAVICONS := ./insert_favicons.sh CSSFILE := common.css COLORS = 1 +START=`date` # put last the ones referring to the others docs := intro.tex csub.tex idl.tex subroutines.tex facilities.tex install.tex @@ -160,14 +162,14 @@ install.html: $(style) healpix.perl cssfile mkdir -p $(HTMLDIR) -cp $(HTMLDIR)/*labels.pl /tmp -$(LATEX2HTML) $(L2HFLAGS) -toc_depth 8 -split 3 -prefix $(FULL) -external_file ./$(FULL) -t $(TITLE) $(LONGTITLES) $(FULL) - ###-$(EQNFIX) $(HTMLDIR)/$(PREFIX) 1> /dev/null 2>&1 +#### ####-$(EQNFIX) $(HTMLDIR)/$(PREFIX) 1> /dev/null 2>&1 -$(FIXHTML5) $(HTMLDIR)/$(PREFIX) -$(SHORTEN) $(HTMLDIR)/$(PREFIX) -$(IMPROVEHTML) $(HTMLDIR)/$(PREFIX) -$(INSERTFAVICONS) $(HTMLDIR)/$(PREFIX) mv -f $(HTMLDIR)/WARNINGS $(HTMLDIR)/WARNINGS_$(FULL) ln -sf $(CSSFILE) $(HTMLDIR)/$(FULL).css - #######ln -sf $(PREFIX)$(TTL).htm $(HTMLDIR)/$(FULL).htm +### #######ln -sf $(PREFIX)$(TTL).htm $(HTMLDIR)/$(FULL).htm -cp $(HTMLDIR)/*labels.pl /tmp @echo "created$(BLUE_COLOR) $(HTMLDIR)/$(FULL).htm $(NO_COLOR)" @@ -183,7 +185,7 @@ intro.html: $(style) healpix.perl cssfile mkdir -p $(HTMLDIR) -cp $(HTMLDIR)/*labels.pl /tmp -$(LATEX2HTML) $(L2HFLAGS) -toc_depth 8 -split 4 -prefix $(PREFIX) -external_file ./$(FULL) -t $(TITLE) $(LONGTITLES) $(FULL) - ###-$(EQNFIX) $(HTMLDIR)/$(PREFIX) 1> /dev/null 2>&1 +## ###-$(EQNFIX) $(HTMLDIR)/$(PREFIX) 1> /dev/null 2>&1 -$(FIXHTML5) $(HTMLDIR)/$(PREFIX) -$(SHORTEN) $(HTMLDIR)/$(PREFIX) -$(IMPROVEHTML) $(HTMLDIR)/$(PREFIX) @@ -207,7 +209,7 @@ idl.html: $(style) healpix.perl cssfile mkdir -p $(HTMLDIR) -cp $(HTMLDIR)/*labels.pl /tmp -$(LATEX2HTML) $(L2HFLAGS) -toc_depth 8 -split 4 -prefix $(PREFIX) -external_file ./$(FULL) -t $(TITLE) $(LONGTITLES) $(FULL) - ###-$(EQNFIX) $(HTMLDIR)/$(PREFIX) 1> /dev/null 2>&1 +### ###-$(EQNFIX) $(HTMLDIR)/$(PREFIX) 1> /dev/null 2>&1 -$(FIXHTML5) $(HTMLDIR)/$(PREFIX) -$(SHORTEN) $(HTMLDIR)/$(PREFIX) -$(IMPROVEHTML) $(HTMLDIR)/$(PREFIX) @@ -231,7 +233,7 @@ subroutines.html: $(style) healpix.perl cssfile mkdir -p $(HTMLDIR) -cp $(HTMLDIR)/*labels.pl /tmp -$(LATEX2HTML) $(L2HFLAGS) -toc_depth 4 -toc_stars -split 4 -prefix $(PREFIX) -external_file ./$(FULL) -t $(TITLE) $(LONGTITLES) $(FULL) - ###-$(EQNFIX) $(HTMLDIR)/$(PREFIX) 1> /dev/null 2>&1 +### ###-$(EQNFIX) $(HTMLDIR)/$(PREFIX) 1> /dev/null 2>&1 -$(FIXHTML5) $(HTMLDIR)/$(PREFIX) -$(SHORTEN) $(HTMLDIR)/$(PREFIX) -$(IMPROVEHTML) $(HTMLDIR)/$(PREFIX) @@ -255,7 +257,7 @@ facilities.html: $(style) healpix.perl cssfile mkdir -p $(HTMLDIR) -cp $(HTMLDIR)/*labels.pl /tmp -$(LATEX2HTML) $(L2HFLAGS) -toc_depth 8 -split 4 -prefix $(PREFIX) -external_file ./$(FULL) -t $(TITLE) $(LONGTITLES) $(FULL) - ###-$(EQNFIX) $(HTMLDIR)/$(PREFIX) 1> /dev/null 2>&1 +### ###-$(EQNFIX) $(HTMLDIR)/$(PREFIX) 1> /dev/null 2>&1 -$(FIXHTML5) $(HTMLDIR)/$(PREFIX) -$(SHORTEN) $(HTMLDIR)/$(PREFIX) -$(IMPROVEHTML) $(HTMLDIR)/$(PREFIX) @@ -279,7 +281,7 @@ csub.html: $(style) healpix.perl cssfile mkdir -p $(HTMLDIR) -cp $(HTMLDIR)/*labels.pl /tmp -$(LATEX2HTML) $(L2HFLAGS) -toc_depth 8 -split 4 -prefix $(PREFIX) -external_file ./$(FULL) -t $(TITLE) $(LONGTITLES) $(FULL) - ###-$(EQNFIX) $(HTMLDIR)/$(PREFIX) 1> /dev/null 2>&1 +### ###-$(EQNFIX) $(HTMLDIR)/$(PREFIX) 1> /dev/null 2>&1 -$(FIXHTML5) $(HTMLDIR)/$(PREFIX) -$(SHORTEN) $(HTMLDIR)/$(PREFIX) -$(IMPROVEHTML) $(HTMLDIR)/$(PREFIX) @@ -299,7 +301,7 @@ epub: main.html @echo "$(GREEN_COLOR)==================================$(NO_COLOR)" $(EBOOK) @mkdir -p $(EPUBDIR) - #@cp $(epub) $(EPUBDIR) +### #@cp $(epub) $(EPUBDIR) intro.epub: $(EBOOK) intro @@ -348,6 +350,7 @@ allpdf: empty crossref all: empty crossref crosshtml epub @echo "$(GREEN_COLOR) All PDF+HTML+EPUB Done ! $(NO_COLOR)" + @echo $(START) ... `date` package: all cd $(DOCDIR) ; \ diff --git a/doc/TeX/fig/new_dir_tree.pdf b/doc/TeX/fig/new_dir_tree.pdf index 2f105f76..dd64b2a0 100644 Binary files a/doc/TeX/fig/new_dir_tree.pdf and b/doc/TeX/fig/new_dir_tree.pdf differ diff --git a/doc/TeX/fig/new_dir_tree.png b/doc/TeX/fig/new_dir_tree.png deleted file mode 120000 index 60ea5c8a..00000000 --- a/doc/TeX/fig/new_dir_tree.png +++ /dev/null @@ -1 +0,0 @@ -new_dir_tree_382.png \ No newline at end of file diff --git a/doc/TeX/fig/new_dir_tree.png b/doc/TeX/fig/new_dir_tree.png new file mode 100644 index 00000000..d24923ae Binary files /dev/null and b/doc/TeX/fig/new_dir_tree.png differ diff --git a/doc/TeX/fig/new_dir_tree_383.pdf b/doc/TeX/fig/new_dir_tree_383.pdf new file mode 100644 index 00000000..dd64b2a0 Binary files /dev/null and b/doc/TeX/fig/new_dir_tree_383.pdf differ diff --git a/doc/TeX/fig/new_dir_tree_383.png b/doc/TeX/fig/new_dir_tree_383.png new file mode 100644 index 00000000..d24923ae Binary files /dev/null and b/doc/TeX/fig/new_dir_tree_383.png differ diff --git a/doc/TeX/fig/new_dir_tree_383.tex b/doc/TeX/fig/new_dir_tree_383.tex new file mode 100644 index 00000000..5b51afbb --- /dev/null +++ b/doc/TeX/fig/new_dir_tree_383.tex @@ -0,0 +1,47 @@ +%====================== +\documentclass{article} +\usepackage{dirtree} +\textheight = 14cm +\textwidth = 14cm +\oddsidemargin = 0cm +\topmargin = -2cm +\input{hpxversion} +%---------------------- +% LaTeX file generated by make_dir_tree.csh +%---------------------- +\begin{document} +\thispagestyle{empty} +\small{ +\fbox{ +\parbox{0.97\textwidth}{ +\dirtree{% + .1 Healpix\_\hpxversion/. + .1 data/. + .1 doc/. + .2 epub/. + .2 html/. + .2 pdf/. + .1 src/. + .2 C/. + .3 autotools/, subs/. + .2 common\_libraries/. + .3 libsharp/. + .2 cxx/. + .3 Healpix\_cxx/, autom4te.cache/, autotools/, cxxsupport/, m4/, test/. + .2 f90/. + .3 alteralm/, anafast/, hotspot/, lib/, map2gif/, median\_filter/, mod/, ngsims\_full\_sky/, plmgen/, process\_mask/, smoothing/, synfast/, ud\_grade/. + .2 healpy/. + .3 bin/, cextern/, lib/, src/, test/. + .2 idl/. + .3 examples/, fits/, interfaces/, misc/, toolkit/, visu/, zzz\_external/. + .2 java/. + .3 lib/, src/. + .2 python/. + .1 test/. +} +} +} +} +\end{document} +%---------------------- +%====================== diff --git a/doc/TeX/hpxversion.tex b/doc/TeX/hpxversion.tex index 2f286661..220af9cb 100644 --- a/doc/TeX/hpxversion.tex +++ b/doc/TeX/hpxversion.tex @@ -20,5 +20,7 @@ % \newcommand{\hpxverstex}{3\_80} % \newcommand{\hpxversion}{3.81} % \newcommand{\hpxverstex}{3\_81} -\newcommand{\hpxversion}{3.82} -\newcommand{\hpxverstex}{3\_82} +% \newcommand{\hpxversion}{3.82} +% \newcommand{\hpxverstex}{3\_82} +\newcommand{\hpxversion}{3.83} +\newcommand{\hpxverstex}{3\_83} diff --git a/doc/TeX/hpyversion.tex b/doc/TeX/hpyversion.tex index ec38f948..c774a7ef 100644 --- a/doc/TeX/hpyversion.tex +++ b/doc/TeX/hpyversion.tex @@ -14,5 +14,7 @@ % \newcommand{\hpyversion}{1.15.0}% 2021-05-?? (3.80) % \newcommand{\hpyversion}{1.15.1}% 2022-01-?? (3.81) % \newcommand{\hpyversion}{1.15.2}% 2022-01-2? (3.81) -\newcommand{\hpyversion}{1.16.1}% 2022-07-29? (3.82) +% \newcommand{\hpyversion}{1.16.1}% 2022-07-29? (3.82) +% \newcommand{\hpysite}{https://github.com/healpy/healpy} +\newcommand{\hpyversion}{1.17.3}% 2024-10-09? (3.83) \newcommand{\hpysite}{https://github.com/healpy/healpy} diff --git a/doc/TeX/install.tex b/doc/TeX/install.tex index 6dae28b9..2fa0df16 100644 --- a/doc/TeX/install.tex +++ b/doc/TeX/install.tex @@ -273,16 +273,20 @@ \section{Installation Requirements} \healpix package simpler. The \healpix \textbf{Fortran 90}, \textbf{C++}, \textbf{C} and \textbf{Python} distributions also -require the publicly available CFITSIO library. Note that the -\textbf{Fortran 90} routines require -version 3.20 or more (post August 2009) -of CFITSIO on most platforms, except on Apple's ARM (M1 and M2) chips, which -require version 4.1.0 (March 2022) or more. Out of security concerns, the CFITSIO developers recommend using version 3.44 (April 2018) or more. +require the publicly available CFITSIO library. +Versions 4.2.0 (Nov 2022) or higher are recommended since they simultaneously meet +\textbf{Fortran 90} routines requirements, fix previous security vulnerabilities +and are compatible with Apple's ARM chips. +% Note that the +% \textbf{Fortran 90} routines require +% version 3.20 or more (post August 2009) +% of CFITSIO on most platforms, except on Apple's ARM (M1 and M2) chips, which +% require version 4.1.0 (March 2022) or more. Out of security concerns, the CFITSIO developers recommend using version 3.44 (April 2018) or more. \begin{tabular}{p{0.3\hsize} p{0.6\hsize}} \hline \textbf{Software Package} & \textbf{Source} \\ \hline & \\ %%% for presentation - CFITSIO V 3.44 (4.1.0) or more + CFITSIO V 4.2.0 or more & \url{https://heasarc.gsfc.nasa.gov/fitsio/} \\ & \\ \hline %%% for presentation @@ -322,7 +326,9 @@ \section{Installation Requirements} As it was already the case in version 1.20, users no longer need to acquire the \textbf{IDL} -Astronomy User's Library (\url{https://idlastro.gsfc.nasa.gov/homepage.html}) +Astronomy User's Library +%(\url{https://idlastro.gsfc.nasa.gov/homepage.html}) +(\url{https://github.com/wlandsman/IDLAstro}) or the COBE (IDL) Analysis Software (\url{https://lambda.gsfc.nasa.gov/product/cobe/cgis.cfm}), although we do recommend these packages to the user. The 100-odd routines required for version \hpxversion\ are contained in the @@ -337,9 +343,9 @@ \section{Installation Requirements} \begin{tabular}{p{0.3\hsize} p{0.6\hsize}} \hline \textbf{Software Package} & \textbf{Source} \\ \hline & \\ %%% for presentation -Python 3.6 or more & \url{https://www.python.org} +Python 3.9 or more & \url{https://www.python.org} \\ -Numpy 1.13 or more & \url{https://numpy.scipy.org} +Numpy 2.0 or more & \url{https://numpy.scipy.org} \\ Matplotlib 0.91.2 or more & \url{https://matplotlib.sourceforge.net} \\ @@ -959,7 +965,9 @@ \subsection{Free Fortran90/95 Compilers} They all support the few Fortran 2003 features used in \healpixns. \begin{itemize} % - \item {\bf Intel Fortran} compiler (\texttt{ifort}) for Linux based computers (versions + \item {\bf Intel Fortran} compilers for Linux based computers \texttt{ifx} + (since version 2021) and previously + \texttt{ifort} (versions 11.* to 19.*\footnote{problems have been reported with one of the code (\texttt{sky\_ng\_sim}) when compiled with \texttt{ifort 14.0.1.106}}) \hfill \\ \url{https://software.intel.com/en-us/fortran-compilers} @@ -1383,8 +1391,13 @@ \subsection{Mac OS X, X11 and IDL cursor} \item with Xquartz (default under Moutain Lion (10.8.*), Mavericks (10.9.*) and Yosemite (10.10.*), available for download for El Capitan (10.11.*), Sierra (10.12.*), High Sierra (10.13.*), Mojave (10.14.*), -Catalina (10.15.*), Big Sur (11.0.*) and Monterey (12.*)):\\ -{\texttt{defaults write org.macosforge.xquartz.X11 wm\_click\_through -bool true}} +Catalina (10.15.*), Big Sur (11.*), Monterey (12.*), Ventura (13.*), Sonoma +(14.*) and Sequoia (15.*)):\\ +{\texttt{defaults write org.macosforge.xquartz.X11 wm\_click\_through -bool + true}} for Xquartz $\le$ 2.7.*, %https://www.xquartz.org/FAQs.html +or \\ +{\texttt{defaults write org.xquartz.X11 wm\_click\_through -bool true}}\\ +for Xquartz $\ge$ 2.8.* \item with MacPort's X11 (package xorg-server):\\ {\texttt{defaults write org.macports.X11 wm\_click\_through -bool true}} \end{itemize} @@ -1660,7 +1673,7 @@ \subsubsection*{Impact of FL limitations on \healpix} \section{Appendix I: Recent Changes and New Features} \label{sec:newfeatures} %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% BEGIN LATEST CHANGES %%%%%%%%%%%%% -\subsection{Bug corrections and Improvements in Version \hpxversion}%2022-07-?? +\subsection{Bug corrections and Improvements in Version \hpxversion}%2024-10-?? % ------------ % \subsubsection[General]{General} % \subsubsection[C]{\linklatexhtml{C}{csub.pdf}{csub.htm}} @@ -1671,7 +1684,52 @@ \subsection{Bug corrections and Improvements in Version \hpxversion}%2022-07-?? % \subsubsection[IDL]{\linklatexhtml{IDL}{idl.pdf}{idl.htm}} % \subsubsection[Java]{\htmladdnormallink{Java}{\healpixwebpage/html/java/index.html}} % \subsubsection[Python]{\htmladdnormallink{Python}{https://healpy.readthedocs.io/en/latest/}} +% ------------ +\subsubsection[General]{General} +\begin{itemize} + \item Support for intel \texttt{ifx} compiler + \item Proper detection of \texttt{python} versions above 3.9 +\end{itemize} +% \subsubsection[C]{\linklatexhtml{C}{csub.pdf}{csub.htm}} +\subsubsection[C++]{\htmladdnormallink{C++}{\healpixwebpage/html/index_cxx.htm}} +\begin{itemize} +\item bug fix in \texttt{query\_polygon} where pixels might be missing in some situations + where polygon edges were parallel to the equator. + (\url{https://github.com/healpy/healpy/issues/904}). +\item bug fix in \texttt{query\_disc\_inclusive} where pixels could be missing at locations + exactly azimuthally opposite to the disc center. + (\url{https://github.com/healpy/healpy/issues/968}) +\end{itemize} +% \subsubsection[Fortran]{% +% Fortran 90 \linklatexhtml{facilities}{facilities.pdf}{facilities.htm} and +% \linklatexhtml{subroutines}{subroutines.pdf}{subroutines.htm}} +\subsubsection[IDL]{\linklatexhtml{IDL}{idl.pdf}{idl.htm}} +\begin{itemize} +\item update of the required + \htmladdnormallink{\texttt{IDL-astron} library}{https://github.com/wlandsman/IDLAstro} + routines (2024-09-27).% +\end{itemize} +% \subsubsection[Java]{\htmladdnormallink{Java}{\healpixwebpage/html/java/index.html}} +\subsubsection[Python]{\htmladdnormallink{Python}{https://healpy.readthedocs.io/en/latest/}} +\begin{itemize} +\item Switch to + \htmladdnormallink{\texttt{healpy \hpyversion}}{\hpysite/releases} + (\htmladdnormallink{CHANGELOG}{\hpysite/blob/master/CHANGELOG.rst}) + \begin{itemize} + \item scipy and matplotlib are now optional dependencies + \item wheels available for MacOS arm64 + \item now supports $ 3.9 \le$ \texttt{python}$\le 3.12$. + \item addition of \texttt{resize\_alm} + \item bugs correction in ???? +\end{itemize} +\end{itemize} +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% END LATEST CHANGES %%%%%%%%%%%%% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% +%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% %------------ +\subsection{Bug corrections and Improvements in Version 3.82}%2022-07-?? % \subsubsection[General]{General} \subsubsection[C]{\linklatexhtml{C}{csub.pdf}{csub.htm}} \begin{itemize} @@ -1720,11 +1778,6 @@ \subsection{Bug corrections and Improvements in Version \hpxversion}%2022-07-?? \item Added colorbar ticks and normalization \end{itemize} \end{itemize} -%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% END LATEST CHANGES %%%%%%%%%%%%% -%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% -%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% -%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% -%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%% \subsection{Bug corrections and Improvements in Version 3.81}%2022-01-25 \label{sec:v381}\mytarget{install:v381} \subsubsection[C++]{C++} diff --git a/doc/TeX/mollcursor_idl.tex b/doc/TeX/mollcursor_idl.tex index 4002b05d..3d3e039a 100644 --- a/doc/TeX/mollcursor_idl.tex +++ b/doc/TeX/mollcursor_idl.tex @@ -77,10 +77,12 @@ {\footnotesize {\tt defaults write com.apple.x11 wm\_click\_through -bool true}} \\ or, under Leopard (10.5), Snow Leopard (10.6), Lion (10.7): \\ {\footnotesize {\tt defaults write org.x.x11 wm\_click\_through -bool true}} \\ -If you are using Xquartz (for eg, Montain Lion (10.8), Mavericks (10.9), -Yosemite (10.10), El Capitan (10.11), Sierra (10.12), High Sierra (10.13), -Mojave (10.14), Catalina (10.15), Big Sur (11.0) or Monterey (12)): \\ -{\footnotesize {\tt defaults write org.macosforge.xquartz.X11 wm\_click\_through -bool true}}\\ +If you are using Xquartz (from, Montain Lion (10.8) to Sequoia (15.*)): \\ +{\footnotesize {\tt defaults write org.macosforge.xquartz.X11 wm\_click\_through + -bool true}} for Xquartz $\le$ 2.7, \\ +or +{\footnotesize {\tt defaults write org.xquartz.X11 wm\_click\_through -bool + true}} for Xquartz $\ge$ 2.8,\\ and if you are using MacPort's X11 (package xorg-server):\\ {\footnotesize {\tt defaults write org.macports.X11 wm\_click\_through -bool true}}\\ (see diff --git a/getit b/getit index 2709ed82..09940d46 100755 --- a/getit +++ b/getit @@ -27,7 +27,7 @@ echoRed (){ WRKDIR="/tmp" #healpytag="1.15.2" -healpytag="1.16.1" +healpytag="1.17.3" healpytag_git="" #healpytag_git=${healpytag} healpygit=0 # 1: uses GIT, 0: uses tar.gz diff --git a/hpxconfig_functions.sh b/hpxconfig_functions.sh index b377e601..afbb3a41 100644 --- a/hpxconfig_functions.sh +++ b/hpxconfig_functions.sh @@ -918,7 +918,7 @@ Cpp_config () { #------------- -Healpy_config () { # for healpy 1.7.0 +Healpy_config () { # for healpy >= 1.7.0 HPY_PYTHON="$PYTHON" tmpfile=to_be_removed @@ -939,7 +939,8 @@ Healpy_config () { # for healpy 1.7.0 #python_reqrd="2.4" # minimal version supported #python_reqrd="2.6" # minimal version supported #python_reqrd="2.7" # minimal version supported (1.12.8) - python_reqrd="3.6" # minimal version supported (1.15.0) + #python_reqrd="3.6" # minimal version supported (1.15.0) + python_reqrd="3.9" # minimal version supported (1.17.3) #p_v1=`echo ${python_version} | ${AWK} '{print $1*10}'` # does not work properly for eg 3.10 #p_v2=`echo ${python_reqrd} | ${AWK} '{print $1*10}'` p_v1=`echo ${python_version} | ${AWK} -F. '{print $1*10000+$2*100+$3}'` @@ -1596,16 +1597,18 @@ EOF FFLAGS_=`eval echo ${FFLAGS_}` # ${} -> value ${FC} ${FFLAGS_} ${tmpfile}${suffix} -o ${tmpfile}.x -L${FITSDIR} -l${LIBFITS} ${CFITSIOCURL} ${F90_WLRPATH_} #CFITSIOVREQ="3.14" # required version of CFITSIO (in Healpix 3.00) - CFITSIOVREQ="3.20" # required version of CFITSIO (in Healpix 3.30) - CFITSIOVREC="3.44" # recommended version of CFITSIO (according to NASA) - CFITSIOVARM="4.01" # stands for 4.1.0, required by F90 on Apple's ARM M1 and M2 chips + #CFITSIOVREQ="3.20" # required version of CFITSIO (in Healpix 3.30) + #CFITSIOVREC="3.44" # recommended version of CFITSIO (according to NASA) + CFITSIOVREQ="3.44" # required + CFITSIOVREC="4.2.0" # recommended version of CFITSIO (according to NASA) + CFITSIOVARM="4.1.0" # required by F90 on Apple's ARM M1 and M2 chips # run if executable if [ -x ${tmpfile}.x ]; then CFITSIOVERSION=`${tmpfile}.x` || CFITSIOVERSION=-1 # available version of CFITSIO - v1=`echo ${CFITSIOVERSION} | ${AWK} '{print $1*1000}'` # multiply by 1000 to get integer - v2=`echo ${CFITSIOVREQ} | ${AWK} '{print $1*1000}'` - v3=`echo ${CFITSIOVREC} | ${AWK} '{print $1*1000}'` - v4=`echo ${CFITSIOVARM} | ${AWK} '{print $1*1000}'` + v1=`echo ${CFITSIOVERSION} | ${AWK} -F. '{print $1*10000+$2*100+$3}'` # deal with x.y.z + v2=`echo ${CFITSIOVREQ} | ${AWK} -F. '{print $1*10000+$2*100+$3}'` + v3=`echo ${CFITSIOVREC} | ${AWK} -F. '{print $1*10000+$2*100+$3}'` + v4=`echo ${CFITSIOVARM} | ${AWK} -F. '{print $1*10000+$2*100+$3}'` if [ $v1 -lt 0 ]; then echo echo "The code compiled with" @@ -1894,7 +1897,7 @@ IdentifyF90Compiler () { DO_F90_SHARED=0 # do NOT know how to create a shared library nima=`$FC -V 2>&1 | ${GREP} -i imagine1 | ${WC} -l` nnag=`$FC -V 2>&1 | ${GREP} -i nagware | ${WC} -l` - nifc=`$FC -V 2>&1 | ${GREP} -i intel | ${WC} -l` + nifc=`$FC -V 2>&1 | ${GREP} -io intel | ${WC} -l` #npgf=`$FC -V 2>&1 | ${GREP} -i portland | ${WC} -l` npgf=`$FC -V 2>&1 | ${GREP} PGI | ${WC} -l` nlah=`$FC --version 2>&1 | ${GREP} -i lahey | ${WC} -l` @@ -1920,28 +1923,39 @@ IdentifyF90Compiler () { FI8FLAG="-double" # change default INTEGER and FLOAT to 64 bits MODDIR="-mdir " # output location of modules elif [ $nifc != 0 ] ; then - ifc_modules - FCNAME="Intel Fortran Compiler" - junk=`$FC -v 2>&1 | grep -i version | sed "s|[ifort,version,Version, ]||g"` - intelversion=`echo $junk | awk -F. '{print $1}'` - #if [ $intelversion -le 17 ] ; then # old syntax, supported up to version 17 included - if [ $intelversion -lt 15 ] ; then # old syntax, supported up to version 17 included - FFLAGS="$IFCINC -cm -w -sox -vec_report0" - PRFLAGS="-openmp -openmp_report0" # Open MP enabled # June 2007 - else # new syntax, supported since version 15, required in 18 - FFLAGS="$IFCINC -cm -w -sox -qopt-report=0" - PRFLAGS="-qopenmp" # Open MP enabled # Sept 2017 - fi - MOD="$IFCMOD" - FTYPE="$IFCVERSION" + ifc_modules + nifort=`$FC --version | ${GREP} -io ifort | ${WC} -l` + nifx=`$FC --version | ${GREP} -io ifx | ${WC} -l` + junk=`$FC -v 2>&1 | grep -i version | sed "s|[ifort,ifx,version,Version, ]||g"` + intelversion=`echo $junk | awk -F. '{print $1}'` + #if [ $intelversion -le 17 ] ; then # old syntax, supported up to version 17 included + if [ $intelversion -lt 15 ] ; then # old syntax, supported up to version 17 included + FFLAGS="$IFCINC -cm -w -sox -vec_report0" + PRFLAGS="-openmp -openmp_report0" # Open MP enabled # June 2007 + elif [ $intelversion -lt 2020 ] ; then # new syntax, supported since version 15, required in 18 + FFLAGS="$IFCINC -qopt-report=0" + PRFLAGS="-qopenmp" # Open MP enabled # Sept 2017 + else + FFLAGS="$IFCINC -qopt-report=0" + PRFLAGS="-qopenmp" # Open MP enabled + fi + MOD="$IFCMOD" + FTYPE="$IFCVERSION" + if [ $nifx != 0 ] ; then + FCNAME="Intel Fortran Compiler (ifx)" + EMULATE_IFORT_DEFAULTS="-assume noieee_compares,nan_compares" + OFLAGS="-O3 -xHost ${EMULATE_IFORT_DEFAULTS}" + else + FCNAME="Intel Fortran Compiler (ifort)" OFLAGS="-O3" - FI8FLAG="-i8" # change default INTEGER to 64 bits -## FI8FLAG="-integer-size 64" # change default INTEGER to 64 bits - CFLAGS="$CFLAGS -DINTEL_COMPILER" # to combine C and F90 - MODDIR="-module " # output location of modules - [ $OS = "Linux" ] && F90_WLRPATH="-Wl,-R" - [ $OS = "Darwin" ] && F90_WLRPATH="-Wl,-rpath," - DO_F90_SHARED=1 + fi + FI8FLAG="-i8" # change default INTEGER to 64 bits + ## FI8FLAG="-integer-size 64" # change default INTEGER to 64 bits + CFLAGS="$CFLAGS -DINTEL_COMPILER" # to combine C and F90 + MODDIR="-module " # output location of modules + [ $OS = "Linux" ] && F90_WLRPATH="-Wl,-R" + [ $OS = "Darwin" ] && F90_WLRPATH="-Wl,-rpath," + DO_F90_SHARED=1 elif [ $npgf != 0 ] ; then #FCNAME="Portland Group Compiler" FCNAME="PGI Compiler" diff --git a/pack b/pack index 3bde6a7b..88810baa 100755 --- a/pack +++ b/pack @@ -216,6 +216,7 @@ echoRed (){ } #--------------- +tstart=`date` revision=`svnversion . | sed "s|[A-Z]*||g"` echo "Revision=${revision}" setTopDefaults @@ -443,6 +444,8 @@ echo "SVN url: svn://svn.code.sf.net/p/healpix/code/branches/" >> ${rnfile} echo "SVN revision: ${revision}" >> ${rnfile} cat $rnfile cd ${here} +tend=`date` +echo "$tstart ... $tend" exit diff --git a/src/cxx/Healpix_cxx/alice3.cc b/src/cxx/Healpix_cxx/alice3.cc index 7869e2a7..41c6b255 100644 --- a/src/cxx/Healpix_cxx/alice3.cc +++ b/src/cxx/Healpix_cxx/alice3.cc @@ -29,56 +29,44 @@ * \author David Larson \author Martin Reinecke */ -#include -#include "announce.h" -#include "paramfile.h" -#include "healpix_map_fitsio.h" +#include "alice3.h" #include "lsconstants.h" #include "arr.h" -#include "fitshandle.h" #include "vec3.h" -#include "string_utils.h" #include "alm.h" #include "alm_healpix_tools.h" -#include "planck_rng.h" #include "healpix_map.h" using namespace std; -class PolarizationHolder +void PolarizationHolder::getQU(const pointing &p, double &q, double &u) const { - public: - Healpix_Map Q, U; - - void getQU(const pointing &p, double &q, double &u) const - { - fix_arr pix; - fix_arr wgt; - Q.get_interpol(p,pix,wgt); - q=u=0.f; - for (tsize i=0;i<4;++i) {q+=Q[pix[i]]*wgt[i];u+=U[pix[i]]*wgt[i]; } - } + fix_arr pix; + fix_arr wgt; + Q.get_interpol(p,pix,wgt); + q=u=0.f; + for (tsize i=0;i<4;++i) {q+=Q[pix[i]]*wgt[i];u+=U[pix[i]]*wgt[i]; } + } - vec3 getQUDir(const vec3 &loc) const - { - double q,u; - getQU(loc,q,u); - vec3 east(1,0,0); - if (abs(loc.x)+abs(loc.y) > 0.0) - east = vec3(-loc.y,loc.x,0).Norm(); - vec3 north = crossprod(loc, east); - double angle = 0.5*safe_atan2(u,q); - return north*(-cos(angle)) + east*sin(angle); - } +vec3 PolarizationHolder::getQUDir(const vec3 &loc) const + { + double q,u; + getQU(loc,q,u); + vec3 east(1,0,0); + if (abs(loc.x)+abs(loc.y) > 0.0) + east = vec3(-loc.y,loc.x,0).Norm(); + vec3 north = crossprod(loc, east); + double angle = 0.5*safe_atan2(u,q); + return north*(-cos(angle)) + east*sin(angle); + } - // Return the magnitude of the polarization at some pointing. - double getQUMagnitude(const pointing& p) const - { - double q,u; - getQU(p,q,u); - return sqrt(q*q + u*u); - } - }; +// Return the magnitude of the polarization at some pointing. +double PolarizationHolder::getQUMagnitude(const pointing& p) const + { + double q,u; + getQU(p,q,u); + return sqrt(q*q + u*u); + } /*! Steps from loc in direction dir for an angle theta and updates loc and dir. */ void get_step(const PolarizationHolder &ph, vec3 &loc, vec3 &dir, double theta) @@ -219,68 +207,3 @@ void lic_main(const Healpix_Map &Q, const Healpix_Map &U, const for (int i=0; i Q, U; - // Load a polarized fits file, with Q and U as the second - // and third columns (the standard form). - read_Healpix_map_from_fits(params.find("in"), Q, 2, 2); - read_Healpix_map_from_fits(params.find("in"), U, 3, 2); - - int nside = params.find("nside"); - int steps = params.find("steps",100); - double step_radian=arcmin2rad*params.find("step_arcmin",10.); - int kernel_steps = params.find("kernel_steps",50); - double polmin = params.find("polmin",-1e30), - polmax = params.find("polmax",1e30); - string out = params.find("out"); - - Healpix_Map th(nside,RING,SET_NSIDE); - if (params.param_present("texture")) - read_Healpix_map_from_fits(params.find("texture"),th); - else - { - planck_rng rng(params.find("rand_seed",42)); - if (params.param_present("ell")) - { - int ell = params.find("ell"); - if (ell<0) ell=2*nside; - Alm > a(ell,ell); - a.SetToZero(); - cout << "Background texture using ell = " << ell << endl; - - a(ell,0)=fcomplex(rng.rand_gauss(),0.); - for (int m=0; m<=ell; m++) - { a(ell,m).real(rng.rand_gauss()); a(ell,m).imag(rng.rand_gauss()); } - alm2map(a, th); - } - else - { - for (int i=0; i hit(nside,RING,SET_NSIDE), - tex(nside,RING,SET_NSIDE), - mag(nside,RING,SET_NSIDE); - - { - PolarizationHolder ph; - ph.Q = Q; - ph.U = U; - - for (int i=0; i Q, U; + void getQU(const pointing &p, double &q, double &u) const; + vec3 getQUDir(const vec3 &loc) const; + double getQUMagnitude(const pointing& p) const; +}; + void lic_main(const Healpix_Map &Q, const Healpix_Map &U, const Healpix_Map &th, Healpix_Map &hit, Healpix_Map &tex, Healpix_Map &mag, int steps, int kernel_steps, double step_radian, double polmin, double polmax); diff --git a/src/cxx/Healpix_cxx/alice3_main.cc b/src/cxx/Healpix_cxx/alice3_main.cc new file mode 100644 index 00000000..2f21991a --- /dev/null +++ b/src/cxx/Healpix_cxx/alice3_main.cc @@ -0,0 +1,112 @@ +/* + * This file is part of Healpix_cxx. + * + * Healpix_cxx is free software; you can redistribute it and/or modify + * it under the terms of the GNU General Public License as published by + * the Free Software Foundation; either version 2 of the License, or + * (at your option) any later version. + * + * Healpix_cxx is distributed in the hope that it will be useful, + * but WITHOUT ANY WARRANTY; without even the implied warranty of + * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the + * GNU General Public License for more details. + * + * You should have received a copy of the GNU General Public License + * along with Healpix_cxx; if not, write to the Free Software + * Foundation, Inc., 51 Franklin St, Fifth Floor, Boston, MA 02110-1301 USA + * + * For more information about HEALPix, see http://healpix.sourceforge.net + */ + +/* + * Healpix_cxx is being developed at the Max-Planck-Institut fuer Astrophysik + * and financially supported by the Deutsches Zentrum fuer Luft- und Raumfahrt + * (DLR). + */ + +/*! \file alice3.cc + * Copyright (C) 2005-2015 David Larson, Max-Planck-Society + * \author David Larson \author Martin Reinecke + */ + +#include +#include "alice3.h" +#include "announce.h" +#include "paramfile.h" +#include "healpix_map_fitsio.h" +#include "lsconstants.h" +#include "arr.h" +#include "fitshandle.h" +#include "vec3.h" +#include "string_utils.h" +#include "alm.h" +#include "alm_healpix_tools.h" +#include "planck_rng.h" +#include "healpix_map.h" + +using namespace std; + +int main(int argc, const char** argv) + { + module_startup ("alice3", argc, argv); + paramfile params (getParamsFromCmdline(argc,argv)); + + Healpix_Map Q, U; + // Load a polarized fits file, with Q and U as the second + // and third columns (the standard form). + read_Healpix_map_from_fits(params.find("in"), Q, 2, 2); + read_Healpix_map_from_fits(params.find("in"), U, 3, 2); + + int nside = params.find("nside"); + int steps = params.find("steps",100); + double step_radian=arcmin2rad*params.find("step_arcmin",10.); + int kernel_steps = params.find("kernel_steps",50); + double polmin = params.find("polmin",-1e30), + polmax = params.find("polmax",1e30); + string out = params.find("out"); + + Healpix_Map th(nside,RING,SET_NSIDE); + if (params.param_present("texture")) + read_Healpix_map_from_fits(params.find("texture"),th); + else + { + planck_rng rng(params.find("rand_seed",42)); + if (params.param_present("ell")) + { + int ell = params.find("ell"); + if (ell<0) ell=2*nside; + Alm > a(ell,ell); + a.SetToZero(); + cout << "Background texture using ell = " << ell << endl; + + a(ell,0)=fcomplex(rng.rand_gauss(),0.); + for (int m=0; m<=ell; m++) + { a(ell,m).real(rng.rand_gauss()); a(ell,m).imag(rng.rand_gauss()); } + alm2map(a, th); + } + else + { + for (int i=0; i hit(nside,RING,SET_NSIDE), + tex(nside,RING,SET_NSIDE), + mag(nside,RING,SET_NSIDE); + + { + PolarizationHolder ph; + ph.Q = Q; + ph.U = U; + + for (int i=0; i template double x = (cosrbig-z*z0)*xa; double ysq = 1-z*z-x*x; double dphi=-1; + bool fullcircle = false; if (ysq<=0) // no intersection, ring completely inside or outside - dphi = (fct==1) ? 0: pi-1e-15; + { + if (fct==1) + dphi = 0; + else + { + fullcircle = true; + dphi = pi-1e-15; + } + } else dphi = atan2(sqrt(ysq),x); if (dphi>0) @@ -231,6 +240,16 @@ template template I ip_lo = ifloor(nr*inv_twopi*(ptg.phi-dphi) - shift)+1; I ip_hi = ifloor(nr*inv_twopi*(ptg.phi+dphi) - shift); + if (fullcircle) // make sure we test the entire ring + { + if (ip_hi-ip_lo0) + --ip_lo; + else + ++ip_hi; + } + } if (fct>1) { @@ -417,24 +436,27 @@ template template { double x = (cosrbig[j]-z*z0[j])*xa[j]; double ysq = 1.-z*z-x*x; - double dphi = (ysq<=0) ? pi-1e-15 : atan2(sqrt(ysq),x); - I ip_lo = ifloor(nr*inv_twopi*(ptg[j].phi-dphi) - shift)+1; - I ip_hi = ifloor(nr*inv_twopi*(ptg[j].phi+dphi) - shift); - if (fct>1) + if (ysq>0) { - while ((ip_lo<=ip_hi) && check_pixel_ring - (*this,b2,ip_lo,nr,ipix1,fct,z0[j],ptg[j].phi,cosrsmall[j],cpix[j])) - ++ip_lo; - while ((ip_hi>ip_lo) && check_pixel_ring - (*this,b2,ip_hi,nr,ipix1,fct,z0[j],ptg[j].phi,cosrsmall[j],cpix[j])) - --ip_hi; + double dphi = atan2(sqrt(ysq),x); + I ip_lo = ifloor(nr*inv_twopi*(ptg[j].phi-dphi) - shift)+1; + I ip_hi = ifloor(nr*inv_twopi*(ptg[j].phi+dphi) - shift); + if (fct>1) + { + while ((ip_lo<=ip_hi) && check_pixel_ring + (*this,b2,ip_lo,nr,ipix1,fct,z0[j],ptg[j].phi,cosrsmall[j],cpix[j])) + ++ip_lo; + while ((ip_hi>ip_lo) && check_pixel_ring + (*this,b2,ip_hi,nr,ipix1,fct,z0[j],ptg[j].phi,cosrsmall[j],cpix[j])) + --ip_hi; + } + if (ip_hi>=nr) + { ip_lo-=nr; ip_hi-=nr;} + if (ip_lo<0) + tr.remove(ipix1+ip_hi+1,ipix1+ip_lo+nr); + else + tr.intersect(ipix1+ip_lo,ipix1+ip_hi+1); } - if (ip_hi>=nr) - { ip_lo-=nr; ip_hi-=nr;} - if (ip_lo<0) - tr.remove(ipix1+ip_hi+1,ipix1+ip_lo+nr); - else - tr.intersect(ipix1+ip_lo,ipix1+ip_hi+1); } pixset.append(tr); } diff --git a/src/cxx/Healpix_cxx/hpxtest.cc b/src/cxx/Healpix_cxx/hpxtest.cc index 712181a1..92683f6c 100644 --- a/src/cxx/Healpix_cxx/hpxtest.cc +++ b/src/cxx/Healpix_cxx/hpxtest.cc @@ -864,6 +864,18 @@ void check_issue_229 (Healpix_Ordering_Scheme scheme) } } +void check_issue_968 () + { + cout << "checking issue #968" << endl; + int nside=4; + Healpix_Base base (nside,RING,SET_NSIDE); + pointing ptg(174*pi/180., 45*pi/180.); + vector res; + base.query_disc_inclusive (ptg, 9.9*pi/180., res, 4); + if (find(res.begin(), res.end(), 190) == res.end()) + FAIL(cout << " PROBLEM: issue 968" << endl) + } + void check_query_disc_strict (Healpix_Ordering_Scheme scheme) { cout << "testing whether all pixels found by query_disc() really" << endl @@ -1586,6 +1598,7 @@ int main(int argc, const char **argv) check_query_polygon(); check_ringweights(); check_fullweights(); + check_issue_968(); #ifdef UNITTESTS if (errcount>0) planck_fail("unit test errors"); #endif diff --git a/src/cxx/Makefile.am b/src/cxx/Makefile.am index da725939..07248207 100644 --- a/src/cxx/Makefile.am +++ b/src/cxx/Makefile.am @@ -67,7 +67,8 @@ src_healpix_cxx= \ Healpix_cxx/moc_query.cc \ Healpix_cxx/weight_utils.h \ Healpix_cxx/weight_utils.cc \ - Healpix_cxx/mask_tools.cc + Healpix_cxx/mask_tools.cc \ + Healpix_cxx/alice3.cc src_healpix_cxx_fits= \ Healpix_cxx/healpix_data_io.cc \ Healpix_cxx/healpix_data_io.h \ @@ -129,7 +130,7 @@ libhealpix_cxx_la_LIBADD = $(SHARP_LIBS) $(CFITSIO_LIBS) # - Always increase the revision value. # - Increase the current value whenever an interface has been added, removed or changed. # - Increase the age value only if the changes made to the ABI are backward compatible. -libhealpix_cxx_la_LDFLAGS = -version-info 3:4:0 +libhealpix_cxx_la_LDFLAGS = -version-info 4:5:0 bin_PROGRAMS = alm2map_cxx anafast_cxx calc_powspec hotspots_cxx map2tga \ median_filter_cxx mult_alm rotalm_cxx smoothing_cxx syn_alm_cxx udgrade_cxx \ @@ -163,7 +164,7 @@ compute_weights_SOURCES = Healpix_cxx/compute_weights.cc Healpix_cxx/compute_wei compute_weights_LDADD = libhealpix_cxx.la needlet_tool_SOURCES = Healpix_cxx/needlet_tool.cc Healpix_cxx/needlet_tool_module.cc needlet_tool_LDADD = libhealpix_cxx.la -alice3_SOURCES = Healpix_cxx/alice3.cc +alice3_SOURCES = Healpix_cxx/alice3_main.cc alice3_LDADD = libhealpix_cxx.la hpxtest_SOURCES=Healpix_cxx/hpxtest.cc hpxtest_LDADD = libhealpix_cxx.la diff --git a/src/cxx/NEWS b/src/cxx/NEWS index fec2e190..564f614c 100644 --- a/src/cxx/NEWS +++ b/src/cxx/NEWS @@ -1,3 +1,11 @@ +Changes since 3.82: +- bug fix in query_polygon where pixels might be missing in some situations + where polygon edges were parallel to the equator. + (https://github.com/healpy/healpy/issues/904). +- bug fix in query_disc_inclusive where pixels could be missing at locations + exactly azimuthally opposite to the disc center. + (https://github.com/healpy/healpy/issues/968) + Changes since 3.50: - Configuration mechanism was completely switched to autotools - major performance increase for spherical harmonic transforms thanks to diff --git a/src/cxx/configure.ac b/src/cxx/configure.ac index 3d99dd01..91dc7a4e 100644 --- a/src/cxx/configure.ac +++ b/src/cxx/configure.ac @@ -1,4 +1,4 @@ -AC_INIT([healpix_cxx],[3.82.0]) +AC_INIT([healpix_cxx],[3.83.0]) AM_INIT_AUTOMAKE([foreign subdir-objects -Wall -Werror]) AM_MAINTAINER_MODE([enable]) @@ -36,10 +36,6 @@ AC_OPENMP CXXFLAGS="$CXXFLAGS $OPENMP_CFLAGS" AC_LANG_POP([C++]) -PKG_CHECK_MODULES([ZLIB], [zlib], , [ZLIB_LIBS=-lz]) -CFLAGS="$CFLAGS $ZLIB_CFLAGS" -LIBS="$LIBS $ZLIB_LIBS" - dnl dnl Determine the compiler flags (CFITSIO_CFLAGS) dnl and linker flags (CFITSIO_LIBS) required to build against libcfitsio. @@ -56,10 +52,6 @@ dnl pkg-config, CFITSIO_LIBS defaults to "-lcfitsio". dnl PKG_CHECK_MODULES([CFITSIO], [cfitsio], , [CFITSIO_LIBS=-lcfitsio]) dnl -dnl Linking against libcfitsio requires libm too. -dnl -CFITSIO_LIBS="$CFITSIO_LIBS -lm" -dnl dnl With pkg-config < 0.24, PKG_CHECK_MODULES does not AC_SUBST the _CFLAGS dnl and _LIBS variables. dnl diff --git a/src/f90/mod/healpix_types.F90 b/src/f90/mod/healpix_types.F90 index f9cd1845..2e6b8d7d 100644 --- a/src/f90/mod/healpix_types.F90 +++ b/src/f90/mod/healpix_types.F90 @@ -39,7 +39,7 @@ MODULE healpix_types ! Mars 2008: i8b same as i4b on machines not supporting 64 bits (NO64BITS flag set) ! Feb 2009: introduce healpix_version ! - character(len=*), PARAMETER, public :: healpix_version = '3.82' + character(len=*), PARAMETER, public :: healpix_version = '3.83' INTEGER, PARAMETER, public :: i4b = SELECTED_INT_KIND(9) #ifdef NO64BITS INTEGER, PARAMETER, public :: i8b = i4b diff --git a/src/idl/HEALPix_startup b/src/idl/HEALPix_startup index c04e21a1..0c569368 100644 --- a/src/idl/HEALPix_startup +++ b/src/idl/HEALPix_startup @@ -15,6 +15,7 @@ ; 2008-02-24 E. Hivon Use path_sep(/search) to separate directories ; 2008-03-17 E. Hivon Use IDL_PATH to set !path ; 2008-10-24 E. Hivon Print welcome message +; 2023-12-13 E. Hivon Make sure to delete internal variables upon exit ; ;********************************************************************* ; @@ -66,11 +67,11 @@ ; compile routines ; ; check that init_healpix is accessible -pathtab = expand_path(!path,/array) -junk = file_search(pathtab+path_sep()+'init_healpix.pro', count=count) +__hsu_pathtab__ = expand_path(!path,/array) +__hsu_junk__ = file_search(__hsu_pathtab__+path_sep()+'init_healpix.pro', count=__hsu_count__) ; run init_healpix to define Healpix variables, and print welcome message -if (count gt 0) then begin $ +if (__hsu_count__ gt 0) then begin $ init_healpix & $ print,'**************************' & $ print,' Welcome to Healpix '+!healpix.version & $ @@ -81,7 +82,9 @@ endif else begin $ print,'!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!!' & $ endelse -if (count gt 0 && is_gdl()) then !PROMPT = 'HGDL> ' +if (__hsu_count__ gt 0 && is_gdl()) then !PROMPT = 'HGDL> ' + +delvar, __hsu_count__, __hsu_junk__, __hsu_pathtab__ ; ; return to interactive mode diff --git a/src/idl/misc/init_healpix.pro b/src/idl/misc/init_healpix.pro index dc6ee57f..f4c59beb 100644 --- a/src/idl/misc/init_healpix.pro +++ b/src/idl/misc/init_healpix.pro @@ -70,10 +70,10 @@ pro init_healpix, verbose=verbose healpix_sysvar = '!HEALPIX' ; Healpix version -version = '3.82' +version = '3.83' ; release data -date = '2022-07-29' +date = '2024-10-09' ; Healpix directory diff --git a/src/idl/zzz_external/README b/src/idl/zzz_external/README index 67d51b49..7465a721 100644 --- a/src/idl/zzz_external/README +++ b/src/idl/zzz_external/README @@ -11,12 +11,12 @@ libraries apply for these procedures. o ./astron/ : required routines from THE IDL ASTRONOMY USER'S LIBRARY - (https://idlastro.gsfc.nasa.gov/homepage.html) + (https://github.com/wlandsman/IDLAstro) including their supporting D. Fanning's COYOTE routines - (http://www.idlcoyote.com/documents/programs.php) + (now in https://asd.gsfc.nasa.gov/archive/idlastro/ftp/coyote_astron.tar.gz) o ./cgis/ : required routines from the COBE cgis library - (used to be in http://space.gsfc.nasa.gov/astro/cobe/cgis.html) + (https://lambda.gsfc.nasa.gov/product/cobe/cgis.cfm) o ./obsolete_astron/ : routines from the Astron library which are now considered obsolete, but may still be needed by Healpix (or by user-developped applications). @@ -27,7 +27,7 @@ o ./epstopdf/ : Perl script to turn (encapsulated) PostScript file into PDF and its documentation see ./epstopdf/README for details - (added 2015-03) + (added 2015-03, updated 2024-09) o ./textoidl/ : IDL routines to emulate a subset of TeX commands in IDL see ./textoidl/README for details @@ -38,6 +38,7 @@ updated 2007-05-15 updated 2013-02-08 updated 2017-06-20 + updated 2024-09-30 AJB, KMG, EH ---------------- @@ -286,8 +287,17 @@ FITS_INFO FXADDPAR MATCH MRDFITS SXADDPAR SXPAR WRITEFITS 2 routines updated in astron(11) CGGETCOLORSTATE FITS_INFO mrdfits was not updated as it fails some tests - (10) This version of astron requires IDL v6.4 or newer. + (11) This version of astron requires IDL v6.4 or newer. Done with version 2022-07-27 2022-07-27 +---------------- + +2 routines updated in astron(12) MRDFITS FXBREAD + + (12) This version of astron requires IDL v6.4 or newer. + Done with version 2022-11-22 + + 2024-09-27 + EH diff --git a/src/idl/zzz_external/astron/fxbread.pro b/src/idl/zzz_external/astron/fxbread.pro index 0fd274fa..548336e0 100644 --- a/src/idl/zzz_external/astron/fxbread.pro +++ b/src/idl/zzz_external/astron/fxbread.pro @@ -134,8 +134,12 @@ ; Version 17, William Thompson/Terje Fredvik, 30-Aug-2018, preserve ; original dimensionality ; Version 18, William Thompson, 31-Aug-2018, correction to v17 +; Version 19, William Thompson, 09-Nov-2022, fix bug when reading +; multi-dimensional arrays over multiple lines. +; Version 20, William Thompson, 18-Nov-2022, fix bug introduced in +; version 19 when reading string arrays ; Version : -; Version 18, 31-Aug-2018 +; Version 20, 18-Nov-2022 ;- ; @fxbintable @@ -320,8 +324,11 @@ CHECK_ROW: DATA = MAKE_ARRAY(TYPE=DATATYPE,DIMENSION=DIMS) DATA = REFORM(DATA,DIMS,/OVERWRITE) READU,UNIT,DATA + DIMS2 = DIMS END ELSE BEGIN DIMS2 = [DIMS, ROW2-ROW1+1] + IF (N_ELEMENTS(DIMS) EQ 1) AND (DIMS[0] EQ 1) THEN $ + DIMS2 = DIMS2[1] DATA = MAKE_ARRAY(TYPE=DATATYPE, DIMENSION=DIMS2) DATA = REFORM(DATA, DIMS2, /OVERWRITE) TEMPDATA = MAKE_ARRAY(TYPE=DATATYPE, DIMENSION=DIMS) @@ -339,6 +346,7 @@ CHECK_ROW: ; IF IDLTYPE[ICOL,ILUN] EQ 7 THEN BEGIN DATA = STRING(DATA) + IF N_ELEMENTS(DIMS2) EQ 1 THEN DIMS2 = 1 ELSE DIMS2 = DIMS2[1:*] COUNT = 0 ; ; Otherwise, if necessary, then convert the data to the native format of the @@ -369,11 +377,11 @@ CHECK_ROW: BSCALE = TSCAL[ICOL,ILUN] IF (BSCALE NE 0) AND (BSCALE NE 1) THEN DATA *= BSCALE IF BZERO NE 0 THEN DATA += BZERO - IF N_ELEMENTS(DIMS) NE 1 THEN BEGIN - DDIMS = DIMS + IF N_ELEMENTS(DIMS2) NE 1 THEN BEGIN + DDIMS = DIMS2 IF (SIZE(DATA,/TNAME) EQ 'STRING') AND $ - (PRODUCT(DIMS) GT N_ELEMENTS(DATA)) THEN $ - DDIMS = DIMS[1:*] + (PRODUCT(DIMS2) GT N_ELEMENTS(DATA)) THEN $ + DDIMS = DIMS2[1:*] IF N_ELEMENTS(DDIMS) NE 1 THEN $ DATA = REFORM(DATA, DDIMS, /OVERWRITE) ENDIF diff --git a/src/idl/zzz_external/astron/mrdfits.pro b/src/idl/zzz_external/astron/mrdfits.pro index aeb3bf23..c6c049c8 100644 --- a/src/idl/zzz_external/astron/mrdfits.pro +++ b/src/idl/zzz_external/astron/mrdfits.pro @@ -171,8 +171,9 @@ ; user specifies the same value for the STRUCTYP keyword ; in calls to MRDFITS in the same IDL session for extensions ; which have different structures. -; /UNSIGNED - For integer data with appropriate zero points and scales -; read the data into unsigned integer arrays. +; /UNSIGNED - For integer image data with appropriate zero points and scales, +; read the data into unsigned integer arrays. This is the +; default for binary tables. ; /USE_COLNUM - When creating column names for binary and ASCII tables ; MRDFITS attempts to use the appropriate TTYPE keyword ; values. If USE_COLNUM is specified and non-zero then @@ -385,8 +386,9 @@ ; V2.23 Use 64 bit for very large files WL April 2014 ; V2.24 Binary table is allowed to have zero columns WL September 2018 ; V2.25 Use long64 for ASCII table integers longer than I12 WL October 2020 -; 2021-06-2*: replaced -9223372036854775808LL by 2LL^63 (line 984), -; same value but accepted by FL (https://bitbucket.org/fawlty/fl) +; V2.26 Use '8000000000000000'xll long64 offset for GDL/FL compatibility WL Aug 2021 +; V2.27 Allow different columns to have different datatypes for TSCALn and TZEROn +; Use ULONG64() when necessary WL Sep 2021 ;- PRO mrd_fxpar, hdr, xten, nfld, nrow, rsize, fnames, fforms, scales, offsets compile_opt idl2, hidden @@ -441,8 +443,8 @@ compile_opt idl2, hidden ;; The others fnames = strarr(n_mforms) fforms = strarr(n_mforms) - scales = dblarr(n_mforms) - offsets = dblarr(n_mforms) + scales = ptrarr(n_mforms, /all) + offsets = ptrarr(n_mforms, /all) ;;comments = strarr(n_mnames) @@ -457,7 +459,6 @@ compile_opt idl2, hidden match, keyword, scales_names, mkey_scales, mscales, count = N_mscales match, keyword, offsets_names, mkey_offsets, moffsets,count = N_moffsets - FOR in=0L, nnames-1 DO BEGIN CASE names[in] OF @@ -489,6 +490,7 @@ compile_opt idl2, hidden ENDCASE ;;help,matches,nmatches + ptr = size(result,/tname) EQ 'POINTER' ;Is it a pointer? ; ; Extract the parameter field from the specified header lines. If one of the @@ -570,6 +572,7 @@ NEXT_APOST: NOT_COMPLEX: ON_IOERROR, GOT_VALUE value = test + IF ~VALID_NUM(value) THEN GOTO, GOT_VALUE IF (STRPOS(value,'.') GE 0) || (STRPOS(value,'E') $ @@ -581,9 +584,13 @@ NOT_COMPLEX: ENDIF ELSE BEGIN lmax = long64(2)^31 - 1 lmin = -long64(2)^31 - value = long64(value) + if strmid(value,0,1) NE '-' then begin + value = ulong64(value) + if value lt ulong64(2)^63-1 then value = long64(value) + endif else value = long64(value) if (value GE lmin) && (value LE lmax) THEN $ value = LONG(value) + ENDELSE ; @@ -591,22 +598,23 @@ GOT_VALUE: ON_IOERROR, NULL ENDELSE ENDELSE ; if string + ; ; Add to vector if required. ; - - result[tmatches[i]] = value + if ptr then $ + *result[tmatches[i]] = value else $ + result[tmatches[i]] = value ENDFOR - + CASE names[in] OF 'TTYPE': fnames[number] = strtrim(result, 2) 'TFORM': fforms[number] = strtrim(result, 2) - 'TSCAL': scales[number] = result - 'TZERO': offsets[number] = result + 'TSCAL': scales[number] = result + 'TZERO': offsets[number] = result ELSE: message,'What?' ENDCASE - ; ; Error point for keyword not found. ; @@ -616,8 +624,8 @@ GOT_VALUE: ENDFOR + END - ; Get a tag name give the column name and index function mrd_dofn, name, index, use_colnum, alias=alias @@ -734,7 +742,7 @@ compile_opt idl2, hidden if scale eq 1 then begin if (bitpix eq 16 && zero eq 32768L) || $ (bitpix eq 32 && zero eq 2147483648UL) || $ - (bitpix eq 64 && zero eq 9223372036854775808ULL) then return,1 + (bitpix eq 64 && zero eq '8000000000000000'xll ) then return,1 endif return, 0 @@ -753,7 +761,7 @@ end ; Return the currrent version string for MRDFITS function mrd_version compile_opt idl2, hidden - return, '2.25 ' + return, '2.26 ' end ;===================================================================== ; END OF GENERAL UTILITY FUNCTIONS =================================== @@ -981,7 +989,7 @@ compile_opt idl2, hidden return endif ; Special test for long64 integers - if (ftype EQ 'I') && (lenarr[i] GT 12) then sclstr[j] = 2LL^63 ; -9223372036854775808LL + if (ftype EQ 'I') && (lenarr[i] GT 12) then sclstr[j] = '8000000000000000'xll fvalues[i] = ftype NE 'A' ? sclstr[j] : $ 'string(replicate(32b,'+strtrim(flen,2)+'))' @@ -2141,7 +2149,6 @@ compile_opt idl2, hidden if range[0] gt 0 then mrd_skip, unit, rsize*range[0] readu,unit, table if N_elements(rows) GT 0 then table = table[rows- range[0]] - ; Move to the beginning of the heap -- we may have only read some rows of ; the data. if range[1] lt nrows-1 then begin @@ -2309,8 +2316,9 @@ pro mrd_table, header, structyp, use_colnum, $ ;; Use scale=1 if not found if nnames GT 0 then begin - wsc=where(scales EQ 0.0d,nwsc) - IF nwsc NE 0 THEN scales[wsc] = 1.0d + for i = 0,N_elements(scales)-1 do $ + if *scales[i] EQ 0.0d then *scales[i] = 1.0d + endif xten = strtrim(xten,2) @@ -2404,7 +2412,7 @@ pro mrd_table, header, structyp, use_colnum, $ ; Add in the structure label. ; - + ; Handle variable length columns. if (ftype eq 'P') || (ftype eq 'Q') then begin @@ -2425,10 +2433,9 @@ pro mrd_table, header, structyp, use_colnum, $ vcls[i] = 1 - xunsigned = mrd_chkunsigned(bitpix[ppos], scales[i], $ offsets[i], $ - unsigned=unsigned) + unsigned=1) if (xunsigned) then begin @@ -2447,14 +2454,13 @@ pro mrd_table, header, structyp, use_colnum, $ for j=0, n_elements(types) - 1 do begin if ftype eq types[j] then begin - - xunsigned = mrd_chkunsigned(bitpix[j], scales[i], $ - offsets[i], $ - unsigned=unsigned) + xunsigned = mrd_chkunsigned(bitpix[j], *scales[i], $ + *offsets[i], $ + unsigned=1) if xunsigned then begin fxaddpar, header, 'TZERO'+istr, 0, 'Modified by MRDFITS V'+mrd_version() - offsets[i] = 0 ;; C. Markwardt Aug 2007 - reset to zero so offset is not applied twice' + *offsets[i] = 0 ;; C. Markwardt Aug 2007 - reset to zero so offset is not applied twice' endif if dim eq 0 then begin @@ -2662,7 +2668,6 @@ function mrdfits, file, extension, header, $ status = -2 return, 0 endif - mrd_hread, unit, header, status, SILENT = silent, ERRMSG = errmsg if status lt 0 then begin diff --git a/src/idl/zzz_external/astron/update_idl_astron_lib.s b/src/idl/zzz_external/astron/update_idl_astron_lib.s index 7f3452a6..f066d92c 100755 --- a/src/idl/zzz_external/astron/update_idl_astron_lib.s +++ b/src/idl/zzz_external/astron/update_idl_astron_lib.s @@ -13,6 +13,7 @@ # 2014-01-06: deal with latest version # 2016-08-22: detect duplicates # Note: do not use github because it does not include the Coyote directory +# 2024-09-27: switch to github (with a hand made link to coyote directory) # # directory with new routines set dir = /Applications/itt/external_contributions/astron/pro/ diff --git a/src/idl/zzz_external/epstopdf/README b/src/idl/zzz_external/epstopdf/README index 7eaaae33..56f02d32 100644 --- a/src/idl/zzz_external/epstopdf/README +++ b/src/idl/zzz_external/epstopdf/README @@ -1,12 +1,12 @@ -$Id: README 42921 2017-01-10 23:39:44Z karl $ +$Id: README 71121 2024-04-29 17:27:25Z karl $ This file is public domain. (Originally written by Karl Berry, 2009.) This is the README for the epstopdf script distribution. -Primary distribution point: http://ctan.org/pkg/epstopdf - (list of mirrors at: http://ctan.org/mirrors) +Primary distribution point: https://ctan.org/pkg/epstopdf + (list of mirrors at: https://ctan.org/mirrors) -Home page: http://tug.org/epstopdf/ +Home page: https://tug.org/epstopdf/ Run epstopdf --help for the usual list of options, examples, etc. @@ -18,7 +18,7 @@ options, so the problem can be reproduced. Various test files and a Makefile to exercise them are in the source repository, which is currently a subdirectory of the texlive Subversion repo, purely for the developers' convenience: - http://tug.org/svn/texlive/trunk/Build/source/extra/epstopdf/ + http://tug.org/svn/texlive/trunk/Build/extra/epstopdf/ The test-binary and test-bin2 files there were supplied by Akira Kakuto and Reinhard Kotucha. They contain binary data. They are public domain. diff --git a/src/idl/zzz_external/epstopdf/epstopdf.1 b/src/idl/zzz_external/epstopdf/epstopdf.1 index 3e64f1ab..cf993d31 100644 --- a/src/idl/zzz_external/epstopdf/epstopdf.1 +++ b/src/idl/zzz_external/epstopdf/epstopdf.1 @@ -1,36 +1,36 @@ -.TH EPSTOPDF 1 "17 September 2018" -.\" $Id: epstopdf.1 48681 2018-09-16 23:03:58Z karl $ +.TH EPSTOPDF 1 "29 April 2024" +.\" $Id: epstopdf.1 71121 2024-04-29 17:27:25Z karl $ .SH NAME epstopdf, repstopdf \- convert an EPS file to PDF .SH SYNOPSIS \fBepstopdf\fP [\fIoptions\fP] [\fIepsfile\fP [\fIpdffile\fP.pdf]] .SH DESCRIPTION -By default, \fBepstopdf\fP converts the input PostScript file to PDF, +\fBepstopdf\fP converts the input PostScript file to PDF, by default using Ghostscript. .PP -\fBEpstopdf\fP transforms the Encapsulated PostScript file \fIepsfile\fP -(or standard input) so that it is guaranteed to start at the 0,0 -coordinate, and it sets a page size exactly corresponding to the -BoundingBox. Thus, the result needs no cropping, and the PDF MediaBox -is correct. +In more detail: \fBepstopdf\fP transforms the Encapsulated PostScript +file \fIepsfile\fP (or standard input) so that it is guaranteed to start +at the 0,0 coordinate, and it sets a page size exactly corresponding to +the BoundingBox. Thus, the result needs no cropping, and the PDF +MediaBox is correct. .PP By default, the output name is the input name with any extension replaced by \fB.pdf\fP. An output name ending with .pdf can also be given as a second argument on the command line, or the \fB--outfile\fP (\fB-o\fP) option can be used with any name. .PP -The output is PDF 1.5 by default; use, e.g., +The output is PDF 1.5 by default. To change this, use, for example .nf --gsopt=-dCompatibilityLevel=1.7 .fi -to change this. (Until epstopdf 2.28 (released September 2018), the +(Until epstopdf 2.28 (released September 2018), the PDF version was whatever the underlying Ghostscript or other interpreter produced by default.) .PP PJL commands at the start of a file are removed. DOS EPS binary files -(TN 5002) are supported. +(TN 5002) are supported. Seeking from a pipe is not supported. .PP -If the bounding box in the input is incorrect, of course there will +If the bounding box in the input is incorrect, inevitably there will be resulting problems. .SH OPTIONS Options may start with either "\fB-\fP" or "\fB--\fP", and may be @@ -48,7 +48,8 @@ write result to \fIfile\fP. If this option is not given, and otherwise, the default is to construct the output file name by replacing any extension in the input file with `.pdf'. .IP "\fB--\fP[\fBno\fP]\fBdebug\fP" -write debugging info (default: false). +write debugging info (default: false). For maximum output, use \fB--debug\fP +as the first option. .IP "\fB--\fP[\fBno\fP]\fBexact\fP" scan ExactBoundingBox (default: false). .IP "\fB--\fP[\fBno\fP]\fBfilter\fP" @@ -62,13 +63,16 @@ is, the input PostScript as modified by \fBepstopdf\fP. scan HiresBoundingBox (default: false). .IP "\fB--restricted\fP=\fIval\fP" turn on restricted mode (default: [true for repstopdf, else false]); -this forbids the use of \fB--gscmd\fP and other options and imposes +this forbids the use of \fB--gscmd\fP, among other options, and imposes restrictions on the input and output file names according to the values -of openin_any and openout_any (see the Web2c manual, http://tug.org/web2c). +of openin_any and openout_any (see the Web2c manual, https://tug.org/web2c). +On Windows, the Ghostscript command is forced to be the TeX Live builtin +gs, installed under \fB.../tlpkg/tlgs/bin/\fP. .PP Options for Ghostscript (more info below): .IP "\fB--gscmd\fP=\fIval\fP" -pipe output to \fIval\fP (default: [\fBgswin32c\fP on Windows, else \fBgs\fP]) +pipe output to \fIval\fP (default: [\fBgswin64c.exe\fP on 64-bit Windows, +\fBgswin32c.exe\fP on 32-bit Windows, else \fBgs\fP]) .IP "\fB--gsopt\fP=\fIval\fP" include \fIval\fP as one argument in the gs command (can be repeated). .IP "\fB--gsopts\fP=\fIval\fP" @@ -79,15 +83,15 @@ set AutoRotatePages (default: None); recognized \fIval\fP choices: None, All, PageByPage. For EPS files, PageByPage is equivalent to All. .IP "\fB--\fP[\fBno\fP]\fBcompress\fP" use compression in the output (default: true); if turned off, passes -.IR -dUseFlateCompression=false . +.BR -dUseFlateCompression=false . .IP "\fB--device\fP=\fIdev\fP" -use -sDEVICE=\fIdev\fP (default: pdfwrite); not allowed in restricted mode. +use \fB-sDEVICE=\fIdev\fR (default: pdfwrite); not allowed in restricted mode. .IP "\fB--\fP[\fBno\fP]\fBembed\fP" embed fonts (default: true); passes -.I -dMaxSubsetPct=100 -dSubsetFonts=true -dEmbedAllFonts=true. +.B -dMaxSubsetPct=100 -dSubsetFonts=true -dEmbedAllFonts=true. .IP "\fB--\fP[\fBno\fP]\fBgray\fP" grayscale output (default: false); passes -.I -sColorConversionStrategy=Gray -dProcessColorModel=/DeviceGray. +.B -sColorConversionStrategy=Gray -dProcessColorModel=/DeviceGray. .IP "\fB--pdfsettings\fP=\fIval\fP" use -dPDFSETTINGS=/\fIval\fP (default is `prepress' if \fB--embed\fP, else empty); recognized \fIval\fP choices: screen, ebook, printer, @@ -95,26 +99,29 @@ prepress, default. .IP "\fB--\fP[\fBno\fP]\fBquiet\fP" use -q, a.k.a. -dQUIET (default: false). .IP "\fB--res\fP=\fIdpi, dpi\fPx\fIdpi\fP" -set image resolution (default: [use gs default]); ignored if -\fB--debug\fP is set. +set image resolution (default: [use gs default]). .IP "\fB--\fP[\fBno\fP]\fBsafer\fP" -use -d(NO)QUIET (default: true). +use -d(NO)SAFER (default: true). .PP In addition to the specific options above, additional options to be used with gs can be specified with either or both of the two cumulative options \fB--gsopts\fP and \fB--gsopt.\fP .PP \fB--gsopts\fP takes a single string of options, which is split at -whitespace, each resulting word then added to the gs command line +whitespace; each resulting word then added to the gs command line individually. .PP \fB--gsopt\fP adds its argument as a single option to the gs command -line. It can be used multiple times to specify options separately, -and is necessary if an option or its value contains whitespace. +line. It can be used multiple times to specify options separately. +This form must be used if a gs option or its value contains whitespace. .PP In restricted mode, options are limited to those with names and values known to be safe. Some options taking booleans, integers or fixed names are allowed, those taking general strings are not. +.PP +In order to give a comprehensible error message, epstopdf checks whether +kpsewhich and (the specified) gs are found in the current PATH, or +executable if they are specified as absolute names. .SH EXAMPLES These examples all equivalently convert `test.eps' to `test.pdf': @@ -132,24 +139,26 @@ epstopdf --hires test.eps .PP Example for \fBepstopdf\fP's attempt at correcting PostScript: .nf -$program --nogs test.ps >testcorr.ps +epstopdf --nogs test.ps >testcorr.ps .fi .PP -In all cases, you can add \fB--debug\fP (\fB-d\fP) to see more about -what \fBepstopdf\fP is doing. +In all cases, you can add \fB--debug\fP to see more about +what \fBepstopdf\fP is doing. Use \fB--debug\fP as the first option for +maximum output. .SH BUGS The case of "%%BoundingBox: (atend)" when input is not seekable (e.g., from a pipe) is not supported. .PP -Report bugs in the program or this man page to tex-k@tug.org. When -reporting bugs, please include an input file and the command line -options specified, so the problem can be reproduced. +Report bugs in the program or this man page to tex-k@tug.org +(https://lists.tug.org/tex-k). When reporting bugs, please include an +input file and the command line options specified, so the problem can be +reproduced. .SH SEE ALSO \fBgs\fP(1), \fBpdfcrop\fP(1). .PP -The epstopdf LaTeX package, part of the oberdiek bundle, which automates -running this script on the fly under TeX: http://ctan.org/pkg/epstopdf-pkg. +The epstopdf LaTeX package, which automates running this script on the +fly under LaTeX: https://ctan.org/pkg/epstopdf-pkg. .SH AUTHOR Originally written by Sebastian Rahtz, for Elsevier Science, with subsequent contributions from Thomas Esser, Gerben Wierda, Heiko @@ -157,6 +166,11 @@ Oberdiek, and many others. Currently maintained by Karl Berry. .PP Man page originally written by Jim Van Zandt. .PP -epstopdf home page: http://tug.org/epstopdf. +epstopdf package page on CTAN: https://ctan.org/pkg/epstopdf. +.PP +epstopdf home page: https://tug.org/epstopdf. .PP You may freely use, modify and/or distribute this man page. +The epstopdf script is released under the modified BSD license. +.PP +$Id: epstopdf.1 71121 2024-04-29 17:27:25Z karl $ diff --git a/src/idl/zzz_external/epstopdf/epstopdf.man1.pdf b/src/idl/zzz_external/epstopdf/epstopdf.man1.pdf index 7263dd3d..c824099b 100644 Binary files a/src/idl/zzz_external/epstopdf/epstopdf.man1.pdf and b/src/idl/zzz_external/epstopdf/epstopdf.man1.pdf differ diff --git a/src/idl/zzz_external/epstopdf/epstopdf.pl b/src/idl/zzz_external/epstopdf/epstopdf.pl index 5a956761..4fa1a590 100755 --- a/src/idl/zzz_external/epstopdf/epstopdf.pl +++ b/src/idl/zzz_external/epstopdf/epstopdf.pl @@ -1,5 +1,6 @@ #!/usr/bin/env perl -# $Id: epstopdf.pl 48681 2018-09-16 23:03:58Z karl $ +use warnings; +# $Id: epstopdf.pl 71777 2024-07-11 21:24:57Z karl $ # (Copyright lines below.) # # Redistribution and use in source and binary forms, with or without @@ -35,7 +36,47 @@ # # emacs-page # -my $ver = "2.28"; +my $ver = "2.36"; +# 2024/07/11 2.36 (Karl Berry) +# * regexp syntax for OS/2 test, found by John Collins. +# 2024/06/21 2.35 (Karl Berry) +# * path_sep for OS/2 is also ";". +# 2024/04/29 2.34 (Karl Berry) +# * if --debug is first argument, give more output. +# * do not check for kpsewhich in PATH unless restricted. +# * minor wording and doc changes. +# 2024/04/14 (John Collins) +# * use warnings. +# * Msys PATH separator is :. +# * Do immediate decomposition of path to array on startup, and use array +# instead of separate uses of split. +# * On Windows, Msys and Cygwin, normalize directory separator to /. +# * Detect invocation via Windows TL (and epstopdf.exe wrapper script) by +# presence of TL's private gs in PATH: a directory ending in /tlgs/bin. +# In this case, change behavior under Cygwin to be like that of Windows +# instead of Unix. +# * On Cygwin and Msys, put temporary file in current directory instead of +# default, which is normally /tmp. That's so that the pathname to the +# temporary file remains valid no matter which kind of gs it's passed to: +# native Windows, Msys or Cygwin. +# * Prettyprint PATH, one directory per line, in error about program +# not in PATH. +# Original report from Pablo Gonzalez L, +# https://tug.org/pipermail/tex-k/2024-April/004036.html +# 2023/09/15 2.33 (Karl Berry) +# * Cygwin PATH separator is :. Report from Alois Steindl, +# https://tug.org/pipermail/tex-live/2023-September/049474.html +# 2023/07/08 2.32 (Karl Berry) +# * check that kpsewhich and gs are in PATH. +# * correct TL path for kpsewhich to bin/windows. +# 2023/03/06 v2.31 (Karl Berry) +# * disallow --nosafer in restricted mode. +# * disallow output to pipes in restricted mode. +# Report from nikolay.ermishkin to tlsecurity. +# 2022/09/05 v2.30 (Siep Kroonenberg) +# * still use gswin32c if gswin64c.exe not on PATH. +# 2022/08/29 v2.29 (Karl Berry) +# * use gswin64c.exe on 64-bit Windows. # 2018/09/17 v2.28 (Karl Berry) # * -dCompatibilityLevel=1.5 by default, since gs9.25 switched to 1.7. # 2017/09/14 v2.27 (Karl Berry) @@ -189,9 +230,9 @@ ### emacs-page ### program identification my $program = "epstopdf"; -my $ident = '($Id: epstopdf.pl 48681 2018-09-16 23:03:58Z karl $)' . " $ver"; +my $ident = '($Id: epstopdf.pl 71777 2024-07-11 21:24:57Z karl $)' . " $ver"; my $copyright = < @@ -200,14 +241,111 @@ END_COPYRIGHT my $title = "$program $ident\n"; -my $on_windows = $^O =~ /^(MSWin|msys$)/; -my $on_windows_or_cygwin = $on_windows || $^O eq "cygwin"; +### message functions. +sub debug { print STDERR "* @_\n" if $::opt_debug; } +sub warning { print STDERR "==> Warning: @_\n"; } +sub error { die "$title!!! Error: @_\n"; } +sub errorUsage { die "$program: Error: @_ (try --help for more information)\n"; } +sub warnerr { $restricted ? error(@_) : warning(@_); } + +# Check specially for --debug or -d (exactly) as first argument, so we can +# generate debugging output during initialization. +$::opt_debug = 1 if @ARGV && ($ARGV[0] eq "--debug" || $ARGV[0] eq "-d"); + +# Different Windows cases. +my $on_cygwin = ($^O eq 'cygwin'); +my $on_msys = ($^O eq 'msys'); +my $on_windows = ($^O =~ /^MSWin/) || $on_msys; +my $on_windows_or_cygwin = $on_windows || $on_cygwin; +debug "on_windows=$on_windows, on_windows_or_cygwin=$on_windows_or_cygwin"; +debug " on_cygwin=$on_cygwin, on_msys=$on_msys"; + +# Split PATH and use / as directory separator. +# +my $path_sep = ($^O =~ /^(OS2|MSWin)/i) ? ';' : ':'; # not msys +my @pdirs = split($path_sep, $ENV{"PATH"}); +# Normalize directory separators to /. Always valid on Windows. +if ($on_windows_or_cygwin) { + foreach (@pdirs) { s !\\!/!g; } +} +debug "Normalized PATH to: @pdirs"; + +# Default values for commands. +# Ghostscript, which is always needed. +my $GS = 'gs'; +# Kpsewhich, only used in restricted mode. +my $kpsewhich = 'kpsewhich'; -### ghostscript command name -my $GS = $on_windows ? "gswin32c" : "gs"; +# Determine if we were invoked from a standard Windows TL installation via the +# wrapper script epstopdf.exe: +my $TL_Windows_bin = undef; +my $TL_tlgs = undef; +if ($on_windows_or_cygwin) { + debug "Looking for symptoms of Windows TL gs and wrapper .exe:"; + for (@pdirs) { + if (m!^(.+)/tlpkg/tlgs/bin$!) { + debug "Found Windows tlgs item '$_' in PATH"; + # We were probably invoked via runscript by .exe file in native TL + # Windows, since then a tlgs/bin item is inserted in PATH, + # so that Windows TL's private installation of gs, with its executables + # gswin64c.exe and/or gswin32c.exe gets used. + # Anything else giving the same symptom is surely a deliberate + # configuration to imitate that the TL Windows behavior. + my $TL_root = $1; + $TL_tlgs = $_; + $TL_Windows_bin = "$TL_root/bin/windows"; + last; + } + } + if ($TL_tlgs) { + # Confirm by existence of expected directories and files. + # If those do not exist, we don't have a standard native + # Windows TL installation. + if (-x "$TL_Windows_bin/kpsewhich.exe" + && (-x "$TL_tlgs/gswin64c.exe" || -x "$TL_tlgs/gswin32c.exe") + ) { + # The needed files exist. + # The runscript wrapper ensures that the tlgs and the binary directory + # of its own installation are in PATH ahead of any directories that + # may contain other versions. + } + else { + warning(<test.pdf @@ -404,8 +542,8 @@ Example for producing epstopdf's attempt at corrected PostScript: \$ $program --nogs test.ps >testcorr.ps -In all cases, you can add --debug (-d) to see more about what epstopdf -is doing. +In all cases, you can use --debug to see more about what epstopdf +is doing. For maximum output, use --debug as the first option. More about the options for Ghostscript: Additional options to be used with gs can be specified @@ -427,7 +565,7 @@ options so the problem can be reproduced. Report bugs to: tex-k\@tug.org -epstopdf home page: +epstopdf home page: END_OF_USAGE ### process options @@ -462,29 +600,60 @@ ### restricted option $restricted = 1 if $::opt_restricted; -### help functions -sub debug { print STDERR "* @_\n" if $::opt_debug; } -sub warning { print STDERR "==> Warning: @_\n"; } -sub error { die "$title!!! Error: @_\n"; } -sub errorUsage { die "$program: Error: @_ (try --help for more information)\n"; } -sub warnerr { $restricted ? error(@_) : warning(@_); } - ### debug messages debug "Restricted mode activated" if $restricted; -### safer external commands for Windows in restricted mode -my $kpsewhich = 'kpsewhich'; -if ($restricted && $on_windows) { - use File::Basename; - my $mydirname = dirname $0; - # $mydirname is the location of the Perl script - $kpsewhich = "$mydirname/../../../bin/win32/$kpsewhich"; - $GS = "$mydirname/../../../tlpkg/tlgs/bin/$GS"; +### check that PROG is in PATH and executable, abort if not. It'd be +# better to actually try running the program, but then we'd have to +# either replicate Perl's logic for finding the command interpreter +# (trivial on Unix, complicated on Windows), or do a fork/exec and close +# the file descriptors ourselves, which seems too painful. Nor do we +# want to load/assume File::Which. Instead we'll look along PATH +# ourselves, which is good enough in practice for us, since the only +# goal here is to give a better error message if the program isn't +# available. +sub check_prog_exists { + my ($prog) = @_; + my @w_ext = ("exe", "com", "bat"); + debug " Checking if $prog is in PATH"; + # absolute unix + if (! $on_windows_or_cygwin && $prog =~ m,^((\.(\.)?)?/),) { + return 1 if -x $prog; # absolute or explicitly relative + error "Required program $prog not found, given with explicit directory"; + + # absolute windows: optional drive letter, then . or .., then \ or /. + } elsif ($on_windows_or_cygwin + && $prog =~ m,^(([a-zA-Z]:)?(\.(\.)?)?[/\\]),) { + return 1 if -x $prog; + for my $ext (@w_ext) { + return 1 if (-x "$prog.$ext"); + } + error "Required program $prog not found, given explicit Windows directory"; + } + + # not absolute, check path + for my $dir (@pdirs) { + $dir = "." if $dir eq ""; # empty path element + debug " Checking dir $dir"; + if (-x "$dir/$prog") { + return 1; + } elsif ($on_windows_or_cygwin) { + for my $ext (@w_ext) { + return 1 if (-x "$dir/$prog.$ext"); + } + } + } + + # if made it through the whole loop, not found, so quit. + my @path_pretty = (); + for (@pdirs) { push @path_pretty, " '$_'\n"; } + error "Required program $prog not found in PATH, which contains:\n", + @path_pretty; } -debug "kpsewhich command: $kpsewhich"; +check_prog_exists ($kpsewhich) if $restricted; # only needed if restricted ### check if a name is "safe" according to kpse's open(in|out)_any -# return true if name is ok, false otherwise +# return true if name is ok, false if not. sub safe_name { my ($mode, $name) = @_; my $option = ""; @@ -492,7 +661,8 @@ sub safe_name { $option = '-safe-out-name' if $mode eq 'out'; error "Unknown check mode in safe_name(): $mode" unless $option; my @args = ($kpsewhich, '-progname', 'repstopdf', $option, $name); - my $bad = system {$args[0]} @args; + debug "Checking safe_name with: @args"; + my $bad = system { $args[0] } @args; return ! $bad; } @@ -548,11 +718,24 @@ sub safe_name { $GS = $::opt_gscmd; } } +debug "GS command: $GS"; +check_prog_exists ($GS); + +### option (no)safer +my $gs_opt_safer = "-dSAFER"; +if (! $::opt_safer) { + if ($restricted) { + error "Option forbidden in restricted mode: --nosafer"; + } else { + debug "Switching from $gs_opt_safer to -dNOSAFER"; + $gs_opt_safer = "--nosafer"; + } +} ### start building GS command line for the pipe my @GS = ($GS); push @GS, '-q' if $::opt_quiet; -push @GS, $::opt_safer ? '-dSAFER' : '-dNOSAFER'; +push @GS, $gs_opt_safer; push @GS, '-dNOPAUSE'; push @GS, '-dBATCH'; push @GS, '-dCompatibilityLevel=1.5'; @@ -589,7 +772,13 @@ sub safe_name { $OutputFilename = "-"; } } -$OutputFilename =~ s/%/%%/g; # we will do the escaping for gs +# +# gs -sOutputFilename opens pipes itself if the string starts with +# %pipe or |. Disallow this in restricted mode. +if ($restricted && $OutputFilename =~ /^(%pipe|\|)/) { + error "Output to pipe forbidden in restricted mode: $OutputFilename"; +} +$OutputFilename =~ s/%/%%/g; # stop gs interpretation of % characters debug "Output filename:", $OutputFilename; push @GS, "-sOutputFile=$OutputFilename"; @@ -707,8 +896,15 @@ sub safe_name { debug "Ghostscript pipe: @GS"; open($OUT, '|-', @GS) or error "Cannot open Ghostscript for piped input: @GS"; - } else { # use a temporary file on Windows/Cygwin. - ($OUT, $tmp_filename) = tempfile(UNLINK => 1); + } else { + # use a temporary file on Windows/msys/Cygwin. + if ($on_cygwin || $on_msys) { + # Use current directory for temporary file, to avoid problems of + # translation of directory name if native Windows gs gets invoked. + ($OUT, $tmp_filename) = tempfile(UNLINK => 1, DIR => '.'); + } else { + ($OUT, $tmp_filename) = tempfile(UNLINK => 1); + } debug "Using temporary file '$tmp_filename'"; } $outname = $GS; @@ -717,6 +913,7 @@ sub safe_name { debug "No Ghostscript: opening $OutputFilename"; if ($OutputFilename eq "-") { $OUT = *STDOUT; + $outname = "-"; } else { open($OUT, '>', $OutputFilename) || error ("Cannot write \"$OutputFilename\": $!"); @@ -775,7 +972,7 @@ sub safe_name { debug " No checksum"; } else { - debug " checksum: $checksum"; + debug " Checksum: $checksum"; my $cs = 0; map { $cs ^= $_ } unpack('n14', $header); if ($cs != $checksum) { diff --git a/test/alm.fits b/test/alm.fits index 074a3c44..276c97c7 100644 --- a/test/alm.fits +++ b/test/alm.fits @@ -1,4 +1,4 @@ -SIMPLE = T / file does conform to FITS standard BITPIX = 32 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H DATE = '2022-07-28T14:24:16' / file creation date (YYYY-MM-DDThh:mm:ss UT) END XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 12 / width of table in bytes NAXIS2 = 33153 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 3 / number of fields in each row COMMENT **************************************************************** COMMENT HISTORY alm generated by CREATE_ALM_2.1.0 from following power spectrum COMMENT COMMENT ---------------------------------------------------- COMMENT Planck Power Spectrum Description Specific Keywords COMMENT ---------------------------------------------------- COMMENT Input power spectrum in : COMMENT cl.fits COMMENT COMMENT Quadrupole COMMENT C(2) = 1.278940E+03 uK^2 COMMENT COMMENT COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- BCROSS = F / Magnetic cross terms included (True/False) COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- TEMPTYPE= 'THERMO ' / temperature type either THERMO or ANTENNA POLNORM = 'CMBFAST ' / CMBFAST (EB) convention for polar. spectra COMMENT **************************************************************** COMMENT ----------------------------------------------- COMMENT Map Analysis Specific Keywords COMMENT ----------------------------------------------- EXTNAME = 'SIMULATED a_lms (TEMPERATURE)' COMMENT CREATOR = 'SYNFAST ' / Software creating the FITS file VERSION = '3.82 ' / Version of the simulation software COMMENT MAX-LPOL= 256 / Maximum L multipole order MAX-MPOL= 256 / Maximum M multipole degree RANDSEED= -1 / Random generator seed COMMENT COMMENT The real and imaginary part of the a_lm with m>=0 COMMENT TTYPE1 = 'INDEX ' / i = l^2 + l + m + 1 TFORM1 = '1J ' / data format of field: 4-byte INTEGER TUNIT1 = ' ' / index COMMENT TTYPE2 = 'REAL ' / REAL a_lm TFORM2 = '1E ' / data format of field: 4-byte REAL TUNIT2 = 'uK ' / alm units COMMENT TTYPE3 = 'IMAG ' / IMAGINARY a_lm TFORM3 = '1E ' / data format of field: 4-byte REAL TUNIT3 = 'uK ' / alm units COMMENT COORDSYS= 'unknown ' / Input map coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial POLAR = T / Polarisation included (True/False) HISTORY File with input C(l): HISTORY cl.fits HISTORY These alms are multiplied by pixel and beam window functions NSIDE = 128 / Resolution parameter for HEALPIX FWHM = 5.00000000E-01 / [deg] FWHM of gaussian symmetric beam HISTORY MIN-LPOL= 0 / Minimum L multipole order END Œ8qAq ץ BA0=5lZA~ؿ8A AgR\>/1@ލlWi @ך`Q!@Aj"AzA^#Ae$%]l+G~,@KA?-?3AD6/.AgR)y7/?,A08z@Ae1\9@0:&WWANe;@Oj,{Ep?o A@?d@XIAJLJg?3KX ?عL@aLw'YMNkW~O?QP>bjQAѳr[@aZ\Aھ|]e ^4h&X_@Xm(ѿ` +SIMPLE = T / file does conform to FITS standard BITPIX = 32 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H DATE = '2024-10-08T15:50:33' / file creation date (YYYY-MM-DDThh:mm:ss UT) END XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 12 / width of table in bytes NAXIS2 = 33153 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 3 / number of fields in each row COMMENT **************************************************************** COMMENT HISTORY alm generated by CREATE_ALM_2.1.0 from following power spectrum COMMENT COMMENT ---------------------------------------------------- COMMENT Planck Power Spectrum Description Specific Keywords COMMENT ---------------------------------------------------- COMMENT Input power spectrum in : COMMENT cl.fits COMMENT COMMENT Quadrupole COMMENT C(2) = 1.278940E+03 uK^2 COMMENT COMMENT COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- BCROSS = F / Magnetic cross terms included (True/False) COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- TEMPTYPE= 'THERMO ' / temperature type either THERMO or ANTENNA POLNORM = 'CMBFAST ' / CMBFAST (EB) convention for polar. spectra COMMENT **************************************************************** COMMENT ----------------------------------------------- COMMENT Map Analysis Specific Keywords COMMENT ----------------------------------------------- EXTNAME = 'SIMULATED a_lms (TEMPERATURE)' COMMENT CREATOR = 'SYNFAST ' / Software creating the FITS file VERSION = '3.83 ' / Version of the simulation software COMMENT MAX-LPOL= 256 / Maximum L multipole order MAX-MPOL= 256 / Maximum M multipole degree RANDSEED= -1 / Random generator seed COMMENT COMMENT The real and imaginary part of the a_lm with m>=0 COMMENT TTYPE1 = 'INDEX ' / i = l^2 + l + m + 1 TFORM1 = '1J ' / data format of field: 4-byte INTEGER TUNIT1 = ' ' / index COMMENT TTYPE2 = 'REAL ' / REAL a_lm TFORM2 = '1E ' / data format of field: 4-byte REAL TUNIT2 = 'uK ' / alm units COMMENT TTYPE3 = 'IMAG ' / IMAGINARY a_lm TFORM3 = '1E ' / data format of field: 4-byte REAL TUNIT3 = 'uK ' / alm units COMMENT COORDSYS= 'unknown ' / Input map coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial POLAR = T / Polarisation included (True/False) HISTORY File with input C(l): HISTORY cl.fits HISTORY These alms are multiplied by pixel and beam window functions NSIDE = 128 / Resolution parameter for HEALPIX FWHM = 5.00000000E-01 / [deg] FWHM of gaussian symmetric beam HISTORY MIN-LPOL= 0 / Minimum L multipole order END Œ8qAq ץ BA0=5lZA~ؿ8A AgR\>/1@ލlWi @ך`Q!@Aj"AzA^#Ae$%]l+G~,@KA?-?3AD6/.AgR)y7/?,A08z@Ae1\9@0:&WWANe;@Oj,{Ep?o A@?d@XIAJLJg?3KX ?عL@aLw'YMNkW~O?QP>bjQAѳr[@aZ\Aھ|]e ^4h&X_@Xm(ѿ` zn@a@c?-?'bY%;cA@d^ֿoA6֯p3S}q@@r@o&A9sخt@T_ u@bXA v?Տ?w@#qjgx%GyAT՘"Arr̳4P@u@%_ɾfؐ5A6A(hsw?nS@`@@û))@0k#GLV ? ?q@6V@K,Ys@@@4@7GuC9[m"@:t 4AW x ɿC >m@m?&֎2?sO~@a4@P@#A >|q|@ȿbo_3T¾@4?i%?{C@U @L.?J&)?WK߰ҾƷ@[<@bϹbGھ2*A$|???)R>q@U]?ÿ U`/#Zk @Jfx@>iP@>.R@>Z'ef@JL>Bi?6ј>F?~5@i@ }@?>cL8P0B@?L"%pz@S@B7@ @@ -1138,7 +1138,7 @@ M> >J>fHl>&>WfD>k+<}<@[ھ4>Na=Uo2>`f:Cj>@ K ׊>c=T~>6=:>F>l=>(>ҾY>=1Pa>2 jb>3?Gsgއ>V> nJ>G>7þi>Y< ż>g[>됬>̱Ǽ=g)Ⱦg6?Nɾldʾ)˽y̾le>*Cͼ~>hξ_0Q6O>Y=)Rн3]>9=c3ҽI>o.f>WA1>>mq<%ֽ >[u׽ZI>eؾJ;r=! =Ē<=qg;b>ܾ~>Kݾ,%i;=ϙ߾hཟ>qιR>>w=g$Pɔn>V[1=׾>y3?p>Sij,> -ý~=|g@>=n>=/P=N;@w=lb>Vu  dG>6:4>M>C½<=A^>;,g=)>ұ4l"z>>G>#?>܊e [y<9^=މBmK>_E>|x U= *I{XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 12 / width of table in bytes NAXIS2 = 33153 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 3 / number of fields in each row COMMENT **************************************************************** COMMENT HISTORY alm generated by CREATE_ALM_2.1.0 from following power spectrum COMMENT COMMENT ---------------------------------------------------- COMMENT Planck Power Spectrum Description Specific Keywords COMMENT ---------------------------------------------------- COMMENT Input power spectrum in : COMMENT cl.fits COMMENT COMMENT Quadrupole COMMENT C(2) = 1.278940E+03 uK^2 COMMENT COMMENT COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- BCROSS = F / Magnetic cross terms included (True/False) COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- TEMPTYPE= 'THERMO ' / temperature type either THERMO or ANTENNA POLNORM = 'CMBFAST ' / CMBFAST (EB) convention for polar. spectra COMMENT **************************************************************** COMMENT ----------------------------------------------- COMMENT Map Analysis Specific Keywords COMMENT ----------------------------------------------- EXTNAME = 'SIMULATED a_lms (GRAD / ELECTRIC component)' COMMENT CREATOR = 'SYNFAST ' / Software creating the FITS file VERSION = '3.82 ' / Version of the simulation software COMMENT MAX-LPOL= 256 / Maximum L multipole order MAX-MPOL= 256 / Maximum M multipole degree RANDSEED= -1 / Random generator seed COMMENT COMMENT The real and imaginary part of the a_lm with m>=0 COMMENT TTYPE1 = 'INDEX ' / i = l^2 + l + m + 1 TFORM1 = '1J ' / data format of field: 4-byte INTEGER TUNIT1 = ' ' / index COMMENT TTYPE2 = 'REAL ' / REAL a_lm TFORM2 = '1E ' / data format of field: 4-byte REAL TUNIT2 = 'uK ' / alm units COMMENT TTYPE3 = 'IMAG ' / IMAGINARY a_lm TFORM3 = '1E ' / data format of field: 4-byte REAL TUNIT3 = 'uK ' / alm units COMMENT COORDSYS= 'unknown ' / Input map coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial POLAR = T / Polarisation included (True/False) HISTORY File with input C(l): HISTORY cl.fits HISTORY These alms are multiplied by pixel and beam window functions NSIDE = 128 / Resolution parameter for HEALPIX FWHM = 5.00000000E-01 / [deg] FWHM of gaussian symmetric beam HISTORY MIN-LPOL= 0 / Minimum L multipole order END C#={ \J >]O+s1$%>4=Z>:^ n><-lgt>\j>p=z#>ޗ$=,细+Fk,i=MhD- =.=*=ޒ/=Tr_=f0<>=-j[1[1^f9:m=Ո;gu=^=>d<]Ko=n>=/P=N;@w=lb>Vu  dG>6:4>M>C½<=A^>;,g=)>ұ4l"z>>G>#?>܊e [y<9^=މBmK>_E>|x U= *I{XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 12 / width of table in bytes NAXIS2 = 33153 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 3 / number of fields in each row COMMENT **************************************************************** COMMENT HISTORY alm generated by CREATE_ALM_2.1.0 from following power spectrum COMMENT COMMENT ---------------------------------------------------- COMMENT Planck Power Spectrum Description Specific Keywords COMMENT ---------------------------------------------------- COMMENT Input power spectrum in : COMMENT cl.fits COMMENT COMMENT Quadrupole COMMENT C(2) = 1.278940E+03 uK^2 COMMENT COMMENT COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- BCROSS = F / Magnetic cross terms included (True/False) COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- TEMPTYPE= 'THERMO ' / temperature type either THERMO or ANTENNA POLNORM = 'CMBFAST ' / CMBFAST (EB) convention for polar. spectra COMMENT **************************************************************** COMMENT ----------------------------------------------- COMMENT Map Analysis Specific Keywords COMMENT ----------------------------------------------- EXTNAME = 'SIMULATED a_lms (GRAD / ELECTRIC component)' COMMENT CREATOR = 'SYNFAST ' / Software creating the FITS file VERSION = '3.83 ' / Version of the simulation software COMMENT MAX-LPOL= 256 / Maximum L multipole order MAX-MPOL= 256 / Maximum M multipole degree RANDSEED= -1 / Random generator seed COMMENT COMMENT The real and imaginary part of the a_lm with m>=0 COMMENT TTYPE1 = 'INDEX ' / i = l^2 + l + m + 1 TFORM1 = '1J ' / data format of field: 4-byte INTEGER TUNIT1 = ' ' / index COMMENT TTYPE2 = 'REAL ' / REAL a_lm TFORM2 = '1E ' / data format of field: 4-byte REAL TUNIT2 = 'uK ' / alm units COMMENT TTYPE3 = 'IMAG ' / IMAGINARY a_lm TFORM3 = '1E ' / data format of field: 4-byte REAL TUNIT3 = 'uK ' / alm units COMMENT COORDSYS= 'unknown ' / Input map coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial POLAR = T / Polarisation included (True/False) HISTORY File with input C(l): HISTORY cl.fits HISTORY These alms are multiplied by pixel and beam window functions NSIDE = 128 / Resolution parameter for HEALPIX FWHM = 5.00000000E-01 / [deg] FWHM of gaussian symmetric beam HISTORY MIN-LPOL= 0 / Minimum L multipole order END C#={ \J >]O+s1$%>4=Z>:^ n><-lgt>\j>p=z#>ޗ$=,细+Fk,i=MhD- =.=*=ޒ/=Tr_=f0<>=-j[1[1^f9:m=Ո;gu=^=>d<]Ko@b;)!]4<#<}.`m <:!; u5&3VR4[;'5xB6H;75;8:rﻷ @@ -2194,7 +2194,7 @@ H; Qjvk)sOlBкYm7<"3Gn@OC+D< < .<QW<:;Q;aB9D7#_;s1a;uB< -:Gd; w< s<'d;'*#j;A;;6\r87"(;2;mIMNm:8;$;n;/5:;e;;v;=ו;n;;ʻznmQu:Qf;(<1z!6D9_n@ۻNy:槕ܼ0q;eݼ L߃޺$_߻#;(3j=0 COMMENT TTYPE1 = 'INDEX ' / i = l^2 + l + m + 1 TFORM1 = '1J ' / data format of field: 4-byte INTEGER TUNIT1 = ' ' / index COMMENT TTYPE2 = 'REAL ' / REAL a_lm TFORM2 = '1E ' / data format of field: 4-byte REAL TUNIT2 = 'uK ' / alm units COMMENT TTYPE3 = 'IMAG ' / IMAGINARY a_lm TFORM3 = '1E ' / data format of field: 4-byte REAL TUNIT3 = 'uK ' / alm units COMMENT COORDSYS= 'unknown ' / Input map coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial POLAR = T / Polarisation included (True/False) HISTORY File with input C(l): HISTORY cl.fits HISTORY These alms are multiplied by pixel and beam window functions NSIDE = 128 / Resolution parameter for HEALPIX FWHM = 5.00000000E-01 / [deg] FWHM of gaussian symmetric beam HISTORY MIN-LPOL= 0 / Minimum L multipole order END   !"#$+,-./019:;<=>?@IJKLMNOPQ[\]^_`abcdopqrstuvwxy !3456789:;<=>?@ABCDWXYZ[\]^_`abcdefghi}~  +:Gd; w< s<'d;'*#j;A;;6\r87"(;2;mIMNm:8;$;n;/5:;e;;v;=ו;n;;ʻznmQu:Qf;(<1z!6D9_n@ۻNy:槕ܼ0q;eݼ L߃޺$_߻#;(3j=0 COMMENT TTYPE1 = 'INDEX ' / i = l^2 + l + m + 1 TFORM1 = '1J ' / data format of field: 4-byte INTEGER TUNIT1 = ' ' / index COMMENT TTYPE2 = 'REAL ' / REAL a_lm TFORM2 = '1E ' / data format of field: 4-byte REAL TUNIT2 = 'uK ' / alm units COMMENT TTYPE3 = 'IMAG ' / IMAGINARY a_lm TFORM3 = '1E ' / data format of field: 4-byte REAL TUNIT3 = 'uK ' / alm units COMMENT COORDSYS= 'unknown ' / Input map coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial POLAR = T / Polarisation included (True/False) HISTORY File with input C(l): HISTORY cl.fits HISTORY These alms are multiplied by pixel and beam window functions NSIDE = 128 / Resolution parameter for HEALPIX FWHM = 5.00000000E-01 / [deg] FWHM of gaussian symmetric beam HISTORY MIN-LPOL= 0 / Minimum L multipole order END   !"#$+,-./019:;<=>?@IJKLMNOPQ[\]^_`abcdopqrstuvwxy !3456789:;<=>?@ABCDWXYZ[\]^_`abcdefghi}~     )*+,-./0123456789:;<=>?@YZ[\]^_`abcdefghijklmnopq     -./0123456789:;<=>?@ABCDEFGHIghijklmnopqrstuvwxyz{|}~!"#$%&'()*+,-./0123456789:;<=>?@Acdefghijklmnopqrstuvwxyz{|}~     56789:;<=>?@ABCDEFGHIJKLMNOPQRSTUVWXY !"#$%&'()*+,-./0123456789:;<=>?@ijklmnopqrstuvwxyz{|}~ !"#$%&'()*+,-./0123456789efghijklmnopqrstuvwxyz{|}~ !"#$%&'()*+,-./0123456789:;<=>?@ABCDstuvwxyz{|}~ 1 2 3 4 5 6 7 8 9 : ; < = > ? @ A B C D E F G H I J K L M N O P Q R S T U V W X Y Z [ \ ] ^ _ ` a diff --git a/test/almdec.fits b/test/almdec.fits index 9e5005c4..0772b0cc 100644 --- a/test/almdec.fits +++ b/test/almdec.fits @@ -1,4 +1,4 @@ -SIMPLE = T / file does conform to FITS standard BITPIX = 32 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H DATE = '2022-07-28T14:24:17' / file creation date (YYYY-MM-DDThh:mm:ss UT) END XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 12 / width of table in bytes NAXIS2 = 33153 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 3 / number of fields in each row COMMENT **************************************************************** COMMENT HISTORY alm generated by CREATE_ALM_2.1.0 from following power spectrum COMMENT COMMENT ---------------------------------------------------- COMMENT Planck Power Spectrum Description Specific Keywords COMMENT ---------------------------------------------------- COMMENT Input power spectrum in : COMMENT cl.fits COMMENT COMMENT Quadrupole COMMENT C(2) = 1.278940E+03 uK^2 COMMENT COMMENT COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- BCROSS = F / Magnetic cross terms included (True/False) COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- TEMPTYPE= 'THERMO ' / temperature type either THERMO or ANTENNA POLNORM = 'CMBFAST ' / CMBFAST (EB) convention for polar. spectra COMMENT **************************************************************** COMMENT ----------------------------------------------- COMMENT Map Analysis Specific Keywords COMMENT ----------------------------------------------- COMMENT CREATOR = 'SYNFAST ' / Software creating the FITS file VERSION = '3.81 ' / Version of the simulation software COMMENT RANDSEED= -1 / Random generator seed COMMENT COMMENT The real and imaginary part of the a_lm with m>=0 COMMENT TTYPE1 = 'INDEX ' / i = l^2 + l + m + 1 TFORM1 = '1J ' / data format of field: 4-byte INTEGER TUNIT1 = ' ' / index COMMENT TTYPE2 = 'REAL ' / REAL a_lm TFORM2 = '1E ' / data format of field: 4-byte REAL TUNIT2 = 'uK ' / alm units COMMENT TTYPE3 = 'IMAG ' / IMAGINARY a_lm TFORM3 = '1E ' / data format of field: 4-byte REAL TUNIT3 = 'uK ' / alm units COMMENT COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial POLAR = T / Polarisation included (True/False) HISTORY File with input C(l): HISTORY cl.fits HISTORY These alms are multiplied by pixel and beam window functions HISTORY FWHM = 0.00000000E+00 / [deg] FWHM of gaussian symmetric beam NSIDE = 128 / Resolution parameter for HEALPIX MAX-LPOL= 256 / Maximum L multipole order MIN-LPOL= 0 / Minimum L multipole order MAX-MPOL= 256 / Maximum M multipole degree COORDSYS= ' ' / Coordinates system EPOCH = 2.000000000000E+03 / Coordinates system epoch HISTORY file alm.fits HISTORY modified by ALTERALM 3.82 HISTORY changed FWHM END ŒC9As jK BA0@9lXA <A Ag3W>(@ޕ!<lޫi% @ץQ!@Ak"AyAf #Amy$%+G;,@K"A?-?3ADD.Agc>yJI/?A!Q0C4@At*1fؿ 9@#:&gANy;@^ξ 9V?{A@?c@iIAJfJ?3KX(>?L@ahDM3ON~Ob?%P> ~QA0[@a:\AY|] 4F^R&r_@q(w` +SIMPLE = T / file does conform to FITS standard BITPIX = 32 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H DATE = '2024-10-08T15:50:35' / file creation date (YYYY-MM-DDThh:mm:ss UT) END XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 12 / width of table in bytes NAXIS2 = 33153 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 3 / number of fields in each row COMMENT **************************************************************** COMMENT HISTORY alm generated by CREATE_ALM_2.1.0 from following power spectrum COMMENT COMMENT ---------------------------------------------------- COMMENT Planck Power Spectrum Description Specific Keywords COMMENT ---------------------------------------------------- COMMENT Input power spectrum in : COMMENT cl.fits COMMENT COMMENT Quadrupole COMMENT C(2) = 1.278940E+03 uK^2 COMMENT COMMENT COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- BCROSS = F / Magnetic cross terms included (True/False) COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- TEMPTYPE= 'THERMO ' / temperature type either THERMO or ANTENNA POLNORM = 'CMBFAST ' / CMBFAST (EB) convention for polar. spectra COMMENT **************************************************************** COMMENT ----------------------------------------------- COMMENT Map Analysis Specific Keywords COMMENT ----------------------------------------------- COMMENT CREATOR = 'SYNFAST ' / Software creating the FITS file VERSION = '3.82 ' / Version of the simulation software COMMENT RANDSEED= -1 / Random generator seed COMMENT COMMENT The real and imaginary part of the a_lm with m>=0 COMMENT TTYPE1 = 'INDEX ' / i = l^2 + l + m + 1 TFORM1 = '1J ' / data format of field: 4-byte INTEGER TUNIT1 = ' ' / index COMMENT TTYPE2 = 'REAL ' / REAL a_lm TFORM2 = '1E ' / data format of field: 4-byte REAL TUNIT2 = 'uK ' / alm units COMMENT TTYPE3 = 'IMAG ' / IMAGINARY a_lm TFORM3 = '1E ' / data format of field: 4-byte REAL TUNIT3 = 'uK ' / alm units COMMENT COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial POLAR = T / Polarisation included (True/False) HISTORY File with input C(l): HISTORY cl.fits HISTORY These alms are multiplied by pixel and beam window functions HISTORY FWHM = 0.00000000E+00 / [deg] FWHM of gaussian symmetric beam NSIDE = 128 / Resolution parameter for HEALPIX MAX-LPOL= 256 / Maximum L multipole order MIN-LPOL= 0 / Minimum L multipole order MAX-MPOL= 256 / Maximum M multipole degree COORDSYS= ' ' / Coordinates system EPOCH = 2.000000000000E+03 / Coordinates system epoch HISTORY file alm.fits HISTORY modified by ALTERALM 3.83 HISTORY changed FWHM END ŒC9As jK BA0@9lXA <A Ag3W>(@ޕ!<lޫi% @ץQ!@Ak"AyAf #Amy$%+G;,@K"A?-?3ADD.Agc>yJI/?A!Q0C4@At*1fؿ 9@#:&gANy;@^ξ 9V?{A@?c@iIAJfJ?3KX(>?L@ahDM3ON~Ob?%P> ~QA0[@a:\AY|] 4F^R&r_@q(w` Y@aa@c?-ZbYcA#@6Dd_?oA6p4$\q@@Gr@o|A9sOt@m2&u@bA 8v?չ:? w@#hݕ<xByAT# CAazҁ@"@%G;1"{;A('??@`t@1R@$kY}7O ?a=? &@b@KYB@%@+%@_y@lfuCopymR@yY 8AW= ! }>m@n5?)?͵6#@u;@0bE@aA9>jL+K@)-_y4¾F@\?i?{ʀV6d R @Lym?Jp?W*t@茾k<@V Z?ٿ a2A ju_@J=@X>@>~@d>m=7'@J>C1?P ^>0,?@@ @ة?u>/Ud @@ -1157,7 +1157,7 @@ w R?.=!ż9>?9 L? HǼV=Ⱦ!?Qpɿʾp˾Qͽ85>7ξSX>̽}8оBN>z=ҽ>rM>>y?>=׽_m>ؾ:@"=}%>j=Tn6;9>;mܾ;>ݾ:˿1_n;ɻ>#߾Vq86k>!砾k>>A>d;=w8v¿Y>߿K;<演(pj)>²׺?g?#My>Z-1=Ƽk2>e>U>T=i!G2tﾗ0=о#M>2 QH>HG>fw=Ԁ/>ﰖ;=X$?%V~> >ѽ:e6>ɳ?->+4 a..*'GŽ -j>H>TGXu,=k\66XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 12 / width of table in bytes NAXIS2 = 33153 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 3 / number of fields in each row COMMENT **************************************************************** COMMENT HISTORY alm generated by CREATE_ALM_2.1.0 from following power spectrum COMMENT COMMENT ---------------------------------------------------- COMMENT Planck Power Spectrum Description Specific Keywords COMMENT ---------------------------------------------------- COMMENT Input power spectrum in : COMMENT cl.fits COMMENT COMMENT Quadrupole COMMENT C(2) = 1.278940E+03 uK^2 COMMENT COMMENT COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- BCROSS = F / Magnetic cross terms included (True/False) COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- TEMPTYPE= 'THERMO ' / temperature type either THERMO or ANTENNA POLNORM = 'CMBFAST ' / CMBFAST (EB) convention for polar. spectra COMMENT **************************************************************** COMMENT ----------------------------------------------- COMMENT Map Analysis Specific Keywords COMMENT ----------------------------------------------- COMMENT CREATOR = 'SYNFAST ' / Software creating the FITS file VERSION = '3.81 ' / Version of the simulation software COMMENT RANDSEED= -1 / Random generator seed COMMENT COMMENT The real and imaginary part of the a_lm with m>=0 COMMENT TTYPE1 = 'INDEX ' / i = l^2 + l + m + 1 TFORM1 = '1J ' / data format of field: 4-byte INTEGER TUNIT1 = ' ' / index COMMENT TTYPE2 = 'REAL ' / REAL a_lm TFORM2 = '1E ' / data format of field: 4-byte REAL TUNIT2 = 'uK ' / alm units COMMENT TTYPE3 = 'IMAG ' / IMAGINARY a_lm TFORM3 = '1E ' / data format of field: 4-byte REAL TUNIT3 = 'uK ' / alm units COMMENT COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial POLAR = T / Polarisation included (True/False) HISTORY File with input C(l): HISTORY cl.fits HISTORY These alms are multiplied by pixel and beam window functions HISTORY FWHM = 0.00000000E+00 / [deg] FWHM of gaussian symmetric beam NSIDE = 128 / Resolution parameter for HEALPIX MAX-LPOL= 256 / Maximum L multipole order MIN-LPOL= 0 / Minimum L multipole order MAX-MPOL= 256 / Maximum M multipole degree COORDSYS= ' ' / Coordinates system EPOCH = 2.000000000000E+03 / Coordinates system epoch HISTORY file alm.fits HISTORY modified by ALTERALM 3.82 HISTORY changed FWHM END Cʤ= ]J~ >_,-ü1&>16=Z>:cS(>K&<3¾gz>]JjK>pHv#>巽'$=6w+R,i`=Mu- =.=:4=/=T=v0<>=-u1e_l9<:Õ=;=m1=>Βʝd<]mo Vs5Q»_v}aA<<1:OH>TGXu,=k\66XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 12 / width of table in bytes NAXIS2 = 33153 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 3 / number of fields in each row COMMENT **************************************************************** COMMENT HISTORY alm generated by CREATE_ALM_2.1.0 from following power spectrum COMMENT COMMENT ---------------------------------------------------- COMMENT Planck Power Spectrum Description Specific Keywords COMMENT ---------------------------------------------------- COMMENT Input power spectrum in : COMMENT cl.fits COMMENT COMMENT Quadrupole COMMENT C(2) = 1.278940E+03 uK^2 COMMENT COMMENT COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- BCROSS = F / Magnetic cross terms included (True/False) COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- TEMPTYPE= 'THERMO ' / temperature type either THERMO or ANTENNA POLNORM = 'CMBFAST ' / CMBFAST (EB) convention for polar. spectra COMMENT **************************************************************** COMMENT ----------------------------------------------- COMMENT Map Analysis Specific Keywords COMMENT ----------------------------------------------- COMMENT CREATOR = 'SYNFAST ' / Software creating the FITS file VERSION = '3.82 ' / Version of the simulation software COMMENT RANDSEED= -1 / Random generator seed COMMENT COMMENT The real and imaginary part of the a_lm with m>=0 COMMENT TTYPE1 = 'INDEX ' / i = l^2 + l + m + 1 TFORM1 = '1J ' / data format of field: 4-byte INTEGER TUNIT1 = ' ' / index COMMENT TTYPE2 = 'REAL ' / REAL a_lm TFORM2 = '1E ' / data format of field: 4-byte REAL TUNIT2 = 'uK ' / alm units COMMENT TTYPE3 = 'IMAG ' / IMAGINARY a_lm TFORM3 = '1E ' / data format of field: 4-byte REAL TUNIT3 = 'uK ' / alm units COMMENT COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial POLAR = T / Polarisation included (True/False) HISTORY File with input C(l): HISTORY cl.fits HISTORY These alms are multiplied by pixel and beam window functions HISTORY FWHM = 0.00000000E+00 / [deg] FWHM of gaussian symmetric beam NSIDE = 128 / Resolution parameter for HEALPIX MAX-LPOL= 256 / Maximum L multipole order MIN-LPOL= 0 / Minimum L multipole order MAX-MPOL= 256 / Maximum M multipole degree COORDSYS= ' ' / Coordinates system EPOCH = 2.000000000000E+03 / Coordinates system epoch HISTORY file alm.fits HISTORY modified by ALTERALM 3.83 HISTORY changed FWHM END Cʤ= ]J~ >_,-ü1&>16=Z>:cS(>K&<3¾gz>]JjK>pHv#>巽'$=6w+R,i`=Mu- =.=:4=/=T=v0<>=-u1e_l9<:Õ=;=m1=>Βʝd<]mo Vs5Q»_v}aA<<1:O<ܑ;?< ȧC@:ai9)6AuB_(B\C;;("D:- W:JX N;Y;ueёZoxl@Tkԝڇ:9<:) w;~һu^z;G<ԺKtoռB+;<{j;׹S<,;<=9;( ;4;<}NۼE~F"ܼ,ӼK:E:q޻{:(<໽A;>+ <&'1ā⻆;D;u<NG:I<`r;";7]b)?.񼃹};ب;3E;I<_ <ʩJ`z=0 COMMENT TTYPE1 = 'INDEX ' / i = l^2 + l + m + 1 TFORM1 = '1J ' / data format of field: 4-byte INTEGER TUNIT1 = ' ' / index COMMENT TTYPE2 = 'REAL ' / REAL a_lm TFORM2 = '1E ' / data format of field: 4-byte REAL TUNIT2 = 'uK ' / alm units COMMENT TTYPE3 = 'IMAG ' / IMAGINARY a_lm TFORM3 = '1E ' / data format of field: 4-byte REAL TUNIT3 = 'uK ' / alm units COMMENT COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial POLAR = T / Polarisation included (True/False) HISTORY File with input C(l): HISTORY cl.fits HISTORY These alms are multiplied by pixel and beam window functions HISTORY FWHM = 0.00000000E+00 / [deg] FWHM of gaussian symmetric beam NSIDE = 128 / Resolution parameter for HEALPIX MAX-LPOL= 256 / Maximum L multipole order MIN-LPOL= 0 / Minimum L multipole order MAX-MPOL= 256 / Maximum M multipole degree COORDSYS= ' ' / Coordinates system EPOCH = 2.000000000000E+03 / Coordinates system epoch HISTORY file alm.fits HISTORY modified by ALTERALM 3.82 HISTORY changed FWHM END   !"#$+,-./019:;<=>?@IJKLMNOPQ[\]^_`abcdopqrstuvwxy !3456789:;<=>?@ABCDWXYZ[\]^_`abcdefghi}~  +7;}?<$/$] \]0\XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 12 / width of table in bytes NAXIS2 = 33153 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 3 / number of fields in each row COMMENT **************************************************************** COMMENT HISTORY alm generated by CREATE_ALM_2.1.0 from following power spectrum COMMENT COMMENT ---------------------------------------------------- COMMENT Planck Power Spectrum Description Specific Keywords COMMENT ---------------------------------------------------- COMMENT Input power spectrum in : COMMENT cl.fits COMMENT COMMENT Quadrupole COMMENT C(2) = 1.278940E+03 uK^2 COMMENT COMMENT COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- BCROSS = F / Magnetic cross terms included (True/False) COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- TEMPTYPE= 'THERMO ' / temperature type either THERMO or ANTENNA POLNORM = 'CMBFAST ' / CMBFAST (EB) convention for polar. spectra COMMENT **************************************************************** COMMENT ----------------------------------------------- COMMENT Map Analysis Specific Keywords COMMENT ----------------------------------------------- COMMENT CREATOR = 'SYNFAST ' / Software creating the FITS file VERSION = '3.82 ' / Version of the simulation software COMMENT RANDSEED= -1 / Random generator seed COMMENT COMMENT The real and imaginary part of the a_lm with m>=0 COMMENT TTYPE1 = 'INDEX ' / i = l^2 + l + m + 1 TFORM1 = '1J ' / data format of field: 4-byte INTEGER TUNIT1 = ' ' / index COMMENT TTYPE2 = 'REAL ' / REAL a_lm TFORM2 = '1E ' / data format of field: 4-byte REAL TUNIT2 = 'uK ' / alm units COMMENT TTYPE3 = 'IMAG ' / IMAGINARY a_lm TFORM3 = '1E ' / data format of field: 4-byte REAL TUNIT3 = 'uK ' / alm units COMMENT COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial POLAR = T / Polarisation included (True/False) HISTORY File with input C(l): HISTORY cl.fits HISTORY These alms are multiplied by pixel and beam window functions HISTORY FWHM = 0.00000000E+00 / [deg] FWHM of gaussian symmetric beam NSIDE = 128 / Resolution parameter for HEALPIX MAX-LPOL= 256 / Maximum L multipole order MIN-LPOL= 0 / Minimum L multipole order MAX-MPOL= 256 / Maximum M multipole degree COORDSYS= ' ' / Coordinates system EPOCH = 2.000000000000E+03 / Coordinates system epoch HISTORY file alm.fits HISTORY modified by ALTERALM 3.83 HISTORY changed FWHM END   !"#$+,-./019:;<=>?@IJKLMNOPQ[\]^_`abcdopqrstuvwxy !3456789:;<=>?@ABCDWXYZ[\]^_`abcdefghi}~     )*+,-./0123456789:;<=>?@YZ[\]^_`abcdefghijklmnopq     -./0123456789:;<=>?@ABCDEFGHIghijklmnopqrstuvwxyz{|}~!"#$%&'()*+,-./0123456789:;<=>?@Acdefghijklmnopqrstuvwxyz{|}~     56789:;<=>?@ABCDEFGHIJKLMNOPQRSTUVWXY !"#$%&'()*+,-./0123456789:;<=>?@ijklmnopqrstuvwxyz{|}~ !"#$%&'()*+,-./0123456789efghijklmnopqrstuvwxyz{|}~ !"#$%&'()*+,-./0123456789:;<=>?@ABCDstuvwxyz{|}~ 1 2 3 4 5 6 7 8 9 : ; < = > ? @ A B C D E F G H I J K L M N O P Q R S T U V W X Y Z [ \ ] ^ _ ` a diff --git a/test/cl2maps.fits b/test/cl2maps.fits index ab1b12e0..ccf61973 100644 --- a/test/cl2maps.fits +++ b/test/cl2maps.fits @@ -1 +1 @@ -SIMPLE = T / file does conform to FITS standard BITPIX = 32 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H DATE = '2022-07-28T14:24:17' / file creation date (YYYY-MM-DDThh:mm:ss UT) END XTENSION= 'TABLE ' / ASCII table extension BITPIX = 8 / 8-bit ASCII characters NAXIS = 2 / 2-dimensional ASCII table NAXIS1 = 143 / width of table in characters NAXIS2 = 257 / number of rows in table PCOUNT = 0 / no group parameters (required keyword) GCOUNT = 1 / one data group (required keyword) TFIELDS = 9 / number of fields in each row COMMENT ----------------------------------------------- COMMENT Map Analysis Specific Keywords COMMENT ----------------------------------------------- EXTNAME = 'ANALYSED CROSS POWER SPECTRUM' COMMENT CREATOR = 'ANAFAST ' / Software creating the FITS file VERSION = '3.82 ' / Version of the simulation software COMMENT MAX-LPOL= 256 / Maximum Legendre order L COMMENT POLAR = T / Polarisation included (True/False) BCROSS = T / Magnetic cross terms included (True/False) ASYMCL = T / Asymmetric pol cross terms (XY vs YX) included COMMENT NSIDE = 128 / Resolution Parameter of Input Map COORDSYS= 'unknown ' / Input Map Coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial COMMENT TBCOL1 = 1 / beginning column of field 1 TFORM1 = 'E15.7 ' TTYPE1 = 'TEMPERATURE' / Temperature C(l) TUNIT1 = 'uK^2 ' / square of map units COMMENT TBCOL2 = 17 / beginning column of field 2 TFORM2 = 'E15.7 ' TTYPE2 = 'GRADIENT' / Gradient (=ELECTRIC) polarisation C(l) TUNIT2 = 'uK^2 ' / power spectrum units COMMENT TBCOL3 = 33 / beginning column of field 3 TFORM3 = 'E15.7 ' TTYPE3 = 'CURL ' / Curl (=MAGNETIC) polarisation C(l) TUNIT3 = 'uK^2 ' / power spectrum units COMMENT TBCOL4 = 49 / beginning column of field 4 TFORM4 = 'E15.7 ' TTYPE4 = 'TG ' / Temperature X Gradient cross terms TUNIT4 = 'uK^2 ' / power spectrum units COMMENT TBCOL5 = 65 / beginning column of field 5 TFORM5 = 'E15.7 ' TTYPE5 = 'TC ' / Temperature X Curl cross terms TUNIT5 = 'uK^2 ' / power spectrum units COMMENT TBCOL6 = 81 / beginning column of field 6 TFORM6 = 'E15.7 ' TTYPE6 = 'GC ' / Gradient x Curl cross terms TUNIT6 = 'uK^2 ' / power spectrum units COMMENT TBCOL7 = 97 / beginning column of field 7 TFORM7 = 'E15.7 ' TTYPE7 = 'GT ' / Gradient1 x Temperature2 cross terms TUNIT7 = 'uK^2 ' / power spectrum units COMMENT TBCOL8 = 113 / beginning column of field 8 TFORM8 = 'E15.7 ' TTYPE8 = 'CT ' / Curl1 x Temperature2 cross terms TUNIT8 = 'uK^2 ' / power spectrum units COMMENT TBCOL9 = 129 / beginning column of field 9 TFORM9 = 'E15.7 ' TTYPE9 = 'CG ' / Curl1 x Gradient2 cross terms TUNIT9 = 'uK^2 ' / power spectrum units COMMENT COMMENT The polarisation power spectra have the same definition as in CMBFAST COMMENT CUT-SKY = 0.000000000000E+00 / [deg] Symmetric Cut Sky NITERALM= 0 / Number of iterations for a_lms extraction LREGRESS= 2 / Regression of low multipoles (0/1/2) NMAPS_IN= 2 / Number of maps (co-)analysed (1/2) QUADSCHM= 1 / Quadrature scheme (0/1/2) COMMENT HISTORY Input Map1 = map.fits HISTORY Input Map2 = map.fits END 1.6709244E-08 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 1.3732767E-06 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 1.9208811E+03 1.5580678E-01 4.8352069E-14 1.3119236E+01 1.0511602E-06 5.2924753E-09 1.3119236E+01 1.0511602E-06 5.2924753E-09 8.8083441E+02 1.1366151E-01 2.6074539E-13 7.3459702E+00 -3.0818373E-06 -2.8333609E-08 7.3459702E+00 -3.0818373E-06 -2.8333609E-08 1.9121996E+02 5.2373238E-02 4.9698767E-14 4.2856255E-01 -2.3860011E-07 -2.8506612E-08 4.2856255E-01 -2.3860011E-07 -2.8506612E-08 3.1475549E+02 4.2491779E-02 2.6118541E-13 2.7417312E+00 3.1288841E-06 -3.0129255E-09 2.7417312E+00 3.1288841E-06 -3.0129255E-09 1.8607808E+02 1.2426565E-02 5.1856387E-14 1.1944407E+00 7.2669422E-08 1.1708419E-09 1.1944407E+00 7.2669422E-08 1.1708419E-09 1.0912059E+02 1.1852164E-02 2.6178701E-13 7.5098610E-01 3.5768406E-07 -1.1923338E-08 7.5098610E-01 3.5768406E-07 -1.1923338E-08 9.4294434E+01 3.2661760E-03 5.4879807E-14 2.8261247E-01 8.7458659E-07 6.5774377E-09 2.8261247E-01 8.7458659E-07 6.5774377E-09 5.6273460E+01 2.9558546E-03 2.6257306E-13 2.2497472E-01 -7.5785766E-07 -5.5717333E-09 2.2497472E-01 -7.5785766E-07 -5.5717333E-09 8.8571434E+01 1.8752117E-03 5.8627196E-14 1.8444876E-01 -3.7566878E-07 -4.6674820E-10 1.8444876E-01 -3.7566878E-07 -4.6674820E-10 3.4723320E+01 5.6158280E-04 2.6350954E-13 5.1227380E-02 -1.0769456E-06 9.6749697E-10 5.1227380E-02 -1.0769456E-06 9.6749697E-10 5.5994274E+01 6.4067211E-04 6.3214238E-14 9.9612176E-02 -1.1784223E-07 2.5088120E-10 9.9612176E-02 -1.1784223E-07 2.5088120E-10 3.2573311E+01 5.1920296E-04 2.6477751E-13 6.1285630E-02 -2.0950120E-08 3.0586826E-09 6.1285630E-02 -2.0950120E-08 3.0586826E-09 3.2238415E+01 2.4396315E-04 6.8633819E-14 1.4068934E-02 5.4362783E-08 5.6420063E-10 1.4068934E-02 5.4362783E-08 5.6420063E-10 2.0166826E+01 3.8469082E-04 2.6610138E-13 5.4040551E-02 -4.1566818E-07 -1.5428580E-09 5.4040551E-02 -4.1566818E-07 -1.5428580E-09 1.7658108E+01 1.5379270E-04 7.4891272E-14 1.0539895E-02 -1.0179018E-07 1.1581939E-10 1.0539895E-02 -1.0179018E-07 1.1581939E-10 1.2040778E+01 1.5634559E-04 2.6756307E-13 1.6746340E-02 -5.6590626E-08 -7.2038403E-11 1.6746340E-02 -5.6590626E-08 -7.2038403E-11 1.5882023E+01 2.1458072E-04 8.1940205E-14 2.1327939E-02 -3.5841433E-07 -7.1803763E-10 2.1327939E-02 -3.5841433E-07 -7.1803763E-10 1.0771794E+01 1.3890110E-04 2.6932100E-13 1.6515872E-02 3.9482069E-07 2.9083890E-11 1.6515872E-02 3.9482069E-07 2.9083890E-11 1.8970325E+01 1.1791504E-04 8.9891311E-14 3.0103255E-02 -6.7887918E-08 -3.0744440E-10 3.0103255E-02 -6.7887918E-08 -3.0744440E-10 1.3997983E+01 1.4761774E-04 2.7132601E-13 2.8791601E-02 -1.4400408E-07 -3.7484099E-10 2.8791601E-02 -1.4400408E-07 -3.7484099E-10 6.9224439E+00 1.0474593E-04 9.8745278E-14 1.1323366E-02 9.5958264E-09 -1.5929134E-10 1.1323366E-02 9.5958264E-09 -1.5929134E-10 1.0003628E+01 1.1038726E-04 2.7351968E-13 1.8730281E-02 1.6434619E-07 -1.8579314E-10 1.8730281E-02 1.6434619E-07 -1.8579314E-10 1.0017974E+01 1.4789449E-04 1.0846278E-13 2.5550455E-02 -2.2766029E-07 -6.9938094E-10 2.5550455E-02 -2.2766029E-07 -6.9938094E-10 1.3921675E+01 1.4326723E-04 2.7591693E-13 2.3117559E-02 1.6280067E-07 4.9930360E-10 2.3117559E-02 1.6280067E-07 4.9930360E-10 9.4554539E+00 9.5202442E-05 1.1905914E-13 1.6183496E-02 5.9010745E-08 8.5714956E-11 1.6183496E-02 5.9010745E-08 8.5714956E-11 8.6376410E+00 1.4232975E-04 2.7854794E-13 1.6754905E-02 1.2739095E-07 5.1627247E-10 1.6754905E-02 1.2739095E-07 5.1627247E-10 5.6569176E+00 1.1266072E-04 1.3058180E-13 5.8259335E-03 -2.3682645E-09 1.1920283E-10 5.8259335E-03 -2.3682645E-09 1.1920283E-10 6.8044815E+00 1.1551985E-04 2.8138250E-13 9.1398750E-03 1.2900847E-07 1.1770511E-09 9.1398750E-03 1.2900847E-07 1.1770511E-09 8.3943834E+00 1.2213606E-04 1.4307009E-13 1.3593781E-02 5.0303452E-08 2.2174775E-10 1.3593781E-02 5.0303452E-08 2.2174775E-10 8.8008337E+00 1.7417122E-04 2.8448725E-13 1.3756079E-02 -1.8060780E-08 -1.9156582E-10 1.3756079E-02 -1.8060780E-08 -1.9156582E-10 9.2416582E+00 1.9039912E-04 1.5654310E-13 1.1598191E-02 1.8111442E-07 4.9434481E-11 1.1598191E-02 1.8111442E-07 4.9434481E-11 5.9690027E+00 1.3854665E-04 2.8785259E-13 7.4966187E-03 -8.2792596E-08 -8.4561924E-10 7.4966187E-03 -8.2792596E-08 -8.4561924E-10 6.6154165E+00 1.7594715E-04 1.7098810E-13 8.2535651E-03 1.0081007E-08 2.7772393E-10 8.2535651E-03 1.0081007E-08 2.7772393E-10 4.9477024E+00 1.5676959E-04 2.9150597E-13 -1.0982341E-03 1.8305812E-07 -3.8797316E-11 -1.0982341E-03 1.8305812E-07 -3.8797316E-11 4.7425060E+00 1.9215028E-04 1.8654016E-13 8.4417500E-03 4.1894197E-08 -7.6851436E-10 8.4417500E-03 4.1894197E-08 -7.6851436E-10 4.9923410E+00 1.8782940E-04 2.9535237E-13 1.0517733E-02 8.9072429E-09 -6.7022693E-10 1.0517733E-02 8.9072429E-09 -6.7022693E-10 3.5748935E+00 2.1360058E-04 2.0306027E-13 6.4345165E-03 3.6215458E-10 6.7966427E-10 6.4345165E-03 3.6215458E-10 6.7966427E-10 5.2434268E+00 2.1643443E-04 2.9950410E-13 8.3864843E-03 -9.9383179E-08 5.3938765E-10 8.3864843E-03 -9.9383179E-08 5.3938765E-10 3.7635739E+00 1.9640426E-04 2.2071245E-13 5.1070000E-03 8.0940488E-08 1.1777066E-09 5.1070000E-03 8.0940488E-08 1.1777066E-09 5.4213471E+00 2.5829003E-04 3.0395131E-13 9.6298093E-03 4.3039725E-07 -2.8753067E-10 9.6298093E-03 4.3039725E-07 -2.8753067E-10 4.3534036E+00 2.1423829E-04 2.3945564E-13 8.1508758E-04 -7.4801655E-08 7.3462003E-10 8.1508758E-04 -7.4801655E-08 7.3462003E-10 3.5252440E+00 2.1963776E-04 3.0876170E-13 2.3995279E-03 -1.0476371E-07 6.3604294E-10 2.3995279E-03 -1.0476371E-07 6.3604294E-10 3.8818378E+00 2.3064886E-04 2.5942071E-13 1.5731046E-03 1.5351223E-08 -6.1599176E-10 1.5731046E-03 1.5351223E-08 -6.1599176E-10 3.3869541E+00 2.5392856E-04 3.1382202E-13 1.8893357E-03 2.9237915E-08 -1.1600810E-09 1.8893357E-03 2.9237915E-08 -1.1600810E-09 3.8015990E+00 2.4619431E-04 2.8050441E-13 -5.0806405E-04 4.4362409E-08 3.3435499E-10 -5.0806405E-04 4.4362409E-08 3.3435499E-10 4.0637574E+00 2.6482801E-04 3.1930770E-13 3.9238571E-03 9.3653307E-09 -7.1568845E-10 3.9238571E-03 9.3653307E-09 -7.1568845E-10 3.4207907E+00 2.7267248E-04 3.0293164E-13 3.5970863E-03 -2.5541274E-07 -7.4261697E-10 3.5970863E-03 -2.5541274E-07 -7.4261697E-10 2.7502620E+00 2.7351890E-04 3.2506132E-13 -3.2344339E-03 2.0487516E-08 1.4146884E-09 -3.2344339E-03 2.0487516E-08 1.4146884E-09 2.9286714E+00 2.2570384E-04 3.2656313E-13 -6.4987941E-03 -8.3157175E-08 -6.0048061E-10 -6.4987941E-03 -8.3157175E-08 -6.0048061E-10 2.9461942E+00 2.6674414E-04 3.3123238E-13 -8.7262582E-05 -1.7126274E-08 9.3120051E-10 -8.7262582E-05 -1.7126274E-08 9.3120051E-10 3.5302558E+00 2.4006818E-04 3.5153117E-13 1.9147213E-03 2.8026801E-07 -1.3767842E-09 1.9147213E-03 2.8026801E-07 -1.3767842E-09 3.4332235E+00 2.7609625E-04 3.3787038E-13 -1.0849974E-03 2.4829263E-09 7.5384934E-11 -1.0849974E-03 2.4829263E-09 7.5384934E-11 3.1531720E+00 3.2285869E-04 3.7785619E-13 3.4456691E-03 -4.6111687E-08 4.8703885E-10 3.4456691E-03 -4.6111687E-08 4.8703885E-10 2.4914711E+00 2.7597387E-04 3.4482597E-13 4.9907970E-03 1.0915235E-08 -5.0961585E-10 4.9907970E-03 1.0915235E-08 -5.0961585E-10 2.6640990E+00 3.1714287E-04 4.0568086E-13 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4.7716348E-11 1.8968952E-03 9.9805916E-08 1.0911382E-09 1.8968952E-03 9.9805916E-08 1.0911382E-09 \ No newline at end of file +SIMPLE = T / file does conform to FITS standard BITPIX = 32 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H DATE = '2024-10-08T15:50:34' / file creation date (YYYY-MM-DDThh:mm:ss UT) END XTENSION= 'TABLE ' / ASCII table extension BITPIX = 8 / 8-bit ASCII characters NAXIS = 2 / 2-dimensional ASCII table NAXIS1 = 143 / width of table in characters NAXIS2 = 257 / number of rows in table PCOUNT = 0 / no group parameters (required keyword) GCOUNT = 1 / one data group (required keyword) TFIELDS = 9 / number of fields in each row COMMENT ----------------------------------------------- COMMENT Map Analysis Specific Keywords COMMENT ----------------------------------------------- EXTNAME = 'ANALYSED CROSS POWER SPECTRUM' COMMENT CREATOR = 'ANAFAST ' / Software creating the FITS file VERSION = '3.83 ' / Version of the simulation software COMMENT MAX-LPOL= 256 / Maximum Legendre order L COMMENT POLAR = T / Polarisation included (True/False) BCROSS = T / Magnetic cross terms included (True/False) ASYMCL = T / Asymmetric pol cross terms (XY vs YX) included COMMENT NSIDE = 128 / Resolution Parameter of Input Map COORDSYS= 'unknown ' / Input Map Coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial COMMENT TBCOL1 = 1 / beginning column of field 1 TFORM1 = 'E15.7 ' TTYPE1 = 'TEMPERATURE' / Temperature C(l) TUNIT1 = 'uK^2 ' / square of map units COMMENT TBCOL2 = 17 / beginning column of field 2 TFORM2 = 'E15.7 ' TTYPE2 = 'GRADIENT' / Gradient (=ELECTRIC) polarisation C(l) TUNIT2 = 'uK^2 ' / power spectrum units COMMENT TBCOL3 = 33 / beginning column of field 3 TFORM3 = 'E15.7 ' TTYPE3 = 'CURL ' / Curl (=MAGNETIC) polarisation C(l) TUNIT3 = 'uK^2 ' / power spectrum units COMMENT TBCOL4 = 49 / beginning column of field 4 TFORM4 = 'E15.7 ' TTYPE4 = 'TG ' / Temperature X Gradient cross terms TUNIT4 = 'uK^2 ' / power spectrum units COMMENT TBCOL5 = 65 / beginning column of field 5 TFORM5 = 'E15.7 ' TTYPE5 = 'TC ' / Temperature X Curl cross terms TUNIT5 = 'uK^2 ' / power spectrum units COMMENT TBCOL6 = 81 / beginning column of field 6 TFORM6 = 'E15.7 ' TTYPE6 = 'GC ' / Gradient x Curl cross terms TUNIT6 = 'uK^2 ' / power spectrum units COMMENT TBCOL7 = 97 / beginning column of field 7 TFORM7 = 'E15.7 ' TTYPE7 = 'GT ' / Gradient1 x Temperature2 cross terms TUNIT7 = 'uK^2 ' / power spectrum units COMMENT TBCOL8 = 113 / beginning column of field 8 TFORM8 = 'E15.7 ' TTYPE8 = 'CT ' / Curl1 x Temperature2 cross terms TUNIT8 = 'uK^2 ' / power spectrum units COMMENT TBCOL9 = 129 / beginning column of field 9 TFORM9 = 'E15.7 ' TTYPE9 = 'CG ' / Curl1 x Gradient2 cross terms TUNIT9 = 'uK^2 ' / power spectrum units COMMENT COMMENT The polarisation power spectra have the same definition as in CMBFAST COMMENT CUT-SKY = 0.000000000000E+00 / [deg] Symmetric Cut Sky NITERALM= 0 / Number of iterations for a_lms extraction LREGRESS= 2 / Regression of low multipoles (0/1/2) NMAPS_IN= 2 / Number of maps (co-)analysed (1/2) QUADSCHM= 1 / Quadrature scheme (0/1/2) COMMENT HISTORY Input Map1 = map.fits HISTORY Input Map2 = map.fits END 1.6709244E-08 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 1.3732767E-06 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 1.9208811E+03 1.5580678E-01 4.8352069E-14 1.3119236E+01 1.0511602E-06 5.2924753E-09 1.3119236E+01 1.0511602E-06 5.2924753E-09 8.8083441E+02 1.1366151E-01 2.6074539E-13 7.3459702E+00 -3.0818373E-06 -2.8333609E-08 7.3459702E+00 -3.0818373E-06 -2.8333609E-08 1.9121996E+02 5.2373238E-02 4.9698767E-14 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FITS standard BITPIX = 32 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H DATE = '2022-07-28T14:24:17' / file creation date (YYYY-MM-DDThh:mm:ss UT) END XTENSION= 'TABLE ' / ASCII table extension BITPIX = 8 / 8-bit ASCII characters NAXIS = 2 / 2-dimensional ASCII table NAXIS1 = 95 / width of table in characters NAXIS2 = 257 / number of rows in table PCOUNT = 0 / no group parameters (required keyword) GCOUNT = 1 / one data group (required keyword) TFIELDS = 6 / number of fields in each row COMMENT ----------------------------------------------- COMMENT Map Analysis Specific Keywords COMMENT ----------------------------------------------- EXTNAME = 'ANALYSED AUTO POWER SPECTRUM' COMMENT CREATOR = 'ANAFAST ' / Software creating the FITS file VERSION = '3.82 ' / Version of the simulation software COMMENT MAX-LPOL= 256 / Maximum Legendre order L COMMENT POLAR = T / Polarisation included (True/False) BCROSS = T / Magnetic cross terms included (True/False) ASYMCL = F / Asymmetric pol cross terms (XY vs YX) included COMMENT NSIDE = 128 / Resolution Parameter of Input Map COORDSYS= 'unknown ' / Input Map Coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial COMMENT TBCOL1 = 1 / beginning column of field 1 TFORM1 = 'E15.7 ' TTYPE1 = 'TEMPERATURE' / Temperature C(l) TUNIT1 = 'uK^2 ' / square of map units COMMENT TBCOL2 = 17 / beginning column of field 2 TFORM2 = 'E15.7 ' TTYPE2 = 'GRADIENT' / Gradient (=ELECTRIC) polarisation C(l) TUNIT2 = 'uK^2 ' / power spectrum units COMMENT TBCOL3 = 33 / beginning column of field 3 TFORM3 = 'E15.7 ' TTYPE3 = 'CURL ' / Curl (=MAGNETIC) polarisation C(l) TUNIT3 = 'uK^2 ' / power spectrum units COMMENT TBCOL4 = 49 / beginning column of field 4 TFORM4 = 'E15.7 ' TTYPE4 = 'TG ' / Temperature X Gradient cross terms TUNIT4 = 'uK^2 ' / power spectrum units COMMENT TBCOL5 = 65 / beginning column of field 5 TFORM5 = 'E15.7 ' TTYPE5 = 'TC ' / Temperature X Curl cross terms TUNIT5 = 'uK^2 ' / power spectrum units COMMENT TBCOL6 = 81 / beginning column of field 6 TFORM6 = 'E15.7 ' TTYPE6 = 'GC ' / Gradient x Curl cross terms TUNIT6 = 'uK^2 ' / power spectrum units COMMENT COMMENT The polarisation power spectra have the same definition as in CMBFAST COMMENT CUT-SKY = 0.000000000000E+00 / [deg] Symmetric Cut Sky NITERALM= 0 / Number of iterations for a_lms extraction LREGRESS= 2 / Regression of low multipoles (0/1/2) NMAPS_IN= 1 / Number of maps (co-)analysed (1/2) QUADSCHM= 1 / Quadrature scheme (0/1/2) COMMENT HISTORY Input Map = map.fits END 1.6709244E-08 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 1.3732767E-06 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 1.9208811E+03 1.5580678E-01 4.8352069E-14 1.3119236E+01 1.0511602E-06 5.2924753E-09 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BITPIX = 32 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H DATE = '2024-10-08T15:50:34' / file creation date (YYYY-MM-DDThh:mm:ss UT) END XTENSION= 'TABLE ' / ASCII table extension BITPIX = 8 / 8-bit ASCII characters NAXIS = 2 / 2-dimensional ASCII table NAXIS1 = 95 / width of table in characters NAXIS2 = 257 / number of rows in table PCOUNT = 0 / no group parameters (required keyword) GCOUNT = 1 / one data group (required keyword) TFIELDS = 6 / number of fields in each row COMMENT ----------------------------------------------- COMMENT Map Analysis Specific Keywords COMMENT ----------------------------------------------- EXTNAME = 'ANALYSED AUTO POWER SPECTRUM' COMMENT CREATOR = 'ANAFAST ' / Software creating the FITS file VERSION = '3.83 ' / Version of the simulation software COMMENT MAX-LPOL= 256 / Maximum Legendre order L COMMENT POLAR = T / Polarisation included (True/False) BCROSS = T / Magnetic cross terms included (True/False) ASYMCL = F / Asymmetric pol cross terms (XY vs YX) included COMMENT NSIDE = 128 / Resolution Parameter of Input Map COORDSYS= 'unknown ' / Input Map Coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial COMMENT TBCOL1 = 1 / beginning column of field 1 TFORM1 = 'E15.7 ' TTYPE1 = 'TEMPERATURE' / Temperature C(l) TUNIT1 = 'uK^2 ' / square of map units COMMENT TBCOL2 = 17 / beginning column of field 2 TFORM2 = 'E15.7 ' TTYPE2 = 'GRADIENT' / Gradient (=ELECTRIC) polarisation C(l) TUNIT2 = 'uK^2 ' / power spectrum units COMMENT TBCOL3 = 33 / beginning column of field 3 TFORM3 = 'E15.7 ' TTYPE3 = 'CURL ' / Curl (=MAGNETIC) polarisation C(l) TUNIT3 = 'uK^2 ' / power spectrum units COMMENT TBCOL4 = 49 / beginning column of field 4 TFORM4 = 'E15.7 ' TTYPE4 = 'TG ' / Temperature X Gradient cross terms TUNIT4 = 'uK^2 ' / power spectrum units COMMENT TBCOL5 = 65 / beginning column of field 5 TFORM5 = 'E15.7 ' TTYPE5 = 'TC ' / Temperature X Curl cross terms TUNIT5 = 'uK^2 ' / power spectrum units COMMENT TBCOL6 = 81 / beginning column of field 6 TFORM6 = 'E15.7 ' TTYPE6 = 'GC ' / Gradient x Curl cross terms TUNIT6 = 'uK^2 ' / power spectrum units COMMENT COMMENT The polarisation power spectra have the same definition as in CMBFAST COMMENT CUT-SKY = 0.000000000000E+00 / [deg] Symmetric Cut Sky NITERALM= 0 / Number of iterations for a_lms extraction LREGRESS= 2 / Regression of low multipoles (0/1/2) NMAPS_IN= 1 / Number of maps (co-)analysed (1/2) QUADSCHM= 1 / Quadrature scheme (0/1/2) COMMENT HISTORY Input Map = map.fits END 1.6709244E-08 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 1.3732767E-06 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 1.9208811E+03 1.5580678E-01 4.8352069E-14 1.3119236E+01 1.0511602E-06 5.2924753E-09 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index ceb99d9f..7709604d 100644 --- a/test/cl_w2.fits +++ b/test/cl_w2.fits @@ -1 +1 @@ -SIMPLE = T / file does conform to FITS standard BITPIX = 32 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H DATE = '2022-07-28T14:24:17' / file creation date (YYYY-MM-DDThh:mm:ss UT) END XTENSION= 'TABLE ' / ASCII table extension BITPIX = 8 / 8-bit ASCII characters NAXIS = 2 / 2-dimensional ASCII table NAXIS1 = 95 / width of table in characters NAXIS2 = 257 / number of rows in table PCOUNT = 0 / no group parameters (required keyword) GCOUNT = 1 / one data group (required keyword) TFIELDS = 6 / number of fields in each row COMMENT ----------------------------------------------- COMMENT Map Analysis Specific Keywords COMMENT ----------------------------------------------- EXTNAME = 'ANALYSED AUTO POWER SPECTRUM' COMMENT CREATOR = 'ANAFAST ' / Software creating the FITS file VERSION = '3.82 ' / Version of the simulation software COMMENT MAX-LPOL= 256 / Maximum Legendre order L COMMENT POLAR = T / Polarisation included (True/False) BCROSS = T / Magnetic cross terms included (True/False) ASYMCL = F / Asymmetric pol cross terms (XY vs YX) included COMMENT NSIDE = 128 / Resolution Parameter of Input Map COORDSYS= 'unknown ' / Input Map Coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial COMMENT TBCOL1 = 1 / beginning column of field 1 TFORM1 = 'E15.7 ' TTYPE1 = 'TEMPERATURE' / Temperature C(l) TUNIT1 = 'uK^2 ' / square of map units COMMENT TBCOL2 = 17 / beginning column of field 2 TFORM2 = 'E15.7 ' TTYPE2 = 'GRADIENT' / Gradient (=ELECTRIC) polarisation C(l) TUNIT2 = 'uK^2 ' / power spectrum units COMMENT TBCOL3 = 33 / beginning column of field 3 TFORM3 = 'E15.7 ' TTYPE3 = 'CURL ' / Curl (=MAGNETIC) polarisation C(l) TUNIT3 = 'uK^2 ' / power spectrum units COMMENT TBCOL4 = 49 / beginning column of field 4 TFORM4 = 'E15.7 ' TTYPE4 = 'TG ' / Temperature X Gradient cross terms TUNIT4 = 'uK^2 ' / power spectrum units COMMENT TBCOL5 = 65 / beginning column of field 5 TFORM5 = 'E15.7 ' TTYPE5 = 'TC ' / Temperature X Curl cross terms TUNIT5 = 'uK^2 ' / power spectrum units COMMENT TBCOL6 = 81 / beginning column of field 6 TFORM6 = 'E15.7 ' TTYPE6 = 'GC ' / Gradient x Curl cross terms TUNIT6 = 'uK^2 ' / power spectrum units COMMENT COMMENT The polarisation power spectra have the same definition as in CMBFAST COMMENT CUT-SKY = 0.000000000000E+00 / [deg] Symmetric Cut Sky NITERALM= 0 / Number of iterations for a_lms extraction LREGRESS= 2 / Regression of low multipoles (0/1/2) NMAPS_IN= 1 / Number of maps (co-)analysed (1/2) QUADSCHM= 2 / Quadrature scheme (0/1/2) COMMENT HISTORY Input Map = map.fits END 1.5448977E-08 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 1.4854892E-06 0.0000000E+00 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8.8585132E-11 1.8970133E-03 1.1208419E-07 2.8103480E-09 \ No newline at end of file +SIMPLE = T / file does conform to FITS standard BITPIX = 32 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H DATE = '2024-10-08T15:50:34' / file creation date (YYYY-MM-DDThh:mm:ss UT) END XTENSION= 'TABLE ' / ASCII table extension BITPIX = 8 / 8-bit ASCII characters NAXIS = 2 / 2-dimensional ASCII table NAXIS1 = 95 / width of table in characters NAXIS2 = 257 / number of rows in table PCOUNT = 0 / no group parameters (required keyword) GCOUNT = 1 / one data group (required keyword) TFIELDS = 6 / number of fields in each row COMMENT ----------------------------------------------- COMMENT Map Analysis Specific Keywords COMMENT ----------------------------------------------- EXTNAME = 'ANALYSED AUTO POWER SPECTRUM' COMMENT CREATOR = 'ANAFAST ' / Software creating the FITS file VERSION = '3.83 ' / Version of the simulation software COMMENT MAX-LPOL= 256 / Maximum Legendre order L COMMENT POLAR = T / Polarisation included (True/False) BCROSS = T / Magnetic cross terms included (True/False) ASYMCL = F / Asymmetric pol cross terms (XY vs YX) included COMMENT NSIDE = 128 / Resolution Parameter of Input Map COORDSYS= 'unknown ' / Input Map Coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial COMMENT TBCOL1 = 1 / beginning column of field 1 TFORM1 = 'E15.7 ' TTYPE1 = 'TEMPERATURE' / Temperature C(l) TUNIT1 = 'uK^2 ' / square of map units COMMENT TBCOL2 = 17 / beginning column of field 2 TFORM2 = 'E15.7 ' TTYPE2 = 'GRADIENT' / Gradient (=ELECTRIC) polarisation C(l) TUNIT2 = 'uK^2 ' / power spectrum units COMMENT TBCOL3 = 33 / beginning column of field 3 TFORM3 = 'E15.7 ' TTYPE3 = 'CURL ' / Curl (=MAGNETIC) polarisation C(l) TUNIT3 = 'uK^2 ' / power spectrum units COMMENT TBCOL4 = 49 / beginning column of field 4 TFORM4 = 'E15.7 ' TTYPE4 = 'TG ' / Temperature X Gradient cross terms TUNIT4 = 'uK^2 ' / power spectrum units COMMENT TBCOL5 = 65 / beginning column of field 5 TFORM5 = 'E15.7 ' TTYPE5 = 'TC ' / Temperature X Curl cross terms TUNIT5 = 'uK^2 ' / power spectrum units COMMENT TBCOL6 = 81 / beginning column of field 6 TFORM6 = 'E15.7 ' TTYPE6 = 'GC ' / Gradient x Curl cross terms TUNIT6 = 'uK^2 ' / power spectrum units COMMENT COMMENT The polarisation power spectra have the same definition as in CMBFAST COMMENT CUT-SKY = 0.000000000000E+00 / [deg] Symmetric Cut Sky NITERALM= 0 / Number of iterations for a_lms extraction LREGRESS= 2 / Regression of low multipoles (0/1/2) NMAPS_IN= 1 / Number of maps (co-)analysed (1/2) QUADSCHM= 2 / Quadrature scheme (0/1/2) COMMENT HISTORY Input Map = map.fits END 1.5448977E-08 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 0.0000000E+00 1.4854892E-06 0.0000000E+00 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4.8500475E-08 1.5338657E-09 1.5449342E-01 5.9151618E-05 1.9625577E-11 1.5821594E-03 4.7270230E-08 -2.6355839E-11 1.7861411E-01 6.7486908E-05 6.5640736E-11 2.1245179E-03 5.5962605E-08 -1.2114725E-09 1.8427038E-01 6.6013912E-05 2.0689981E-11 2.0611852E-03 -1.7841114E-07 -2.9112037E-09 1.6919816E-01 6.8032372E-05 7.0048259E-11 1.9940692E-03 2.4123713E-07 2.9320188E-09 1.4857613E-01 6.6503890E-05 2.1595175E-11 1.7627242E-03 -1.3642794E-07 -1.9996134E-09 1.5285006E-01 7.1206727E-05 7.4431739E-11 1.9556046E-03 5.8458351E-08 -2.7034469E-10 1.4172393E-01 6.9630631E-05 2.2292978E-11 1.7682504E-03 -1.5216903E-08 -2.0386579E-09 1.6189575E-01 8.0774233E-05 7.8731376E-11 2.1063813E-03 7.5400962E-08 4.0089563E-09 1.3523257E-01 7.6472905E-05 2.3811463E-11 1.8898976E-03 3.5521278E-08 3.0853067E-10 1.4768484E-01 8.0704544E-05 8.3451364E-11 1.9903211E-03 1.2909912E-07 -6.7448092E-10 1.3509472E-01 8.2717939E-05 2.5493748E-11 2.0095694E-03 -1.7144478E-08 5.6922922E-10 1.2666613E-01 7.5758951E-05 8.8585132E-11 1.8970133E-03 1.1208419E-07 2.8103480E-09 \ No newline at end of file diff --git a/test/distmask.fits b/test/distmask.fits index ecee10b8..a6a8615d 100644 --- a/test/distmask.fits +++ b/test/distmask.fits @@ -1,73 +1,75 @@ -SIMPLE = T / file does conform to FITS standard BITPIX = 32 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H DATE = '2022-07-28T14:24:18' / file creation date (YYYY-MM-DDThh:mm:ss UT) END XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 8192 / width of table in bytes NAXIS2 = 3 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 1 / number of fields in each row COMMENT COMMENT ----------------------------------------------- COMMENT Sky Map Pixelisation Specific Keywords COMMENT ----------------------------------------------- PIXTYPE = 'HEALPIX ' / HEALPIX Pixelisation ORDERING= 'RING ' / Pixel ordering scheme, either RING or NESTED NSIDE = 16 / Resolution parameter for HEALPIX FIRSTPIX= 0 / First pixel # (0 based) LASTPIX = 3071 / Last pixel # (0 based) COORDSYS= 'unknown ' / Pixelisation coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial BAD_DATA= -1.637500000000E+30 / Sentinel value given to bad pixels COMMENT COMMENT ----------------------------------------------- COMMENT Planck Simulation Specific Keywords COMMENT ----------------------------------------------- EXTNAME = 'FULL SKY MAP' CREATOR = 'process_mask' / Software creating the FITS file VERSION = '3.82 ' / Version of the simulation software COMMENT POLCCONV= 'COSMO ' / Coord. convention for polarisation (COSMO/IAU) COMMENT ----------------------------------------------- COMMENT Data Description Specific Keywords COMMENT ----------------------------------------------- COMMENT COMMENT Full sky data OBJECT = 'FULLSKY ' INDXSCHM= 'IMPLICIT' / Indexing : IMPLICIT or EXPLICIT COMMENT POLAR = F / Polarisation included (True/False) DERIV = 0 / Derivative included (0, 1 or 2) COMMENT TUNIT1 = 'RADIANS ' / map unit COMMENT TTYPE1 = 'ANGULAR_DISTANCE' / [RAD] TFORM1 = '1024D ' / data format of field: 8-byte REAL HISTORY Distance to closest hole for HISTORY Input mask: HISTORY mask.fits HISTORY Filled mask: HISTORY NP_MIN = 0 / [pixels] Minimal size END ?:ej? tZ?ּ"e?EzUd?fe,>?_?b%?!_? -Y?uP?'Ia?t,o?1V?d~ ?N, ?W&??ɏƀ ?.?à F>?Qe,>?_?b%?!_? +Y?uP?'Ia?t,o?1V?d~ ?N, ?W&??ɏƀ ?.?à F>?Q -?<:߻X?c*b?WVπ?O#Z?΁?b$N?w?E?"R`kd?䖶?k.~?೟U?O5U|6?݉t{?{+f͐?`70?ށj{V?p̘?:(?=? ?l-3G?O2Dt?˵\?L!?Z %?V1tE?졥pf?/31q?H?1Ӓ?26z?෩?3?25?ے2?23?3?෩?26z?1Ӓ?H?/31p?ol?r9)M?ƿ?8'i?=j .m?3og,?1R?۱IB?ȡ6x?HY(?l=y?㏷G -?OcRp?`b?aAI?V 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PI?斋k&?#G?B''?r/?s.?R?9a?5US?Vxh?5US?Oל?MDl%?q^?녟?ݨ}r#?f`̜?|ׇ?m~Y%?!J? ?WL?p?x?0rYN?}X? ĵ@?;e8/Q?aBm?x˛3,?~|nm?nfރ?FAFx?^K?6?rʓ?AS?L3?u ?0Qk?pz?5??L?Uu?ߎC?Ut?L?gVhi?Pg?d?*ٚ2?R{o6x?ZA$a? ?? ? i?ˡN ?k_?K'7?E?jIo`&?(_ |?i.m ?[%v?Zt,F?`˵?`˵? ?{?nΈ?i ?t?dI"W?nco?2a?]@?[?(L?;?;0?<_?5R?۰ԋK?Hϊ?LH?\(u?렶?lHe?.oӿ?S-?\<0_?bdv?\VK?9jV:?jog?隴8?1jx ?8Am&?ՓyQ?.h?c} ?hL?Y?5I%5?gGu/?w +Q?󍋯e?YϫrK?⧓5??L?Uu?ߎC?Ut?L?gVhi?Pg?d?*ٚ2?R{o6x?ZA$a? ?? ? i?ˡN ?k_?K'7?E?jIo`&?(_ |?i.m ?[%v?Zt,F?`˵?`˵? ?{?n·?i ?t?dI"W?nco?2a?]@?[?(L?;?;0?<_?5R?۰ԋK?Hϊ?LH?\(u?렶?lHe?.oӿ?S-?\<0_?bdv?\VK?9jV:?jog?隴8?1jx ?8Am%?ՓyQ?.h?c} ?hL?Y?5I%5?gGu/?w ؑ?WfH?\ cU?po?ݾ9? - u??R?5$5?TQi?d"a`?Vw?=j?갺g?xfU?>f/?!]i? Z$?Ea?X%? f/?!]i? Z$?Ea?X%? BTB6rBfeqBTB^/BůBBg@@TB$(B#*^3YBTB6rBfeqBTB^/BůBBg@@TB$(B#*^3YQB,VA6BYB:CgB[NE٪Q ¯zʇō:$@G B|B%HAAQK6B-v_J&3!Tf/Xe›JI©sW´1¬N$(BfBܸ@Uy(4K•emBBCBqIB#™®F8 AA diff --git a/test/map.gif b/test/map.gif index 29ca60ea..f3a57cce 100644 Binary files a/test/map.gif and b/test/map.gif differ diff --git a/test/map_LOres.fits b/test/map_LOres.fits index 95fc4abf..02573c18 100644 --- a/test/map_LOres.fits +++ b/test/map_LOres.fits @@ -1,4 +1,4 @@ -SIMPLE = T / file does conform to FITS standard BITPIX = 32 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H DATE = '2022-07-28T14:24:17' / file creation date (YYYY-MM-DDThh:mm:ss UT) END XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 12 / width of table in bytes NAXIS2 = 192 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 3 / number of fields in each row COMMENT COMMENT ----------------------------------------------- COMMENT Sky Map Pixelisation Specific Keywords COMMENT ----------------------------------------------- PIXTYPE = 'HEALPIX ' / HEALPIX Pixelisation ORDERING= 'RING ' / Pixel ordering scheme, either RING or NESTED NSIDE = 4 / Resolution parameter for HEALPIX FIRSTPIX= 0 / First pixel # (0 based) LASTPIX = 191 / Last pixel # (0 based) COORDSYS= 'unknown ' / Pixelisation coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial BAD_DATA= -1.637500000000E+30 / Sentinel value given to bad pixels COMMENT COMMENT ----------------------------------------------- COMMENT Planck Simulation Specific Keywords COMMENT ----------------------------------------------- EXTNAME = 'DEGRADED DATA' CREATOR = 'UD_GRADE' / Software creating the FITS file VERSION = '3.82 ' / Version of the simulation software COMMENT POLCCONV= 'COSMO ' COMMENT ----------------------------------------------- COMMENT Data Description Specific Keywords COMMENT ----------------------------------------------- COMMENT COMMENT Full sky data OBJECT = 'FULLSKY ' INDXSCHM= 'IMPLICIT' / Indexing : IMPLICIT or EXPLICIT COMMENT POLAR = T / Polarisation included (True/False) DERIV = 0 / Derivative included (0, 1 or 2) COMMENT TTYPE1 = 'TEMPERATURE' / Temperature map TFORM1 = '1E ' / data format of field: 4-byte REAL TUNIT1 = 'uK ' / map unit COMMENT TTYPE2 = 'Q_POLARISATION' / Q Polarisation map TFORM2 = '1E ' / data format of field: 4-byte REAL TUNIT2 = 'uK ' / map unit COMMENT TTYPE3 = 'U_POLARISATION' / U Polarisation map TFORM3 = '1E ' / data format of field: 4-byte REAL TUNIT3 = 'uK ' / map unit COMMENT HISTORY Input Map in map.fits HISTORY Input Map resolution NSIDE = 128 COMMENT END Al㲾^:^U>us ߧ1A#g>(U>yU_ӄ!:e>=_p>?:è>˾jk9G}-g>q> A;XQLf==Zs17ؾ;2?t4?@w>B >ChxB7<6)Y~>^b;wfB'==H>Hʒl>x=y>?7@+>+v/QAپþ4&A2˿3" ds$F?5^¹g?T?R1R?3M>=㩾#}͓Řc=澵A\Hc~B=6>ZϵA`^>-~P;>>ԢCXe>jwxח>|9M̽@R{>5B-2B43>\?B3ʕiuBz-pw){>Û?ILȆL?NM? >#ŠMȾ\k!7ζ +SIMPLE = T / file does conform to FITS standard BITPIX = 32 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H DATE = '2024-10-08T15:50:34' / file creation date (YYYY-MM-DDThh:mm:ss UT) END XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 12 / width of table in bytes NAXIS2 = 192 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 3 / number of fields in each row COMMENT COMMENT ----------------------------------------------- COMMENT Sky Map Pixelisation Specific Keywords COMMENT ----------------------------------------------- PIXTYPE = 'HEALPIX ' / HEALPIX Pixelisation ORDERING= 'RING ' / Pixel ordering scheme, either RING or NESTED NSIDE = 4 / Resolution parameter for HEALPIX FIRSTPIX= 0 / First pixel # (0 based) LASTPIX = 191 / Last pixel # (0 based) COORDSYS= 'unknown ' / Pixelisation coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial BAD_DATA= -1.637500000000E+30 / Sentinel value given to bad pixels COMMENT COMMENT ----------------------------------------------- COMMENT Planck Simulation Specific Keywords COMMENT ----------------------------------------------- EXTNAME = 'DEGRADED DATA' CREATOR = 'UD_GRADE' / Software creating the FITS file VERSION = '3.83 ' / Version of the simulation software COMMENT POLCCONV= 'COSMO ' COMMENT ----------------------------------------------- COMMENT Data Description Specific Keywords COMMENT ----------------------------------------------- COMMENT COMMENT Full sky data OBJECT = 'FULLSKY ' INDXSCHM= 'IMPLICIT' / Indexing : IMPLICIT or EXPLICIT COMMENT POLAR = T / Polarisation included (True/False) DERIV = 0 / Derivative included (0, 1 or 2) COMMENT TTYPE1 = 'TEMPERATURE' / Temperature map TFORM1 = '1E ' / data format of field: 4-byte REAL TUNIT1 = 'uK ' / map unit COMMENT TTYPE2 = 'Q_POLARISATION' / Q Polarisation map TFORM2 = '1E ' / data format of field: 4-byte REAL TUNIT2 = 'uK ' / map unit COMMENT TTYPE3 = 'U_POLARISATION' / U Polarisation map TFORM3 = '1E ' / data format of field: 4-byte REAL TUNIT3 = 'uK ' / map unit COMMENT HISTORY Input Map in map.fits HISTORY Input Map resolution NSIDE = 128 COMMENT END Al㲾^:^U>us ߧ1A#g>(U>yU_ӄ!:e>=_p>?:è>˾jk9G}-g>q> A;XQLf==Zs17ؾ;2?t4?@w>B >ChxB7<6)Y~>^b;wfB'==H>Hʒl>x=y>?7@+>+v/QAپþ4&A2˿3" ds$F?5^¹g?T?R1R?3M>=㩾#}͓Řc=澵A\Hc~B=6>ZϵA`^>-~P;>>ԢCXe>jwxח>|9M̽@R{>5B-2B43>\?B3ʕiuBz-pw){>Û?ILȆL?NM? >#ŠMȾ\k!7ζ &Tپ (ML?rAD>%n$>`h=S$V=4kˆ>gསZ?'>{־.BJ!>xBoR>$BnƽU%csBu>h>#t_Б?:|>u– >>± ^՗$/OLA zW?N=[>{з FQ>&B5[lF+l>?#1=XEp:>>x>f.B(>[2zBi>YB .=Ӵ>BSQ>2< xAr=k 6 5>짾 B =D2s=K>>jQ[=~ľ]Bi8sBvd⽁?%B79>su>Apk?&r8;tA̒>DqARE2>rjBl\=1BGjQ=o>@=@>FBiȐ;S=|NA1>G"@B'o=O>fv‡;>=Ɂf>8_̮A"=U)LtByt(B"?\R{@"NL7A>HB%C?3#NAAQ]>+ҽ4A<2n>{AaƾV>Dg(B,s,eAQ>3A-I>LBYJ>t@w2B=3j=R>Lz:==.2B.>,>ӉB?Ai>ʾIC7jB M>+![=B>SB diff --git a/test/map_LOres.gif b/test/map_LOres.gif index 31dfab78..aeb22788 100644 Binary files a/test/map_LOres.gif and b/test/map_LOres.gif differ diff --git a/test/map_ext.fits b/test/map_ext.fits index f65d2eaf..960cd11e 100644 --- a/test/map_ext.fits +++ b/test/map_ext.fits @@ -1,2 +1,2 @@ -SIMPLE = T / file does conform to FITS standard BITPIX = 32 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H DATE = '2022-07-28T14:24:17' / file creation date (YYYY-MM-DDThh:mm:ss UT) END XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 4 / width of table in bytes NAXIS2 = 192 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 1 / number of fields in each row COMMENT COMMENT ----------------------------------------------- COMMENT Sky Map Pixelisation Specific Keywords COMMENT ----------------------------------------------- PIXTYPE = 'HEALPIX ' / HEALPIX Pixelisation ORDERING= 'RING ' / Pixel ordering scheme, either RING or NESTED NSIDE = 4 / Resolution parameter for HEALPIX FIRSTPIX= 0 / First pixel # (0 based) LASTPIX = 191 / Last pixel # (0 based) COORDSYS= 'unknown ' / Pixelisation coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial BAD_DATA= -1.637500000000E+30 / Sentinel value given to bad pixels COMMENT COMMENT ----------------------------------------------- COMMENT Planck Simulation Specific Keywords COMMENT ----------------------------------------------- EXTNAME = 'PEAK MAP' CREATOR = 'HOTSPOTS' / Software creating the FITS file VERSION = '3.82 ' / Version of the simulation software COMMENT POLCCONV= 'COSMO ' / Coord. convention for polarisation (COSMO/IAU) COMMENT ----------------------------------------------- COMMENT Data Description Specific Keywords COMMENT ----------------------------------------------- COMMENT COMMENT Full sky data OBJECT = 'FULLSKY ' INDXSCHM= 'IMPLICIT' / Indexing : IMPLICIT or EXPLICIT COMMENT POLAR = F / Polarisation included (True/False) DERIV = 0 / Derivative included (0, 1 or 2) COMMENT TTYPE1 = 'PEAKS ' / Maxima and Minima TFORM1 = '1E ' / data format of field: 4-byte REAL TUNIT1 = 'unknown ' / map unit COMMENT COMMENT Input Map =test_LOres.fits COMMENT Local Min and Max keep their original value, the rest is set to 0 END Alk9B7^¹gBB3ȆLˆBJ!±B +SIMPLE = T / file does conform to FITS standard BITPIX = 32 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H DATE = '2024-10-08T15:50:34' / file creation date (YYYY-MM-DDThh:mm:ss UT) END XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 4 / width of table in bytes NAXIS2 = 192 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 1 / number of fields in each row COMMENT COMMENT ----------------------------------------------- COMMENT Sky Map Pixelisation Specific Keywords COMMENT ----------------------------------------------- PIXTYPE = 'HEALPIX ' / HEALPIX Pixelisation ORDERING= 'RING ' / Pixel ordering scheme, either RING or NESTED NSIDE = 4 / Resolution parameter for HEALPIX FIRSTPIX= 0 / First pixel # (0 based) LASTPIX = 191 / Last pixel # (0 based) COORDSYS= 'unknown ' / Pixelisation coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial BAD_DATA= -1.637500000000E+30 / Sentinel value given to bad pixels COMMENT COMMENT ----------------------------------------------- COMMENT Planck Simulation Specific Keywords COMMENT ----------------------------------------------- EXTNAME = 'PEAK MAP' CREATOR = 'HOTSPOTS' / Software creating the FITS file VERSION = '3.83 ' / Version of the simulation software COMMENT POLCCONV= 'COSMO ' / Coord. convention for polarisation (COSMO/IAU) COMMENT ----------------------------------------------- COMMENT Data Description Specific Keywords COMMENT ----------------------------------------------- COMMENT COMMENT Full sky data OBJECT = 'FULLSKY ' INDXSCHM= 'IMPLICIT' / Indexing : IMPLICIT or EXPLICIT COMMENT POLAR = F / Polarisation included (True/False) DERIV = 0 / Derivative included (0, 1 or 2) COMMENT TTYPE1 = 'PEAKS ' / Maxima and Minima TFORM1 = '1E ' / data format of field: 4-byte REAL TUNIT1 = 'unknown ' / map unit COMMENT COMMENT Input Map =test_LOres.fits COMMENT Local Min and Max keep their original value, the rest is set to 0 END Alk9B7^¹gBB3ȆLˆBJ!±B .ntBGjBiȐ‡;B%CBB![–B|Bmº \ No newline at end of file diff --git a/test/map_ext.gif b/test/map_ext.gif index fd6d1fe5..e8788073 100644 Binary files a/test/map_ext.gif and b/test/map_ext.gif differ diff --git a/test/map_mf.fits b/test/map_mf.fits index bb1684b4..32c53baf 100644 --- a/test/map_mf.fits +++ b/test/map_mf.fits @@ -1,4 +1,4 @@ -SIMPLE = T / file does conform to FITS standard BITPIX = 32 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H DATE = '2022-07-28T14:24:18' / file creation date (YYYY-MM-DDThh:mm:ss UT) END XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 12288 / width of table in bytes NAXIS2 = 192 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 3 / number of fields in each row COMMENT **************************************************************** COMMENT HISTORY alm generated by CREATE_ALM_2.1.0 from following power spectrum COMMENT COMMENT ---------------------------------------------------- COMMENT Planck Power Spectrum Description Specific Keywords COMMENT ---------------------------------------------------- COMMENT Input power spectrum in : COMMENT cl.fits COMMENT COMMENT Quadrupole COMMENT C(2) = 1.278940E+03 uK^2 COMMENT COMMENT COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- BCROSS = F / Magnetic cross terms included (True/False) COMMENT ----------------------------------------------- COMMENT ----------------------------------------------- TEMPTYPE= 'THERMO ' / temperature type either THERMO or ANTENNA POLNORM = 'CMBFAST ' / CMBFAST (EB) convention for polar. spectra COMMENT **************************************************************** COMMENT COMMENT ----------------------------------------------- COMMENT Sky Map Pixelisation Specific Keywords COMMENT ----------------------------------------------- PIXTYPE = 'HEALPIX ' / HEALPIX Pixelisation ORDERING= 'RING ' / Pixel ordering scheme, either RING or NESTED NSIDE = 128 / Resolution parameter for HEALPIX FIRSTPIX= 0 / First pixel # (0 based) LASTPIX = 196607 / Last pixel # (0 based) COORDSYS= 'unknown ' / Pixelisation coordinate system COMMENT G = Galactic, E = ecliptic, C = celestial = equatorial COMMENT COMMENT ----------------------------------------------- COMMENT Planck Simulation Specific Keywords COMMENT ----------------------------------------------- CREATOR = 'MEDIAN_FILTER' VERSION = '3.82 ' COMMENT MAX-LPOL= 256 / Maximum Legendre order L RANDSEED= -1 / Random generator seed POLCCONV= 'COSMO ' / Coord. convention for polarisation (COSMO/IAU) FWHM = 5.000000000000E-01 / [deg] FWHM of gaussian symmetric beam COMMENT ----------------------------------------------- COMMENT Data Description Specific Keywords COMMENT ----------------------------------------------- COMMENT COMMENT Full sky data OBJECT = 'FULLSKY ' INDXSCHM= 'IMPLICIT' / Indexing : IMPLICIT or EXPLICIT COMMENT POLAR = T / Polarisation included (True/False) DERIV = 0 / Derivative included (0, 1 or 2) COMMENT TTYPE1 = 'TEMPERATURE' / Temperature map TFORM1 = '1024E ' / data format of field: 4-byte REAL TUNIT1 = 'uK ' / map unit COMMENT TTYPE2 = 'Q_POLARISATION' / Q Polarisation map TFORM2 = '1024E ' / data format of field: 4-byte REAL TUNIT2 = 'uK ' / map unit COMMENT TTYPE3 = 'U_POLARISATION' / U Polarisation map TFORM3 = '1024E ' / data format of field: 4-byte REAL TUNIT3 = 'uK ' / map unit COMMENT COMMENT ************************************* COMMENT ----------------------------------------------- HISTORY median filtered map HISTORY input map: map.fits MFRADIUS= 1.500000000000E+00 / [Deg] median filter radius BAD_DATA= -1.63750000E+30 / Sentinel value given to missing data COMMENT ----------------------------------------------- END <'tAהA%!A.AۼA.@6_@VAABA_AהA%!A.AۼA.@6_@VAABA_FyPX'?G-ʇ+|@G Av8BB FAAiAQA ,("BBw§k¬¨TQA=+6A:;AzB(BJ BWfBtB/ B߿kB[NB>BIL‰req[%Z@A_0= z$» #ڀB8IPŠߣu=0Å1D  C¥FC0iQ 3Au;QSd>2 @@ -144,7 +144,7 @@ h un€ơAbBqg«D@g34TlI?£*CxC3+@ )Mn/?D @A`ƒq ‚TEBJBF"n@^o\;~ 3:̦[LL$KŽ-ukE"VO9qa.Z5E®^jğXA@tj1SeIMMG8·mFjQyQHwxMLGVBDAAοv?AlVB?BpjAgAB`B Až ª,@XBQ*TBm[Ok©͸!AZI¬U$¹=¬v:TA?B B~ aj˜//A®9¨|1P)›i©@I^RA9AB$C4 (C2ʪBuQ0z]A B B޳B:@@QABXAasp֥‚vBXB;A޼"I!ir@A e& Ÿm\PB ĻB4+u —)>B+tBYPRrBBBoBpB B?lBl(B/uMAϡyAd8PA{OBx9>BJB\`?hVNBVSBḄUBBeB6*BZBtCi C~C>B|B~BUC BABFB{BC4@#B-BjB9@BBB+ $KRAYB!B*•h›vA.!­ҙ<$S6£y@`9¹ʟ¿h -8x0K{Í«TVaplA=bGԹpvo•R7AzAB?{_T(%-·L_|tJ[°g1!_ɧh$d•¹ $ªq2Lz,#2° b\řf:^zZ`9/Yb(X&L!*"Pz£9&Q*|BY8K>—\¢W%W"S2»šKo¡­A˦WŠ((yB-BgA;%B;@@0B!Bf}P@Y`´=|ҍuªtB~>CfAtq؜̬]907i˜2@neˆŽAA[ 0=ZhS&Z|1€@@+?Q]*LC.˔Kb`\9`<0VJ? N,t@;>ALASAAiA2AA>{AYܗAi.@n)@A¿'ACA/AԵA(AuYA'AA|\AT]A+@m@w?Ďҿ+:x%LIpn1U"^0iV9uQQH$Bi6?:P@lA/?A|8ZA AzAAgA AAQAa{AAaA)_@vG@"@8wo?n8GeI(Tp'mM)p.OXM*GkqӐ?zpv{S 'em?{@mA@\Ae4AA1AA䗏ARAAaAAA3Ak\A6A@]@Dy@?C)EkFN(&M|pP)uQ\XeoO8\Xx,[19B̓i\6lz@G4@GA!IAZZeA]AAqA^A၅A\#A/6A5Aҕ"AMA&ARAtAQA4AA A@ diff --git a/test/map_sm.gif b/test/map_sm.gif index 6db2dc8a..8cb88b47 100644 Binary files a/test/map_sm.gif and b/test/map_sm.gif differ