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Pipeline for SO delensing study (L3.3)

This package contains Python codes for constructing B-mode lensing template from cosmic microwave background anisotropies (CMB) in curvedsky.

Dependencies

The current code depends on the following python modules:

Files

The main files for the analysis are as follows:

  • simmap.py: generate simulated signal and noise maps for each frequency and patch
  • cmb_map2alm.py: spherical harmonic transform of map to alm at each frequency and patch, and compute power spectra
  • cmb_wiener.py: Optimally-combined alms from LAT and SAT with Wiener filtering.
  • delens.py: construct lensing B-mode template and compute auto and cross spectra between lensing template and SAT B-modes
  • gen_mass_sims.py: generate random Gaussian fields from the covariance of the mass-tracers.
  • prjlib.py: read and define parameters and filename for analysis and some functions
  • params.ini: parameter file

Contacts

Toshiya Namikawa (namikawa at slac.stanford.edu) Anton Baleato (a.baleatolizancos at ast.cam.ac.uk) Emilie Hertig (emh83 at cam.ac.uk)

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Code for delensing studies (L3.3)

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