Light field geometry estimator for plenoptic cameras
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Updated
Mar 11, 2025 - Python
Light field geometry estimator for plenoptic cameras
Gravitational microlensing classification engine using machine learning
The fastest gravitational (quasar) microlensing code on the planet. A parallel Barnes-Hut tree code optimized for GPUs, written in OpenCL
MAGIC: Microlensing Analysis Guided by Intelligent Computation. A PyTorch framework for automatic analysis of realistic microlensing light curves.
Implementation of automatic differentiation in VBozza's BinaryLensing
muLAn: MICROlensing Analysis software
Amoeba: an AGN Model of Optical Emissions Beyond steady-state Accretion disks
The goal of this project is to create an all-encompassing collection of Jupyter notebooks—your trusty companions for engaging exercises related to microlensing. Through these notebooks, the insights and experiences of microlensing elders can light your path as you embark on your journey of discovery and exploration through scientific research.
Code to provide approximate magnification probability distributions under microlensing by compact objects such as stars or PBHs of strongly lensed stars.
GPU code for quasar and supernovae microlensing simulations
Simone La Porta's Master thesis in gravitational lensing with applications of automatic differentiation @ Alma Mater Studiorum - Università di Bologna
Code for "Predicting High Magnification Events in Microlensed Quasars in the Era of LSST using Recurrent Neural Networks"
Implementation of the Witt (1993) method to compute gravitational microlensing light curves for an ensemble of point masses with shear
A fortran program based on FEM, it recovers LD profile of distant stars from gravitational microlensing light curves
Open source implementation of the analytical method by Witt (1990,1991) in gravitational microlensing to find the locations of critical curves and caustics for an abritrary number of stars.
python implementation to compute images of gravitational microlensed circular sources and light curves for an ensemble of point masses with shear.
Anomaly detection for Microlensing Single lens fitters.
Gravitational microlensing
code to calculate the critical curves and caustics of micro-lensing star fields
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