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PopSyCLE stands for Population Synthesis for Compact-object Lensing Events. This is a python add-on to the Galaxia modeling code that will make a fake Milky Way populated with stars, white dwarfs, neutron stars, and black holes. The synthetic population can be “observed” for microlensing events.
Running
galaxia-v3andrun.pyonPopSyCLE
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NIRC2/OSIRIS Imager Pipeline (request access) is a python-based (with IRAF dependencies) data reduction pipeline for the NIRC2 and OSIRIS adaptive optics imagers at the W. M. Keck Observatory. This pipeline was built to construct images of star fields to be used for high-precision photometry and astrometry. It does typical image reduction tasks as well as correcting for differential atmospheric refraction, instrumental distortions, and unique instrumental aspects of each instrument (e.g. noisy columns in NIRC2). When combined with StarFinder or AIROPA, this pipeline will also extract positions and fluxes from the images. The code is currently not public (but may be used upon request) as it has dependencies on a number of other non-public codes.
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