MultiRack is a software host that gives FOH and Monitor engineers the power to run the same Waves plug-ins used in recording studios and mixing rooms the world over. PSPL: point-source, point-lens with parallaxįSPL: finite-source, point-lens (currently testing further)Īll models support fitting data with single or multi-band photometry only, astrometry only, or joint fitting of photometry and astrometry (recommended).Waves presents MultiRack, a plug-in platform designed especially for Live Sound. It is currently under development and alpha-testing.ĪIROPA is a source extraction package to handle Anisoplanatic and Instrumental Reconstruction of Off-Axis PSFs for AO.īAGLE - Bayesian Analysis of Gravitational Lensing EventsīAGLE allows modeling of gravitational microlensing events both photometrically and astrometrically.
The code is currently still in alpha-testing.įlyStar is a tool for cross-matching and transforming starlists for high-precision astrometry projects. When combined with StarFinder or AIROPA, this pipeline will also extract positions and fluxes from the images. 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.
This pipeline was built to construct images of star fields to be used for high-precision photometry and astrometry. The KAI (Keck AO Imager) Imager Pipeline is a python-based (with IRAF dependencies) data reduction pipeline for the NIRC2 and OSIRIS adaptive optics imagers at the W. NIRC2 and OSIRIS Image Reduction Pipeline The synthetic population can be “observed” for microlensing events. PopS圜LE 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. PopS圜LE - Population Synthesis for Compact-object Lensing Events
Make a spectrum of a star cluster in integrated light Make a star cluster at any age with an unusual IMF and multiplicity Make a cluster isochrone in many filters using different stellar models
Here is a brief list of things that SPISEA can do: Stellar multiplicity and Initial Mass Function Total extinction, differential extinction, and extinction law It gives the user control over many parameters:Ĭluster characteristics (age, metallicity, mass, distance) SPISEA ( docs) is an python package that generates single-age, single-metallicity populations (i.e. SPISEA - Stellar Population Interface for Stellar Evolution and Atmospheres The MU Lab develops tools for studies of resolved stellar populations in the Milky Way, microlensing, orbits, and high-precision astrometry from space-based telescopes and with adaptive optics on ground-based telescopes.