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The astrophysical models that we mentioned during our meeting today that we'd like to at least investigate adding to Eureka are:
catwoman (for asymmetric transits)
spiderman (for phase curves and eclipse mapping); may not be worthwhile given how extremely time-consuming it is. If we do add it, we should sparsely compute it and interpolate in time
starry (for transits, eclipse mapping, and phase curves. This depends on pymc3; I have already started adding starry while working on Issue Add PyMC3 as a S5 sampling method #265)
eigencurves/eigenmapping (Megan's code for eclipse mapping)
Code of Conduct
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The text was updated successfully, but these errors were encountered:
FYI, I now have well functioning and modular code for starry+pymc3 that just needs tests and documentation. I'll try to have a PR submitted for that before the end of the month in prep for the MIRI ERS observations
Instrument
Light curve fitting (Stages 4-6)
What is your suggestion?
The astrophysical models that we mentioned during our meeting today that we'd like to at least investigate adding to Eureka are:
Code of Conduct
The text was updated successfully, but these errors were encountered: