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[ascl:2002.008] ExoSim: Simulator for predicting signal and noise in transit spectroscopy observations

ExoSim models host star and planet transit events, simulating the temporal change in stellar flux due to the light curve. It is wavelength-dependent, using an input planet spectrum to determine the light curve depth for any given wavelength and can capture temporal effects, such as correlated noise. ExoSim's star spot simulator produces simulated observations that include spot and facula contamination. The code is flexible and can be generically applied to different instruments that simulate specific time-dependent processes.

Code site:
https://github.com/ExoSim/ExoSimPublic
Used in:
https://ui.adsabs.harvard.edu/abs/2018ExA....46...67Z
Described in:
https://ui.adsabs.harvard.edu/abs/2020arXiv200203739S
Bibcode:
2020ascl.soft02008S

Views: 128

ascl:2002.008
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