An exoplanet eclipse depth tool
Project description
Erebus is a rocky-exoplanet secondary eclipse aperture-photometry lightcurve fitting pipeline made for use with the Mid Infra-Red Instrument aboard the James Webb Space Telescope, starting with calints.fits files available on the Barbara A. Mikulski Archive for Space Telescopes.
For issue reporting or feedback suggestions click here.
For the setup used when writing Connors et al. (in prep) click here.
If you use Erebus in a scientific publication we will ask you cite our paper (information will be included here once it has been published).
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The following attestation bundles were made for erebus_exoplanet-0.7.1.tar.gz:
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publish_to_pypi.yaml on nicholasconnors/erebus
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