Abstract: eleanor extracts target pixel files from TESS Full Frame Images and produces systematics-corrected light curves for any star observed by the TESS mission. eleanor takes a TIC ID, a Gaia source ID, or (RA, Dec) coordinates of a star observed by TESS and returns, as a single object, a light curve and accompanying target pixel data. The process can be customized, allowing, for example, examination of intermediate data products and changing the aperture used for light curve extraction. eleanor also offers tools that make it easier to work with stars observed in multiple TESS sectors.
Credit: Feinstein, Adina D.; Montet, Benjamin T.; Foreman-Mackey, Daniel; Bedell, Megan E.; Saunders, Nicholas; Bean, Jacob L.; Christiansen, Jessie L.; Hedges, Christina; Luger, Rodrigo; Scolnic, Daniel; Cardoso, Jose Vinicius de Miranda
Preferred citation method: https://ui.adsabs.harvard.edu/abs/2019arXiv190309152F; please see additional citation information here: http://adina.feinste.in/eleanor/getting ... d/faq.html