Photometry of 10 Million Stars from the First Two Years of TESS Full Frame Images: Part I
Chelsea X. HuangKavli Institute for Astrophysics and Space Research, MIT, USA; [email protected]Andrew VanderburgDepartment of Astronomy, University of Wisconsin-Madison, USAAndrás PálKavli Institute for Astrophysics and Space Research, MIT, USA; [email protected]Lizhou ShaDepartment of Astronomy, University of Wisconsin-Madison, USALiang YuKavli Institute for Astrophysics and Space Research, MIT, USA; [email protected]W. FongKavli Institute for Astrophysics and Space Research, MIT, USA; [email protected]Michael FausnaughKavli Institute for Astrophysics and Space Research, MIT, USA; [email protected]Avi ShporerKavli Institute for Astrophysics and Space Research, MIT, USA; [email protected]Natalia GuerreroKavli Institute for Astrophysics and Space Research, MIT, USA; [email protected]R. VanderspekKavli Institute for Astrophysics and Space Research, MIT, USA; [email protected]G. RickerKavli Institute for Astrophysics and Space Research, MIT, USA; [email protected]
2020en
ABI
Аннотация
Abstract The Transiting Exoplanet Survey Satellite (TESS) is the first high-precision full-sky photometric survey in space. We extracted light curves from a magnitude limited set of stars and other stationary luminous objects from the TESS Full Frame Images using the MIT Quick Look Pipeline. Here, we describe the techniques used to create light curves.
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