Статья

Photometry of 10 Million Stars from the First Two Years of TESS Full Frame Images: Part II

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 We present light curves from a magnitude limited set of stars and other stationary luminous objects from the TESS Full Frame Images, as reduced by the MIT Quick Look Pipeline (QLP). Our light curves cover the full two-year TESS Primary Mission and include ∼14,770,000 and ∼9,600,000 individual light curve segments in the Southern and Northern ecliptic hemispheres, respectively. We describe the detrending techniques we used to create the light curves, and compare the noise properties with theoretical expectations. All of the QLP light curves are available at MAST as a High Level Science Product (HLSP) via doi: 10.17909/t9-r086-e880 ( https://archive.stsci.edu/hlsp/qlp ). This is the largest collection of TESS photometry available to the public to date.

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Идентификаторы

DOI: 10.3847/2515-5172/abca2d

Цитирования и источники

Цитирований: 3Использованных источников: 0

Показатели — AkademScholar