The TESS Input Catalog and Candidate Target List

Astronomical Journal - Tập 156 Số 3 - Trang 102 - 2018
Keivan G. Stassun1,2,3, Ryan J. Oelkers2,3, Joshua Pepper4,2, Martin Paegert5,2, Nathan De Lee6,2, Guillermo Torres5, David W. Latham5, S. Charpinet7, Courtney D. Dressing8, Daniel Huber9, Stephen R. Kane10, Sébastien Lépine11, Andrew W. Mann12, Philip S. Muirhead13, Bárbara Rojas-Ayala14, R. Silvotti15, Scott W. Fleming16, A. M. Levine17, Peter Plavchan18
1Fisk University, USA
2Vanderbilt Initiative in Data-intensive Astrophysics (VIDA), 6301 Stevenson Center Lane, Nashville, TN 37235, USA
3Vanderbilt University, Department of Physics & Astronomy, 6301 Stevenson Center Ln., Nashville, TN 37235, USA
4Lehigh University, Department of Physics, 16 Memorial Drive East, Bethlehem, PA, 18015, USA
5Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
6Department of Physics, Geology, and Engineering Technology, Northern Kentucky University, Highland Heights, KY, 41099, USA
7Institut de Recherche en Astrophysique et Planétologie, CNRS, Université de Toulouse, 14 avenue Edouard Belin, F-31400 Toulouse, France
8Astronomy Department, University of California, Berkeley, CA 94720 USA
9Institute for Astronomy, University of Hawaiì, 2680 Woodlawn Drive, Honolulu, HI 96822, USA
10Department of Earth Sciences University of California Riverside, CA 92521 USA
11Department of Physics & Astronomy, Georgia State University, 25 Park Pl. NE, Atlanta, GA 30303, USA
12Department of Physics and Astronomy, University of North Carolina at Chapel Hill, Chapel Hill, NC 27599 USA
13Department of Astronomy & The Institute for Astrophysical Research, Boston University, 725 Commonwealth Ave., Boston, MA 02215, USA
14Departamento de Ciencias Fisicas, Universidad Andrés Bello, Fernandez Concha 700, Las Condes, Santiago, Chile
15INAF-Osservatorio Astrofisico di Torino, via Osservatorio 20, 10025 Pino Torinese, Italy
16Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
17Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, 77 Massachusetts Ave., 37-241, Cambridge, MA 02139, USA
18Department of Physics & Astronomy, George Mason University, 4400 University Drive MS 3F3, Fairfax,VA 22030, USA

Tóm tắt

Abstract The Transiting Exoplanet Survey Satellite (TESS) will be conducting a nearly all-sky photometric survey over two years, with a core mission goal to discover small transiting exoplanets orbiting nearby bright stars. It will obtain 30 minute cadence observations of all objects in the TESS fields of view, along with two-minute cadence observations of 200,000–400,000 selected stars. The choice of which stars to observe at the two-minute cadence is driven by the need to detect small transiting planets, which leads to the selection of primarily bright, cool dwarfs. We describe the catalogs assembled and the algorithms used to populate the TESS Input Catalog (TIC), including plans to update the TIC with the incorporation of the Gaia second data release in the near future. We also describe a ranking system for prioritizing stars according to the smallest transiting planet detectable, and assemble a Candidate Target List (CTL) using that ranking. We discuss additional factors that affect the ability to photometrically detect and dynamically confirm small planets, and we note additional stellar populations of interest that may be added to the final target list. The TIC is available on the STScI MAST server, and an enhanced CTL is available through the Filtergraph data visualization portal system at the URL http://filtergraph.com/tess_ctl.

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