The Asteroseismic Target List for Solar-like Oscillators Observed in 2 minute Cadence with the Transiting Exoplanet Survey Satellite

被引:63
|
作者
Schofield, Mathew [1 ,2 ]
Chaplin, William J. [1 ,2 ]
Huber, Daniel [3 ]
Campante, Tiago L. [1 ,4 ,5 ]
Davies, Guy R. [1 ,2 ]
Miglio, Andrea [1 ,2 ]
Ball, Warrick H. [1 ,2 ]
Appourchaux, Thierry [6 ]
Basu, Sarbani [7 ]
Bedding, Timothy R. [2 ,8 ]
Christensen-Dalsgaard, Jorgen [2 ]
Creevey, Orlagh [9 ]
Garcia, Rafael A. [10 ]
Handberg, Rasmus [2 ]
Kawaler, Steven D. [11 ]
Kjeldsen, Hans [2 ]
Latham, David W. [12 ]
Lund, Mikkel N. [2 ]
Metcalfe, Travis S. [13 ,14 ]
Ricker, George R. [15 ]
Serenelli, Aldo [16 ,17 ]
Aguirre, Victor Silva [2 ]
Stello, Dennis [2 ,8 ,18 ]
Vanderspek, Roland [15 ]
机构
[1] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
[2] Aarhus Univ, Stellar Astrophys Ctr, Dept Phys & Astron, Ny Munkegade 120, DK-8000 Aarhus C, Denmark
[3] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA
[4] Univ Porto, Inst Astrofis & Ciencias Espaco, Rua Estrelas, PT-4150762 Porto, Portugal
[5] Univ Porto, Dept Fis & Astron, Fac Ciencias, Rua Campo Alegre S-N, PT-4169007 Porto, Portugal
[6] Univ Paris Sud, CNRS, Inst Astrophys Spatiale, UMR 8617, Batiment 121, F-91405 Orsay, France
[7] Yale Univ, Dept Astron, POB 208101, New Haven, CT 06520 USA
[8] Univ Sydney, Sch Phys, SIfA, Sydney, NSW 2006, Australia
[9] Univ Coe Azur, Lab Lagrange, CNRS, Observ Cote Azur, Bd Observ,CS 34229, F-06304 Nice 4, France
[10] Univ Paris Diderot, Ctr Saclay, Lab AIM, CEA DSM CNRS,IRFU SAp, F-91191 Gif Sur Yvette, France
[11] Iowa State Univ, Dept Phys & Astron, Ames, IA 50011 USA
[12] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[13] Space Sci Inst, 4750 Walnut St,Suite 205, Boulder, CO 80301 USA
[14] Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany
[15] MIT, Kavli Inst Astrophys & Space Res, 70 Vassar St, Cambridge, MA 02139 USA
[16] CSIC, Inst Space Sci ICE, Campus UAB,Carrer Can Magrans S-N, E-08193 Barcelona, Spain
[17] IEEC, C Gran Capita 2-4, E-08034 Barcelona, Spain
[18] UNSW, Sch Phys, Sydney, NSW 2052, Australia
来源
基金
新加坡国家研究基金会; 英国科学技术设施理事会;
关键词
catalogs; space vehicles: instruments; stars: fundamental parameters; stars: oscillations; surveys; STARS; DIAMETERS;
D O I
10.3847/1538-4365/ab04f5
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the target list of solar-type stars to be observed in short-cadence (2 minute) for asteroseismology by the NASA Transiting Exoplanet Survey Satellite (TESS) during its 2 year nominal survey mission. The solar-like Asteroseismic Target List (ATL) is comprised of bright, cool main-sequence and subgiant stars and forms part of the larger target list of the TESS Asteroseismic Science Consortium. The ATL uses the Gaia Data Release 2 and the Extended Hipparcos Compilation (XHIP) to derive fundamental stellar properties, to calculate detection probabilities, and to produce a rank-ordered target list. We provide a detailed description of how the ATL was produced and calculate expected yields for solar-like oscillators based on the nominal photometric performance by TESS. We also provide a publicly available source code that can be used to reproduce the ATL, thereby enabling comparisons of asteroseismic results from TESS with predictions from synthetic stellar populations.
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页数:10
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