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

被引：64

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：

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES | 2019年 / 241卷 / 01期

基金：

英国科学技术设施理事会; 新加坡国家研究基金会;

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.

引用

页数：10

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