The TESS-HERMES survey data release 1: High-resolution spectroscopy of the TESS southern continuous viewing zone

被引：0

作者：

Sharma S. ^{[1
]}

Stello D. ^{[1
,2
,3
]}

Buder S. ^{[4
,5
]}

Kos J. ^{[1
]}

Bland-Hawthorn J. ^{[1
]}

Asplund M. ^{[6
]}

Duong L. ^{[6
]}

Lin J. ^{[6
]}

Lind K. ^{[4
,7
]}

Ness M. ^{[4
]}

Huber D. ^{[8
,9
,10
,11
]}

Zwitter T. ^{[12
]}

Traven G. ^{[12
]}

Hon M. ^{[2
]}

Kafle P.R. ^{[13
]}

Khanna S. ^{[1
]}

Saddon H. ^{[2
]}

Anguiano B. ^{[14
,15
]}

Casey A.R. ^{[16
,17
]}

Freeman K. ^{[6
]}

Martell S. ^{[2
]}

De Silva G.M. ^{[1
,18
]}

Simpson J.D. ^{[19
]}

Wittenmyer R.A. ^{[19
]}

Zucker D.B. ^{[15
,18
,20
]}

机构：

[1] Sydney Institute for Astronomy, School of Physics, University of Sydney, 2006, NSW

[2] School of Physics, University of New South Wales, Sydney, 2052, NSW

[3] Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Aarhus C

[4] Max Planck Institute for Astronomy (MPIA), Koenigstuhl 17, Heidelberg

[5] Fellow of the International Max Planck Research School for Astronomy and Cosmic Physics, University of Heidelberg

[6] Research School of Astronomy and Astrophysics, Australian National University, 2611, ACT

[7] Department of Physics and Astronomy, Uppsala University, Box 516, Uppsala

[8] Institute for Astronomy, University of Hawai'i, 2680 Woodlawn Drive, Honolulu, 96822, HI

[9] Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney, 2006, NSW

[10] SETI Institute, 189 Bernardo Avenue, Mountain View, 94043, CA

[11] Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, Aarhus C

[12] Faculty of Mathematics and Physics, University of Ljubljana, Jadranska 19, Ljubljana

[13] International Centre for Radio Astronomy Research (ICRAR), TheUniversity ofWestern Australia, 35 Stirling Highway, Crawley, 6009, WA

[14] Department of Astronomy, University of Virginia, Charlottesville, 22904-4325, VA

[15] Department of Physics and Astronomy, Macquarie University, Sydney, 2109, NSW

[16] School of Physics and Astronomy, Monash University, Clayton, 3800, VIC

[17] Faculty of Information Technology, Monash University, Clayton, 3800, VIC

[18] Australian Astronomical Observatory, 105 Delhi Rd, North Ryde, 2113, NSW

[19] University of Southern Queensland, Computational Engineering and Science Research Centre, Toowoomba, 4350, QLD

[20] Research Centre in Astronomy, Astrophysics and Astrophotonics, Macquarie University, Sydney, 2109, NSW

来源：

| 2004年 / Oxford University Press卷 / 473期

基金：

澳大利亚研究理事会; 美国国家航空航天局;

关键词：

Catalogues; Galaxy: stellar content; Planetary systems; Stars: fundamental parameters; Surveys; Techniques: spectroscopic;

D O I：

10.1093/MNRAS/STX2582

中图分类号：

学科分类号：

摘要：

The Transiting Exoplanet Survey Satellite (TESS) will provide high-precision time series photometry for millions of stars with at least a half-hour cadence. Of particular interest are the circular regions of 12° radius centred around the ecliptic poles that will be observed continuously for a full year. Spectroscopic stellar parameters are desirable to characterize and select suitable targets for TESS, whether they are focused on exploring exoplanets, stellar astrophysics or Galactic archaeology. Here, we present spectroscopic stellar parameters (Teff, log g, [Fe/H], v sin i, vmicro) for about 16 000 dwarf and subgiant stars in TESS' southern continuous viewing zone. For almost all the stars, we also present Bayesian estimates of stellar properties including distance, extinction, mass, radius and age using theoretical isochrones. Stellar surface gravity and radius are made available for an additional set of roughly 8500 red giants. All our target stars are in the range 10 < V < 13.1. Among them, we identify and list 227 stars belonging to the Large Magellanic Cloud. The data were taken using the High Efficiency and Resolution Multi-Element Spectrograph (HERMES; R ~ 28 000) at the Anglo-Australian Telescope as part of the TESS-HERMES survey. Comparing our results with the TESS Input Catalogue (TIC) shows that the TIC is generally efficient in separating dwarfs and giants, but it has flagged more than 100 cool dwarfs (Teff < 4800 K) as giants, which ought to be high-priority targets for the exoplanet search. The catalogue can be accessed via http://www.physics.usyd.edu.au/tess-hermes/, or atMikulski Archive for Space Telescopes (MAST). © 2018 The Author(s).

引用

页码：2004 / 2019

页数：15

共 30 条

[1] The TESS-HERMES survey data release 1: high-resolution spectroscopy of the TESS southern continuous viewing zone
Sharma, Sanjib
Stello, Dennis
Buder, Sven
Kos, Janez
Bland-Hawthorn, Joss
Asplund, Martin
Duong, Ly
Lin, Jane
Lind, Karin
Ness, Melissa
Huber, Daniel
Zwitter, Tomaz
Traven, Gregor
Hon, Marc
Kafle, Prajwal R.
Khanna, Shourya
Saddon, Hafiz
Anguiano, Borja
Casey, Andrew R.
Freeman, Ken
Martell, Sarah
De Silva, Gayandhi M.
Simpson, Jeffrey D.
Wittenmyer, Rob A.
Zucker, Daniel B.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2018, 473 (02) : 2004 - 2019
[2] TESS Stellar Rotation up to 80 Days in the Southern Continuous Viewing Zone
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Beaton, Rachael L.
ASTROPHYSICAL JOURNAL, 2024, 962 (01):
[3] Activity and Rotation of Nearby Field M Dwarfs in the TESS Southern Continuous Viewing Zone
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Curtis, Jason L.
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ASTRONOMICAL JOURNAL, 2022, 163 (06):
[4] Periodic variable A-F spectral type stars in the southern TESS continuous viewing zone
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ASTRONOMY & ASTROPHYSICS, 2024, 688
[5] Variability of OB stars from TESS southern Sectors 1-13 and high-resolution IACOB and OWN spectroscopy
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[6] The ASAS-SN catalogue of variable stars III: variables in the southern TESS continuous viewing zone
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Pawlak, M.
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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2019, 485 (01) : 961 - 971
[7] Detection of period-spacing patterns due to the gravity modes of rotating dwarfs in the TESS southern continuous viewing zone
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ASTRONOMY & ASTROPHYSICS, 2022, 662
[8] Analysis of high-resolution FEROS spectroscopy for a sample of variable B-type stars assembled from TESS photometry
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ASTRONOMY & ASTROPHYSICS, 2022, 665
[9] The ESO UVES/FEROS Large Programs of TESS OB pulsators I. Global stellar parameters from high-resolution spectroscopy
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Tkachenko, Andrew
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ASTRONOMY & ASTROPHYSICS, 2023, 676
[10] Solar System Objects Observed with TESS-First Data Release: Bright Main-belt and Trojan Asteroids from the Southern Survey
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Kiss, Csaba
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Kiss, Laszlo L.
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