{"article_type":"original","year":"2020","publisher":"IOP Publishing","day":"01","date_published":"2020-02-01T00:00:00Z","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"main_file_link":[{"url":"https://arxiv.org/abs/1912.07604","open_access":"1"}],"scopus_import":"1","quality_controlled":"1","title":"Detection and characterization of oscillating red giants: First results from the TESS satellite","issue":"2","oa_version":"Preprint","intvolume":"       889","language":[{"iso":"eng"}],"status":"public","external_id":{"arxiv":["1912.07604"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa":1,"acknowledgement":"This Letter includes data collected by the TESS mission, which are publicly available from the Mikulski Archive for Space Telescopes (MAST). Funding for the TESS mission is provided by NASA's Science Mission directorate. Funding for the TESS Asteroseismic Science Operations Centre is provided by the Danish National Research Foundation (grant agreement No. DNRF106), ESA PRODEX (PEA 4000119301), and Stellar Astrophysics Centre (SAC) at Aarhus University. V.S.A. acknowledges support from the Independent Research Fund Denmark (Research grant 7027-00096B). D.B. is supported in the form of work contract FCT/MCTES through national funds and by FEDER through COMPETE2020 in connection to these grants: UID/FIS/04434/2019; PTDC/FIS-AST/30389/2017 & POCI-01-0145-FEDER-030389. L.B., R.A.G., and B.M. acknowledge the support from the CNES/PLATO grant. D.B. acknowledges NASA grant NNX16AB76G. T.L.C. acknowledges support from the European Union's Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No. 792848 (PULSATION). This work was supported by FCT/MCTES through national funds (UID/FIS/04434/2019). E.C. is funded by the European Union's Horizon 2020 research and innovation program under the Marie Skłodowska-Curie grant agreement No. 664931. R.H. and M.N.L. acknowledge the support of the ESA PRODEX programme. T.S.R. acknowledges financial support from Premiale 2015 MITiC (PI B. Garilli). K.J.B. is supported by the National Science Foundation under Award AST-1903828. M.S.L. is supported by the Carlsberg Foundation (grant agreement No. CF17-0760). M.C. is funded by FCT//MCTES through national funds and by FEDER through COMPETE2020 through these grants: UID/FIS/04434/2019, PTDC/FIS-AST/30389/2017 & POCI-01-0145-FEDER-030389, CEECIND/02619/2017. The research leading to the presented results has received funding from the European Research Council under the European Community's Seventh Framework Programme (FP7/2007-2013)/ERC grant agreement no 338251 (StellarAges). A.M. acknowledges support from the European Research Council Consolidator Grant funding scheme (project ASTEROCHRONOMETRY, grant agreement No. 772293, http://www.asterochronometry.eu). A.M.S. is partially supported by MINECO grant ESP2017-82674-R. J.C.S. acknowledges funding support from Spanish public funds for research under projects ESP2017-87676-2-2, and from project RYC-2012-09913 under the 'Ramón y Cajal' program of the Spanish Ministry of Science and Education. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center for the production of the SPOC data products.","article_processing_charge":"No","citation":{"apa":"Aguirre, V. S., Stello, D., Stokholm, A., Mosumgaard, J. R., Ball, W. H., Basu, S., … Vanderspek, R. (2020). Detection and characterization of oscillating red giants: First results from the TESS satellite. <i>The Astrophysical Journal Letters</i>. IOP Publishing. <a href=\"https://doi.org/10.3847/2041-8213/ab6443\">https://doi.org/10.3847/2041-8213/ab6443</a>","chicago":"Aguirre, Víctor Silva, Dennis Stello, Amalie Stokholm, Jakob R. Mosumgaard, Warrick H. Ball, Sarbani Basu, Diego Bossini, et al. “Detection and Characterization of Oscillating Red Giants: First Results from the TESS Satellite.” <i>The Astrophysical Journal Letters</i>. IOP Publishing, 2020. <a href=\"https://doi.org/10.3847/2041-8213/ab6443\">https://doi.org/10.3847/2041-8213/ab6443</a>.","ista":"Aguirre VS, Stello D, Stokholm A, Mosumgaard JR, Ball WH, Basu S, Bossini D, Bugnet LA, Buzasi D, Campante TL, Carboneau L, Chaplin WJ, Corsaro E, Davies GR, Elsworth Y, García RA, Gaulme P, Hall OJ, Handberg R, Hon M, Kallinger T, Kang L, Lund MN, Mathur S, Mints A, Mosser B, Çelik Orhan Z, Rodrigues TS, Vrard M, Yıldız M, Zinn JC, Örtel S, Beck PG, Bell KJ, Guo Z, Jiang C, Kuszlewicz JS, Kuehn CA, Li T, Lundkvist MS, Pinsonneault M, Tayar J, Cunha MS, Hekker S, Huber D, Miglio A, F. G. Monteiro MJP, Slumstrup D, Winther ML, Angelou G, Benomar O, Bódi A, De Moura BL, Deheuvels S, Derekas A, Di Mauro MP, Dupret M-A, Jiménez A, Lebreton Y, Matthews J, Nardetto N, do Nascimento JD, Pereira F, Rodríguez Díaz LF, Serenelli AM, Spitoni E, Stonkutė E, Suárez JC, Szabó R, Van Eylen V, Ventura R, Verma K, Weiss A, Wu T, Barclay T, Christensen-Dalsgaard J, Jenkins JM, Kjeldsen H, Ricker GR, Seager S, Vanderspek R. 2020. Detection and characterization of oscillating red giants: First results from the TESS satellite. The Astrophysical Journal Letters. 889(2), L34.","ieee":"V. S. Aguirre <i>et al.</i>, “Detection and characterization of oscillating red giants: First results from the TESS satellite,” <i>The Astrophysical Journal Letters</i>, vol. 889, no. 2. IOP Publishing, 2020.","mla":"Aguirre, Víctor Silva, et al. “Detection and Characterization of Oscillating Red Giants: First Results from the TESS Satellite.” <i>The Astrophysical Journal Letters</i>, vol. 889, no. 2, L34, IOP Publishing, 2020, doi:<a href=\"https://doi.org/10.3847/2041-8213/ab6443\">10.3847/2041-8213/ab6443</a>.","ama":"Aguirre VS, Stello D, Stokholm A, et al. Detection and characterization of oscillating red giants: First results from the TESS satellite. <i>The Astrophysical Journal Letters</i>. 2020;889(2). doi:<a href=\"https://doi.org/10.3847/2041-8213/ab6443\">10.3847/2041-8213/ab6443</a>","short":"V.S. Aguirre, D. Stello, A. Stokholm, J.R. Mosumgaard, W.H. Ball, S. Basu, D. Bossini, L.A. Bugnet, D. Buzasi, T.L. Campante, L. Carboneau, W.J. Chaplin, E. Corsaro, G.R. Davies, Y. Elsworth, R.A. García, P. Gaulme, O.J. Hall, R. Handberg, M. Hon, T. Kallinger, L. Kang, M.N. Lund, S. Mathur, A. Mints, B. Mosser, Z. Çelik Orhan, T.S. Rodrigues, M. Vrard, M. Yıldız, J.C. Zinn, S. Örtel, P.G. Beck, K.J. Bell, Z. Guo, C. Jiang, J.S. Kuszlewicz, C.A. Kuehn, T. Li, M.S. Lundkvist, M. Pinsonneault, J. Tayar, M.S. Cunha, S. Hekker, D. Huber, A. Miglio, M.J.P. F. G. Monteiro, D. Slumstrup, M.L. Winther, G. Angelou, O. Benomar, A. Bódi, B.L. De Moura, S. Deheuvels, A. Derekas, M.P. Di Mauro, M.-A. Dupret, A. Jiménez, Y. Lebreton, J. Matthews, N. Nardetto, J.D. do Nascimento, F. Pereira, L.F. Rodríguez Díaz, A.M. Serenelli, E. Spitoni, E. Stonkutė, J.C. Suárez, R. Szabó, V. Van Eylen, R. Ventura, K. Verma, A. Weiss, T. Wu, T. Barclay, J. Christensen-Dalsgaard, J.M. Jenkins, H. Kjeldsen, G.R. Ricker, S. Seager, R. Vanderspek, The Astrophysical Journal Letters 889 (2020)."},"month":"02","date_created":"2022-07-18T13:52:54Z","_id":"11612","doi":"10.3847/2041-8213/ab6443","author":[{"full_name":"Aguirre, Víctor Silva","first_name":"Víctor Silva","last_name":"Aguirre"},{"last_name":"Stello","full_name":"Stello, Dennis","first_name":"Dennis"},{"first_name":"Amalie","full_name":"Stokholm, Amalie","last_name":"Stokholm"},{"first_name":"Jakob R.","full_name":"Mosumgaard, Jakob R.","last_name":"Mosumgaard"},{"full_name":"Ball, Warrick H.","first_name":"Warrick H.","last_name":"Ball"},{"full_name":"Basu, Sarbani","first_name":"Sarbani","last_name":"Basu"},{"last_name":"Bossini","first_name":"Diego","full_name":"Bossini, Diego"},{"full_name":"Bugnet, Lisa Annabelle","first_name":"Lisa Annabelle","orcid":"0000-0003-0142-4000","last_name":"Bugnet","id":"d9edb345-f866-11ec-9b37-d119b5234501"},{"first_name":"Derek","full_name":"Buzasi, Derek","last_name":"Buzasi"},{"first_name":"Tiago L.","full_name":"Campante, Tiago L.","last_name":"Campante"},{"last_name":"Carboneau","full_name":"Carboneau, Lindsey","first_name":"Lindsey"},{"first_name":"William J.","full_name":"Chaplin, William J.","last_name":"Chaplin"},{"full_name":"Corsaro, Enrico","first_name":"Enrico","last_name":"Corsaro"},{"last_name":"Davies","full_name":"Davies, Guy R.","first_name":"Guy R."},{"first_name":"Yvonne","full_name":"Elsworth, Yvonne","last_name":"Elsworth"},{"full_name":"García, Rafael A.","first_name":"Rafael A.","last_name":"García"},{"last_name":"Gaulme","first_name":"Patrick","full_name":"Gaulme, Patrick"},{"last_name":"Hall","full_name":"Hall, Oliver J.","first_name":"Oliver J."},{"first_name":"Rasmus","full_name":"Handberg, Rasmus","last_name":"Handberg"},{"last_name":"Hon","full_name":"Hon, Marc","first_name":"Marc"},{"first_name":"Thomas","full_name":"Kallinger, Thomas","last_name":"Kallinger"},{"last_name":"Kang","full_name":"Kang, Liu","first_name":"Liu"},{"first_name":"Mikkel N.","full_name":"Lund, Mikkel N.","last_name":"Lund"},{"full_name":"Mathur, Savita","first_name":"Savita","last_name":"Mathur"},{"full_name":"Mints, Alexey","first_name":"Alexey","last_name":"Mints"},{"full_name":"Mosser, Benoit","first_name":"Benoit","last_name":"Mosser"},{"last_name":"Çelik Orhan","full_name":"Çelik Orhan, Zeynep","first_name":"Zeynep"},{"last_name":"Rodrigues","full_name":"Rodrigues, Thaíse S.","first_name":"Thaíse S."},{"full_name":"Vrard, Mathieu","first_name":"Mathieu","last_name":"Vrard"},{"last_name":"Yıldız","full_name":"Yıldız, Mutlu","first_name":"Mutlu"},{"last_name":"Zinn","full_name":"Zinn, Joel C.","first_name":"Joel C."},{"first_name":"Sibel","full_name":"Örtel, Sibel","last_name":"Örtel"},{"first_name":"Paul G.","full_name":"Beck, Paul G.","last_name":"Beck"},{"last_name":"Bell","full_name":"Bell, Keaton J.","first_name":"Keaton J."},{"first_name":"Zhao","full_name":"Guo, Zhao","last_name":"Guo"},{"last_name":"Jiang","first_name":"Chen","full_name":"Jiang, Chen"},{"full_name":"Kuszlewicz, James S.","first_name":"James S.","last_name":"Kuszlewicz"},{"last_name":"Kuehn","full_name":"Kuehn, Charles A.","first_name":"Charles A."},{"first_name":"Tanda","full_name":"Li, Tanda","last_name":"Li"},{"last_name":"Lundkvist","full_name":"Lundkvist, Mia S.","first_name":"Mia S."},{"last_name":"Pinsonneault","first_name":"Marc","full_name":"Pinsonneault, Marc"},{"last_name":"Tayar","first_name":"Jamie","full_name":"Tayar, Jamie"},{"first_name":"Margarida S.","full_name":"Cunha, Margarida S.","last_name":"Cunha"},{"full_name":"Hekker, Saskia","first_name":"Saskia","last_name":"Hekker"},{"last_name":"Huber","full_name":"Huber, Daniel","first_name":"Daniel"},{"last_name":"Miglio","first_name":"Andrea","full_name":"Miglio, Andrea"},{"first_name":"Mario J. P.","full_name":"F. G. Monteiro, Mario J. P.","last_name":"F. G. Monteiro"},{"first_name":"Ditte","full_name":"Slumstrup, Ditte","last_name":"Slumstrup"},{"last_name":"Winther","full_name":"Winther, Mark L.","first_name":"Mark L."},{"last_name":"Angelou","first_name":"George","full_name":"Angelou, George"},{"last_name":"Benomar","first_name":"Othman","full_name":"Benomar, Othman"},{"last_name":"Bódi","first_name":"Attila","full_name":"Bódi, Attila"},{"first_name":"Bruno L.","full_name":"De Moura, Bruno L.","last_name":"De Moura"},{"first_name":"Sébastien","full_name":"Deheuvels, Sébastien","last_name":"Deheuvels"},{"full_name":"Derekas, Aliz","first_name":"Aliz","last_name":"Derekas"},{"full_name":"Di Mauro, Maria Pia","first_name":"Maria Pia","last_name":"Di Mauro"},{"first_name":"Marc-Antoine","full_name":"Dupret, Marc-Antoine","last_name":"Dupret"},{"last_name":"Jiménez","first_name":"Antonio","full_name":"Jiménez, Antonio"},{"first_name":"Yveline","full_name":"Lebreton, Yveline","last_name":"Lebreton"},{"last_name":"Matthews","first_name":"Jaymie","full_name":"Matthews, Jaymie"},{"first_name":"Nicolas","full_name":"Nardetto, Nicolas","last_name":"Nardetto"},{"full_name":"do Nascimento, Jose D.","first_name":"Jose D.","last_name":"do Nascimento"},{"last_name":"Pereira","first_name":"Filipe","full_name":"Pereira, Filipe"},{"full_name":"Rodríguez Díaz, Luisa F.","first_name":"Luisa F.","last_name":"Rodríguez Díaz"},{"first_name":"Aldo M.","full_name":"Serenelli, Aldo M.","last_name":"Serenelli"},{"last_name":"Spitoni","full_name":"Spitoni, Emanuele","first_name":"Emanuele"},{"last_name":"Stonkutė","full_name":"Stonkutė, Edita","first_name":"Edita"},{"first_name":"Juan Carlos","full_name":"Suárez, Juan Carlos","last_name":"Suárez"},{"last_name":"Szabó","full_name":"Szabó, Robert","first_name":"Robert"},{"last_name":"Van Eylen","first_name":"Vincent","full_name":"Van Eylen, Vincent"},{"last_name":"Ventura","full_name":"Ventura, Rita","first_name":"Rita"},{"full_name":"Verma, Kuldeep","first_name":"Kuldeep","last_name":"Verma"},{"full_name":"Weiss, Achim","first_name":"Achim","last_name":"Weiss"},{"full_name":"Wu, Tao","first_name":"Tao","last_name":"Wu"},{"full_name":"Barclay, Thomas","first_name":"Thomas","last_name":"Barclay"},{"last_name":"Christensen-Dalsgaard","full_name":"Christensen-Dalsgaard, Jørgen","first_name":"Jørgen"},{"first_name":"Jon M.","full_name":"Jenkins, Jon M.","last_name":"Jenkins"},{"first_name":"Hans","full_name":"Kjeldsen, Hans","last_name":"Kjeldsen"},{"last_name":"Ricker","full_name":"Ricker, George R.","first_name":"George R."},{"full_name":"Seager, Sara","first_name":"Sara","last_name":"Seager"},{"first_name":"Roland","full_name":"Vanderspek, Roland","last_name":"Vanderspek"}],"publication_status":"published","publication":"The Astrophysical Journal Letters","abstract":[{"text":"Since the onset of the \"space revolution\" of high-precision high-cadence photometry, asteroseismology has been demonstrated as a powerful tool for informing Galactic archeology investigations. The launch of the NASA Transiting Exoplanet Survey Satellite (TESS) mission has enabled seismic-based inferences to go full sky—providing a clear advantage for large ensemble studies of the different Milky Way components. Here we demonstrate its potential for investigating the Galaxy by carrying out the first asteroseismic ensemble study of red giant stars observed by TESS. We use a sample of 25 stars for which we measure their global asteroseimic observables and estimate their fundamental stellar properties, such as radius, mass, and age. Significant improvements are seen in the uncertainties of our estimates when combining seismic observables from TESS with astrometric measurements from the Gaia mission compared to when the seismology and astrometry are applied separately. Specifically, when combined we show that stellar radii can be determined to a precision of a few percent, masses to 5%–10%, and ages to the 20% level. This is comparable to the precision typically obtained using end-of-mission Kepler data.","lang":"eng"}],"article_number":"L34","date_updated":"2022-08-22T07:25:51Z","volume":889,"extern":"1","type":"journal_article","publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]}}