Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Cynthia S K Ho"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 520:4103-4117
We investigate the effect of observing cadence on the precision of radius ratio values obtained from transit light curves by performing uniform Markov Chain Monte Carlo fits of 46 exoplanets observed by the Transiting Exoplanet Survey Satellite (TESS
Autor:
Cynthia S. K. Ho, Vincent Van Eylen
The characteristics of the radius valley, i.e., an observed lack of planets between 1.5-2 Earth radii at periods shorter than about 100 days, provide insights into the formation and evolution of close-in planets. We present a novel view of the radius
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1f67c5ea3b33c87bab593f5bd2701d8c
Autor:
Daniel Huber, Timothy R. White, Travis S. Metcalfe, Ashley Chontos, Michael M. Fausnaugh, Cynthia S. K. Ho, Vincent Van Eylen, Warrick H. Ball, Sarbani Basu, Timothy R. Bedding, Othman Benomar, Diego Bossini, Sylvain Breton, Derek L. Buzasi, Tiago L. Campante, William J. Chaplin, Jørgen Christensen-Dalsgaard, Margarida S. Cunha, Morgan Deal, Rafael A. García, Antonio García Muñoz, Charlotte Gehan, Lucía González-Cuesta, Chen Jiang, Cenk Kayhan, Hans Kjeldsen, Mia S. Lundkvist, Stéphane Mathis, Savita Mathur, Mário J. P. F. G. Monteiro, Benard Nsamba, Jia Mian Joel Ong, Erika Pakštienė, Aldo M. Serenelli, Victor Silva Aguirre, Keivan G. Stassun, Dennis Stello, Sissel Norgaard Stilling, Mark Lykke Winther, Tao Wu, Thomas Barclay, Tansu Daylan, Maximilian N. Günther, J. J. Hermes, Jon M. Jenkins, David W. Latham, Alan M. Levine, George R. Ricker, Sara Seager, Avi Shporer, Joseph D. Twicken, Roland K. Vanderspek, Joshua N. Winn
Publikováno v:
Huber, D, White, T R, Metcalfe, T S, Chontos, A, Fausnaugh, M M, Ho, C S K, Van Eylen, V, Ball, W H, Basu, S, Bedding, T R, Benomar, O, Bossini, D, Breton, S, Buzasi, D L, Campante, T L, Chaplin, W J, Christensen-Dalsgaard, J, Cunha, M S, Deal, M, Garciá, R A, Garciá Munoz, A, Gehan, C, González-Cuesta, L, Jiang, C, Kayhan, C, Kjeldsen, H, Lundkvist, M S, Mathis, S, Mathur, S, Monteiro, M J P F G, Nsamba, B, Ong, J M J, Pakštiene, E, Serenelli, A M, Silva Aguirre, V, Stassun, K G, Stello, D, Norgaard Stilling, S, Lykke Winther, M, Wu, T, Barclay, T, Daylan, T, Günther, M N, Hermes, J J, Jenkins, J M, Latham, D W, Levine, A M, Ricker, G R, Seager, S, Shporer, A, Twicken, J D, Vanderspek, R K & Winn, J N 2022, ' A 20 Second Cadence View of Solar-type Stars and Their Planets with TESS : Asteroseismology of Solar Analogs and a Recharacterization of p Men c ', Astronomical Journal, vol. 163, no. 2, 79 . https://doi.org/10.3847/1538-3881/ac3000
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomical journal, Bristol : IOP publishing Ltd, 2022, vol. 163, iss. 2, art. no. 79, p. [1-17]
The Astronomical Journal
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomical journal, Bristol : IOP publishing Ltd, 2022, vol. 163, iss. 2, art. no. 79, p. [1-17]
The Astronomical Journal
We present an analysis of the first 20 second cadence light curves obtained by the TESS space telescope during its extended mission. We find improved precision of 20 second data compared to 2 minute data for bright stars when binned to the same caden
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6529dbc7a86d6cf4620e431b2c68fd0c
http://hdl.handle.net/10261/279517
http://hdl.handle.net/10261/279517