Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/30434
Campo DC | Valore | Lingua |
---|---|---|
dc.contributor.author | Huber, Daniel | en_US |
dc.contributor.author | Chaplin, William J. | en_US |
dc.contributor.author | Chontos, Ashley | en_US |
dc.contributor.author | Kjeldsen, Hans | en_US |
dc.contributor.author | Christensen-Dalsgaard, Jørgen | en_US |
dc.contributor.author | Bedding, Timothy R. | en_US |
dc.contributor.author | Ball, Warrick | en_US |
dc.contributor.author | Brahm, Rafael | en_US |
dc.contributor.author | Espinoza, Nestor | en_US |
dc.contributor.author | Henning, Thomas | en_US |
dc.contributor.author | Jordán, Andrés | en_US |
dc.contributor.author | Sarkis, Paula | en_US |
dc.contributor.author | Knudstrup, Emil | en_US |
dc.contributor.author | Albrecht, Simon | en_US |
dc.contributor.author | Grundahl, Frank | en_US |
dc.contributor.author | Fredslund Andersen, Mads | en_US |
dc.contributor.author | Pallé, Pere L. | en_US |
dc.contributor.author | Crossfield, Ian | en_US |
dc.contributor.author | Fulton, Benjamin | en_US |
dc.contributor.author | Howard, Andrew W. | en_US |
dc.contributor.author | Isaacson, Howard T. | en_US |
dc.contributor.author | Weiss, Lauren M. | en_US |
dc.contributor.author | Handberg, Rasmus | en_US |
dc.contributor.author | Lund, Mikkel N. | en_US |
dc.contributor.author | Serenelli, Aldo M. | en_US |
dc.contributor.author | Rørsted Mosumgaard, Jakob | en_US |
dc.contributor.author | Stokholm, Amalie | en_US |
dc.contributor.author | Bieryla, Allyson | en_US |
dc.contributor.author | Buchhave, Lars A. | en_US |
dc.contributor.author | Latham, David W. | en_US |
dc.contributor.author | Quinn, Samuel N. | en_US |
dc.contributor.author | Gaidos, Eric | en_US |
dc.contributor.author | Hirano, Teruyuki | en_US |
dc.contributor.author | Ricker, George R. | en_US |
dc.contributor.author | Vanderspek, Roland K. | en_US |
dc.contributor.author | Seager, Sara | en_US |
dc.contributor.author | Jenkins, Jon M. | en_US |
dc.contributor.author | Winn, Joshua N. | en_US |
dc.contributor.author | Antia, H. M. | en_US |
dc.contributor.author | Appourchaux, Thierry | en_US |
dc.contributor.author | Basu, Sarbani | en_US |
dc.contributor.author | Bell, Keaton J. | en_US |
dc.contributor.author | Benomar, Othman | en_US |
dc.contributor.author | BONANNO, Alfio Maurizio | en_US |
dc.contributor.author | Buzasi, Derek L. | en_US |
dc.contributor.author | Campante, Tiago L. | en_US |
dc.contributor.author | Çelik Orhan, Z. | en_US |
dc.contributor.author | CORSARO, ENRICO MARIA NICOLA | en_US |
dc.contributor.author | Cunha, Margarida S. | en_US |
dc.contributor.author | Davies, Guy R. | en_US |
dc.contributor.author | Deheuvels, Sebastien | en_US |
dc.contributor.author | Grunblatt, Samuel K. | en_US |
dc.contributor.author | Hasanzadeh, Amir | en_US |
dc.contributor.author | DI MAURO, Maria Giuseppina | en_US |
dc.contributor.author | García, Rafael A. | en_US |
dc.contributor.author | Gaulme, Patrick | en_US |
dc.contributor.author | GIRARDI, Leo Alberto | en_US |
dc.contributor.author | Guzik, Joyce A. | en_US |
dc.contributor.author | Hon, Marc | en_US |
dc.contributor.author | Jiang, Chen | en_US |
dc.contributor.author | Kallinger, Thomas | en_US |
dc.contributor.author | Kawaler, Steven D. | en_US |
dc.contributor.author | Kuszlewicz, James S. | en_US |
dc.contributor.author | Lebreton, Yveline | en_US |
dc.contributor.author | Li, Tanda | en_US |
dc.contributor.author | Lucas, Miles | en_US |
dc.contributor.author | Lundkvist, Mia S. | en_US |
dc.contributor.author | Mann, Andrew W. | en_US |
dc.contributor.author | Mathis, Stéphane | en_US |
dc.contributor.author | Mathur, Savita | en_US |
dc.contributor.author | Mazumdar, Anwesh | en_US |
dc.contributor.author | Metcalfe, Travis S. | en_US |
dc.contributor.author | MIGLIO, ANDREA | en_US |
dc.contributor.author | Monteiro, Mário J. P. F. G. | en_US |
dc.contributor.author | Mosser, Benoit | en_US |
dc.contributor.author | Noll, Anthony | en_US |
dc.contributor.author | Nsamba, Benard | en_US |
dc.contributor.author | Ong, Jia Mian Joel | en_US |
dc.contributor.author | Örtel, S. | en_US |
dc.contributor.author | Pereira, Filipe | en_US |
dc.contributor.author | Ranadive, Pritesh | en_US |
dc.contributor.author | Régulo, Clara | en_US |
dc.contributor.author | Da Silva Rodrigues, Thaise | en_US |
dc.contributor.author | Roxburgh, Ian W. | en_US |
dc.contributor.author | Silva Aguirre, Victor | en_US |
dc.contributor.author | Smalley, Barry | en_US |
dc.contributor.author | Schofield, Mathew | en_US |
dc.contributor.author | Sousa, Sérgio G. | en_US |
dc.contributor.author | Stassun, Keivan G. | en_US |
dc.contributor.author | Stello, Dennis | en_US |
dc.contributor.author | Tayar, Jamie | en_US |
dc.contributor.author | White, Timothy R. | en_US |
dc.contributor.author | Verma, Kuldeep | en_US |
dc.contributor.author | Vrard, Mathieu | en_US |
dc.contributor.author | Yıldız, M. | en_US |
dc.contributor.author | Baker, David | en_US |
dc.contributor.author | Bazot, Michaël | en_US |
dc.contributor.author | Beichmann, Charles | en_US |
dc.contributor.author | Bergmann, Christoph | en_US |
dc.contributor.author | Bugnet, Lisa | en_US |
dc.contributor.author | Cale, Bryson | en_US |
dc.contributor.author | Carlino, Roberto | en_US |
dc.contributor.author | Cartwright, Scott M. | en_US |
dc.contributor.author | Christiansen, Jessie L. | en_US |
dc.contributor.author | Ciardi, David R. | en_US |
dc.contributor.author | Creevey, Orlagh | en_US |
dc.contributor.author | Dittmann, Jason A. | en_US |
dc.contributor.author | Do Nascimento, Jose-Dias, Jr. | en_US |
dc.contributor.author | Van Eylen, Vincent | en_US |
dc.contributor.author | Fürész, Gabor | en_US |
dc.contributor.author | Gagné, Jonathan | en_US |
dc.contributor.author | Gao, Peter | en_US |
dc.contributor.author | Gazeas, Kosmas | en_US |
dc.contributor.author | Giddens, Frank | en_US |
dc.contributor.author | Hall, Oliver J. | en_US |
dc.contributor.author | Hekker, Saskia | en_US |
dc.contributor.author | Ireland, Michael J. | en_US |
dc.contributor.author | Latouf, Natasha | en_US |
dc.contributor.author | LeBrun, Danny | en_US |
dc.contributor.author | Levine, Alan M. | en_US |
dc.contributor.author | Matzko, William | en_US |
dc.contributor.author | Natinsky, Eva | en_US |
dc.contributor.author | Page, Emma | en_US |
dc.contributor.author | Plavchan, Peter | en_US |
dc.contributor.author | Mansouri-Samani, Masoud | en_US |
dc.contributor.author | McCauliff, Sean | en_US |
dc.contributor.author | Mullally, Susan E. | en_US |
dc.contributor.author | Orenstein, Brendan | en_US |
dc.contributor.author | Garcia Soto, Aylin | en_US |
dc.contributor.author | Paegert, Martin | en_US |
dc.contributor.author | van Saders, Jennifer L. | en_US |
dc.contributor.author | Schnaible, Chloe | en_US |
dc.contributor.author | Soderblom, David R. | en_US |
dc.contributor.author | Szabó, Róbert | en_US |
dc.contributor.author | Tanner, Angelle | en_US |
dc.contributor.author | Tinney, C. G. | en_US |
dc.contributor.author | Teske, Johanna | en_US |
dc.contributor.author | Thomas, Alexandra | en_US |
dc.contributor.author | Trampedach, Regner | en_US |
dc.contributor.author | Wright, Duncan | en_US |
dc.contributor.author | Yuan, Thomas T. | en_US |
dc.contributor.author | Zohrabi, Farzaneh | en_US |
dc.date.accessioned | 2021-02-17T15:01:24Z | - |
dc.date.available | 2021-02-17T15:01:24Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 0004-6256 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30434 | - |
dc.description.abstract | We present the discovery of HD 221416 b, the first transiting planet identified by the Transiting Exoplanet Survey Satellite (TESS) for which asteroseismology of the host star is possible. HD 221416 b (HIP 116158, TOI-197) is a bright (V = 8.2 mag), spectroscopically classified subgiant that oscillates with an average frequency of about 430 μHz and displays a clear signature of mixed modes. The oscillation amplitude confirms that the redder TESS bandpass compared to Kepler has a small effect on the oscillations, supporting the expected yield of thousands of solar-like oscillators with TESS 2 minute cadence observations. Asteroseismic modeling yields a robust determination of the host star radius (R <SUB>⋆</SUB> = 2.943 ± 0.064 R <SUB>☉</SUB>), mass (M <SUB>⋆</SUB> = 1.212 ± 0.074 M <SUB>☉</SUB>), and age (4.9 ± 1.1 Gyr), and demonstrates that it has just started ascending the red-giant branch. Combining asteroseismology with transit modeling and radial-velocity observations, we show that the planet is a “hot Saturn” (R <SUB>p</SUB> = 9.17 ± 0.33 R <SUB>⊕</SUB>) with an orbital period of ∼14.3 days, irradiance of F = 343 ± 24 F <SUB>⊕</SUB>, and moderate mass (M <SUB>p</SUB> = 60.5 ± 5.7 M <SUB>⊕</SUB>) and density (ρ <SUB>p</SUB> = 0.431 ± 0.062 g cm<SUP>-3</SUP>). The properties of HD 221416 b show that the host-star metallicity-planet mass correlation found in sub-Saturns (4-8 R <SUB>⊕</SUB>) does not extend to larger radii, indicating that planets in the transition between sub-Saturns and Jupiters follow a relatively narrow range of densities. With a density measured to ∼15%, HD 221416 b is one of the best characterized Saturn-size planets to date, augmenting the small number of known transiting planets around evolved stars and demonstrating the power of TESS to characterize exoplanets and their host stars using asteroseismology. | en_US |
dc.language.iso | eng | en_US |
dc.title | A Hot Saturn Orbiting an Oscillating Late Subgiant Discovered by TESS | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-3881/ab1488 | en_US |
dc.identifier.scopus | 2-s2.0-85072292342 | en_US |
dc.identifier.isi | 000469975500005 | en_US |
dc.identifier.url | https://iopscience.iop.org/article/10.3847/1538-3881/ab1488 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 157 | en_US |
dc.relation.issue | 6 | en_US |
dc.relation.firstpage | 245 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | THE ASTRONOMICAL JOURNAL | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2019AJ....157..245H | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.grantfulltext | open | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 0004-6256 | - |
crisitem.journal.ance | E016224 | - |
crisitem.author.dept | O.A. Catania | - |
crisitem.author.dept | O.A. Catania | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.orcid | 0000-0003-3175-9776 | - |
crisitem.author.orcid | 0000-0001-8835-2075 | - |
crisitem.author.orcid | 0000-0001-7801-7484 | - |
crisitem.author.orcid | 0000-0002-6301-3269 | - |
crisitem.author.orcid | 0000-0002-9414-339X | - |
È visualizzato nelle collezioni: | 1.01 Articoli in rivista |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
huber.pdf | Pdf editoriale | 15.18 MB | Adobe PDF | Visualizza/apri |
30434-huber_P01.pdf | Miur | 6.54 MB | Adobe PDF | Visualizza/apri |
30434-huber_P02.pdf | Miur | 8.71 MB | Adobe PDF | Visualizza/apri |
Page view(s)
95
controllato il 11-set-2024
Download(s)
63
controllato il 11-set-2024
Google ScholarTM
Check
Altmetric
Altmetric
Tutti i documenti in DSpace sono pubblicati ad Accesso Aperto, salvo diversa indicazione per alcuni documenti specifici.