CARLEO, Ilaria, Davide GANDOLFI, Oscar BARRAGAN, John H. LIVINGSTON, Carina M. PERSSON, Kristine W. F. LAM, Aline VIDOTTO, Michael B. LUND, Carolina Villarr D'ANGELO, Karen A. COLLINS, Luca FOSSATI, Andrew W. HOWARD, Daria KUBYSHKINA, Rafael BRAHM, Antonija OKLOPCIC, Paul MOLLIERE, Seth REDFIELD, Luisa Maria SERRANO, Fei DAI, Malcolm FRIDLUND, Francesco BORSA, Judith KORTH, Massimiliano ESPOSITO, Matias R. DIAZ, Louise Dyregaard NIELSEN, Coel HELLIER, Savita MATHUR, Hans J. DEEG, Artie P. HATZES, Serena BENATTI, Florian RODLER, Javier ALARCON, Lorenzo SPINA, Angela R. G. SANTOS, Iskra GEORGIEVA, Rafael A. GARCIA, Lucia GONZALEZ-CUESTA, George R. RICKER, Roland VANDERSPEK, David W. LATHAM, Sara SEAGER, Joshua N. WINN, Jon M. JENKINS, Simon ALBRECHT, Natalie M. BATALHA, Corey BEARD, Patricia T. BOYD, Francois BOUCHY, Jennifer A. BURT, R. Paul BUTLER, Juan CABRERA, Ashley CHONTOS, David R. CIARDI, William D. COCHRAN, Kevin I. COLLINS, Jeffrey D. CRANE, Ian CROSSFIELD, Szilard CSIZMADIA, Diana DRAGOMIR, Courtney DRESSING, Philipp EIGMULLER, Michael ENDL, Anders ERIKSON, Nestor ESPINOZA, Michael FAUSNAUGH, Fabo FENG, Erin FLOWERS, Benjamin FULTON, Erica J. GONZALES, Nolan GRIEVES, Sascha GRZIWA, Eike W. GUENTHER, Natalia M. GUERRERO, Thomas HENNING, Diego HIDALGO, Teruyuki HIRANO, Maria HJORTH, Daniel HUBER, Howard ISAACSON, Matias JONES, Andres JORDAN, Petr KABATH, Stephen R. KANE, Emil KNUDSTRUP, Jack LUBIN, Rafael LUQUE, Ismael MIRELES, Norio NARITA, David NESPRAL, Prajwal NIRAULA, Grzegorz NOWAK, Enric PALLE, Martin PATZOLD, Erik A. PETIGURA, Jorge PRIETO-ARRANZ, Heike RAUER, Paul ROBERTSON, Mark E. ROSE, Arpita ROY, Paula SARKIS, Joshua E. SCHLIEDER, Damien SEGRANSAN, Stephen SHECTMAN, Marek SKARKA, Alexis M. S. SMITH, Jeffrey C. SMITH, Keivan STASSUN, Johanna TESKE, Joseph D. TWICKEN, Vincent VAN EYLEN, Sharon WANG, Lauren M. WEISS a Aurelien WYTTENBACH. The Multiplanet System TOI-421: A Warm Neptune and a Super Puffy Mini-Neptune Transiting a G9 V Star in a Visual Binary. Astronomical Journal. Bristol: IOP Publishing Ltd., 2020, roč. 160, č. 3, s. 1-23. ISSN 0004-6256. Dostupné z: https://dx.doi.org/10.3847/1538-3881/aba124.
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Základní údaje
Originální název The Multiplanet System TOI-421: A Warm Neptune and a Super Puffy Mini-Neptune Transiting a G9 V Star in a Visual Binary
Autoři CARLEO, Ilaria, Davide GANDOLFI, Oscar BARRAGAN, John H. LIVINGSTON, Carina M. PERSSON, Kristine W. F. LAM, Aline VIDOTTO, Michael B. LUND, Carolina Villarr D'ANGELO, Karen A. COLLINS, Luca FOSSATI, Andrew W. HOWARD, Daria KUBYSHKINA, Rafael BRAHM, Antonija OKLOPCIC, Paul MOLLIERE, Seth REDFIELD, Luisa Maria SERRANO, Fei DAI, Malcolm FRIDLUND, Francesco BORSA, Judith KORTH, Massimiliano ESPOSITO, Matias R. DIAZ, Louise Dyregaard NIELSEN, Coel HELLIER, Savita MATHUR, Hans J. DEEG, Artie P. HATZES, Serena BENATTI, Florian RODLER, Javier ALARCON, Lorenzo SPINA, Angela R. G. SANTOS, Iskra GEORGIEVA, Rafael A. GARCIA, Lucia GONZALEZ-CUESTA, George R. RICKER, Roland VANDERSPEK, David W. LATHAM, Sara SEAGER, Joshua N. WINN, Jon M. JENKINS, Simon ALBRECHT, Natalie M. BATALHA, Corey BEARD, Patricia T. BOYD, Francois BOUCHY, Jennifer A. BURT, R. Paul BUTLER, Juan CABRERA, Ashley CHONTOS, David R. CIARDI, William D. COCHRAN, Kevin I. COLLINS, Jeffrey D. CRANE, Ian CROSSFIELD, Szilard CSIZMADIA, Diana DRAGOMIR, Courtney DRESSING, Philipp EIGMULLER, Michael ENDL, Anders ERIKSON, Nestor ESPINOZA, Michael FAUSNAUGH, Fabo FENG, Erin FLOWERS, Benjamin FULTON, Erica J. GONZALES, Nolan GRIEVES, Sascha GRZIWA, Eike W. GUENTHER, Natalia M. GUERRERO, Thomas HENNING, Diego HIDALGO, Teruyuki HIRANO, Maria HJORTH, Daniel HUBER, Howard ISAACSON, Matias JONES, Andres JORDAN, Petr KABATH, Stephen R. KANE, Emil KNUDSTRUP, Jack LUBIN, Rafael LUQUE, Ismael MIRELES, Norio NARITA, David NESPRAL, Prajwal NIRAULA, Grzegorz NOWAK, Enric PALLE, Martin PATZOLD, Erik A. PETIGURA, Jorge PRIETO-ARRANZ, Heike RAUER, Paul ROBERTSON, Mark E. ROSE, Arpita ROY, Paula SARKIS, Joshua E. SCHLIEDER, Damien SEGRANSAN, Stephen SHECTMAN, Marek SKARKA (203 Česká republika, domácí), Alexis M. S. SMITH, Jeffrey C. SMITH, Keivan STASSUN, Johanna TESKE, Joseph D. TWICKEN, Vincent VAN EYLEN, Sharon WANG, Lauren M. WEISS a Aurelien WYTTENBACH.
Vydání Astronomical Journal, Bristol, IOP Publishing Ltd. 2020, 0004-6256.
Další údaje
Originální jazyk angličtina
Typ výsledku Článek v odborném periodiku
Obor 10308 Astronomy
Stát vydavatele Velká Británie a Severní Irsko
Utajení není předmětem státního či obchodního tajemství
WWW URL
Impakt faktor Impact factor: 6.263
Kód RIV RIV/00216224:14310/20:00117944
Organizační jednotka Přírodovědecká fakulta
Doi http://dx.doi.org/10.3847/1538-3881/aba124
UT WoS 000561609000001
Klíčová slova anglicky Exoplanet astronomy; Exoplanet systems; Exoplanets; Mini Neptunes; Hot Neptunes; Fundamental parameters of stars; High resolution spectroscopy; Transit photometry; Radial velocity
Štítky rivok
Příznaky Mezinárodní význam, Recenzováno
Změnil Změnila: Mgr. Marie Šípková, DiS., učo 437722. Změněno: 21. 1. 2021 15:14.
Anotace
We report the discovery of a warm Neptune and a hot sub-Neptune transiting TOI-421 (BD-14 1137, TIC 94986319), a bright (V = 9.9) G9 dwarf star in a visual binary system observed by the Transiting Exoplanet Survey Satellite (TESS) space mission in Sectors 5 and 6. We performed ground-based follow-up observations-comprised of Las Cumbres Observatory Global Telescope transit photometry, NIRC2 adaptive optics imaging, and FIbre-fed Echelle Spectrograph, CORALIE, High Accuracy Radial velocity Planet Searcher, High Resolution echelle Spectrometer, and Planet Finder Spectrograph high-precision Doppler measurements-and confirmed the planetary nature of the 16 day transiting candidate announced by the TESS team. We discovered an additional radial velocity signal with a period of five days induced by the presence of a second planet in the system, which we also found to transit its host star. We found that the inner mini-Neptune, TOI-421 b, has an orbital period of P-b = 5.19672 +/- 0.00049 days, a mass of M-b = 7.17 +/- 0.66 M-circle plus, and a radius of R-b = R-circle plus, whereas the outer warm Neptune, TOI-421 c, has a period of P-c = 16.06819 +/- 0.00035 days, a mass of M-c = 16.42(-1.04)(+1.06)M(circle plus), a radius of R-c = 5.09(-0.15)(+0.16)R(circle plus), and a density of rho(c) = 0.685(-0.072)(+0.080) cm(-3). With its characteristics, the outer planet (rho(c) = 0.685(-0.0072)(+0.080) cm(-3)) is placed in the intriguing class of the super-puffy mini-Neptunes. TOI-421 b and TOI-421 c are found to be well-suited for atmospheric characterization. Our atmospheric simulations predict significant Ly alpha transit absorption, due to strong hydrogen escape in both planets, as well as the presence of detectable CH4 in the atmosphere of TOI-421 c if equilibrium chemistry is assumed.
VytisknoutZobrazeno: 24. 4. 2024 16:01