HAT-P-27b: A HOT JUPITER TRANSITING A G STAR ON A 3 DAY ORBIT
dc.contributor.author | Beky, B. | |
dc.contributor.author | Bakos, G. A. | |
dc.contributor.author | Hartman, J. | |
dc.contributor.author | Torres, G. | |
dc.contributor.author | Latham, D. W. | |
dc.contributor.author | Jordan, A. | |
dc.contributor.author | Arriagada, P. | |
dc.contributor.author | Bayliss, D. | |
dc.contributor.author | Kiss, L. L. | |
dc.contributor.author | Kovacs, Geza | |
dc.contributor.author | Quinn, S. N. | |
dc.contributor.author | Marcy, G. W. | |
dc.contributor.author | Howard, A. W. | |
dc.contributor.author | Fischer, D. A. | |
dc.contributor.author | Johnson, J. A. | |
dc.contributor.author | Esquerdo, G. A. | |
dc.contributor.author | Noyes, R. W. | |
dc.contributor.author | Buchhave, L. A. | |
dc.contributor.author | Sasselov, D. D. | |
dc.contributor.author | Stefanik, R. P. | |
dc.contributor.author | Perumpilly, G. | |
dc.contributor.author | Lazar, J. | |
dc.contributor.author | Papp, I. | |
dc.contributor.author | Sari, P. | |
dc.date.accessioned | 2025-01-21T00:01:47Z | |
dc.date.available | 2025-01-21T00:01:47Z | |
dc.date.issued | 2011 | |
dc.description.abstract | We report the discovery of HAT-P-27b, an exoplanet transiting the moderately bright G8 dwarf star GSC 0333-00351 (V = 12.214). The orbital period is 3.039586 +/- 0.000012 days, the reference epoch of transit is 2455186.01879 +/- 0.00054 (BJD), and the transit duration is 0.0705 +/- 0.0019 days. The host star with its effective temperature 5300 +/- 90 K is somewhat cooler than the Sun and is more metal-rich with a metallicity of +0.29 +/- 0.10. Its mass is 0.94 +/- 0.04 M-circle dot and radius is 0.90(-0.04)(+0.05) R-circle dot. For the planetary companion we determine a mass of 0.660 +/- 0.033 M-J and radius of 1.038(-0.058)(+0.077) R-J. For the 30 known transiting exoplanets between 0.3 M-J and 0.8 M-J, a negative correlation between host star metallicity and planetary radius and an additional dependence of planetary radius on equilibrium temperature are confirmed at a high level of statistical significance. | |
dc.fuente.origen | WOS | |
dc.identifier.doi | 10.1088/0004-637X/734/2/109 | |
dc.identifier.eissn | 1538-4357 | |
dc.identifier.issn | 0004-637X | |
dc.identifier.uri | https://doi.org/10.1088/0004-637X/734/2/109 | |
dc.identifier.uri | https://repositorio.uc.cl/handle/11534/95395 | |
dc.identifier.wosid | WOS:000291386500037 | |
dc.issue.numero | 2 | |
dc.language.iso | en | |
dc.revista | Astrophysical journal | |
dc.rights | acceso restringido | |
dc.subject | planetary systems | |
dc.subject | stars: individual (HAT-P-27, GSC 0333-00351) | |
dc.subject | techniques: photometric | |
dc.subject | techniques: spectroscopic | |
dc.subject.ods | 13 Climate Action | |
dc.subject.odspa | 13 Acción por el clima | |
dc.title | HAT-P-27b: A HOT JUPITER TRANSITING A G STAR ON A 3 DAY ORBIT | |
dc.type | artículo | |
dc.volumen | 734 | |
sipa.index | WOS | |
sipa.trazabilidad | WOS;2025-01-12 |