4.7 Article

HAT-P-25b: A HOT-JUPITER TRANSITING A MODERATELY FAINT G STAR

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ASTROPHYSICAL JOURNAL
卷 745, 期 1, 页码 -

出版社

IOP PUBLISHING LTD
DOI: 10.1088/0004-637X/745/1/80

关键词

planetary systems; stars: individual (HAT-P-25, GSC 1788-01237); techniques: photometric techniques: spectroscopic

资金

  1. NASA [NNG04GN74G, NNX08AF23G, NNX09AF59G]
  2. SAO IRD
  3. NSF [AST-0702843, AST-0702821]
  4. Kepler Mission under NASA [NCC2-1390]
  5. Hungarian Scientific Research Foundation (OTKA) [K-81373]
  6. NASA [118994, NNX09AF59G] Funding Source: Federal RePORTER

向作者/读者索取更多资源

We report the discovery of HAT-P-25b, a transiting extrasolar planet orbiting the V = 13.19 G5 dwarf star GSC 1788-01237, with a period P = 3.652836 +/- 0.000019 days, transit epoch T-c = 2455176.85173 +/- 0.00047 (BJD-barycentric Julian dates throughout the paper are calculated from Coordinated Universal Time, UTC), and transit duration 0.1174 +/- 0.0017 days. The host star has a mass of 1.01 +/- 0.03 M-circle dot, radius of 0.96(-0.04)(+0.05)R(circle dot), effective temperature 5500 +/- 80 K, and metallicity [Fe/H] = +0.31 +/- 0.08. The planetary companion has a mass of 0.567 +/- 0.022 M-J and radius of 1.190(-0.056)(+0.081) R-J yielding a mean density of 0.42 +/- 0.07 g cm(-3).

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