HAT-P-24b: An inflated hot Jupiter on a 3.36 day period transiting a hot, metal-poor star

Astrophysical Journal

Volumn 725, Issue 2, 2010, Pages 2017-2028

  Kipping, D M ^a,b   Bakos, G A ^a   Hartman, J ^a   Torres, G ^a   Shporer, A ^c,d   Latham, D W ^a   Kovács, Géza ^e   Noyes, R W ^a   Howard, A W ^f   Fischer, D A ^g   Johnson, J A ^h   Marcy, G W ^f   Beky B ^a   Perumpilly, G ^a   Esquerdo, G A ^a   Sasselov, D D ^a   Stefanik, R P ^a   Lazar J ⁱ   Papp, I ⁱ   Sari P ⁱ  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b UNIVERSITY COLLEGE LONDON   (United Kingdom)

^c LAS CUMBRES OBSERVATORY GLOBAL TELESCOPE NETWORK   (United States)

^d UNIVERSITY OF CALIFORNIA   (United States)

^e KONKOLY OBSERVATORY   (Hungary)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g YALE UNIVERSITY   (United States)

^h CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

ⁱ HUNGARIAN ASTRONOMICAL ASSOCIATION   (Hungary)

Author keywords

Planetary systems; Stars: individual (HAT P 24); Techniques: photometric; Techniques: spectroscopic

Indexed keywords

EID: 78650101129     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/725/2/2017     Document Type: Article

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