HAT-P-34b-HAT-P-37b: Four transiting planets more massive than Jupiter orbiting moderately bright stars

Astronomical Journal

Volumn 144, Issue 1, 2012, Pages

  Bakos, G A ^a,b   Hartman, J D ^a,b   Torres, G ^b   Beky B ^b   Latham, D W ^b   Buchhave, L A ^c,l   Csubry, Z ^a,b   Kovacs G ^d   Bieryla, A ^b   Quinn, S ^b   Szklenar T ^b   Esquerdo, G A ^b   Shporer, A ^e,f   Noyes, R W ^b   Fischer, D A ^g   Johnson, J A ^h   Howard, A W ⁱ   Marcy, G W ⁱ   Sato, B ^j   Penev, K ^a,b   Everett, M ^b   Sasselov, D D ^b   Fresz G ^b   Stefanik, R P ^b   Lazar J ^k   Papp, I ^k   Sari P ^k   more..

^a PRINCETON UNIVERSITY   (United States)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c UNIVERSITY OF COPENHAGEN   (Denmark)

^d KONKOLY OBSERVATORY   (Hungary)

^e LCOGT   (United States)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g YALE UNIVERSITY   (United States)

^h CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

ⁱ UNIVERSITY OF CALIFORNIA   (United States)

^j TOKYO INSTITUTE OF TECHNOLOGY   (Japan)

^k HUNGARIAN ASTRONOMICAL ASSOCIATION   (Hungary)

^l UNIVERSITY OF COPENHAGEN   (Denmark)

more..

Author keywords

planetary systems; stars: individual (HAT P 34, GSC 1622 01261, HAT P 35, GSC 0203 01079, HAT P 36, ); techniques: photometric; techniques: spectroscopic

Indexed keywords

EID: 84862509055     PISSN: 00046256     EISSN: None     Source Type: Journal    
DOI: 10.1088/0004-6256/144/1/19     Document Type: Article

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