HAT-P-18b and HAT-P-19b: Two low-density Saturn-mass planets transiting metal-rich K stars

Astrophysical Journal

Volumn 726, Issue 1, 2011, Pages

  Hartman, J D ^a   Bakos, G A ^a   Sato, B ^b   Torres, G ^a   Noyes, R W ^a   Latham, D W ^a   Kovacs G ^c   Fischer, D A ^d   Howard, A W ^e   Johnson, J A ^f   Marcy, G W ^e   Buchhave, L A ^a,g   Furesz G ^a   Perumpilly, G ^a,h   Beky B ^a   Stefanik, R P ^a   Sasselov, D D ^a   Esquerdo, G A ^a   Everett, M ^a   Csubry, Z ^a   Lazar J ⁱ   Papp, I ⁱ   Sari P ⁱ   more..

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b TOKYO INSTITUTE OF TECHNOLOGY   (Japan)

^c KONKOLY OBSERVATORY   (Hungary)

^d SAN FRANCISCO STATE UNIVERSITY   (United States)

^e UNIVERSITY OF CALIFORNIA   (United States)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g UNIVERSITY OF COPENHAGEN   (Denmark)

^h University of South Dakota   (United States)

ⁱ HUNGARIAN ASTRONOMICAL ASSOCIATION   (Hungary)

Author keywords

GSC 2283 00589); Planetary systems; Stars: individual (HAT P 18, GSC 2594 00646, HAT P 19; Techniques: photometric; Techniques: spectroscopic

Indexed keywords

EID: 84891243650     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/726/1/52     Document Type: Article

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