HAT-P-11b: A super-neptune planet transiting a bright K star in the kepler field

Astrophysical Journal

Volumn 710, Issue 2, 2010, Pages 1724-1745

  Bakos, G A ^a   Torres, G ^a   Pal A ^a,b   Hartman, J ^a   Kovács, Géza ^c   Noyes, R W ^a   Latham, D W ^a   Sasselov, D D ^a   Sipocz B ^a,b   Esquerdo, G A ^a   Fischer, D A ^d   Johnson, J A ^e   Marcy, G W ^f   Butler, R P ^g   Isaacson, H ^d   Howard, A ^f   Vogt, S ^h   Kovács, Gbor ^a   Fernandez, J ^a   Moor A ^c   Stefanik, R P ^a   Lazar J ⁱ   Papp, I ⁱ   Sari P ⁱ   more..

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^b EÖTVÖS LORÁND UNIVERSITY   (Hungary)

^c KONKOLY OBSERVATORY   (Hungary)

^d SAN FRANCISCO STATE UNIVERSITY   (United States)

^e UNIVERSITY OF HAWAII   (United States)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g GEOPHYSICAL LABORATORY   (United States)

^h University of California at Santa Cruz   (United States)

ⁱ HUNGARIAN ASTRONOMICAL ASSOCIATION   (Hungary)

Author keywords

Planetary systems; Stars: individual (HAT P 11, GSC 03561 02092); Techniques: photometric; Techniques: spectroscopic

Indexed keywords

EID: 77149164433     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/710/2/1724     Document Type: Article

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