Kepler's optical phase curve of the exoplanet HAT-P-7b

Science

Volumn 325, Issue 5941, 2009, Pages 709-

  Borucki, W J ^a   Koch, D ^a   Jenkins, J ^b   Sasselov, D ^c   Gilliland, R ^d   Batalha, N ^e   Latham, D W ^c   Caldwell, D ^b   Basri, G ^f   Brown, T ^g   Christensen Dalsgaard, J ^h   Cochran, W D ⁱ   DeVore, E ^b   Dunham, E ^j   Dupree, A K ^c   Gautier, T ^k   Geary, J ^c   Gould, A ^l   Howell, S ^m   Kjeldsen, H ^h   Lissauer, J ^a   Marcy, G ^f   Meibom, S ^c   Morrison, D ^a   Tarter, J ^b   more..

^a NASA AMES RESEARCH CENTER   (United States)

^b SETI INSTITUTE   (United States)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d STScI   (United States)

^e SAN JOSE STATE UNIVERSITY   (United States)

^f UNIVERSITY OF CALIFORNIA   (United States)

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

^h AARHUS UNIVERSITY   (Denmark)

ⁱ UNIVERSITY OF TEXAS AT AUSTIN   (United States)

^j LOWELL OBSERVATORY   (United States)

^k CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^l Lawrence Hall of Science ^*  (United States)

^m NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

more..

Author keywords

[No Author keywords available]

Indexed keywords

OPTICAL METHOD;

ASTRONOMY; ATMOSPHERE; NIGHT; PHOTOMETRY; PREDICTION; PRIORITY JOURNAL; SHORT SURVEY; TEMPERATURE;

EID: 68449083318     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1178312     Document Type: Short Survey

References (9)

1. W. J. Boracki, A. L. Summers, Icarus 58, 121 (1984).
2. http://exoplanet.eu
3. A. Pal et al., Astrophys. J. 680, 1450 (2008).
4. Materials and methods are available on Science Online.
5. M. Lopez-Morales, S. Seager, Astrophys. J. 667, L191 (2007).
6. J. J. Fortney, K. Lodders, M. S. Marley, R. S. Freedman, Astrophys. J. 678, 1419 (2008).
7. I. A. G. Snellen, E. J. W. de Mooij, S. Albrecht, Nature 459, 543 (2009).
8. R. Alonso et al., http://arxiv.org/abs/0906.2814v1 (2009).
9. We acknowledge the contributions of hundreds of individuals across NASA, Ball Aerospace, and the scientific community who made this mission possible. Funding was provided by the NASA Discovery program.