Article (Scientific journals)
The Transit Light Curve Project. VII. The Not-So-Bloated Exoplanet HAT-P-1b
Winn, Joshua N; Holman, Matthew J; Bakos, Gaspar Á et al.
2007In Astronomical Journal, 134, p. 1707-1712
Peer Reviewed verified by ORBi
 

Files


Full Text
205953.web.pdf
Publisher postprint (1.69 MB)
Download

All documents in ORBi are protected by a user license.

Send to



Details



Abstract :
[en] We present photometry of the G0 star HAT-P-1 during six transits of its close-in giant planet, and we refine the estimates of the system parameters. Relative to Jupiter's properties, HAT-P-1b is 1.20 ± 0.05 times larger, and its surface gravity is 2.7 ± 0.2 times weaker. Although it remains the case that HAT-P-1b is among the least dense of the known sample of transiting exoplanets, its properties are in accord with previously published models of strongly irradiated, coreless, solar-composition giant planets. The times of the transits have a typical accuracy of 1 minute and do not depart significantly from a constant period.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Winn, Joshua N;  Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
Holman, Matthew J;  Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
Bakos, Gaspar Á;  Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA ; Hubble Fellow
Pál, András;  Department of Astronomy, Eötvös Loránd University, Pf. 32, H-1518 Budapest, Hungary
Johnson, John Asher;  Department of Astronomy, University of California, Mail Code 3411, Berkeley, CA 94720, USA
Williams, Peter K G;  Department of Astronomy, University of California, Mail Code 3411, Berkeley, CA 94720, USA
Shporer, Avi;  Wise Observatory, Raymond and Beverly Sackler Faculty of Exact Sciences, Tel Aviv University, Tel Aviv 69978, Israel
Mazeh, Tsevi;  Wise Observatory, Raymond and Beverly Sackler Faculty of Exact Sciences, Tel Aviv University, Tel Aviv 69978, Israel
Fernandez, José;  Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA ; Department of Astronomy, Pontificia Universidad Católica, Casilla 306, Santiago 22, Chile
Latham, David W;  Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
Gillon, Michaël  ;  Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique et traitement de l'image
Language :
English
Title :
The Transit Light Curve Project. VII. The Not-So-Bloated Exoplanet HAT-P-1b
Publication date :
01 October 2007
Journal title :
Astronomical Journal
ISSN :
0004-6256
eISSN :
1538-3881
Publisher :
Univ Chicago Press, Chicago, United States - Illinois
Volume :
134
Pages :
1707-1712
Peer reviewed :
Peer Reviewed verified by ORBi
Commentary :
http://de.arxiv.org/abs/0707.1908
Available on ORBi :
since 30 October 2009

Statistics


Number of views
74 (3 by ULiège)
Number of downloads
181 (0 by ULiège)

Scopus citations®
 
67
Scopus citations®
without self-citations
47
OpenCitations
 
91

Bibliography


Similar publications



Contact ORBi