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WASP-4b: a 12th-magnitude transiting hot-Jupiter in the Southern hemisphere

Wilson, D. M.; Gillon, M.; Hellier, C.; Maxted, P. F. L.; Pepe, F.; Queloz, D.; Anderson, D. R.; Collier-Cameron, A.; Smalley, B.; Lister, T. A.; Bentley, S. J.; Blecha, A.; Christian, D. J.; Enoch, B.; Haswell, C. A.; Hebb, L.; Horne, K.; Irwin, J.; Joshi, Y. C.; Kane, S. R.; Marmier, M.; Mayor, M.; Parley, N.; Pollacco, D.; Pont, F.; Ryans, R.; Segransan, D.; Skillen, I.; Street, R. A.; Udry, S.; West, R. G. and Wheatley, P. J. (2008). WASP-4b: a 12th-magnitude transiting hot-Jupiter in the Southern hemisphere. Astrophysical Journal Letters, 675 L113-L116.

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URL: http://www.journals.uchicago.edu/doi/abs/10.1086/5...
DOI (Digital Object Identifier) Link: http://dx.doi.org/10.1086/586735
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Abstract

We report the discovery of WASP-4b, a large transiting gas-giant planet with an orbital period of 1.34 days. This is the first planet to be discovered by the SuperWASP-South observatory and CORALIE collaboration and the first planet orbiting a star brighter than 16th magnitude to be discovered in the southern hemisphere. A simultaneous fit to high-quality light curves and precision radial velocity measurements leads to a planetary mass of 1.22 M and a planetary radius of 1.42 R . The host star is USNO-B1.0 0479−0948995, a G7 V star of visual magnitude 12.5. As a result of the short orbital period, the predicted surface temperature of the planet is 1761 K, making it an ideal candidate for detections of the secondary eclipse at infrared wavelengths.

Item Type: Journal Article
ISSN: 1538-4357
Extra Information: Click here to view other publications available on this repository relating to the SuperWASP Project.
Academic Unit/Department: Science > Physical Sciences
Science > Physical Sciences
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 10770
Depositing User: Astrid Peterkin
Date Deposited: 28 May 2008
Last Modified: 05 Dec 2010 05:56
URI: http://oro.open.ac.uk/id/eprint/10770
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