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WASP-36b : a new transiting planet around a metal-poor G-Dwarf, and an investigation into analyses based on a single transit light curve

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Smith, A. M. S., Anderson, D. R., Collier Cameron, A., Gillon, M., Hellier, C., Lendl, M., Maxted, P. F. L., Queloz, D., Smalley, B., Triaud, A. H. M. J., West, Richard G., Barros, S. C. C., Jehin, E., Pepe, F., Pollacco, Don, Segransan, D., Southworth, J., Street, R. A. and Udry, S. (2012) WASP-36b : a new transiting planet around a metal-poor G-Dwarf, and an investigation into analyses based on a single transit light curve. The Astronomical Journal, Volume 143 (Number 4). Article number 81. doi:10.1088/0004-6256/143/4/81

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Official URL: http://dx.doi.org/10.1088/0004-6256/143/4/81

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Abstract

We report the discovery, from WASP and CORALIE, of a transiting exoplanet in a 1.54 day orbit. The host star, WASP-36, is a magnitude V = 12.7, metal-poor G2 dwarf ($\mbox{$T_{\rm eff}$}= 5959\pm 134$ K), with [Fe/H] =–0.26 ± 0.10. We determine the planet to have mass and radius, respectively, 2.30 ± 0.07 and 1.28 ± 0.03 times that of Jupiter. We have eight partial or complete transit light curves, from four different observatories, which allow us to investigate the potential effects on the fitted system parameters of using only a single light curve. We find that the solutions obtained by analyzing each of these light curves independently are consistent with our global fit to all the data, despite the apparent presence of correlated noise in at least two of the light curves.

Item Type: Journal Article
Divisions: Faculty of Science > Physics
Journal or Publication Title: The Astronomical Journal
Publisher: Institute of Physics Publishing, Inc.
ISSN: 0004-6256
Official Date: February 2012
Dates:
DateEvent
February 2012Published
Volume: Volume 143
Number: Number 4
Article Number: Article number 81
DOI: 10.1088/0004-6256/143/4/81
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Restricted or Subscription Access

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