WASP-40b: Independent Discovery of the 0.6 M Transiting Exoplanet HAT-P-27b
- Anderson, D. R.
- Barros, S. C. C.
- Boisse, I.
- Bouchy, F.
- Collier Cameron, A.
- Faedi, F.
- Hebrard, G.
- Hellier, C.
- Lendl, M.
- Moutou, C.
- Pollacco, D.
- Santerne, A.
- Smalley, B.
- Smith, A. M. S.
- Todd, I.
- Triaud, A H M J
- West, R. G.
- Wheatley, P. J.
- Bento, J.
- Enoch, B.
- Gillon, Michaël
- Maxted, P. F. L.
- McCormac, J.
- Queloz, D.
- Simpson, E. K.
- Skillen, I.
Publication date
May 2011
DOI Publisher
University of Chicago Press for the Astronomical Society of the PacificAbstract
peer reviewedFrom WASP photometry and SOPHIE radial velocities we report the discovery of WASP-40b (HAT-P-27b), a 0.6 M planet that transits its 12th magnitude host star every 3.04 days. The host star is of late G-type or early K-type and likely has a metallicity greater than solar ([Fe/H]=0.14±0.11). The planet's mass and radius are typical of the known hot Jupiters, thus adding another system to the apparent pileup of transiting planets with periods near 3-4 days. Our parameters match those of the recent HATnet announcement of the same planet, thus giving confidence in the techniques used. We report a possible indication of stellar activity in the host star
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