WASP-40b: Independent Discovery of the 0.6 M Transiting Exoplanet HAT-P-27b

D.R. Anderson; S.C.C. Barros; I. Boisse; F. Bouchy; A. Collier Cameron; F. Faedi; [No Value] Hebrard; Don Pollacco; A. Santerne; B. Smalley; A.M.S. Smith; I. Todd; A.H.M.J. Triaud; R.G. West; P. Wheatley

doi:10.1086/660135

WASP-40b: Independent Discovery of the 0.6 M Transiting Exoplanet HAT-P-27b

D.R. Anderson, S.C.C. Barros, I. Boisse, F. Bouchy, A. Collier Cameron, F. Faedi, [No Value] Hebrard, Don Pollacco, A. Santerne, B. Smalley, A.M.S. Smith, I. Todd, A.H.M.J. Triaud, R.G. West, P. Wheatley

Research output: Contribution to journal › Article › peer-review

16 Citations (Scopus)

Abstract

From 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.

Original language	English
Pages (from-to)	555-560
Number of pages	6
Journal	Publications of the Astronomical Society of the Pacific
Volume	123
Issue number	903
DOIs	https://doi.org/10.1086/660135
Publication status	Published - May 2011

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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Anderson, D. R., Barros, S. C. C., Boisse, I., Bouchy, F., Collier Cameron, A., Faedi, F., Hebrard, N. V., Pollacco, D., Santerne, A., Smalley, B., Smith, A. M. S., Todd, I., Triaud, A. H. M. J., West, R. G., & Wheatley, P. (2011). WASP-40b: Independent Discovery of the 0.6 M Transiting Exoplanet HAT-P-27b. Publications of the Astronomical Society of the Pacific, 123(903), 555-560. https://doi.org/10.1086/660135

Anderson, D.R. ; Barros, S.C.C. ; Boisse, I. ; Bouchy, F. ; Collier Cameron, A. ; Faedi, F. ; Hebrard, [No Value] ; Pollacco, Don ; Santerne, A. ; Smalley, B. ; Smith, A.M.S. ; Todd, I. ; Triaud, A.H.M.J. ; West, R.G. ; Wheatley, P. / WASP-40b: Independent Discovery of the 0.6 M Transiting Exoplanet HAT-P-27b. In: Publications of the Astronomical Society of the Pacific. 2011 ; Vol. 123, No. 903. pp. 555-560.

@article{37bf39488dbb49b79492e334f75f5b15,

title = "WASP-40b: Independent Discovery of the 0.6 M Transiting Exoplanet HAT-P-27b",

abstract = "From 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.",

author = "D.R. Anderson and S.C.C. Barros and I. Boisse and F. Bouchy and {Collier Cameron}, A. and F. Faedi and Hebrard, {[No Value]} and Don Pollacco and A. Santerne and B. Smalley and A.M.S. Smith and I. Todd and A.H.M.J. Triaud and R.G. West and P. Wheatley",

year = "2011",

month = may,

doi = "10.1086/660135",

language = "English",

volume = "123",

pages = "555--560",

journal = "Publications of the Astronomical Society of the Pacific",

issn = "0004-6280",

publisher = "University of Chicago",

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Anderson, DR, Barros, SCC, Boisse, I, Bouchy, F, Collier Cameron, A, Faedi, F, Hebrard, NV, Pollacco, D, Santerne, A, Smalley, B, Smith, AMS, Todd, I, Triaud, AHMJ, West, RG & Wheatley, P 2011, 'WASP-40b: Independent Discovery of the 0.6 M Transiting Exoplanet HAT-P-27b', Publications of the Astronomical Society of the Pacific, vol. 123, no. 903, pp. 555-560. https://doi.org/10.1086/660135

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, [No Value]; Pollacco, Don; Santerne, A.; Smalley, B.; Smith, A.M.S.; Todd, I.; Triaud, A.H.M.J.; West, R.G.; Wheatley, P.

In: Publications of the Astronomical Society of the Pacific, Vol. 123, No. 903, 05.2011, p. 555-560.

Research output: Contribution to journal › Article › peer-review

TY - JOUR

T1 - WASP-40b: Independent Discovery of the 0.6 M Transiting Exoplanet HAT-P-27b

AU - Anderson, D.R.

AU - Barros, S.C.C.

AU - Boisse, I.

AU - Bouchy, F.

AU - Collier Cameron, A.

AU - Faedi, F.

AU - Hebrard, [No Value]

AU - Pollacco, Don

AU - Santerne, A.

AU - Smalley, B.

AU - Smith, A.M.S.

AU - Todd, I.

AU - Triaud, A.H.M.J.

AU - West, R.G.

AU - Wheatley, P.

PY - 2011/5

Y1 - 2011/5

N2 - From 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.

AB - From 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.

U2 - 10.1086/660135

DO - 10.1086/660135

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JO - Publications of the Astronomical Society of the Pacific

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