Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b

C. Hellier; D. R. Anderson; A. Collier Cameron; L. Delrez; M. Gillon; E. Jehin; M. Lendl; P. F. L. Maxted; F. Pepe; D. Pollacco; D. Queloz; D. Ségransan; B. Smalley; A. M. S. Smith; J. Southworth; A. H. M. J. Triaud; S. Udry; R. G. West

doi:10.1093/mnras/stu410

Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b

C. Hellier, D. R. Anderson, A. Collier Cameron, L. Delrez, M. Gillon, E. Jehin, M. Lendl, P. F. L. Maxted, F. Pepe, D. Pollacco, D. Queloz, D. Ségransan, B. Smalley, A. M. S. Smith, J. Southworth, A. H. M. J. Triaud, S. Udry, R. G. West

Physics and Astronomy

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Abstract

We report the discovery of the transiting exoplanets WASP-95b, WASP-96b, WASP-97b, WASP-98b, WASP-99b, WASP-100b and WASP-101b. All are hot Jupiters with orbital periods in the range 2.1-5.7 d, masses of 0.5-2.8 M_Jup and radii of 1.1-1.4 R_Jup. The orbits of all the planets are compatible with zero eccentricity. WASP-99b produces the shallowest transit yet found by WASP-South, at 0.4 per cent. The host stars are of spectral type F2-G8. Five have metallicities of [Fe/H] from -0.03 to +0.23, while WASP-98 has a metallicity of -0.60, exceptionally low for a star with a transiting exoplanet. Five of the host stars are brighter than V = 10.8, which significantly extends the number of bright transiting systems available for follow-up studies. WASP-95 shows a possible rotational modulation at a period of 20.7 d. We discuss the completeness of WASP survey techniques by comparing to the HATnet project.

Original language	English
Pages (from-to)	1982-1992
Number of pages	11
Journal	Royal Astronomical Society. Monthly Notices
Volume	440
DOIs	https://doi.org/10.1093/mnras/stu410
Publication status	Published - 3 Apr 2014

Keywords

planetary systems

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Hellier, C., Anderson, D. R., Cameron, A. C., Delrez, L., Gillon, M., Jehin, E., Lendl, M., Maxted, P. F. L., Pepe, F., Pollacco, D., Queloz, D., Ségransan, D., Smalley, B., Smith, A. M. S., Southworth, J., Triaud, A. H. M. J., Udry, S., & West, R. G. (2014). Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b. Royal Astronomical Society. Monthly Notices, 440, 1982-1992. https://doi.org/10.1093/mnras/stu410

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title = "Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b",

abstract = "We report the discovery of the transiting exoplanets WASP-95b, WASP-96b, WASP-97b, WASP-98b, WASP-99b, WASP-100b and WASP-101b. All are hot Jupiters with orbital periods in the range 2.1-5.7 d, masses of 0.5-2.8 MJup and radii of 1.1-1.4 RJup. The orbits of all the planets are compatible with zero eccentricity. WASP-99b produces the shallowest transit yet found by WASP-South, at 0.4 per cent. The host stars are of spectral type F2-G8. Five have metallicities of [Fe/H] from -0.03 to +0.23, while WASP-98 has a metallicity of -0.60, exceptionally low for a star with a transiting exoplanet. Five of the host stars are brighter than V = 10.8, which significantly extends the number of bright transiting systems available for follow-up studies. WASP-95 shows a possible rotational modulation at a period of 20.7 d. We discuss the completeness of WASP survey techniques by comparing to the HATnet project. ",

keywords = "planetary systems",

author = "C. Hellier and Anderson, {D. R.} and Cameron, {A. Collier} and L. Delrez and M. Gillon and E. Jehin and M. Lendl and Maxted, {P. F. L.} and F. Pepe and D. Pollacco and D. Queloz and D. S{\'e}gransan and B. Smalley and Smith, {A. M. S.} and J. Southworth and Triaud, {A. H. M. J.} and S. Udry and West, {R. G.}",

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Hellier, C, Anderson, DR, Cameron, AC, Delrez, L, Gillon, M, Jehin, E, Lendl, M, Maxted, PFL, Pepe, F, Pollacco, D, Queloz, D, Ségransan, D, Smalley, B, Smith, AMS, Southworth, J, Triaud, AHMJ, Udry, S & West, RG 2014, 'Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b', Royal Astronomical Society. Monthly Notices, vol. 440, pp. 1982-1992. https://doi.org/10.1093/mnras/stu410

TY - JOUR

T1 - Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b

AU - Hellier, C.

AU - Anderson, D. R.

AU - Cameron, A. Collier

AU - Delrez, L.

AU - Gillon, M.

AU - Jehin, E.

AU - Lendl, M.

AU - Maxted, P. F. L.

AU - Pepe, F.

AU - Pollacco, D.

AU - Queloz, D.

AU - Ségransan, D.

AU - Smalley, B.

AU - Smith, A. M. S.

AU - Southworth, J.

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

AU - Udry, S.

AU - West, R. G.

PY - 2014/4/3

Y1 - 2014/4/3

N2 - We report the discovery of the transiting exoplanets WASP-95b, WASP-96b, WASP-97b, WASP-98b, WASP-99b, WASP-100b and WASP-101b. All are hot Jupiters with orbital periods in the range 2.1-5.7 d, masses of 0.5-2.8 MJup and radii of 1.1-1.4 RJup. The orbits of all the planets are compatible with zero eccentricity. WASP-99b produces the shallowest transit yet found by WASP-South, at 0.4 per cent. The host stars are of spectral type F2-G8. Five have metallicities of [Fe/H] from -0.03 to +0.23, while WASP-98 has a metallicity of -0.60, exceptionally low for a star with a transiting exoplanet. Five of the host stars are brighter than V = 10.8, which significantly extends the number of bright transiting systems available for follow-up studies. WASP-95 shows a possible rotational modulation at a period of 20.7 d. We discuss the completeness of WASP survey techniques by comparing to the HATnet project.

AB - We report the discovery of the transiting exoplanets WASP-95b, WASP-96b, WASP-97b, WASP-98b, WASP-99b, WASP-100b and WASP-101b. All are hot Jupiters with orbital periods in the range 2.1-5.7 d, masses of 0.5-2.8 MJup and radii of 1.1-1.4 RJup. The orbits of all the planets are compatible with zero eccentricity. WASP-99b produces the shallowest transit yet found by WASP-South, at 0.4 per cent. The host stars are of spectral type F2-G8. Five have metallicities of [Fe/H] from -0.03 to +0.23, while WASP-98 has a metallicity of -0.60, exceptionally low for a star with a transiting exoplanet. Five of the host stars are brighter than V = 10.8, which significantly extends the number of bright transiting systems available for follow-up studies. WASP-95 shows a possible rotational modulation at a period of 20.7 d. We discuss the completeness of WASP survey techniques by comparing to the HATnet project.

KW - planetary systems

U2 - 10.1093/mnras/stu410

DO - 10.1093/mnras/stu410

M3 - Article

SN - 0035-8711

VL - 440

SP - 1982

EP - 1992

JO - Royal Astronomical Society. Monthly Notices

JF - Royal Astronomical Society. Monthly Notices

ER -

Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b

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Keywords

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