Pierre Maxted p.maxted@keele.ac.uk
Five transiting hot Jupiters discovered using WASP-South, Euler and TRAPPIST: WASP-119 b, WASP-124 b, WASP-126 b, WASP-129 b and WASP-133 b
Maxted, P.F.L.; Anderson, D.R.; Collier Cameron, A.; Delrez, L.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; -VanMalle, M.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A.M.S.; Southworth, J.; Triaud, A.H.M.J.; Udry, S.; Wagg, T.; West, R.G.
Authors
D.R. Anderson
A. Collier Cameron
L. Delrez
M. Gillon
Coel Hellier c.hellier@keele.ac.uk
E. Jehin
M. Lendl
M. -VanMalle
F. Pepe
D. Pollacco
D. Queloz
D. Ségransan
Barry Smalley b.smalley@keele.ac.uk
A.M.S. Smith
Dr John Taylor j.k.taylor@keele.ac.uk
A.H.M.J. Triaud
S. Udry
T. Wagg
R.G. West
Abstract
We have used photometry from the WASP-South instrument to identify 5 stars showing planet-like transits in their light curves. The planetary nature of the companions to these stars has been confirmed using photometry from the EulerCam instrument on the Swiss Euler 1.2-m telescope and the TRAPPIST telescope, and spectroscopy obtained with the CORALIE spectrograph. The planets discovered are hot Jupiter systems with orbital periods in the range 2.17 to 5.75 days, masses from 0.3M$_{\rm Jup}$ to 1.2M$_{\rm Jup}$ and with radii from 1R$_{\rm Jup}$ to 1.5R$_{\rm Jup}$. These planets orbit bright stars (V = 11-13) with spectral types in the range F9 to G4. WASP-126 is the brightest planetary system in this sample and hosts a low-mass planet with a large radius (0.3 M$_{\rm Jup}$ , 0.95R$_{\rm Jup}$), making it a good target for transmission spectroscopy. The high density of WASP-129 A suggests that it is a helium-rich star similar to HAT-P-11 A. WASP-133 has an enhanced surface lithium abundance compared to other old G-type stars, particularly other planet host stars. These planetary systems are good targets for follow-up observations with ground-based and space-based facilities to study their atmospheric and dynamical properties.
Citation
Maxted, P., Anderson, D., Collier Cameron, A., Delrez, L., Gillon, M., Hellier, C., Jehin, E., Lendl, M., -VanMalle, M., Pepe, F., Pollacco, D., Queloz, D., Ségransan, D., Smalley, B., Smith, A., Southworth, J., Triaud, A., Udry, S., Wagg, T., & West, R. (2016). Five transiting hot Jupiters discovered using WASP-South, Euler and TRAPPIST: WASP-119 b, WASP-124 b, WASP-126 b, WASP-129 b and WASP-133 b. Astronomy and Astrophysics, 591, Article A55. https://doi.org/10.1051/0004-6361/201628250
Journal Article Type | Article |
---|---|
Acceptance Date | Apr 24, 2016 |
Online Publication Date | Jun 10, 2016 |
Publication Date | 2016-07 |
Journal | Astronomy and Astrophysics |
Print ISSN | 2329-1273 |
Electronic ISSN | 2329-1265 |
Publisher | Hans Publishers |
Peer Reviewed | Peer Reviewed |
Volume | 591 |
Article Number | A55 |
DOI | https://doi.org/10.1051/0004-6361/201628250 |
Keywords | planetary systems |
Public URL | https://keele-repository.worktribe.com/output/405672 |
Publisher URL | https://doi.org/10.1051/0004-6361/201628250 |
Files
1602.01740v1.pdf
(1.3 Mb)
PDF
You might also like
Glancing through the debris disk: Photometric analysis of DE Boo with CHEOPS
(2023)
Journal Article
Limb darkening measurements from TESS and Kepler light curves of transiting exoplanets
(2023)
Journal Article
Connecting photometric and spectroscopic granulation signals with CHEOPS and ESPRESSO
(2023)
Journal Article