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Mocnik, T ORCID: https://orcid.org/0000-0003-4603-556X, Anderson, DR, Brown, DJA, Collier Cameron, A, Delrez, L, Gillon, M, Hellier, C
ORCID: https://orcid.org/0000-0002-3439-1439, Jehin, E, Lendl, M, Maxted, PFL
ORCID: https://orcid.org/0000-0003-3794-1317, Neveu-VanMalle, M, Pepe, F, Pollacco, D, Queloz, D, Segransan, D, Smalley, B
ORCID: https://orcid.org/0000-0002-3456-087X, Taylor, J, Triaud, AHMJ, Udry, S and West, RG
(2016)
WASP-157b, a Transiting Hot Jupiter Observed with K2.
Publications of the Astronomical Society of the Pacific, 128 (970).
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teo_1603.05638v2-1.pdf - Accepted Version Available under License Creative Commons Attribution Non-commercial. Download (619kB) | Preview |
Abstract
We announce the discovery of the transiting hot Jupiter WASP-157b in a 3.95-d orbit around a V = 12.9 G2 main-sequence star. This moderately inflated planet has a Saturn-like density, with a mass of 0.57 ± 0.10 MJup and a radius of 1.06 ± 0.05 RJup. We do not detect any rotational or phase curve modulations, nor the secondary eclipse, with conservative semi-amplitude upper limits of 250 and 20 ppm, respectively.
Item Type: | Article |
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Additional Information: | © 2016 IOP Publishing, The Authors. This is the accepted author manuscript (AAM). The published version (Močnik, T. et al., 2016. WASP-157b, a Transiting Hot Jupiter Observed with K2. Publications of the Astronomical Society of the Pacific, 128(970), p.124403) is available online via IOP Publishing at http://dx.doi.org/10.1088/1538-3873/128/970/124403. Please refer to any applicable terms of use of the publisher. |
Uncontrolled Keywords: | astrophysics, astronomy, physics |
Subjects: | Q Science > QB Astronomy Q Science > QC Physics |
Divisions: | Faculty of Natural Sciences > School of Physical and Geographical Sciences |
Depositing User: | Symplectic |
Date Deposited: | 23 Nov 2016 09:31 |
Last Modified: | 08 Apr 2019 09:02 |
URI: | https://eprints.keele.ac.uk/id/eprint/2480 |
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