The Hot Jupiter WASP-12b
Early UV ingress in WASP 12b: measuring planetary magnetic fields
... 5. CONCLUSION Motivated by the recent observation on the light curve asymmetry of the transit hot-Jupiter WASP-12b (Fossati et al. 2010a), we proposed a model where the interaction of the ...
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WASP 190b : tomographic discovery of a transiting hot Jupiter
... most hot Jupiters will settle into a circular orbit on a shorter timescale than their lifetimes ( Pont et ...days, WASP-190b is entering the regime where eccentricity may ...
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WASP 157b, a transiting hot jupiter observed with K2
... al. WASP-South is hosted by the South African Astronom- ical Observatory and SuperWASP-North by the Isaac Newton Group of Telescopes and the Instituto de As- trofisica de ...
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From dense hot Jupiter to low density Neptune : the discovery of WASP 127b, WASP 136b, and WASP 138b
... of WASP-136 and ...of WASP-136 and WASP-138 are ...of WASP-127 is too low for a sensible ...of WASP-136 and WASP-138, which may have arisen as a result of tidal interac- ...
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WASP 20b and WASP 28b : a hot Saturn and a hot Jupiter in near aligned orbits around solar type stars
... of WASP-20: 12 m s −1 for the CORALIE RVs and 7 m s − 1 for the HARPS RVs; no jitter was required for ...of WASP-20 into two sets: those taken on the night of the spectroscopic transit obser- vation of 2009 ...
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WASP 77 Ab: A Transiting Hot Jupiter Planet in a Wide Binary System
... The WASP light curves show a weak, periodic modulation with an amplitude of about ...in WASP-77 A caused by starspots modulating the apparent brightness as the star ...rotates. WASP-77 B may ...
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The well aligned orbit of Wasp 84b : evidence for disk migration of a hot Jupiter
... misaligned and that tides changed the initial distribution either by realigning the orbits or by destroying misaligned planets. 6.1. Giant-planet migration As tides become ineffective with suf fi cient distance from the ...
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WASP 94 A and B planets : hot Jupiter cousins in a twin star system
... discussions. WASP-South is hosted by the South African Astronomical Observatory and we are grateful for their ongoing sup- port and ...for WASP comes from consortium universities and from the UK’s Science ...
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WASP 135b : a highly irradiated, inflated hot Jupiter orbiting a G5V star
... This age discrepancy could be evidence of tidal spin-up of the star, due to its massive, short period planet. On the other hand, lithium is detected in the stellar spectrum, and the age estimate of 0.60 +1.40 −0.35 Gyr ...
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KELT-14b and KELT-15b: an independent discovery of WASP-122b and a new hot Jupiter
... a hot Jupiter provide a direct measurement of thermal emission from the planet ʼs dayside and allow constraints on the connection between the atmospheric structure and climate and irradiation from the host ...
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WASP 180Ab : Doppler tomography of an hot Jupiter orbiting the primary star in a visual binary
... of WASP-180Ab, a hot Jupiter confirmed by the detection of its Doppler shadow and by measuring its mass using radial ...light. WASP-180Ab therefore adds to a small sample of transiting ...
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WASP 121 b : a hot Jupiter close to tidal disruption transiting an active F star
... the WASP-South survey of WASP-121 b, a new remarkable short-period transiting hot ...of WASP-121 b is that its orbital semimajor axis is only ...
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WASP 167b/KELT 13b : joint discovery of a hot Jupiter transiting a rapidly rotating F1V star
... in WASP-118. We have looked for the pulsations in the WASP and KELT photometry, but do not detect any signal, with an upper limit of ...the WASP data are not par- ticularly suitable for searching for ...
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WASP South hot Jupiters : WASP 178b, WASP 184b, WASP 185b & WASP 192b
... of hot Jupiters and bloated radii is now well established ...2018). WASP-178b is at the upper end of such a relationship, as illustrated for known planets in ...hottest hot Jupiters to be more ...
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WASP 71b : a bloated hot Jupiter in a 2 9 day, prograde orbit around an evolved F8 star
... the WASP transit survey of a highly-irradiated, massive ...planet, WASP-71b, is larger than Jupiter ...confidence. WASP-71, with an effective temperature of 6059 ± 98 K, therefore fits the ...
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Defocused transmission spectroscopy: a potential detection of sodium in the atmosphere of WASP-12b
... The typical precision required to detect an exoplanet at- mosphere is of the order of ∼ 0.1%. Due to the systematics associated with ground-based observations, the technique of transmission spectroscopy provides a unique ...
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Three irradiated and bloated hot Jupiters: WASP 76b, WASP 82b, and WASP 90b
... transiting hot Jupiter planets, discovered from the WASP surveys, which we combine with radial velocities from OHP/SOPHIE and Euler/CORALIE and photometry from Euler and ...planets WASP-76b, ...
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Thermal emission at 3 6 8 μm from WASP 19b: a hot Jupiter without a stratosphere orbiting an active star
... We considered whether stellar variability could have affected our measured occultation depths. One potential issue is that the stellar brightness may have varied significantly during one or more of the observations. ...
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Optical transmission spectroscopy of hot Jupiter atmospheres
... Similar to HAT-P-18b, the atmosphere of WASP-80b favoured a Rayleigh scattering slope over a flat transmission spectrum, although it did not provide a good fit to the entire data set (Ch[r] ...
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WASP 169, WASP 171, WASP 175 and WASP 182 : three hot Jupiters and one bloated sub Saturn mass planet discovered by WASP south
... WASP-171b is found to have a mass of 1.0841 ± 0.094 M Jup and radius 0.98 +0.07 − 0.04 R Jup , fitting the characteristics of a fairly typical hot Jupiter. The orbital period is 3.82 d, making it the ...
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