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The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue
Aims. Pointed observations with XMM-Newton provide the basis for creating catalogues of X-ray sources detected serendipitously in each field. This paper describes the creation and characteristics ofExpand
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WASP-12b: The hottest transiting extrasolar planet yet discovered
TLDR
We report on the discovery of WASP-12b, a new transiting extrasolar planet with the largest radius of any transiting planet yet detected. Expand
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The WASP project and the superWASP cameras
TLDR
ABSTRACT The SuperWASP cameras are wide‐field imaging systems at the Observatorio del Roque de los Muchachos on the island of La Palma in the Canary Islands, and at the Sutherland Station of the South African Astronomical Observatory. Expand
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WASP-19b: The Shortest Period Transiting Exoplanet Yet Discovered
We report on the discovery of a new extremely short period transiting extrasolar planet, WASP-19b. The planet has mass M pl = 1.15 ± 0.08 MJ , radius R pl = 1.31 ± 0.06 RJ , and orbital period P =Expand
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An orbital period of 0.94 days for the hot-Jupiter planet WASP-18b
The ‘hot Jupiters’ that abound in lists of known extrasolar planets are thought to have formed far from their host stars, but migrate inwards through interactions with the proto-planetary disk fromExpand
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Line-profile tomography of exoplanet transits - II. A gas-giant planet transiting a rapidly rotating A5 star
TLDR
We use photometry and time-series spectroscopy to confirm the existence of a gas-giant planet with an orbital period of 1.22 d in orbit around HD 15082. Expand
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A high C/O ratio and weak thermal inversion in the atmosphere of exoplanet WASP-12b
The carbon-to-oxygen ratio (C/O) in a planet provides critical information about its primordial origins and subsequent evolution. A primordial C/O greater than 0.8 causes a carbide-dominatedExpand
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WASP-1b and WASP-2b: Two new transiting exoplanets detected with SuperWASP and SOPHIE
TLDR
We have detected low-amplitude radial-velocity variations in two stars, USNO-B1.0 1219‐ 0005465 (GSC 02265‐00107 = WASP‐1) and WASP-2.0 0964‐0543604, which are likely host stars of transiting exoplanets. Expand
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Stellar rotation in the Hyades and Praesepe: gyrochronology and braking time-scale
We present the results of photometric surveys for stellar rotation in the Hyades and in Praesepe, using data obtained as part of the SuperWASP exoplanetary transit-search programme. We determinedExpand
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On the orbit of exoplanet WASP-12b
TLDR
We observed two secondary eclipses of the exoplanet WASP-12b using the Infrared Array Camera on the Spitzer Space Telescope. Expand
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