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19972023
most citedWASP-12b: The hottest transiting planet yet discovered

399 citations · 3.4k across the 51 of their papers we have counts for

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astro-ph2009★ 399 cited

WASP-12b: The hottest transiting planet yet discovered

L. Hebb, A. Collier-Cameron, B. Loeillet +15

We report on the discovery of WASP-12b, a new transiting extrasolar planet with and . The planet and host star propertie…

astro-ph2008★ 75 cited

Updated parameters for the transiting exoplanet WASP-3b using RISE, a new fast camera for the Liverpool Telescope

N. P. Gibson, D. Pollacco, E. K. Simpson +9

Some of the first results are reported from RISE - a new fast camera mounted on the Liverpool Telescope primarily designed to obtain high time resolution light curves of transiting…

astro-ph2008★ 22 cited

Use of neural networks for the identification of new z>=3.6 QSOs from FIRST-SDSS DR5

R. Carballo, J. I. Gonzalez-Serrano, C. R. Benn +1

We aim to obtain a complete sample of redshift > 3.6 radio QSOs from FIRST sources having star-like counterparts in the SDSS DR5 photometric survey (r<=20.2). We found that simple…

astro-ph2008★ 64 cited

Physical Conditions in Quasar Outflows: VLT Observations of QSO 2359-1241

Kirk Korista, Manuel Bautista, Nahum Arav +3

We analyze the physical conditions of the outflow seen in QSO 2359-1241 (NVSS J235953-124148), based on high resolution spectroscopic VLT observations. This object was previously s…

astro-ph2008★ 13 cited

Searching for transit timing variations in transiting exoplanet systems

Marie Hrudková, Ian Skillen, Chris Benn +5

Searching for transit timing variations in the known transiting exoplanet systems can reveal the presence of other bodies in the system. Here we report such searches for two transi…

astro-ph2008★ 91 cited

Measuring Column Densities in Quasar Outflows: VLT Observations of QSO 2359-1241

Nahum Arav, Maxwell Moe, Elisa Costantini +3

We present high resolution spectroscopic VLT observations of the outflow seen in QSO 2359-1241. These data contain absorption troughs from five resonance Fe II lines with a resolut…