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20042026
most citedThe PLATO 2.0 Mission

1.3k citations · 9.1k across the 85 of their papers we have counts for

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Showing 2011 · astro-ph.EPShow all

6 papers · 2 filters

astro-ph.EP2011★ 50 cited

High precision transit observations of the exoplanet WASP-13b with the RISE instrument

S. C. C. Barros, D. L. Pollacco, N. P. Gibson +3

WASP-13b is a sub-Jupiter mass exoplanet orbiting a G1V type star with a period of 4.35 days. The current uncertainty in its impact parameter (0 < b < 0.46) resulted in poorly defi…

astro-ph.EP2011★ 44 cited

A lower mass for the exoplanet WASP-21b

S. C. C. Barros, D. L. Pollacco, N. P. Gibson +6

We present high precision transit observations of the exoplanet WASP-21b, obtained with the RISE instrument mounted on 2.0m Liverpool Telescope. A transit model is fitted, coupled…

astro-ph.EP2011★ 84 cited

WASP-35b, WASP-48b and WASP-51b: Two new planets and an independent discovery of HAT-P-30b

B. Enoch, D. R. Anderson, S. C. C. Barros +36

We report the detection of WASP-35b, a planet transiting a metal-poor ([Fe/H] = -0.15) star in the Southern hemisphere, WASP-48b, an inflated planet which may have spun-up its slig…

astro-ph.EP2011★ 129 cited

WASP-39b: a highly inflated Saturn-mass planet orbiting a late G-type star

F. Faedi, S. C. C. Barros, D. R. Anderson +30

We present the discovery of WASP-39b, a highly inflated transiting Saturn-mass planet orbiting a late G-type dwarf star with a period of \,d, Transit Epoch T…

astro-ph.EP2011★ 25 cited

WASP-40b: independent discovery of the 0.6-Mjup transiting exoplanet HAT-P-27b

D. R. Anderson, S. C. C. Barros, I. Boisse +23

From WASP photometry and SOPHIE radial velocities we report the discovery of WASP-40b (HAT-P-27b), a 0.6 Mjup planet that transits its 12th magnitude host star every 3.04 days. The…

astro-ph.EP2011★ 58 cited

Thermal emission from WASP-33b, the hottest known planet

A. M. S. Smith, D. R. Anderson, I. Skillen +2

We report ground-based observations at 0.91 microns of the occultation of the hot Jupiter WASP-33b by its A5 host star. We measure the planet to be 0.109 +/- 0.030 per cent as brig…