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20112025
most citedSOPHIE velocimetry of Kepler transit candidates XVII. The physical properties of giant exoplanets within 400 days of period

273 citations · 1.3k across the 36 of their papers we have counts for

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astro-ph.EP2025★ 5 cited

The star HIP 41378 potentially misaligned with its cohort of long-period planets

S. Grouffal, A. Santerne, V. Bourrier +29

The obliquity between the stellar spin axis and the planetary orbit, detected via the Rossiter-McLaughlin (RM) effect, is a tracer of the formation history of planetary systems. Wh…

astro-ph.EP2025★ 1 cited

A Swarm of WASP Planets: Nine giant planets identified by the WASP survey

Nicole Schanche, Guillaume Hébrard, Keivan G. Stassun +52

The Wide Angle Search for Planets (WASP) survey provided some of the first transiting hot Jupiter candidates. With the addition of the Transiting Exoplanet Survey Satellite (TESS),…

astro-ph.EP2020★ 6 cited

A dayside thermal inversion in the atmosphere of WASP-19b

A. S. Rajpurohit, F. Allard, D. Homeier +2

Observations of ultra-hot Jupiters indicate the existence of thermal inversion in their atmospheres with day-side temperatures greater than 2200 K. Various physical mechanisms such…

astro-ph.EP2016★ 32 cited

EPIC211089792 b: an aligned and inflated hot jupiter in a young visual binary

A. Santerne, G. Hébrard, J. Lillo-Box +71

In the present paper we report the discovery of a new hot Jupiter, EPIC211089792 b, first detected by the Super-WASP observatory and then by the K2 space mission during its campaig…

astro-ph.EP2016★ 12 cited

K2-30b and K2-34b: two inflated hot-Jupiters around Solar-type stars

J. Lillo-Box, O. Demangeon, A. Santerne +23

We report the discovery of the two hot-Jupiters K2-30b and K2-34b. The two planets were detected transiting their main-sequence star with periods 4.099 and 2.996 days…

astro-ph.EP2015★ 273 cited

SOPHIE velocimetry of Kepler transit candidates XVII. The physical properties of giant exoplanets within 400 days of period

A. Santerne, C. Moutou, M. Tsantaki +19

While giant extrasolar planets have been studied for more than two decades now, there are still some open questions such as their dominant formation and migration process, as well…