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20122026
most citedESPRESSO@VLT -- On-sky performance and first results

537 citations · 11.3k across the 206 of their papers we have counts for

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Showing 2019Show all

19 papers · 1 filter

astro-ph.EP2019★ 75 cited

Wind of Change: retrieving exoplanet atmospheric winds from high-resolution spectroscopy

J. V. Seidel, D. Ehrenreich, L. Pino +5

Context. The atmosphere of exoplanets has been studied extensively in recent years, using numerical models to retrieve chemical composition, dynamical circulation or temperature fr…

astro-ph.EP2019★ 51 cited

The SOPHIE search for northern extrasolar planets. XVI. HD 158259: A compact planetary system in a near-3:2 mean motion resonance chain

N. C. Hara, F. Bouchy, M. Stalport +32

Since 2011, the SOPHIE spectrograph has been used to search for Neptunes and super-Earths in the Northern Hemisphere. As part of this observational program, 290 radial velocity mea…

astro-ph.EP2019★ 46 cited

WASP-52b. The effect of starspot correction on atmospheric retrievals

Giovanni Bruno, Nikole K. Lewis, Munazza K. Alam +13

We perform atmospheric retrievals on the full optical to infrared () transmission spectrum of the inflated hot Jupiter WASP-52b by combining HST/STIS, WFC3 IR…

astro-ph.EP2019★ 26 cited

Multi-season optical modulation phased with the orbit of the super-Earth 55 Cnc e

S. Sulis, D. Dragomir, M. Lendl +13

Context. 55 Cnc e is a transiting super-Earth orbiting a solar-like star with an orbital period of 17.7 hours. In 2011, using the MOST space telescope, a quasi-sinusoidal modulatio…

astro-ph.EP2019★ 81 cited

Optical phase curve of the ultra-hot Jupiter WASP-121b

V. Bourrier, D. Kitzmann, T. Kuntzer +28

We present the analysis of TESS optical photometry of WASP-121b, which reveal the phase curve of this transiting ultra-hot Jupiter. Its hotspot is located at the substellar point,…

astro-ph.SR2019★ 65 cited

The detection and characterisation of 54 massive companions with the SOPHIE spectrograph -- 7 new brown dwarfs and constraints on the BD desert

F. Kiefer, G. Hébrard, J. Sahlmann +35

Brown-dwarfs are substellar objects with masses intermediate between planets and stars within about 13-80Mjup. While isolated BDs are most likely produced by gravitational collapse…