activity
19982023
most citedThe prevalence of dust on the exoplanet HD 189733b from Hubble and Spitzer observations

440 citations · 958 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2023★ 10 cited

EI Eridani: a star under the influence -- The effect of magnetic activity in the short and long term

L. Kriskovics, Zs. Kővári, B. Seli +5

We use our photometric time series of more than forty years to analyze the long-term behaviour of EI Eri. Flare activity is investigated using space-borne photometric data obtained…

astro-ph.EP2023★ 7 cited

The Hubble PanCET program: The near-ultraviolet transmission spectrum of WASP-79b

A. Gressier, A. Lecavelier des Etangs, D. K. Sing +11

We present Hubble Space Telescope (HST) transit observations of the Hot-Jupiter WASP-79b acquired with the Space Telescope Imaging Spectrograph (STIS) in the near ultraviolet (NUV)…

astro-ph.EP2023★ 73 cited

DREAM I. Orbital architecture orrery

V. Bourrier, O. Attia, M. Mallonn +28

The distribution of close-in exoplanets is shaped by a complex interplay between atmospheric and dynamical processes. The Desert-Rim Exoplanets Atmosphere and Migration (DREAM) pro…

astro-ph.EP2022★ 35 cited

The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc

R. Luque, B. J. Fulton, M. Kunimoto +64

We report the discovery of a multi-planetary system transiting the M0 V dwarf HD 260655 (GJ 239, TOI-4599). The system consists of at least two transiting planets, namely HD 260655…

astro-ph.SR2021★ 5 cited

Automated photometry of Cassiopeiae:the last roundup

Myron A. Smith, G. W. Henry

Gamma Cas (B0.5IVe) is the noted prototype of a subgroup of classical Be stars exhibiting hard thermal X-ray emission. This paper reports results from a 23-year optical campaign wi…

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…