activity
20042026
most citedDetection of Thermal Emission from an Extrasolar Planet

655 citations · 4.8k across the 65 of their papers we have counts for

collaborators
Showing 2018Show all

8 papers · 1 filter

astro-ph.EP2018★ 22 cited

Detection and characterization of an ultra-dense sub-Neptune planet orbiting the Sun-like star HD 119130

R. Luque, G. Nowak, E. Pallé +51

We present the discovery and characterization of a new transiting planet from Campaign 17 of the Kepler extended mission K2. HD 119130 b is a warm sub-Neptune on a 17-d orbit aroun…

astro-ph.EP2018★ 3 cited

The role of host star variability in the detectability of planetary phase curves

Diego Hidalgo, Roi Alonso, Enric Palle

Phase curves, or the change in observed illumination of the planet as it orbits around its host star, help us to characterize their atmospheres. However, the variability of the hos…

astro-ph.EP2018★ 27 cited

Detection and Doppler monitoring of EPIC 246471491, a system of four transiting planets smaller than Neptune

E. Palle, G. Nowak, R. Luque +43

The Kepler extended mission, also known as K2, has provided the community with a wealth of planetary candidates that orbit stars typically much brighter than the targets of the ori…

astro-ph.EP2018★ 14 cited

A 4.6-year period brown-dwarf companion interacting with the hot-Jupiter CoRoT-20 b

J. Rey, F. Bouchy, M. Stalport +18

We report the discovery of an additional substellar companion in the CoRoT-20 system based on six years of HARPS and SOPHIE radial velocity follow-up. CoRoT-20 c has a minimum mass…

astro-ph.IM2018★ 19 cited

SPECULOOS: a network of robotic telescopes to hunt for terrestrial planets around the nearest ultracool dwarfs

Laetitia Delrez, Michael Gillon, Didier Queloz +18

We present here SPECULOOS, a new exoplanet transit search based on a network of 1m-class robotic telescopes targeting the 1200 ultracool (spectral type M7 and later) dwarfs b…

astro-ph.EP2018★ 22 cited

Characterization of Exoplanets: Secondary Eclipses

Roi Alonso

When an exoplanet passes behind its host star, we can measure the time of the occultation, its depth, and its color. In this chapter we describe how these observables can be used t…