activity
20182022
most citedSPECULOOS Northern Observatory: searching for red worlds in the northern skies

33 citations · 87 across the 6 of their papers we have counts for

collaborators

8 papers

astro-ph.IM202233 cited

SPECULOOS Northern Observatory: searching for red worlds in the northern skies

Artem Y. Burdanov, Julien de Wit, Michaël Gillon +14

SPECULOOS is a ground-based transit survey consisting of six identical 1-m robotic telescopes. The immediate goal of the project is to detect temperate terrestrial planets transiti…

astro-ph.SR202228 cited

A Study of Flares in the Ultra-Cool Regime from SPECULOOS-South

C. A. Murray, D. Queloz, M. Gillon +22

We present a study of photometric flares on 154 low-mass () objects observed by the SPECULOOS-South Observatory from 1st June 2018 to 23rd March 2020.…

astro-ph.EP2021

A large sub-Neptune transiting the thick-disk M4V TOI-2406

R. D. Wells, B. V. Rackham, N. Schanche +71

Large sub-Neptunes are uncommon around the coolest stars in the Galaxy and are rarer still around those that are metal-poor. However, owing to the large planet-to-star radius ratio…

astro-ph.EP202010 cited

Strong H emission in the young planetary mass companion 2MASS J0249-0557 c

P. Chinchilla, V. J. S. Béjar, N. Lodieu +2

Aims: Our objective is the optical and near-infrared spectroscopic characterisation of 2MASS J0249-0557 c, a recently discovered young planetary mass companion to the Pictoris…

astro-ph.SR2020

Two close binaries across the hydrogen-burning limit in the Praesepe open cluster

N. Lodieu, C. del Burgo, E. Manjavacas +7

We present Keck I/OSIRIS and Keck II/NIRC2 adaptive optics imaging of two member candidates of the Praesepe stellar cluster (d=186.180.11 pc; 590-790 Myr), UGC J08451066+21481…

astro-ph.EP201916 cited

USco1621 B and USco1556 B: Two wide companions at the deuterium-burning mass limit in Upper Scorpius

Patricia Chinchilla, Víctor J. S. Béjar, Nicolas Lodieu +6

(Abridged) Our aim is to identify analogues of gas giant planets, as companions at wide separations of very young stars. To identify these objects, we cross correlated the Visible…