activity
20172022
most citedThe EBLM Project IV. Spectroscopic orbits of over 100 eclipsing M dwarfs masquerading as transiting hot-Jupiters

98 citations · 277 across the 9 of their papers we have counts for

collaborators

8 papers

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.EP202221 cited

TESS discovery of a sub-Neptune orbiting a mid-M dwarf TOI-2136

Tianjun Gan, Abderahmane Soubkiou, Sharon X. Wang +60

We present the discovery of TOI-2136b, a sub-Neptune planet transiting every 7.85 days a nearby M4.5V-type star, identified through photometric measurements from the TESS mission.…

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.EP20196 cited

Gemini-GRACES high-quality spectra of Kepler evolved stars with transiting planets I. Detailed characterization of multi-planet systems Kepler-278 and Kepler-391

E. Jofré, J. M. Almenara, R. Petrucci +10

(abridged) Kepler-278 and Kepler-391 are two of the three evolved stars known to date on the RGB to host multiple short-period transiting planets. Moreover, these planets are among…

astro-ph.SR20197 cited

Fundamental properties of the pre-main sequence eclipsing stars of MML 53 and the mass of the tertiary

Y. Gómez Maqueo Chew, L. Hebb, H. C. Stempels +7

We present the most comprehensive analysis to date of the Upper Centaurus Lupus eclipsing binary MML 53 (2.097892 d), and for the first time, confirm the bound-nature of the third…

astro-ph.GA2018

Massive stars in the SDSS-IV/APOGEE SURVEY. I- OB stars

A. Roman-Lopes, C. RomÁn-ZÚÑiga, Mauricio Tapia +10

In this work we make use of DR14 APOGEE spectroscopic data to study a sample of 92 known OB stars. We developed a near-infrared semi-empirical spectral classification method that w…