activity
20202026
most citedSPECULOOS -- Ultracool Dwarf Transit Survey: Target List and Strategy

106 citations · 959 across the 54 of their papers we have counts for

collaborators
Showing 2021Show all

13 papers · 1 filter

astro-ph.EP2021★ 32 cited

BEBOP III. Observations and an independent mass measurement of Kepler-16 (AB) b -- the first circumbinary planet detected with radial velocities

Amaury H. M. J. Triaud, Matthew R. Standing, Neda Heidari +30

The radial velocity method is amongst the most robust and most established means of detecting exoplanets. Yet, it has so far failed to detect circumbinary planets despite their rel…

astro-ph.EP2021

BEBOP II: Sensitivity to sub-Saturn circumbinary planets using radial-velocities

Matthew R. Standing, Amaury H. M. J. Triaud, João P. Faria +14

BEBOP is a radial-velocity survey that monitors a sample of single-lined eclipsing binaries, in search of circumbinary planets by using high-resolution spectrographs. Here, we desc…

astro-ph.EP2021

TOI-712: a system of adolescent mini-Neptunes extending to the habitable zone

Sydney Vach, Samuel N. Quinn, Andrew Vanderburg +40

As an all-sky survey, NASA's mission is able to detect the brightest and rarest types of transiting planetary systems, including young planets that enable study of the evolu…

astro-ph.EP2021★ 1 cited

TOI-3362b: A Proto-Hot Jupiter Undergoing High-Eccentricity Tidal Migration

Jiayin Dong, Chelsea X. Huang, George Zhou +39

High-eccentricity tidal migration is a possible way for giant planets to be emplaced in short-period orbits. If it commonly operates, one would expect to catch proto-Hot Jupiters o…

astro-ph.SR2021★ 15 cited

NGTS clusters survey -- III: A low-mass eclipsing binary in the Blanco 1 open cluster spanning the fully convective boundary

Gareth D. Smith, Edward Gillen, Didier Queloz +27

We present the discovery and characterisation of an eclipsing binary identified by the Next Generation Transit Survey in the 115 Myr old Blanco 1 open cluster. NGTS J0002-29…

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…