activity
20142023
most citedPlanets Transiting Non-Eclipsing Binaries

118 citations · 1.1k across the 31 of their papers we have counts for

collaborators

31 papers

astro-ph.EP2023

A Non-Transiting Coplanar Circumbinary Planet Around Kepler-1660AB

Max Goldberg, Daniel Fabrycky, David V. Martin +3

Over a dozen transiting circumbinary planets have been discovered around eclipsing binaries. Transit detections are biased towards aligned planet and binary orbits, and indeed all…

astro-ph.SR2023★ 5 cited

The Benchmark M Dwarf Eclipsing Binary CM Draconis With TESS: Spots, Flares and Ultra-Precise Parameters

David V. Martin, Ritika Sethi, Tayt Armitage +3

A gold standard for the study of M dwarfs is the eclipsing binary CM Draconis. It is rare because it is bright () and contains twin fully convective stars on an al…

astro-ph.EP2023★ 62 cited

Radial-velocity discovery of a second planet in the TOI-1338/BEBOP-1 circumbinary system

Matthew R. Standing, Lalitha Sairam, David V. Martin +24

We report the detection of a gas-giant planet in orbit around both stars of an eclipsing binary star system that also contains the smaller, inner transiting planet TOI-1338b. The n…

astro-ph.SR2022

Revised Temperatures For Two Benchmark M-dwarfs -- Outliers No More

David V. Martin, Tayt Armitage, Alison Duck +7

Well-characterised M-dwarfs are rare, particularly with respect to effective temperature. In this letter we re-analyse two benchmark M-dwarfs in eclipsing binaries from Kepler/K2:…

astro-ph.SR2022★ 15 cited

The EBLM project X. Benchmark masses, radii and temperatures for two fully convective M-dwarfs using K2

Alison Duck, David V. Martin, Sam Gill +23

M-dwarfs are the most abundant stars in the galaxy and popular targets for exoplanet searches. However, their intrinsic faintness and complex spectra inhibit precise characterisati…

astro-ph.EP2022★ 3 cited

Spectroscopy of TOI-1259B -- an unpolluted white dwarf companion to an inflated warm Saturn

Evan Fitzmaurice, David V. Martin, Romy Rodriguez Martinez +7

TOI-1259 consists of a transiting exoplanet orbiting a main sequence star, with a bound outer white dwarf companion. Less than a dozen systems with this architecture are known. We…