activity
20222026
most citedThe EBLM project X. Benchmark masses, radii and temperatures for two fully convective M-dwarfs using K2

15 citations · 20 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2026

A Sample of Thick-Disk Stars Hosting Hot Jupiters

Victoria DiTomasso, Samuel W. Yee, Romy Rodriguez Martinez +6

We present a homogeneous analysis of 268 confirmed and candidate transiting hot-Jupiter host stars with 4800K < Teff < 6200K. We combine high-resolution TRES spectra, Gaia, 2MASS a…

astro-ph.EP2025

Identifying Flare Locations Through Exoplanet Transit Occultations

Tayt Armitage, David V. Martin, Romy Rodríguez Martínez

M dwarfs are the most common stars in the galaxy, with long lifespans, a high occurrence rate of rocky planets, and close-in habitable zones. However, high stellar activity in the…

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.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…