activity
20172019
most citedA physically motivated and empirically calibrated method to measure effective temperature, metallicity, and Ti abundance of M dwarfs

49 citations · 65 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.SR20199 cited

Magnetic Inflation and Stellar Mass. V. Intensification and saturation of M dwarf absorption lines with Rossby number

Philip S. Muirhead, Mark J. Veyette, Elisabeth R. Newton +2

In young sun-like stars and field M dwarf stars, chromospheric and coronal magnetic activity indicators such as H, X-ray and radio emission are known to saturate with low Rossby…

astro-ph.EP20197 cited

The Effects of Telluric Contamination in Iodine Calibrated Precise Radial Velocities

Sharon Xuesong Wang, Jason T. Wright, Chad Bender +4

We characterized the effects of telluric absorption lines on the radial velocity (RV) precision of stellar spectra taken through an iodine cell. To isolate the effects induced by t…

astro-ph.SR2018

Radii of 88 M Subdwarfs and Updated Radius Relations for Low-Metallicity M Dwarf Stars

Aurora Y. Kesseli, J. Davy Kirkpatrick, Sergio B. Fajardo-Acosta +9

M subdwarfs are low-metallicity M dwarfs that typically inhabit the halo population of the Galaxy. Metallicity controls the opacity of stellar atmospheres; in metal poor stars, hyd…

astro-ph.SR2018

Chemo-kinematic ages of eccentric-planet-hosting M dwarf stars

Mark J. Veyette, Philip S. Muirhead

M dwarf stars are exciting targets for exoplanet investigations; however, their fundamental stellar properties are difficult to measure. Perhaps the most challenging property to me…

astro-ph.SR201749 cited

A physically motivated and empirically calibrated method to measure effective temperature, metallicity, and Ti abundance of M dwarfs

Mark J. Veyette, Philip S. Muirhead, Andrew W. Mann +3

The ability to perform detailed chemical analysis of Sun-like F-, G-, and K-type stars is a powerful tool with many applications including studying the chemical evolution of the Ga…