activity
20142024
most citedSodium and Oxygen Abundances in the Open Cluster NGC 6791 from APOGEE H-Band Spectroscopy

78 citations · 171 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR20247 cited

Quiet Please: Detrending Radial Velocity Variations from Stellar Activity with a Physically Motivated Spot Model

Jared C. Siegel, Samuel Halverson, Jacob K. Luhn +15

For solar-type stars, spots and their associated magnetic regions induce radial velocity perturbations through the Doppler rotation signal and the suppression of convective blueshi…

astro-ph.IM202318 cited

Stable fiber-illumination for extremely precise radial velocities with NEID

Shubham Kanodia, Andrea S. J. Lin, Emily Lubar +24

NEID is a high-resolution red-optical precision radial velocity (RV) spectrograph recently commissioned at the WIYN 3.5 m telescope at Kitt Peak National Observatory, Arizona, USA.…

astro-ph.SR20237 cited

TOI-5375 B: A Very Low Mass Star at the Hydrogen-Burning Limit Orbiting an Early M-type Star

Mika Lambert, Chad F. Bender, Shubham Kanodia +16

The TESS mission detected a companion orbiting TIC 71268730, categorized it as a planet candidate, and designated the system TOI-5375. Our follow-up analysis using radial velocity…

astro-ph.EP20231 cited

An extreme test case for planet formation: a close-in Neptune orbiting an ultracool star

Gudmundur Stefansson, Suvrath Mahadevan, Yamila Miguel +27

In current theories of planet formation, close-orbiting planets as massive as Neptune are expected to be very rare around low-mass stars. We report the discovery of a Neptune-mass…

astro-ph.SR20233 cited

Characterization of low-mass companions to objects of interest observed with APOGEE-N

Caleb I. Cañas, Chad F. Bender, Suvrath Mahadevan +12

We report the characterization of 28 low-mass () companions to objects of interest (KOIs), eight…

astro-ph.EP202111 cited

A hot Mars-sized exoplanet transiting an M dwarf

Caleb I. Cañas, Suvrath Mahadevan, William D. Cochran +21

We validate the planetary nature of an ultra-short period planet orbiting the M dwarf KOI-4777. We use a combination of space-based photometry from Kepler, high-precision, near-inf…