activity
20192026
most citedThe Featureless Transmission Spectra of Two Super-Puff Planets

114 citations · 451 across the 41 of their papers we have counts for

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Showing 2022Show all

7 papers · 1 filter

astro-ph.EP2022★ 15 cited

NEID Reveals that The Young Warm Neptune TOI-2076 b Has a Low Obliquity

Robert C. Frazier, Gudmundur Stefansson, Suvrath Mahadevan +27

TOI-2076 b is a sub-Neptune-sized planet () that transits a young () bright () K-dwarf hosting a system of three transiting…

astro-ph.EP2022★ 50 cited

TOI-5205 b: A Short-period Jovian Planet Transiting a Mid-M Dwarf

Shubham Kanodia, Suvrath Mahadevan, Jessica Libby-Roberts +27

We present the discovery of TOI-5205~b, a transiting Jovian planet orbiting a solar metallicity M4V star, which was discovered using Transiting Exoplanet Survey Satellite photometr…

astro-ph.EP2022★ 14 cited

GJ 3929: High Precision Photometric and Doppler Characterization of an Exo-Venus and its Hot, Mini-Neptune-mass Companion

Corey Beard, Paul Robertson, Shubham Kanodia +31

We detail the follow up and characterization of a transiting exo-Venus identified by TESS, GJ 3929b, (TOI-2013b) and its non-transiting companion planet, GJ 3929c (TOI-2013c). GJ 3…

astro-ph.EP2022★ 8 cited

TOI-1696 and TOI-2136: Constraining the Masses of Two Mini-Neptunes with HPF

Corey Beard, Paul Robertson, Shubham Kanodia +29

We present the validation of two planets orbiting M dwarfs, TOI-1696b and TOI-2136b. Both planets are mini-Neptunes orbiting nearby stars, making them promising prospects for atmos…

astro-ph.EP2022

TOI-3757 b: A low density gas giant orbiting a solar-metallicity M dwarf

Shubham Kanodia, Jessica Libby-Roberts, Caleb I. Canas +32

We present the discovery of a new Jovian-sized planet, TOI-3757 b, the lowest density planet orbiting an M dwarf (M0V). It orbits a solar-metallicity M dwarf discovered using TESS…

astro-ph.SR2022★ 20 cited

Rotational modulation of spectroscopic Zeeman signatures in low-mass stars

Ryan C. Terrien, Allison Keen, Katy Oda +24

Accurate tracers of the stellar magnetic field and rotation are cornerstones for the study of M dwarfs and for reliable detection and characterization of their exoplanetary compani…