activity
20192026
most citedA detailed analysis of the Gl 486 planetary system

47 citations · 246 across the 26 of their papers we have counts for

collaborators
Showing 2024Show all

10 papers · 1 filter

astro-ph.EP2024

A Small Brown Dwarf in an Aligned Orbit around a Young, Fully-Convective M Star

M. Brady, J. Bean, G. Stefánsson +6

A star's spin-orbit angle can give us insight into a system's formation and dynamical history. In this paper, we use MAROON-X observations of the Rossiter-McLaughlin (RM) effect to…

astro-ph.EP2024

A Fourth Planet in the Kepler-51 System Revealed by Transit Timing Variations

Kento Masuda, Jessica E. Libby-Roberts, John H. Livingston +49

Kepler-51 is a -old Sun-like star hosting three transiting planets with radii - and orbital periods -$130\,\mathrm{day…

astro-ph.EP2024★ 4 cited

TOI-3568 b: a super-Neptune in the sub-Jovian desert

E. Martioli, R. P. Petrucci, E. Jofre +42

The sub-Jovian desert is a region in the mass-period and radius-period parameter space, typically encompassing short-period ranges between super-Earths and hot Jupiters, that exhib…

astro-ph.EP2024★ 13 cited

TESS Giants Transiting Giants. VI. Newly Discovered Hot Jupiters Provide Evidence for Efficient Obliquity Damping after the Main Sequence

Nicholas Saunders, Samuel K. Grunblatt, Ashley Chontos +53

The degree of alignment between a star's spin axis and the orbital plane of its planets (the stellar obliquity) is related to interesting and poorly understood processes that occur…

astro-ph.EP2024

An Earth-sized Planet on the Verge of Tidal Disruption

Fei Dai, Andrew W. Howard, Samuel Halverson +95

TOI-6255~b (GJ 4256) is an Earth-sized planet (1.079 ) with an orbital period of only 5.7 hours. With the newly commissioned Keck Planet Finder (KPF) and CARMEN…

astro-ph.EP2024★ 7 cited

The Aligned Orbit of a Hot Jupiter around the M Dwarf TOI-4201

Tianjun Gan, Sharon X. Wang, Fei Dai +12

Measuring the obliquities of stars hosting giant planets may shed light on the dynamical history of planetary systems. Significant efforts have been made to measure the obliquities…

astro-ph.EP2024★ 20 cited

HATS-38 b and WASP-139 b join a growing group of hot Neptunes on polar orbits

Juan I. Espinoza-Retamal, Guðmundur Stefánsson, Cristobal Petrovich +9

We constrain the sky-projected obliquities of two low-density hot Neptune planets, HATS-38 b and WASP-139 b, orbiting nearby G and K stars using Rossiter-McLaughlin (RM) observatio…

astro-ph.EP2024

Early Results from the HUMDRUM Survey: A Small, Earth-mass Planet Orbits TOI-1450A

M. Brady, J. Bean, A. Seifahrt +23

M dwarf stars provide us with an ideal opportunity to study nearby small planets. The HUMDRUM (HUnting for M Dwarf Rocky planets Using MAROON-X) survey uses the MAROON-X spectrogra…

astro-ph.EP2024★ 13 cited

The death of Vulcan: NEID reveals the planet candidate orbiting HD 26965 is stellar activity

Abigail Burrows, Samuel Halverson, Jared C. Siegel +17

We revisit the long-studied radial velocity (RV) target HD26965 using recent observations from the NASA-NSF 'NEID' precision Doppler facility. Leveraging a suite of classical activ…

astro-ph.EP2024★ 29 cited

Searching for Giant Exoplanets around M-dwarf Stars (GEMS) I: Survey Motivation

Shubham Kanodia, Caleb I. Cañas, Suvrath Mahadevan +13

Recent discoveries of transiting giant exoplanets around M-dwarf stars (GEMS), aided by the all-sky coverage of TESS, are starting to stretch theories of planet formation through t…