output
20032026
most citedSwift and NuSTAR observations of GW170817: detection of a blue kilonova

579 citations

Showing astro-ph.EPShow all

8 papers · 1 filter

astro-ph.EP2026

Searching for GEMS: Three warm Saturns and a super-Jupiter orbiting four early M-dwarfs

Pranav H. Premnath, Paul Robertson, Shubham Kanodia +33

We report the confirmation and characterization of four transiting giant planets orbiting early-M dwarfs discovered by the Searching for Giant Exoplanets around M-dwarf Stars (GEMS…

astro-ph.EP20257 cited

The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems

Mark R. Giovinazzi, Cullen H. Blake, Paul Robertson +26

We present a set of companion dynamical masses and orbital parameters of seven star systems from the NEID Earth Twin Survey with significant absolute astrometric accelerations betw…

astro-ph.EP20243 cited

gaspery: Optimized Scheduling of Radial Velocity Follow-Up Observations for Active Host Stars

Christopher Lam, Megan Bedell, Lily L. Zhao +2

Radial velocity (RV) follow-up is a critical complement of transiting exoplanet surveys like the Transiting Exoplanet Survey Satellite (TESS ), both for validating discoveries of e…

astro-ph.EP20247 cited

A Gap in the Densities of Small Planets Orbiting M Dwarfs: Rigorous Statistical Confirmation Using the Open-source Code RhoPop

J. G. Schulze, Ji Wang, J. A. Johnson +4

Using mass-radius-composition models, small planets () are typically classified into three types: iron-rich, nominally Earth-like, and those…

astro-ph.EP202229 cited

Large-scale cryovolcanic resurfacing on Pluto

Kelsi N. Singer, Oliver L. White, Bernard Schmitt +22

The New Horizons spacecraft returned images and compositional data showing that terrains on Pluto span a variety of ages, ranging from relatively ancient, heavily cratered areas to…

astro-ph.EP202145 cited

TOI-431/HIP 26013: a super-Earth and a sub-Neptune transiting a bright, early K dwarf, with a third RV planet

Ares Osborn, David J. Armstrong, Bryson Cale +125

We present the bright (V), multi-planet system TOI-431, characterised with photometry and radial velocities. We estimate the stellar rotation period to be $30.5 \pm…