activity
20182026
most citedPhotometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the 2 Observations

85 citations · 300 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.HE2026★ 1 cited

TDE 2025abcr: A Tidal Disruption Event in the Outskirts of a Massive Galaxy

Robert Stein, Jonathan Carney, Charlotte Ward +27

Tidal disruption events (TDEs) have traditionally been discovered in optical sky surveys through targeted searches of nuclear transients. However, it is expected that some TDEs wil…

astro-ph.HE2026★ 4 cited

AT2024wpp: An Extremely Luminous Fast Ultraviolet Transient Powered by Accretion onto a Black Hole

Daniel A. Perley, Anna Y. Q. Ho, Zoë McGrath +69

We present the discovery of AT 2024wpp ("Whippet"), a fast and luminous 18cow-like transient. At a redshift of z=0.0868, revealed by Keck Cosmic Web Imager spectroscopy of its fain…

astro-ph.EP2024

The Origins of Lithium Enhancement in Polluted White Dwarfs

Benjamin C. Kaiser, J. Christopher Clemens, Simon Blouin +4

The bulk abundances of exoplanetesimals can be measured when they are accreted by white dwarfs. Recently, lithium from the accretion of exoplanetesimals was detected in relatively…

astro-ph.SR2024

Using 3.4-m Variability towards White Dwarfs as a Signpost of Remnant Planetary Systems

Joseph A. Guidry, J. J. Hermes, Kishalay De +3

Roughly 2% of white dwarfs harbor planetary debris disks detectable via infrared excesses, but only a few percent of these disks show a gaseous component, distinguished by their do…

astro-ph.SR2024

A Test of Spectroscopic Age Estimates of White Dwarfs using Wide WD+WD Binaries

Tyler M. Heintz, J. J. Hermes, P. -E. Tremblay +4

White dwarf stars have been used for decades as precise and accurate age indicators. This work presents a test of the reliability of white dwarf total ages when spectroscopic obser…

astro-ph.SR2023

TIC 378898110: A Bright, Short-Period AM CVn Binary in TESS

Matthew J. Green, J. J. Hermes, Brad N. Barlow +22

AM CVn-type systems are ultracompact, helium-accreting binary systems which are evolutionarily linked to the progenitors of thermonuclear supernovae and are expected to be strong G…