activity
20152022
most citedThe Type II-Plateau Supernova 2017eaw in NGC 6946 and Its Red Supergiant Progenitor

84 citations · 779 across the 23 of their papers we have counts for

collaborators

43 papers

astro-ph.GA202281 cited

SpeX near-infrared spectroscopic extinction curves in the Milky Way

Marjorie Decleir, Karl D. Gordon, Jennifer E. Andrews +7

Interstellar dust extinction curves provide valuable information about dust properties, including the composition and size of the dust grains, and are essential to correct observat…

astro-ph.HE202224 cited

The Candidate Progenitor Companion Star of the Type Ib/c SN 2013ge

Ori D. Fox, Schuyler D. Van Dyk, Benjamin F. Williams +17

This Letter presents the detection of a source at the position of the Type Ib/c supernova (SN) 2013ge more than four years after the radioactive component is expected to have faded…

astro-ph.HE202232 cited

Infant-phase reddening by surface Fe-peak elements in a normal Type Ia Supernova

Yuan Qi Ni, Dae-Sik Moon, Maria R. Drout +41

Type Ia Supernovae are thermonuclear explosions of white dwarf stars. They play a central role in the chemical evolution of the Universe and are an important measure of cosmologica…

astro-ph.SR20224 cited

Massive stars dying alone: the remote environment of SN 2010jp and its associated late-time source

Austin Corgan, Nathan Smith, Jennifer E. Andrews +2

We present late-time images of the site of the peculiar jet-driven TypeIIn supernova SN2010jp, including HST images taken 2-5 yr post explosion and deep ground-based images over a…

astro-ph.HE20212 cited

Spitzer's Last Look at Extragalactic Explosions: Long-Term Evolution of Interacting Supernovae

Tamás Szalai, Ori D. Fox, Richard G. Arendt +10

Here we present new - and, nevertheless, last - mid-infrared (mid-IR) data for supernovae (SNe) based on measurements with the Spitzer Space Telescope. Comparing our recent 3.6 and…

astro-ph.HE2021

Enormous explosion energy of Type IIP SN 2017gmr with bipolar Ni-56 ejecta

V. P. Utrobin, N. N. Chugai, J. E. Andrews +7

The unusual Type IIP SN 2017gmr is revisited in order to pinpoint the origin of its anomalous features, including the peculiar light curve after about 100 days. The hydrodynamic mo…