activity
20042023
most citedThe Man Behind the Curtain: X-rays Drive the UV through NIR Variability in the 2013 AGN Outburst in NGC 2617

1.9k citations · 16.7k across the 175 of their papers we have counts for

collaborators

171 papers

astro-ph.SR2023★ 7 cited

Very late-time spectroscopy of SN 2009ip: Constraints on the ongoing H emission

Thallis Pessi, Jose L. Prieto, Luc Dessart

The peculiar supernova (SN) 2009ip is an ambiguous event that spurred many questions regarding its true origins. Here, we present very late-time spectroscopic and photometric obser…

astro-ph.HE2023★ 1 cited

Environmental dependence of Type IIn supernova properties

Takashi J. Moriya, Lluis Galbany, Cristina Jimenez-Palau +9

Type IIn supernovae occur when stellar explosions are surrounded by dense hydrogen-rich circumstellar matter. The dense circumstellar matter is likely formed by extreme mass loss f…

astro-ph.SR2023★ 14 cited

A metallicity dependence on the occurrence of core-collapse supernovae

Thallis Pessi, Joseph P. Anderson, Joseph D. Lyman +5

Core-collapse supernovae (CCSNe) are widely accepted to be caused by the explosive death of massive stars with initial masses M. There is, however, a comparative…

astro-ph.SR2023★ 19 cited

A characterization of ASAS-SN core-collapse supernova environments with VLT+MUSE: I. Sample selection, analysis of local environments, and correlations with light curve properties

Thallis Pessi, Jose L. Prieto, Joseph P. Anderson +17

The analysis of core-collapse supernova (CCSN) environments can provide important information on the life cycle of massive stars and constrain the progenitor properties of these po…

astro-ph.IM2023★ 16 cited

ASAS-SN Sky Patrol V2.0

K. Hart, B. J. Shappee, D. Hey +13

The All-Sky Automated Survey for Supernovae (ASAS-SN) began observing in late-2011 and has been imaging the entire sky with nightly cadence since late 2017. A core goal of ASAS-SN…

astro-ph.SR2022★ 10 cited

The Value-Added Catalog of ASAS-SN Eclipsing Binaries II: Properties of Extra-Physics Systems

D. M. Rowan, T. Jayasinghe, K. Z. Stanek +6

Detached eclipsing binaries are the primary tool used to measure precise masses and radii of stars. In our previous paper estimating the parameters of more than 30,000 detached ecl…