activity
20242026
collaborators

8 papers

astro-ph.IM2026

The Impact of Host Galaxy Properties on Supernova Classification with Hierarchical Labels

V. Ashley Villar, Sebastian Gomez, Edo Berger +1

With the advent of the Vera C. Rubin Observatory, the discovery rate of supernovae (SNe) will surpass the rate of SNe with real time spectroscopic followup by three orders of magni…

astro-ph.HE2026

JWST Reveals Large Reservoirs of Dust and Ongoing Circumstellar Interaction in SN Ibn/Icn 2023xgo over a Year Post-Explosion

Kyle W. Davis, Kirsty Taggart, Samaporn Tinyanont +23

We present infrared (IR) photometric and spectroscopic observations of SN 2023xgo, a recent and nearby Type Ibn/Icn supernova (SN Ibn/Icn) which shows shock interaction with a He/C…

astro-ph.HE2025

Optimizing Kilonova Searches: A Case Study of the Type IIb SN 2025ulz in the Localization Volume of the Low-Significance Gravitational Wave Event S250818k

Noah Franz, Bhagya Subrayan, Charles D. Kilpatrick +54

Kilonovae, the ultraviolet/optical/infrared counterparts to binary neutron star mergers, are an exceptionally rare class of transients. Optical follow-up campaigns are plagued by c…

astro-ph.HE2025

When IIb Ceases To Be: Bridging the Gap Between IIb and Short-plateau Supernovae

Joseph R. Farah, D. Andrew Howell, Daichi Hiramatsu +13

Hydrogen-rich supernovae (SNe) span a range of hydrogen envelope masses at core collapse, producing diverse light curves from extended plateaus in Type II SNe to double-peaked Type…

astro-ph.HE2025

SPLASH: A Rapid Host-Based Supernova Classifier for Wide-Field Time-Domain Surveys

Adam Boesky, V. Ashley Villar, Alexander Gagliano +1

The upcoming Legacy Survey of Space and Time (LSST) conducted by the Vera C. Rubin Observatory will detect millions of supernovae (SNe) and generate millions of nightly alerts, far…

astro-ph.HE2024

Maven: A Multimodal Foundation Model for Supernova Science

Gemma Zhang, Thomas Helfer, Alexander T. Gagliano +2

A common setting in astronomy is the availability of a small number of high-quality observations, and larger amounts of either lower-quality observations or synthetic data from sim…