activity
20242026
collaborators

6 papers

cs.GR2026

Strand-based Hairstyle Generation via Large Reconstruction and Multimodal Models

Conghui Hao, Tao Huang, Yuefan Shen +3

Creating high-quality strand-based hairstyles in current production pipelines remains heavily dependent on skilled artists and time-consuming manual authoring, making it costly and…

astro-ph.HE2026

The Type IIn SN 2025cbj coincidence with the high-energy neutrino IceCube-250421A

S. Garrappa, E. A. Zimmerman, T. Wasserman +14

Context. The origin of the astrophysical high-energy neutrino flux remains uncertain. Core-collapse supernovae with strong CSM interaction (Type IIn) are compelling candidates for…

astro-ph.HE2026

SN 2019vxm: A Shocking Coincidence between Fermi and TESS

Zachary G. Lane, Ryan Ridden-Harper, Sofia Rest +37

Shock breakout and, in some cases, jet-driven high-energy emission are increasingly recognized as key signatures of the earliest phases of core-collapse supernovae, especially in T…

astro-ph.HE2026

Supernovae Exploding within Dense Extended Material: Early Emission Regimes and Degeneracies in Parameter Inference from Observations

Tal Wasserman, Eli Waxman

Early light curves of many core-collapse supernovae (SNe) are thought to be powered by the interaction of the shock wave with optically thick extended material, either a bound enve…

astro-ph.HE2025

The Optical to X-ray Luminosity and Spectrum of Supernova Wind Breakouts

Tal Wasserman, Nir Sapir, Peter Szabo +1

Observations indicate that optically thick circum-stellar medium (CSM) at radii of cm around Type II core-collapse supernovae (SN) progenitors is common (and may…

astro-ph.HE2024

Shock breakouts from compact CSM surrounding core-collapse SN progenitors may contribute significantly to the observed TeV neutrino background

E. Waxman, T. Wasserman, E. Ofek +1

Growing observational evidence suggests that enhanced mass loss from the progenitors of core-collapse supernovae (SNe) is common during yr preceding the explosion, creating…