activity
20232026
most citedThe Optical to X-ray Luminosity and Spectrum of Supernova Wind Breakouts

4 citations · 6 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2026

High-Energy Neutrinos from Supernova Shock Breakouts in Circumstellar Media: Light Curves, Spectra, and Contribution to the Extragalactic Neutrino Background

Tal Wasserman, Eli Waxman, Kohta Murase

Enhanced mass loss from core-collapse supernova (SN) progenitors shortly before explosion appears to be common, creating a compact, optically thick circumstellar medium (CSM) at $\…

astro-ph.HE2025★ 1 cited

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.HE2025

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.HE2025

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★ 4 cited

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…

astro-ph.HE2023★ 1 cited

Resolving the explosion of supernova 2023ixf in Messier 101 within its complex circumstellar environment

E. A. Zimmerman, I. Irani, P. Chen +54

Observing a supernova explosion shortly after it occurs can reveal important information about the physics of stellar explosions and the nature of the progenitor stars of supernova…