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T. Wasserman

4 papers hereh-index 376 citations8 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE4
same name
  • T. Wasserman — 2 papers, h 3
  • T. Wasserman — 1 paper, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators

4 papers

astro-ph.HE2025

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

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 1014−1015 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 ≳10 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 ∼1 yr preceding the explosion, creating…

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