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T. Wagg

21 papers hereh-index 9409 citations22 works total

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

author position
  • first author9
  • middle author7
  • last author3

Across the 19 of 21 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR7
  • astro-ph.HE6
  • astro-ph.GA4
  • astro-ph.IM2
  • cs.DL1
  • gr-qc1
same name
  • T. Wagg — 3 papers, h 3

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

activity
20212026
most citedThe redshift evolution of the binary black hole merger rate: a weighty matter

152 citations · 314 across the 18 of their papers we have counts for

collaborators
Showing 2025Show all

3 papers · 1 filter

astro-ph.SR2025

Implications of modern mass-loss rates for massive stars

JD Merritt, Simon Stevenson, Andreas Sander +7

Massive stars lose a significant fraction of their mass through stellar winds at various stages of their lives, including on the main sequence, during the red supergiant phase, and…

astro-ph.SR2025

Delayed and Displaced: The Impact of Binary Interactions on Core-collapse SN Feedback

Tom Wagg, Julianne J. Dalcanton, Mathieu Renzo +7

Core-collapse supernova feedback models in hydrodynamical simulations typically assume that all stars evolve as single stars. However, the majority of massive stars are formed in b…

astro-ph.SR2025★ 4 cited

Stellar ejection velocities from the binary supernova scenario: A comparison across population synthesis codes

Tom Wagg, David D. Hendriks, Mathieu Renzo +1

The vast majority of binary systems are disrupted at the moment of the first supernova, resulting in an unbound compact object and companion star. These ejected companion stars con…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.