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Joseph P. Anderson

71 papers hereh-index 373.6k citations116 works total

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

author position
  • sole author1
  • first author5
  • middle author55
  • last author1

Across the 62 of 71 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE41
  • astro-ph.GA12
  • astro-ph.SR10
  • astro-ph.CO7
  • astro-ph.IM1
same name
  • Joseph P. Anderson — 18 papers, h 10
  • Joseph P. Anderson — 13 papers, h 6
  • Joseph P. Anderson — 8 papers, h 2
  • Joseph P. Anderson — 6 papers, h 3
  • Joseph P. Anderson — 4 papers, h 2
  • Joseph P. Anderson — 1 paper, h 2

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
20092023
most citedCharacterizing the V-band light-curves of hydrogen-rich type II supernovae

377 citations · 3.6k across the 70 of their papers we have counts for

collaborators
Showing 2012Show all

3 papers · 1 filter

astro-ph.HE2012★ 93 cited

Multi-Wavelength Observations of Supernova 2011ei: Time-Dependent Classification of Type IIb and Ib Supernovae and Implications for their Progenitors

D. Milisavljevic, R. Margutti, A. M. Soderberg +39

We present X-ray, UV/optical, and radio observations of the stripped-envelope, core-collapse supernova (SN) 2011ei, one of the least luminous SNe IIb or Ib observed to date. Our ob…

astro-ph.SR2012★ 20 cited

Evidence for asymmetric distribution of circumstellar material around Type Ia Supernovae

Francisco Förster, Santiago González-Gaitán, Joseph Anderson +5

We study the properties of low-velocity material in the line of sight towards nearby Type Ia Supernovae (SNe Ia) that have measured late phase nebular velocity shifts (v_neb), thou…

astro-ph.CO2012★ 1 cited

The Local Environments of Core-Collapse SNe within Host Galaxies

Joseph P Anderson, Stacey M Habergham, Phil A James +1

We present constraints on core-collapse supernova progenitors through observations of their environments within host galaxies. This is achieved through 2 routes. Firstly, we invest…

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