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researcher

D. Pooley

78 papers hereh-index 374.2k citations196 works total

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

author position
  • first author5
  • middle author46
  • last author16

Across the 67 of 78 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE31
  • astro-ph23
  • astro-ph.GA12
  • astro-ph.CO6
  • astro-ph.SR4
  • astro-ph.EP1
same name
  • D. Pooley — 18 papers, h 11
  • D. Pooley — 9 papers, h 6
  • D. Pooley — 6 papers
  • D. Pooley — 3 papers, h 4
  • D. Pooley — 3 papers, h 13
  • D. Pooley — 1 paper, 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
20012026
most citedSN 2006gy: Discovery of the most luminous supernova ever recorded, powered by the death of an extremely massive star like Eta Carinae

577 citations · 4.5k across the 78 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.HEShow all

3 papers · 2 filters

astro-ph.HE2017★ 69 cited

GW170817 Most Likely Made a Black Hole

David Pooley, Pawan Kumar, J. Craig Wheeler +1

There are two outstanding issues regarding the neutron-star merger event GW170817: the nature of the compact remnant and the interstellar shock. The mass of the remnant of GW170817…

astro-ph.HE2017★ 81 cited

Gaia17biu/SN 2017egm in NGC 3191: The closest hydrogen-poor superluminous supernova to date is in a "normal", massive, metal-rich spiral galaxy

Subhash Bose, Subo Dong, A. Pastorello +55

Hydrogen-poor superluminous supernovae (SLSNe-I) have been predominantly found in low-metallicity, star-forming dwarf galaxies. Here we identify Gaia17biu/SN 2017egm as an SLSN-I o…

astro-ph.HE2017★ 19 cited

Searching for the expelled hydrogen envelope in Type I supernovae via late-time H-alpha emission

J. Vinko, D. Pooley, J. M. Silverman +6

We report the first results from our long-term observational survey aimed at discovering late-time interaction between the ejecta of hydrogen-poor Type I supernovae and the hydroge…

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