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researcher

I. Arcavi

312 papers hereh-index 7620.7k citations526 works total

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

author position
  • sole author4
  • first author12
  • middle author210
  • last author11

Across the 237 of 312 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE174
  • astro-ph.IM63
  • astro-ph.SR36
  • astro-ph.CO24
  • astro-ph.GA13
  • math.CO1
same name
  • I. Arcavi — 3 papers

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
20092026
most citedOptical emission from a kilonova following a gravitational-wave-detected neutron-star merger

622 citations · 20.6k across the 301 of their papers we have counts for

collaborators
Showing 2009Show all

3 papers · 1 filter

astro-ph.CO2009★ 89 cited

On the progenitor and early evolution of the type II supernova 2009kr

M. Fraser, K. Takats, A. Pastorello +13

We report the identification of a source coincident with SN 2009kr in HST pre-explosion images. The object appears to be a single point source with an intrinsic colour V-I = 1.1 an…

astro-ph.CO2009★ 549 cited

Hydrogen-poor superluminous stellar explosions

R. M. Quimby, S. R. Kulkarni, M. M. Kasliwal +24

Supernovae (SNe) are stellar explosions driven by gravitational or thermonuclear energy, observed as electromagnetic radiation emitted over weeks or more. In all known SNe, this ra…

astro-ph.HE2009★ 349 cited

A faint type of supernova from a white dwarf with a helium-rich companion

H. B. Perets, A. Gal-Yam, P. Mazzali +25

Supernovae (SNe) are thought to arise from two different physical processes. The cores of massive, short-lived stars undergo gravitational core collapse and typically eject a few s…

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