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researcher

J. Agarwal

66 papers hereh-index 446.7k citations207 works total

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

author position
  • first author10
  • middle author41
  • last author11

Across the 62 of 66 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP62
  • astro-ph.IM2
  • astro-ph1
  • astro-ph.SR1
same name
  • J. Agarwal — 3 papers, h 2
  • J. Agarwal — 3 papers, h 3
  • J. Agarwal — 2 papers, h 2
  • J. Agarwal — 1 paper, h 3
  • J. Agarwal — 1 paper, h 17
  • J. Agarwal — 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

activity
20062026
most citedThe Active Asteroids

316 citations · 3k across the 66 of their papers we have counts for

collaborators
Showing 2013Show all

4 papers · 1 filter

astro-ph.EP2013★ 94 cited

The Extraordinary Multi-Tailed Main-Belt Comet P/2013 P5

David Jewitt, Jessica Agarwal, Harold Weaver +2

Hubble Space Telescope observations of main-belt comet P/2013 P5 reveal an extraordinary system of six dust tails that distinguish this object from any other. Observations two week…

astro-ph.EP2013★ 126 cited

The Dust Tail of Asteroid (3200) Phaethon

David Jewitt, Jing Li, Jessica Agarwal

We report the discovery of a comet-like tail on asteroid (3200) Phaethon when imaged at optical wavelengths near perihelion. In both 2009 and 2012, the tail appears >=350" (2.5x10^…

astro-ph.EP2013★ 28 cited

Dynamics of Large Fragments in the Tail of Active Asteroid P/2010 A2

Jessica Agarwal, David Jewitt, Harold Weaver

We examine the motions of large fragments at the head of the dust tail of active asteroid P/2010 A2. In previous work we showed that these fragments were ejected from the primary n…

astro-ph.EP2013★ 33 cited

Large Particles in Active Asteroid P/2010 A2

David Jewitt, Masateru Ishiguro, Jessica Agarwal

Previously unknown asteroid P/2010 A2 rose to prominence in 2010 by forming a transient, comet-like tail consisting of ejected dust. The observed dust production was interpreted as…

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