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researcher

J. Richard

37 papers hereh-index 17958 citations37 works total

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

author position
  • first author1
  • middle author29
  • last author1

Across the 31 of 37 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA16
  • astro-ph.CO13
  • astro-ph6
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • J. Richard — 251 papers, h 75
  • J. Richard — 85 papers, h 30
  • J. Richard — 22 papers, h 9
  • J. Richard — 19 papers, h 6
  • J. Richard — 11 papers, h 11
  • J. Richard — 9 papers, h 17

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
20032026
most citedA bright z=5.2 lensed submillimeter galaxy in the field of Abell 773: HLSJ091828.6+514223

133 citations · 1k across the 36 of their papers we have counts for

collaborators
Showing 2026Show all

3 papers · 1 filter

astro-ph.GA2026

A redshift of z=3.20 for the bright arc in eMACSJ2229.9-0808: Comment on Wagner & Falco (2026) "Hamilton's Object revisited: A challenging source redshift of a strong lensing configuration"

Ian Smail, Johan Richard, Harald Ebeling +1

We re-analyse near-infrared and optical spectroscopy from the Subaru, Gemini, and Keck telescopes of the bright gravitational arc seen in the z=0.62 X-ray cluster eMACSJ2229.9-0808…

astro-ph.HE2026

A spectroscopically confirmed, strongly lensed, metal-poor Type II supernova at z = 5.13

David A. Coulter, Conor Larison, Justin D. R. Pierel +88

Observing supernovae (SNe) in the early Universe (z > 3) provides a window into how both galaxies and individual stars have evolved over cosmic time, yet a detailed study of high-r…

astro-ph.GA2026

Spectroscopic characterization of a remarkable temporally varying, triple-lensed quasar at z=2.67

Charlie Lind-Thomsen, Kasper E. Heintz, Albert Sneppen +5

Gravitationally lensed quasars are viable cosmic tools for constraining a diversity of fundamental astrophysical phenomena; They enable identification of faint, low-mass supermassi…

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