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researcher

J. Cohen

50 papers hereh-index 6513.8k citations289 works total

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

author position
  • sole author5
  • first author18
  • middle author19
  • last author6

Across the 48 of 50 papers where every author was matched, so the position is known.

fields
  • astro-ph27
  • astro-ph.GA16
  • astro-ph.SR4
  • astro-ph.IM2
  • astro-ph.CO1
same name
  • J. Cohen — 23 papers, h 103
  • J. Cohen — 9 papers, h 6
  • J. Cohen — 5 papers, h 3
  • J. Cohen — 5 papers, h 3
  • J. Cohen — 4 papers, h 48
  • J. Cohen — 4 papers, 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
19982020
most citedThe Chemical Evolution of the Draco Dwarf Spheroidal Galaxy

213 citations · 1.7k across the 22 of their papers we have counts for

collaborators
Showing 2004 · astro-phShow all

4 papers · 2 filters

astro-ph2004

Chemical Abundance Inhomogeneities in Globular Cluster Stars

Judith G. Cohen

It is now clear that abundance variations from star-to-star among the light elements, particularly C, N, O, Na and Al, are ubiquitous within galactic globular clusters; they appear…

astro-ph2004

Outer Versus Inner Halo Globular Clusters: NGC 7492 Abundances

Judith G. Cohen, Jorge Melendez

We have carried out a detailed abundance analysis for 21 elements in a sample of four RGB stars in the outer halo globular cluster NGC 7492 (R{GC} 25 kpc); we find [Fe/H] = -1.82 d…

astro-ph2004

Abundances in a Large Sample of Stars in M3 and M13

Judith G. Cohen, Jorge Melendez

We have carried out a detailed abundance analysis for 21 elements in a sample of 25 stars with a wide range in luminosity from luminous giants to stars near the main sequence turno…

astro-ph2004

Abundances In Very Metal Poor Dwarf Stars

Judith G. Cohen, Norbert Christlieb, Andrew McWilliam +7

We discuss the detailed composition of 28 extremely metal-poor dwarfs, 22 of which are from the Hamburg/ESO Survey, based on Keck Echelle spectra. Our sample has a median [Fe/H] of…

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