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researcher

G. Martinez

45 papers hereh-index 294.4k citations58 works total

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

author position
  • sole author1
  • first author3
  • middle author29
  • last author1

Across the 34 of 45 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA21
  • hep-ph10
  • astro-ph.HE6
  • astro-ph.CO3
  • astro-ph.EP2
  • astro-ph.SR2
same name
  • G. Martinez — 67 papers, h 117
  • G. Martinez — 16 papers, h 15
  • G. Martinez — 9 papers, h 14
  • G. Martinez — 8 papers, h 12
  • G. Martinez — 7 papers, h 7
  • G. Martinez — 6 papers, h 4

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
20092023
most citedAccurate masses for dispersion-supported galaxies

682 citations · 5.5k across the 45 of their papers we have counts for

collaborators
Showing 2010 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2010★ 97 cited

A Complete Spectroscopic Survey of the Milky Way satellite Segue 1: Dark matter content, stellar membership and binary properties from a Bayesian analysis

Gregory D. Martinez, Quinn E. Minor, James Bullock +3

We introduce a comprehensive analysis of multi-epoch stellar line-of-sight velocities to determine the intrinsic velocity dispersion of the ultrafaint satellites of the Milky Way.…

astro-ph.GA2010★ 287 cited

A Complete Spectroscopic Survey of the Milky Way Satellite Segue 1: The Darkest Galaxy

Joshua D. Simon, Marla Geha, Quinn E. Minor +9

We present the results of a comprehensive Keck/DEIMOS spectroscopic survey of the ultra-faint Milky Way satellite galaxy Segue 1. We have obtained velocity measurements for 98.2% o…

astro-ph.GA2010★ 57 cited

Correcting velocity dispersions of dwarf spheroidal galaxies for binary orbital motion

Quinn E. Minor, Greg Martinez, James Bullock +2

We show that measured velocity dispersions of dwarf spheroidal galaxies from about 4 to 10 km/s are unlikely to be inflated by more than 20% due to the orbital motion of binary sta…

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