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researcher

G. Bryan

187 papers hereh-index 5914.6k citations273 works total

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

author position
  • sole author2
  • first author10
  • middle author110
  • last author58

Across the 180 of 187 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA86
  • astro-ph66
  • astro-ph.CO29
  • astro-ph.HE2
  • astro-ph.IM2
  • astro-ph.SR1
same name
  • G. Bryan — 2 papers, h 2
  • G. Bryan — 1 paper, h 39

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
19942024
most citedStatistical Properties of X-ray Clusters: Analytic and Numerical Comparisons

2.3k citations · 16.5k across the 186 of their papers we have counts for

collaborators
Showing 2002Show all

4 papers · 1 filter

astro-ph2002★ 55 cited

Numerical Simulations of High Redshift Star Formation in Dwarf Galaxies

Konstantinos Tassis, Tom Abel, Greg L. Bryan +1

We present first results from three-dimensional hydrodynamic simulations of the high redshift formation of dwarf galaxies. The simulations use an Eulerian adaptive mesh refinement…

astro-ph2002★ 139 cited

Effects of a Soft X-ray Background on Structure Formation at High Redshift

Marie M. Machacek, Greg L. Bryan, Tom Abel

We use three dimensional hydrodynamic simulations to investigate the effects of a soft X-ray background, that could have been produced by an early generation of mini-quasars, on th…

astro-ph2002

Redshift of Galaxy Clusters from the Sunyaev-Zel'dovich effect

J. M Diego, J. Mohr, J. Silk +1

We develop a new method for estimating the redshift of galaxy clusters through resolved images of the Sunyaev-Zel'dovich effect (SZE). Our method is based on morphological observab…

astro-ph2002★ 123 cited

A Universal Temperature Profile for Galaxy Clusters

C. Loken, M. L. Norman, E. Nelson +3

We investigate the predicted present-day temperature profiles of the hot, X-ray emitting gas in galaxy clusters for two cosmological models - a current best-guess LCDM model and st…

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