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researcher

K. Glazebrook

471 papers hereh-index 10652.4k citations711 works total

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

author position
  • sole author3
  • first author20
  • middle author348
  • last author24

Across the 395 of 471 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA224
  • astro-ph125
  • astro-ph.CO95
  • astro-ph.IM17
  • astro-ph.HE7
  • physics.optics2
same name
  • K. Glazebrook — 14 papers, h 8
  • K. Glazebrook — 8 papers, h 33
  • K. Glazebrook — 6 papers, h 3
  • K. Glazebrook — 1 paper, h 1
  • K. Glazebrook — 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
19932026
most citedDetection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies

4.6k citations · 60.4k across the 464 of their papers we have counts for

collaborators
Showing 2013 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2013★ 223 cited

A substantial population of massive quiescent galaxies at z~4 from ZFOURGE

Caroline M. S. Straatman, Ivo Labbé, Lee R. Spitler +21

We report the likely identification of a substantial population of massive M~10^11M_Sun galaxies at z~4 with suppressed star formation rates (SFRs), selected on rest-frame optical…

astro-ph.GA2013★ 146 cited

Fundamental Mass-Spin-Morphology Relation of Spiral Galaxies

Danail Obreschkow, Karl Glazebrook

This work present high-precision measurements of the specific baryon angular momentum jb, contained in stars, atomic gas, and molecular gas, out to ~10 scale radii, in 16 nearby sp…

astro-ph.GA2013★ 142 cited

DYNAMO I: A Sample of Ha-Luminous Galaxies with Resolved Kinematics

Andrew W. Green, Karl Glazebrook, Peter J. McGregor +8

(abridged) DYNAMO is a multi-wavelength, spatially-resolved survey of local (z∼0.1) star-forming galaxies designed to study evolution through comparison with samples at z~2.…

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