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D. Perley

25 papers hereh-index 6310 citations17 works total

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

author position
  • first author4
  • middle author20

Across the 24 of 25 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE17
  • astro-ph.GA6
  • astro-ph1
  • astro-ph.CO1
same name
  • D. Perley — 264 papers, h 79
  • D. Perley — 65 papers, h 8
  • D. Perley — 3 papers, h 4
  • D. Perley — 1 paper, h 2

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
20082026
most citedLow-Resolution Spectroscopy of Gamma-ray Burst Optical Afterglows: Biases in the Swift Sample and Characterization of the Absorbers

368 citations · 2k across the 25 of their papers we have counts for

collaborators
Showing 2015 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2015★ 135 cited

The Swift Gamma-Ray Burst Host Galaxy Legacy Survey - I. Sample Selection and Redshift Distribution

D. A. Perley, T. Krühler, S. Schulze +20

We introduce the Swift Gamma-Ray Burst Host Galaxy Legacy Survey ("SHOALS"), a multi-observatory high-redshift galaxy survey targeting the largest unbiased sample of long-duration…

astro-ph.GA2015★ 185 cited

The Swift GRB Host Galaxy Legacy Survey - II. Rest-Frame NIR Luminosity Distribution and Evidence for a Near-Solar Metallicity Threshold

D. A. Perley, N. R. Tanvir, J. Hjorth +9

We present rest-frame NIR luminosities and stellar masses for a large and uniformly-selected population of GRB host galaxies using deep Spitzer Space Telescope imaging of 119 targe…

astro-ph.GA2015★ 73 cited

The Optically Unbiased Gamma-Ray Burst Host (TOUGH) Survey. VII. The Host Galaxy Luminosity Function: Probing the Relationship Between GRBs and Star Formation to Redshift ∼6

S. Schulze, R. Chapman, J. Hjorth +12

Gamma-ray bursts (GRBs) offer a route to characterizing star-forming galaxies and quantifying high-z star formation that is distinct from the approach of traditional galaxy surve…

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