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researcher

D. Alexander

48 papers hereh-index 353.6k citations56 works total

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

author position
  • first author3
  • middle author30
  • last author3

Across the 36 of 48 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO21
  • astro-ph.GA14
  • astro-ph7
  • astro-ph.HE6
same name
  • D. Alexander — 238 papers, h 87
  • D. Alexander — 46 papers, h 86
  • D. Alexander — 36 papers, h 26
  • D. Alexander — 13 papers, h 18
  • D. Alexander — 11 papers, h 6
  • D. Alexander — 8 papers, h 0

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
20042019
most citedMultiwavelength study of massive galaxies at z~2. II. Widespread Compton thick AGN and the concurrent growth of black holes and bulges

346 citations · 4.4k across the 48 of their papers we have counts for

collaborators
Showing 2007Show all

3 papers · 1 filter

astro-ph2007★ 177 cited

The Evolution of AGN Host Galaxies: From Blue to Red and the Influence of Large-Scale Structures

J. D. Silverman, V. Mainieri, B. D. Lehmer +14

We present an analysis of 109 moderate-luminosity (41.9 < Log L{0.5-8.0 keV} < 43.7) AGN in the Extended Chandra Deep Field-South survey, which is drawn from 5,549 galaxies from th…

astro-ph2007★ 30 cited

Uncovering the Near-IR Dwarf Galaxy Population of the Coma Cluster with Spitzer IRAC

L. P. Jenkins, A. E. Hornschemeier, B. Mobasher +2

We present the first results of a Spitzer IRAC (Infrared Array Camera) wide-field survey of the Coma cluster. The observations cover two fields of different galaxy densities; the f…

astro-ph2007★ 346 cited

Multiwavelength study of massive galaxies at z~2. II. Widespread Compton thick AGN and the concurrent growth of black holes and bulges

E. Daddi, D. M. Alexander, M. Dickinson +16

Approximately 20-30% of 1.4<z<2.5 galaxies with K<22 (Vega) detected with Spitzer MIPS at 24um show excess mid-IR emission relative to that expected based on the rates of star form…

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