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D. Alexander

5 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 author1
  • middle author2

Across the 3 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph5
same name
  • D. Alexander — 49 papers, h 87
  • D. Alexander — 12 papers, h 26
  • D. Alexander — 2 papers, h 16
  • D. Alexander — 1 paper, h 0
  • D. Alexander — 1 paper, h 6
  • D. Alexander — 1 paper, h 7

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
20042008
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 · 636 across the 4 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.