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C. Conselice

228 papers hereh-index 11149.1k citations1k works total

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

author position
  • sole author15
  • first author17
  • middle author124
  • last author16

Across the 172 of 228 papers where every author was matched, so the position is known.

fields
  • astro-ph108
  • astro-ph.GA83
  • astro-ph.CO25
  • astro-ph.IM7
  • astro-ph.HE3
  • astro-ph.EP2
same name
  • C. Conselice — 7 papers, h 4
  • C. Conselice — 3 papers, h 5
  • C. Conselice — 2 papers, h 1
  • C. Conselice — 2 papers
  • C. Conselice — 1 paper, h 2
  • C. Conselice — 1 paper

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
19962025
most citedStar Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies

2k citations · 12.2k across the 120 of their papers we have counts for

collaborators
Showing 2016Show all

3 papers · 1 filter

astro-ph.GA2016★ 51 cited

The Formation of Bulges, Discs and Two Component Galaxies in the CANDELS Survey at z < 3

Berta Margalef-Bentabol, Christopher J. Conselice, Alice Mortlock +6

We examine a sample of 1495 galaxies in the CANDELS fields to determine the evolution of two component galaxies, including bulges and discs, within massive galaxies at the epoch 1…

astro-ph.GA2016

HST imaging of the dusty filaments and nucleus swirl in NGC4696 at the centre of the Centaurus Cluster

A. C. Fabian, S. A. Walker, H. R. Russell +14

Narrow-band HST imaging has resolved the detailed internal structure of the 10 kpc diameter H alpha+[NII] emission line nebulosity in NGC4696, the central galaxy in the nearby Cent…

astro-ph.GA2016

The structure and evolution of a forming galaxy cluster at z = 1.62

N. A. Hatch, S. I. Muldrew, E. A. Cooke +4

We present a comprehensive picture of the Cl0218.3-0510 protocluster at z=1.623 across 10 co-moving Mpc. Using filters that tightly bracket the Balmer and 4000 Angstrom breaks of…

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