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researcher

C. Pearson

114 papers hereh-index 406.4k citations248 works total

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

author position
  • sole author1
  • first author7
  • middle author83
  • last author5

Across the 96 of 114 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA38
  • astro-ph.CO37
  • astro-ph24
  • astro-ph.IM11
  • astro-ph.HE2
  • astro-ph.EP1
same name
  • C. Pearson — 30 papers, h 30
  • C. Pearson — 24 papers, h 24
  • C. Pearson — 11 papers, h 24
  • C. Pearson — 10 papers, h 14
  • C. Pearson — 9 papers, h 2
  • C. Pearson — 4 papers, h 6

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
20002025
most citedThe Herschel ATLAS

596 citations · 4.8k across the 113 of their papers we have counts for

collaborators
Showing 2009Show all

4 papers · 1 filter

astro-ph.CO2009

The deepest image of the Universe at a wavelength of 15 microns

Rosalind Hopwood, Stephen Serjeant, Mattia Negrello +6

We present photometry, photometric redshifts and extra galactic number counts for ultra deep 15 micron mapping of the gravitational lensing cluster Abell 2218 (A2218), which is the…

astro-ph.CO2009★ 596 cited

The Herschel ATLAS

S. Eales, L. Dunne, D. Clements +94

The Herschel ATLAS is the largest open-time key project that will be carried out on the Herschel Space Observatory. It will survey 510 square degrees of the extragalactic sky, four…

astro-ph.CO2009★ 2 cited

On the nature of the first galaxies selected at 350 microns

Sophia A. Khan, Pierre F. Chanial, S. P. Willner +18

[abridged] We present constraints on the nature of the first galaxies selected at 350 microns. The sample includes galaxies discovered in the deepest blank-field survey at 350 micr…

astro-ph.CO2009★ 24 cited

Submillimetre surveys: The prospects for Herschel

Chris P. Pearson, Sophia A. Khan

Using the observed submillimetre source counts, from 250-1200 microns (including the most recent 250, 350 and 500 micron counts from BLAST), we present a model capable of reproduci…

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