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researcher

P. Petitjean

41 papers hereh-index 262.6k citations57 works total

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

author position
  • sole author1
  • first author1
  • middle author26
  • last author6

Across the 34 of 41 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO14
  • astro-ph12
  • astro-ph.GA12
  • astro-ph.IM3
same name
  • P. Petitjean — 233 papers, h 77
  • P. Petitjean — 41 papers, h 6
  • P. Petitjean — 27 papers, h 20
  • P. Petitjean — 18 papers, h 10
  • P. Petitjean — 5 papers
  • P. Petitjean — 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
19972026
most citedThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 9 Spectroscopic Galaxy Sample

898 citations · 3.6k across the 41 of their papers we have counts for

collaborators
Showing 2010Show all

3 papers · 1 filter

astro-ph.CO2010★ 16 cited

X-ray and optical properties of Broad Absorption Line Quasars in the Canada-France-Hawaii Telescope Legacy Survey

C. S. Stalin, R. Srianand, P. Petitjean

We study the X-ray and optical properties of 16 Broad Absorption Line (BAL) quasars detected in about 3 degree square region common to the wide synoptic (W-1) component of the Cana…

astro-ph.CO2010★ 49 cited

The WIRCAM Deep Infrared Cluster Survey I: Groups and Clusters at z > 1.1

R. M. Bielby, A. Finoguenov, M. Tanaka +12

We use CFHTLS deep optical data, WIRCam Deep Survey (WIRDS) NIR data and XMM data to identify z>1.1 clusters in the CFHTLS D1 and D4 fields. Counterparts to such clusters can not b…

astro-ph.CO2010★ 59 cited

VLT LBG Redshift Survey II: Interactions between galaxies and the IGM at z ~3

N. H. M. Crighton, R. Bielby, T. Shanks +15

We have measured redshifts for 243 z ~3 quasars in nine VLT VIMOS LBG redshift survey areas, each of which is centred on a known bright quasar. Using spectra of these quasars, we m…

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