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researcher

Paul S. Smith

8 papers hereh-index 151.3k citations17 works total

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

author position
  • middle author4
  • last author1

Across the 5 of 8 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE4
  • astro-ph3
  • astro-ph.CO1
same name
  • Paul S. Smith — 84 papers, h 47
  • Paul S. Smith — 9 papers, h 5
  • Paul S. Smith — 8 papers
  • Paul S. Smith — 3 papers, h 2
  • Paul S. Smith — 1 paper, h 2
  • Paul S. Smith — 1 paper, h 1

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
20042020
most citedThe Luminosity Function of X-ray Selected Active Galactic Nuclei: Evolution of Supermassive Black Holes at High Redshift

290 citations · 637 across the 8 of their papers we have counts for

collaborators
Showing astro-phShow all

3 papers · 1 filter

astro-ph2008★ 121 cited

Spitzer/MIPS Observations of Stars in the Beta Pictoris Moving Group

L. M. Rebull, K. R. Stapelfeldt, M. W. Werner +7

We present Multiband Imaging Photometer for Spitzer (MIPS) observations at 24 and 70 microns for 30 stars, and at 160 microns for a subset of 12 stars, in the nearby (~30 pc), youn…

astro-ph2007★ 290 cited

The Luminosity Function of X-ray Selected Active Galactic Nuclei: Evolution of Supermassive Black Holes at High Redshift

J. D. Silverman, P. J. Green, W. A. Barkhouse +9

We present a measure of the hard (2-8 keV) X-ray luminosity function (XLF) of Active Galactic Nuclei up to z~5. At high redshifts, the wide area coverage of the Chandra Multiwaveng…

astro-ph2004★ 97 cited

Hard X-ray emitting Active Galactic Nuclei selected by the Chandra Multi-wavelength Project

J. Silverman, P. Green, W. Barkhouse +13

We present X-ray and optical analysis of 188 AGN identified from 497 hard X-ray (f (2.0-8.0 keV) > 2.7x10^-15 erg cm^-2 s^-1) sources in 20 Chandra fields (1.5 deg^2) forming part…

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