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researcher

S. Veilleux

61 papers hereh-index 304k citations60 works total

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

author position
  • first author6
  • middle author36
  • last author9

Across the 51 of 61 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA34
  • astro-ph15
  • astro-ph.CO9
  • astro-ph.HE3
same name
  • S. Veilleux — 209 papers, h 72
  • S. Veilleux — 38 papers, h 6
  • S. Veilleux — 11 papers, h 6
  • S. Veilleux — 2 papers, h 5
  • S. Veilleux — 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
19992026
most citedSpitzer Quasar and ULIRG Evolution Study (QUEST). IV. Comparison of 1-Jy Ultraluminous Infrared Galaxies with Palomar-Green Quasars

467 citations · 5.3k across the 59 of their papers we have counts for

collaborators
Showing 2015Show all

3 papers · 1 filter

astro-ph.GA2015★ 2 cited

A deep Herschel/PACS observation of CO(40-39) in NGC 1068: a search for the molecular torus

A. W. Janssen, S. Bruderer, E. Sturm +14

Emission from high-J CO lines in galaxies has long been proposed as a tracer of X-ray dominated regions (XDRs) produced by AGN. Of particular interest is the question of whether th…

astro-ph.GA2015★ 290 cited

The multi-phase winds of Markarian 231: from the hot, nuclear, ultra-fast wind to the galaxy-scale, molecular outflow

C. Feruglio, F. Fiore, S. Carniani +9

We present the best sensitivity and angular resolution maps of the molecular disk and outflow of Mrk 231, as traced by CO observations obtained with IRAM/PdBI, and we analyze archi…

astro-ph.GA2015★ 179 cited

The Herschel Comprehensive (U)LIRG Emission Survey (HerCULES): CO Ladders, fine structure lines, and neutral gas cooling

M. J. F. Rosenberg, P. P. van der Werf, S. Aalto +27

(Ultra) Luminous Infrared Galaxies ((U)LIRGs) are objects characterized by their extreme infrared (8-1000 μm) luminosities (LLIRG​>1011L⊙​ and LULIRG​>1012 L…

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