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researcher

A. Smith

14 papers hereh-index 215 citations15 works total

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

author position
  • middle author6

Across the 6 of 14 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO9
  • astro-ph.GA3
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • A. Smith — 86 papers, h 25
  • A. Smith — 80 papers, h 44
  • A. Smith — 73 papers, h 0
  • A. Smith — 56 papers, h 53
  • A. Smith — 52 papers, h 37
  • A. Smith — 50 papers, h 0

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
20102026
most citedHerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies

106 citations · 153 across the 3 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2015★ 47 cited

The HerMES sub-millimetre local and low-redshift luminosity functions

L. Marchetti, M. Vaccari, A. Franceschini +44

We used wide area surveys over 39 deg2 by the HerMES collaboration, performed with the Herschel Observatory SPIRE multi-wavelength camera, to estimate the low-redshift, $0.02<z<…

astro-ph.GA2015★ 106 cited

HerMES: ALMA Imaging of Herschel-selected Dusty Star-forming Galaxies

R. S. Bussmann, D. Riechers, A. Fialkov +25

The Herschel Multi-tiered Extragalactic Survey (HerMES) has identified large numbers of dusty star-forming galaxies (DSFGs) over a wide range in redshift. A detailed understanding…

astro-ph.GA2014

Herschel Observations of Far-Infrared Cooling Lines in intermediate Redshift (Ultra)-luminous Infrared Galaxies

D. Rigopoulou, R. Hopwood, G. E. Magdis +17

We report the first results from a spectroscopic survey of the [CII] 158um line from a sample of intermediate redshift (0.2<z<0.8) (ultra)-luminous infrared galaxies, (U)LIRGs (LIR…

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