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A. Ross

210 papers hereh-index 00 citations0 works total

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

author position
  • first author13
  • middle author140
  • last author4

Across the 157 of 210 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO182
  • astro-ph.IM19
  • astro-ph.GA6
  • astro-ph1
  • hep-ex1
  • quant-ph1
same name
  • A. Ross — 92 papers
  • A. Ross — 69 papers, h 24
  • A. Ross — 50 papers, h 34
  • A. Ross — 38 papers, h 71
  • A. Ross — 28 papers, h 8
  • A. Ross — 24 papers, h 17

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
20082024
most citedThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples

1.9k citations · 37.1k across the 206 of their papers we have counts for

collaborators
Showing 2010Show all

3 papers · 1 filter

astro-ph.CO2010★ 21 cited

Understanding the faint red galaxy population using large-scale clustering measurements from SDSS DR7

Ashley J. Ross, Rita Tojeiro, Will J. Percival

We use data from the SDSS to investigate the evolution of the large-scale galaxy bias as a function of luminosity for red galaxies. We carefully consider correlation functions of g…

astro-ph.CO2010★ 31 cited

The effect of redshift-space distortions on projected 2-pt clustering measurements

Kelly Nock, Will J. Percival, Ashley J. Ross

Although redshift-space distortions only affect inferred distances and not angles, they still distort the projected angular clustering of galaxy samples selected using redshift dep…

astro-ph.CO2010★ 36 cited

Evolution of the Clustering of Photometrically Selected SDSS Galaxies

Ashley J. Ross, Will J. Percival, Robert J. Brunner

We measure the angular auto-correlation functions (w) of SDSS galaxies selected to have photometric redshifts 0.1 < z < 0.4 and absolute r-band magnitudes Mr < -21.2. We split thes…

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