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researcher

D. Scott

159 papers hereh-index 11461.4k citations724 works total

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

author position
  • sole author6
  • first author13
  • middle author74
  • last author24

Across the 117 of 159 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA53
  • astro-ph52
  • astro-ph.CO37
  • astro-ph.IM13
  • physics.pop-ph2
  • astro-ph.HE1
same name
  • D. Scott — 53 papers
  • D. Scott — 24 papers, h 57
  • D. Scott — 6 papers
  • D. Scott — 5 papers, h 5
  • D. Scott — 4 papers, h 12
  • D. Scott — 3 papers

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
19942022
most citedCMB-S4 Science Case, Reference Design, and Project Plan

443 citations · 4.5k across the 79 of their papers we have counts for

collaborators
Showing 2016Show all

4 papers · 1 filter

astro-ph.GA2016

The multiplicity of 250-μm Herschel sources in the COSMOS field

Jillian M. Scudder, Seb Oliver, Peter D. Hurley +5

We investigate the multiplicity of extragalactic sources detected by the Herschel Space Observatory in the COSMOS field. Using 3.6- and 24-μm catalogues, in conjunction with 250-…

astro-ph.CO2016

A new VLA/e-MERLIN limit on central images in the gravitational lens system CLASS B1030+074

Jonathan Quinn, Neal Jackson, Amitpal Tagore +8

We present new VLA 22-GHz and e-MERLIN 5-GHz observations of CLASS B1030+074, a two-image strong gravitational lens system whose background source is a compact flat-spectrum radio…

astro-ph.CO2016

Pi in the sky

Ali Frolop, Douglas Scott

Deviations of the observed cosmic microwave background (CMB) from the standard model, known as "anomalies", are obviously highly significant and deserve to be pursued more aggressi…

astro-ph.CO2016

The information content of cosmic microwave background anisotropies

Douglas Scott, Dagoberto Contreras, Ali Narimani +1

The cosmic microwave background (CMB) contains perturbations that are close to Gaussian and isotropic. This means that its information content, in the sense of the ability to const…

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