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D. Applegate

33 papers hereh-index 243.3k citations46 works total

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

author position
  • first author2
  • middle author25

Across the 27 of 33 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO27
  • astro-ph.GA4
  • astro-ph1
  • astro-ph.HE1
same name
  • D. Applegate — 13 papers, h 21
  • D. Applegate — 2 papers, h 5
  • D. Applegate — 1 paper, h 8
  • D. Applegate — 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
20082021
most citedGalaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey

708 citations · 4.1k across the 33 of their papers we have counts for

collaborators
Showing 2017 · astro-ph.COShow all

3 papers · 2 filters

astro-ph.CO2017★ 33 cited

Galaxy Kinematics and Mass Calibration in Massive SZE Selected Galaxy Clusters to z=1.3

R. Capasso, A. Saro, J. J. Mohr +27

The galaxy phase-space distribution in galaxy clusters provides insights into the formation and evolution of cluster galaxies, and it can also be used to measure cluster mass profi…

astro-ph.CO2017★ 25 cited

Precise weak lensing constraints from deep high-resolution Ks​ images: VLT/HAWK-I analysis of the super-massive galaxy cluster RCS2J232727.7−020437 at z=0.70

Tim Schrabback, Mischa Schirmer, Remco F. J. van der Burg +16

We demonstrate that deep good-seeing VLT/HAWK-I Ks​ images complemented with g+z-band photometry can yield a sensitivity for weak lensing studies of massive galaxy c…

astro-ph.CO2017★ 4 cited

XMM-Newton X-ray and HST weak gravitational lensing study of the extremely X-ray luminous galaxy cluster ClJ120958.9+495352 (z=0.902)

Sophia Thölken, Tim Schrabback, Thomas H. Reiprich +6

Observations of relaxed, massive and distant clusters can provide important tests of standard cosmological models e.g. using the gas mass fraction. We study the very luminous, high…

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