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researcher

R. Demarco

7 papers hereh-index 451 citations7 works total

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

author position
  • middle author3
  • last author1

Across the 4 of 7 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA6
  • astro-ph.CO1
same name
  • R. Demarco — 108 papers, h 38
  • R. Demarco — 28 papers, h 24
  • R. Demarco — 14 papers, h 3
  • R. Demarco — 5 papers, h 3
  • R. Demarco — 1 paper
  • R. Demarco — 1 paper, h 4

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
20142026
most citedResolving CO (2-1) in z~1.6 Gas-Rich Cluster Galaxies with ALMA: Rotating Molecular Gas Disks with Possible Signatures of Gas Stripping

49 citations · 128 across the 5 of their papers we have counts for

collaborators
Showing 2024Show all

3 papers · 1 filter

astro-ph.GA2024★ 12 cited

Wide Area VISTA Extra-galactic Survey (WAVES): Unsupervised star-galaxy separation on the WAVES-Wide photometric input catalogue using UMAP and HDBSCAN

Todd L. Cook, Behnood Bandi, Sam Philipsborn +13

Star-galaxy separation is a crucial step in creating target catalogues for extragalactic spectroscopic surveys. A classifier biased towards inclusivity risks including spurious sta…

astro-ph.GA2024★ 12 cited

RMS asymmetry: a robust metric of galaxy shapes in images with varied depth and resolution

Elizaveta Sazonova, Cameron R Morgan, Michael Balogh +13

Structural disturbances, such as galaxy mergers or instabilities, are key candidates for driving galaxy evolution, so it is important to detect and quantify galaxies hosting these…

astro-ph.GA2024★ 10 cited

Distribution of merging and post-merging galaxies in nearby galaxy clusters

Duho Kim, Yun-Kyeong Sheen, Yara L. Jaffé +10

We study the incidence and spatial distribution of galaxies that are currently undergoing gravitational merging (M) or that have signs of a post merger (PM) in six galaxy clusters…

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