◍wovepaper
SearchResearchersInstitutions
Sign in
researcher

David R. Patton

17 papers hereh-index 8235 citations16 works total

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

author position
  • first author1
  • middle author11
  • last author4

Across the 16 of 17 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA13
  • astro-ph.CO4
same name
  • David R. Patton — 6 papers, h 4
  • David R. Patton — 1 paper
  • David R. Patton — 1 paper, h 2
  • David R. Patton — 1 paper, h 3

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
20112026
most citedGalaxy pairs in the Sloan Digital Sky Survey - VIII: The observational properties of post-merger galaxies

286 citations · 842 across the 17 of their papers we have counts for

collaborators
Showing 2025Show all

3 papers · 1 filter

astro-ph.GA2025

Interacting galaxies in the IllustrisTNG simulations - IX: Mini mergers trigger AGN in cosmological simulations

Shoshannah Byrne-Mamahit, Sara L. Ellison, David R. Patton +3

Galaxy mergers are transformative events that can cause gaseous inflows capable of triggering active galactic nuclei (AGN). Previous studies of AGN in simulations have mainly focus…

astro-ph.GA2025★ 2 cited

UNIONS: The Ultraviolet Near-Infrared Optical Northern Survey

Stephen Gwyn, Alan W. McConnachie, Jean-Charles Cuillandre +86

The Ultraviolet Near-Infrared Optical Northern Survey (UNIONS) is a "collaboration of collaborations" that is using the Canada-France-Hawai'i Telescope, the Pan-STARRS telescopes,…

astro-ph.GA2025

Interacting galaxies in the IllustrisTNG simulations -- VIII: Pericentric star formation rate enhancements are driven both by increased fuelling and efficiency

Lawrence Faria, David R. Patton, Stéphane Courteau +2

Using the TNG100-1 cosmological simulations, we explore how galaxy properties, such as specific star formation rate (sSFR=SFR/M∗​), gas fraction ($\rm f_{gas} \,= \, M_{\rm H…

◍wovepaper

Papers, researchers and institutions, woven together.

Explore
  • Search
  • Researchers
  • Institutions
Account
  • Library
  • Chat
Data
  • arXiv.org
  • Semantic Scholar
  • OpenAlex
  • Latest RSS
AboutContactPrivacyDevelopersllms.txtopenapi.json
Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.