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researcher

R. Allen

28 papers hereh-index 211.6k citations34 works total

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

author position
  • first author2
  • middle author23
  • last author1

Across the 26 of 28 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA24
  • astro-ph.CO2
  • astro-ph.HE1
  • astro-ph.SR1
same name
  • R. Allen — 54 papers, h 25
  • R. Allen — 45 papers, h 37
  • R. Allen — 35 papers, h 31
  • R. Allen — 14 papers, h 24
  • R. Allen — 13 papers, h 21
  • R. Allen — 10 papers, h 9

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
20112025
most citedGalaxy Stellar Mass Functions from ZFOURGE/CANDELS: An Excess of Low-Mass Galaxies Since z=2 and the Rapid Buildup of Quiescent Galaxies

460 citations · 2.5k across the 28 of their papers we have counts for

collaborators
Showing 2017Show all

3 papers · 1 filter

astro-ph.GA2017★ 5 cited

Decoupled Black Hole Accretion and Quenching: The Relationship Between BHAR, SFR, and Quenching in Milky Way and Andromeda-mass Progenitors Since z = 2.5

Michael J. Cowley, Lee R. Spitler, Ryan F. Quadri +13

We investigate the relationship between the black hole accretion rate (BHAR) and star-formation rate (SFR) for Milky Way (MW) and Andromeda (M31)-mass progenitors from z = 0.2 - 2.…

astro-ph.GA2017★ 159 cited

Effect of local environment and stellar mass on galaxy quenching and morphology at 0.5<z<2.0

Lalitwadee Kawinwanichakij, Casey Papovich, Ryan F. Quadri +20

We study galactic star-formation activity as a function of environment and stellar mass over 0.5<z<2.0 using the FourStar Galaxy Evolution (ZFOURGE) survey. We estimate the galaxy…

astro-ph.GA2017★ 49 cited

Discovery of Extreme [OIII]+Hβ Emitting Galaxies Tracing an Overdensity at z~3.5 in CDF-South

Ben Forrest, Kim-Vy H. Tran, Adam Broussard +12

Using deep multi-wavelength photometry of galaxies from ZFOURGE, we group galaxies at 2.5<z<4.0 by the shape of their spectral energy distributions (SEDs). We identify a populati…

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