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researcher

A. Humphrey

73 papers hereh-index 211.6k citations90 works total

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

author position
  • sole author1
  • first author12
  • middle author38
  • last author7

Across the 58 of 73 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA37
  • astro-ph17
  • astro-ph.CO14
  • astro-ph.IM4
  • astro-ph.SR1
same name
  • A. Humphrey — 13 papers, h 3
  • A. Humphrey — 5 papers, h 2
  • A. Humphrey — 3 papers
  • A. Humphrey — 1 paper, h 1
  • A. Humphrey — 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
20022024
most citedKinematically quiet halos around z~2.5 radio galaxies. Keck spectroscopy

132 citations · 2.1k across the 71 of their papers we have counts for

collaborators
Showing 2016Show all

3 papers · 1 filter

astro-ph.GA2016★ 15 cited

Ionization and feedback in Lyα halos around two radio galaxies at z∼2.5

S. G. Morais, A. Humphrey, M. Villar-Martín +6

We present new spectroscopic observations of two high redshift radio galaxies, TXS 0211-122 (z=2.34) and TXS 0828+193 (z=2.57), known to be associated with large Lyα halos. The o…

astro-ph.GA2016★ 20 cited

MUSE 3D Spectroscopy and Kinematics of the gigahertz peaked spectrum Radio Galaxy PKS 1934-63: Interaction, Recently Triggered AGN and Star Formation

Nathan Roche, Andrew Humphrey, Patricio Lagos +4

We observe the radio galaxy PKS 1934-63 (at z=0.1825) using MUSE (Multi Unit Spectroscopic Explorer) on the Very Large Telescope (VLT). The radio source is GigaHertz Peaked Spect…

astro-ph.GA2016★ 73 cited

Ionized outflows in luminous type 2 AGNs at z<0.6: no evidence for significant impact on the host galaxies

Montse Villar-Martin, Santiago Arribas, Bjorn Emonts +5

We investigate the presence of extended ionized outflows in 18 luminous type 2 AGNs (11 quasars and 7 high luminosity Seyfert 2s) at 0.3<z<0.6 based on VLT-FORS2 spectroscopy. We i…

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