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researcher

A. Moore

56 papers hereh-index 252.3k citations134 works total

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

author position
  • first author1
  • middle author48
  • last author3

Across the 52 of 56 papers where every author was matched, so the position is known.

fields
  • astro-ph.IM27
  • astro-ph.HE11
  • astro-ph.GA10
  • astro-ph.SR6
  • astro-ph1
  • astro-ph.CO1
same name
  • A. Moore — 19 papers, h 64
  • A. Moore — 5 papers, h 35
  • A. Moore — 5 papers, h 22
  • A. Moore — 3 papers, h 2
  • A. Moore — 2 papers, h 3
  • A. Moore — 2 papers, h 31

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
20082023
most citedThe Keck Cosmic Web Imager Integral Field Spectrograph

244 citations · 1.5k across the 55 of their papers we have counts for

collaborators
Showing 2014 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2014★ 67 cited

IGM Emission Observations with the Cosmic Web Imager: II. Discovery of Extended, Kinematically-Linked Emission around SSA22 Lyman-alpha Blob 2

D. Christopher Martin, Daphne Chang, Matt Matuszewski +5

The intergalactic medium (IGM) is the dominant reservoir of baryons, delineates the large scale structure at low to moderate overdensities, and provides gas from which galaxies for…

astro-ph.GA2014★ 122 cited

IGM Emission Observations with the Cosmic Web Imager: I. The Circum-QSO Medium of QSO 1549+19, and Evidence for a Filamentary Gas Inflow

D. Christopher Martin, Daphne Chang, Matt Matuszewski +4

The Palomar Cosmic Web Imager (PCWI), an integral field spectrograph designed to detect and map low surface brightness emission, has obtained imaging spectroscopic maps of Ly-alpha…

astro-ph.GA2014★ 47 cited

Prospects for measuring supermassive black hole masses with future extremely large telescopes

Tuan Do, Shelley A. Wright, Aaron J. Barth +6

The next generation of giant-segmented mirror telescopes (> 20 m) will enable us to observe galactic nuclei at much higher angular resolution and sensitivity than ever before. Th…

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