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researcher

A. Mann

225 papers hereh-index 5110.5k citations308 works total

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

author position
  • first author18
  • middle author152
  • last author21

Across the 191 of 225 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP155
  • astro-ph.SR64
  • astro-ph.CO3
  • astro-ph.GA1
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • A. Mann — 243 papers
  • A. Mann — 68 papers
  • A. Mann — 51 papers
  • A. Mann — 44 papers, h 19
  • A. Mann — 33 papers
  • A. Mann — 21 papers, h 18

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
20112024
most citedThe Revised TESS Input Catalog and Candidate Target List

1k citations · 15.3k across the 224 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

3 papers · 1 filter

astro-ph.CO2013★ 16 cited

A Search for Moderate-Redshift Survivors from the Population of Luminous Compact Passive Galaxies at High Redshift

Alan Stockton, Hsin-Yi Shih, Kirsten Larson +1

From a search of a ~ 2400 square degree region covered by both the SDSS and UKIDSS databases, we have attempted to identify galaxies at z ~ 0.5 that are consistent with their being…

astro-ph.CO2013★ 54 cited

The role of galaxy interaction in the SFR-M relation: characterizing morphological properties of Herschel-selected galaxies at 0.2<z<1.5

Chao-Ling Hung, David B. Sanders, Caitlin M. Casey +13

Galaxy interactions/mergers have been shown to dominate the population of IR luminous galaxies (log(LIR)>11.6Lsun) in the local Universe (z<0.25). Recent studies based on the relat…

astro-ph.CO2011★ 241 cited

X-ray/optical classification of cluster mergers and the evolution of the cluster merger fraction

Andrew W. Mann, Harald Ebeling

We present the results of a simple but robust morphological classification of a statis- tically complete sample of 108 of the most X-ray luminous clusters at 0.15 < z < 0.7 observe…

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