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P. Barmby

3 papers here

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

author position
  • middle author2

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph3
ORCID 0000-0003-2767-0090
same name
  • P. Barmby — 126 papers, h 51
  • P. Barmby — 14 papers, h 1
  • P. Barmby — 6 papers, h 1
  • P. Barmby — 2 papers, h 2

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
20012006
most citedSpitzer/MIPS Infrared Imaging of M31: Further Evidence for a Spiral/Ring Composite Structure

186 citations · 275 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph2006★ 186 cited

Spitzer/MIPS Infrared Imaging of M31: Further Evidence for a Spiral/Ring Composite Structure

Karl D. Gordon, J. Bailin, C. W. Engelbracht +16

New images of M31 at 24, 70, and 160 micron taken with the Multiband Imaging Photometer for Spitzer (MIPS) reveal the morphology of the dust in this galaxy. This morphology is well…

astro-ph2005★ 24 cited

Why Optically--Faint AGN Are Faint: The Spitzer Perspective

J. R. Rigby, G. H. Rieke, P. G. Perez-Gonzalez +5

Optically--faint X-ray sources (those with f_X/f_R > 10) constitute about 20% of X-ray sources in deep surveys, and are potentially highly obscured and/or at high redshift. Their f…

astro-ph2001★ 65 cited

Bright X-Ray Sources in M31 Globular Clusters

R. Di Stefano, A. K. H. Kong, M. R. Garcia +4

We have conducted Chandra observations of ~2560 square arcmin (~131 kpc^2) of of M31, and find that the most luminous X-ray sources in our fields are in globular clusters (GCs). Of…

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