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researcher

M. W. Werner

3 papers here

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

author position
  • middle author1

Across the 1 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph2
  • astro-ph.CO1
ORCID 0000-0003-4990-189X
same name
  • M. W. Werner — 1 paper, h 7

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
20052010
most citedAn Excess Due to Small Grains Around The Nearby K0V Star HD69830: Asteroid or Cometary Debris?

194 citations · 415 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.CO2010★ 35 cited

Improving the identification of high-z Herschel sources with position priors and optical/NIR and FIR/mm photometric redshifts

P. G. Pérez-González, E. Egami, M. Rex +36

We present preliminary results about the detection of high redshift (U)LIRGs in the Bullet cluster field by the PACS and SPIRE instruments within the Herschel Lensing Survey (HLS)…

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★ 194 cited

An Excess Due to Small Grains Around The Nearby K0V Star HD69830: Asteroid or Cometary Debris?

C. A. Beichman, G. Bryden, T. N. Gautier +6

Spitzer photometry and spectroscopy of the star HD69830 reveal an excess of emission relative to the stellar photosphere between 8 and 35 μm dominated by strong features attribut…

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