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researcher

M. Meixner

123 papers hereh-index 508.7k citations427 works total

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

author position
  • sole author1
  • first author5
  • middle author96
  • last author14

Across the 116 of 123 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA47
  • astro-ph.SR33
  • astro-ph29
  • astro-ph.CO9
  • astro-ph.IM3
  • astro-ph.EP1
same name
  • M. Meixner — 51 papers, h 26
  • M. Meixner — 16 papers, h 13
  • M. Meixner — 9 papers
  • M. Meixner — 7 papers, h 4
  • M. Meixner — 6 papers, h 16

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
19952023
most citedSpitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE) I: Overview and Initial Results

718 citations · 7.3k across the 122 of their papers we have counts for

collaborators
Showing 2011 · astro-ph.COShow all

3 papers · 2 filters

astro-ph.CO2011★ 31 cited

Late-time Light Curves of Type II Supernovae: Physical Properties of SNe and Their Environment

Masaaki Otsuka, Margaret Meixner, Nino Panagia +9

We present BVRIJHK band photometry of 6 core-collapse supernovae, SNe 1999bw, 2002hh, 2003gd, 2004et, 2005cs, and 2006bc measured at late epochs (>2 yrs) based on Hubble Space Tele…

astro-ph.CO2011★ 236 cited

Non-Standard Grain Properties, Dark Gas Reservoir, and Extended Submillimeter Excess, Probed by Herschel in the Large Magellanic Cloud

F. Galliano, S. Hony, J. -P. Bernard +13

Aims: In this paper, we perform detailed modelling of the Spitzer and Herschel observations of the LMC, in order to: (i) systematically study the uncertainties and biases affecting…

astro-ph.CO2011★ 77 cited

Evidence for Pre-Existing Dust in the Bright Type IIn SN 2010jl

J. E. Andrews, Geoffrey C. Clayton, R. Wesson +11

SN 2010jl was an extremely bright, Type IIn SNe which showed a significant IR excess no later than 90 days after explosion. We have obtained Spitzer 3.6 and 4.5 \mum and JHK observ…

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