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M. Heidelberg

9 papers hereh-index 7280 citations17 works total

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

fields
  • astro-ph4
  • astro-ph.EP1
  • astro-ph.GA1
  • astro-ph.IM1
  • astro-ph.SR1
  • physics.acc-ph1
same name
  • M. Heidelberg — 1 paper, h 2
  • M. Heidelberg — 1 paper, h 1
  • M. Heidelberg — 1 paper, h 2
  • M. Heidelberg — 1 paper, h 1
  • M. Heidelberg — 1 paper, 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
19992019
most citedGamma rays from clusters of galaxies

92 citations · 362 across the 9 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2007★ 44 cited

Host galaxies of bright high redshift quasars: Luminosities and colours

M. Schramm, L. Wisotzki, K. Jahnke

We present the results of a near-infrared imaging study of high redshift (z~3) quasars using the ESO-VLT. Our targets were selected to have luminosities among the highest known (ab…

astro-ph2007

HD97048: a closer look to the disk

Doucet, C., Habart +11

Aims: Today, large ground-based instruments, like VISIR on the VLT, providing diffraction-limited (about 0.3 arcsec) images in the mid-infrared where strong PAH features appear ena…

astro-ph2007★ 92 cited

Gamma rays from clusters of galaxies

Pasquale Blasi, Stefano Gabici, Gianfranco Brunetti

Clusters of galaxies and the large scale filaments that connect neighboring clusters are expected to be sites of acceleration of charged particles and sources of non-thermal radiat…

astro-ph1999

IRAS 17393-3004, a late-type supergiant surrounded by a dust shell

Sabine Philipp, Richard J. Tuffs, Peter G. Mezger +1

Infrared observations of IRAS 17393-3004, including a full scan ISOSWS are presented. The ISOSWS spectrum shows two prominent dust emission peaks at lambda 10.4mu and 17.5mu confir…

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