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R. Wagner

4 papers hereh-index 364.2k citations234 works total

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

author position
  • sole author3
  • middle author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph4
same name
  • R. Wagner — 10 papers
  • R. Wagner — 3 papers
  • R. Wagner — 2 papers, h 8
  • R. Wagner — 1 paper, h 10
  • R. Wagner — 1 paper
  • R. Wagner — 1 paper

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
20032008
most citedSynoptic studies of seventeen blazars detected in very high-energy gamma-rays

63 citations · 70 across the 4 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2008★ 5 cited

Correlated Variability in Blazars

Robert Wagner

Blazars are thought to emit highly-collimated outflows, so-called jets. By their close alignment to our line of sight, relativistic beaming effects enable us to observe these jets…

astro-ph2007★ 63 cited

Synoptic studies of seventeen blazars detected in very high-energy gamma-rays

Robert Wagner

Since 2002, the number of detected blazars at gamma-ray energies above 100 GeV has more than doubled. I study 17 blazars currently known to emit E>100 GeV gamma rays. Their intrins…

astro-ph2007★ 2 cited

AGN Observations in the GeV/TeV Energy Range with the MAGIC Telescope

Robert Wagner

MAGIC currently is the largest imaging atmospheric Cerenkov telescope world-wide. Since 2004, gamma-ray emission from several active galactic nuclei in the GeV/TeV energy range has…

astro-ph2003

A Chandra LETGS observation of V4743 Sagittarius: A Super Soft X-ray Source and a Violently Variable Light Curve

J. -U. Ness, S. Starrfield, V. Burwitz +13

V4743 Sgr (Nova Sgr 2002 No. 3) was discovered on 20 September 2002. We obtained a 5ks ACIS-S spectrum in November 2002 and found that the nova was faint in X-rays. We then obtaine…

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