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S. Lombardi

131 papers hereh-index 469.4k citations285 works total

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

author position
  • first author6
  • middle author26
  • last author2

Across the 34 of 131 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE95
  • astro-ph.IM20
  • astro-ph9
  • astro-ph.CO4
  • astro-ph.GA2
  • hep-ex1
same name
  • S. Lombardi — 139 papers, h 41
  • S. Lombardi — 16 papers
  • S. Lombardi — 7 papers, h 4
  • S. Lombardi — 1 paper, h 0
  • S. Lombardi — 1 paper, h 1
  • S. Lombardi — 1 paper, h 30

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
20062026
most citedVery-High-Energy Gamma Rays from a Distant Quasar: How Transparent Is the Universe?

446 citations · 7.5k across the 125 of their papers we have counts for

collaborators
Showing 2012Show all

3 papers · 1 filter

astro-ph.HE2012★ 27 cited

Detection of VHE γ-rays from HESS J0632+057 during the 2011 February X-ray outburst with the MAGIC Telescopes

The MAGIC Collaboration, J. Aleksić, E. A. Alvarez +158

The very high energy (VHE) γ-ray source HESS J0632+057 has recently been confirmed to be a γ-ray binary. The optical counterpart is the Be star MWC 148, and a compact object of unk…

astro-ph.HE2012★ 67 cited

Discovery of VHE gamma-rays from the blazar 1ES 1215+303 with the MAGIC Telescopes and simultaneous multi-wavelength observations

MAGIC Collaboration, J. Aleksić, E. A. Alvarez +164

Context. We present the discovery of very high energy (VHE, E > 100GeV) gamma-ray emission from the BL Lac object 1ES 1215+303 by the MAGIC telescopes and simultaneous multi-wavele…

astro-ph.HE2012★ 89 cited

Morphological and spectral properties of the W51 region measured with the MAGIC telescopes

MAGIC Collaboration, J. Aleksić, E. A. Alvarez +157

The W51 complex hosts the supernova remnant W51C which is known to interact with the molecular clouds in the star forming region W51B. In addition, a possible pulsar wind nebula CX…

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