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M. Ajello

22 papers hereh-index 2120 citations17 works total

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

author position
  • middle author13
  • last author3

Across the 16 of 22 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE13
  • astro-ph.GA7
  • astro-ph.CO2
same name
  • M. Ajello — 296 papers, h 103
  • M. Ajello — 54 papers, h 14
  • M. Ajello — 33 papers, h 3
  • M. Ajello — 10 papers
  • M. Ajello — 4 papers, h 3
  • M. Ajello — 3 papers, h 1

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
20092026
most citedThe Spectral Energy Distribution of Fermi bright blazars

1k citations · 2.1k across the 22 of their papers we have counts for

collaborators
Showing 2012Show all

4 papers · 1 filter

astro-ph.HE2012★ 57 cited

Unidentifed gamma-ray sources: hunting gamma-ray blazars

F. Massaro, R. D'Abrusco, G. Tosti +2

One of the main scientific objectives of the ongoing Fermi mission is unveiling the nature of the unidentified gamma-ray sources (UGSs). Despite the large improvements of Fermi in…

astro-ph.HE2012★ 109 cited

Infrared Colors of the gamma-ray detected blazars

R. D'Abrusco, F. Massaro. M. Ajello, J. E. Grindlay +2

Blazars constitute the most enigmatic class of extragalactic gamma-ray sources, and their observational features have been ascribed to a relativistic jet closely aligned to the lin…

astro-ph.HE2012★ 172 cited

Identification of the infrared non-thermal emission in Blazars

F. Massaro, R. D'Abrusco, M. Ajello +2

Blazars constitute the most interesting and enigmatic class of extragalactic gamma-ray sources dominated by non-thermal emission. In this Letter, we show how the WISE infrared data…

astro-ph.HE2012★ 55 cited

Discovery of hard-spectrum γ-ray emission from the BL Lac object 1ES 0414+009

The HESS Collaboration, A. Abramowski, F. Acero +199

1ES 0414+009 (z = 0.287) is a distant high-frequency-peaked BL Lac object, and has long been considered a likely emitter of very-high energy (VHE, E>100 GeV) gamma-rays due to its…

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