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researcher

E. Behar

135 papers hereh-index 406.1k citations293 works total

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

author position
  • sole author1
  • first author16
  • middle author68
  • last author32

Across the 117 of 135 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE47
  • astro-ph40
  • astro-ph.GA28
  • astro-ph.CO9
  • astro-ph.IM6
  • astro-ph.SR5
same name
  • E. Behar — 77 papers, h 10
  • E. Behar — 56 papers, h 29
  • E. Behar — 48 papers, h 19

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
20002026
most citedThe Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission

395 citations · 5.4k across the 130 of their papers we have counts for

collaborators
Showing 2021 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2021★ 24 cited

Transient obscuration event captured in NGC~3227 II. Warm absorbers and obscuration events in archival XMM-Newton and NuSTAR observations

Yijun Wang, Jelle Kaastra, Missagh Mehdipour +18

The relation between warm absorber (WA) outflows of AGN and nuclear obscuration activities caused by optically-thick clouds (obscurers) crossing the line of sight is unclear. NGC 3…

astro-ph.GA2021★ 5 cited

The Great Slump: Mrk926 reveals discrete and varying Balmer line satellite components during a drastic phase of decline

Wolfram Kollatschny, Martin W. Ochmann, Shai Kaspi +9

Mrk926 is known to be a highly variable AGN with very broad line profiles. We studied the continuum and line profile variations of this object with high temporal resolution in orde…

astro-ph.GA2021★ 25 cited

The PG-RQS survey. Building the radio spectral distribution of radio-quiet quasars. I. The 45-GHz data

R. D. Baldi, A. Laor, E. Behar +4

The origin of the radio emission in radio-quiet quasars (RQQs) remains unclear. Radio emission may be produced by a scaled-down version of the relativistic jets observed in radio-l…

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