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researcher

E. Semkov

87 papers hereh-index 261.8k citations167 works total

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

author position
  • sole author1
  • first author18
  • middle author43
  • last author6

Across the 68 of 87 papers where every author was matched, so the position is known.

fields
  • astro-ph.SR43
  • astro-ph.HE28
  • astro-ph9
  • astro-ph.CO3
  • astro-ph.GA2
  • astro-ph.EP1
same name
  • E. Semkov — 13 papers, h 7
  • E. Semkov — 8 papers, h 5
  • E. Semkov — 4 papers
  • E. Semkov — 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
20022025
most citedBlazar spectral variability as explained by a twisting inhomogeneous jet

199 citations · 1.8k across the 86 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

3 papers · 1 filter

astro-ph.CO2011★ 65 cited

Quasi-simultaneous two band optical variability of the blazars 1ES 1959+650 and 1ES 2344+514

Haritma Gaur, Alok C. Gupta, A. Strigachev +8

We report the results of quasi-simultaneous two filter optical monitoring of two high-energy peaked blazars, 1ES 1959+650 and 1ES 2344+514, to search for microvariability and short…

astro-ph.CO2011★ 22 cited

Spectral Energy Distribution variation in BL Lacs and FSRQs

Bindu Rani, Alok C. Gupta, R. Bachev +9

We present the results of our study of spectral energy distributions (SEDs) of a sample of ten low- to intermediate-synchrotron-peaked blazars. We investigate some of the physical…

astro-ph.CO2010★ 35 cited

Short Term Flux and Colour Variations in Low-Energy Peaked Blazars

Bindu Rani, Alok C. Gupta, A. Strigachev +11

We have measured multi-band optical flux and colour variations for a sample of 12 low energy peaked blazars on short, day-to-month, timescales. Our sample contains six BL Lacertae…

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