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Krishna Kumar Singh

6 papers hereh-index 467 citations16 works total

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

author position
  • first author1
  • middle author3
  • last author2

Across the 6 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3
  • astro-ph.IM1
  • gr-qc1
  • physics.gen-ph1
same name
  • Krishna Kumar Singh — 23 papers, h 18
  • Krishna Kumar Singh — 7 papers, h 6
  • Krishna Kumar Singh — 5 papers, h 8
  • Krishna kumar Singh — 5 papers, h 4
  • Krishna Kumar Singh — 4 papers, h 3
  • Krishna Kumar Singh — 4 papers, h 2

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
20172024
most citedA time dependent approach to model X-ray and γ--ray light curves of Mrk 421 observed during the flare in February 2010

15 citations · 30 across the 6 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2024★ 3 cited

Central Engine and Spectral Energy Distribution Properties of High Redshift Gamma Ray Blazars

A. Tolamatti, K. K. Singh, K. K. Yadav

We report on the properties of central engines in the γ-ray blazars located at high redshifts beyond z~>~0.4, where the extra-galactic background light (EBL) starts affecting the…

astro-ph.HE2019★ 3 cited

Results from the long-term Fermi-LAT observations of the white dwarf binary pulsar AR Scorpii

Q. Kaplan, P. J. Meintjes, K. K. Singh +3

The discovery of the white dwarf binary system AR Scorpii (AR Sco) with its fascinating non-thermal dominated multi-frequency emission has sparked renewed interest in potential hig…

astro-ph.HE2017★ 15 cited

A time dependent approach to model X-ray and γ--ray light curves of Mrk 421 observed during the flare in February 2010

K K Singh, S Sahayanathan, A Sinha +18

Strong X-ray and γ--ray flares have been detected in February 2010 from the high synchrotron peaked blazar Mrk 421 (z=0.031). With the motivation of understanding the physics inv…

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