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researcher

D. Saikia

94 papers hereh-index 303.2k citations238 works total

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

author position
  • sole author2
  • first author7
  • middle author41
  • last author24

Across the 74 of 94 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO36
  • astro-ph35
  • astro-ph.GA21
  • astro-ph.HE2
same name
  • D. Saikia — 30 papers, h 4
  • D. Saikia — 12 papers, h 7
  • D. Saikia — 1 paper, h 13
  • D. Saikia — 1 paper, h 1
  • D. Saikia — 1 paper, 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
19982023
most citedEMU: Evolutionary Map of the Universe

430 citations · 3.1k across the 94 of their papers we have counts for

collaborators
Showing 2003Show all

4 papers · 1 filter

astro-ph2003★ 8 cited

J1432+158: the most distant giant quasar

A. K. Singal, C. Konar, D. J. Saikia

We present low-frequency, GMRT (Giant Metrewave Radio Telescope) observations at 333 and 617 MHz of the most-distant giant quasar, J1432+158, which is at a redshift of 1.005. The r…

astro-ph2003★ 31 cited

3C459: A highly asymmetric radio galaxy with a starburst

P. Thomasson, D. J. Saikia, T. W. B. Muxlow

Multifrequency radio observations of the radio galaxy 3C459 using MERLIN, VLA and the EVN, and an optical HST image using the F702W filter are presented. The galaxy has a very asym…

astro-ph2003★ 30 cited

Symmetry Parameters of CSS Sources: Evidence of Fuelling?

D. J. Saikia, S. Jeyakumar, F. Mantovani +4

The compact steep spectrum (CSS) and gigahertz peaked spectrum (GPS) sources are widely believed to be young radiosources, with ages <10^6 yr. If the activity in the nucleus is fue…

astro-ph2003★ 37 cited

Polarization asymmetry in CSS sources: evidence of AGN fuel?

D. J. Saikia, Neeraj Gupta

The compact steep spectrum and gigahertz peaked spectrum sources are widely believed to be young radio sources, with ages <10^6 yr. If the activity in the nucleus is fuelled by the…

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