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S. Kumari

12 papers hereh-index 6108 citations33 works total

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

author position
  • first author6
  • middle author3
  • last author3

Across the 12 of 12 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA11
  • astro-ph.HE1
same name
  • S. Kumari — 12 papers, h 5
  • S. Kumari — 10 papers, h 11
  • S. Kumari — 6 papers, h 16
  • S. Kumari — 6 papers, h 8
  • S. Kumari — 5 papers, h 20
  • S. Kumari — 4 papers, h 3

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
20212026
most citedSearch for hybrid morphology radio galaxies from FIRST survey at 1400 MHz

11 citations · 44 across the 12 of their papers we have counts for

collaborators
Showing 2021Show all

4 papers · 1 filter

astro-ph.GA2021★ 11 cited

Search for hybrid morphology radio galaxies from FIRST survey at 1400 MHz

Shobha Kumari, Sabyasachi Pal

Hybrid Morphology Radio Sources (HyMoRS) are a very rare subclass of radio galaxies with apparent mixed FR morphology, i.e. these galaxies seem to have an FR-I structure on one sid…

astro-ph.GA2021

Winged Radio Sources from LOFAR Two-metre Sky Survey First Data Release (LoTSS DR1)

Sabyasachi Pal, Shobha Kumari

Winged radio sources are a small sub-class of extragalactic radio sources which display a pair of low surface brightness radio lobes, known as `wings' aligned at a certain angle wi…

astro-ph.HE2021★ 1 cited

Head Tail Radio Sources from VLA FIRST Survey

Sabyasachi Pal, Shobha Kumari

The study of Head Tail (HT) radio galaxies track the information of associated galaxy clusters. With the help of the VLA FIRST survey at 1.4 GHz, we detected 607 new HT radio sourc…

astro-ph.GA2021★ 10 cited

A new catalogue of head-tail radio galaxies from LoTSS DR1

Sabyasachi Pal, Shobha Kumari

The unique morphology of head-tail (HT) radio galaxies suggests that radio jets and their intra-cluster medium interact strongly. We conducted a systematic search for HT radio gala…

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