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researcher

S. Rakshit

53 papers hereh-index 191.1k citations76 works total

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

author position
  • sole author1
  • first author9
  • middle author33
  • last author5

Across the 48 of 53 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA35
  • astro-ph.HE17
  • astro-ph.SR1
same name
  • S. Rakshit — 14 papers, h 13
  • S. Rakshit — 7 papers, h 4
  • S. Rakshit — 1 paper, h 5
  • S. Rakshit — 1 paper
  • S. Rakshit — 1 paper, h 12
  • S. Rakshit — 1 paper, 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
20172026
most citedHost galaxy properties of quasi-periodically erupting X-ray sources

83 citations · 704 across the 41 of their papers we have counts for

collaborators
Showing 2017Show all

4 papers · 1 filter

astro-ph.GA2017★ 70 cited

PAH features within few hundred parsecs of active galactic nuclei

J. J. Jensen, S. F. Hönig, S. Rakshit +6

Spectral features from PAH molecules observed in the mid-IR range are typically used to infer the amount of recent and ongoing star formation (SF) on kpc scales around AGN where mo…

astro-ph.GA2017

Properties of Narrow line Seyfert 1 galaxies

Suvendu Rakshit, C. S. Stalin, Hum Chand +1

Narrow line Seyfert 1 (NLSy1) galaxies constitute a class of active galactic nuclei characterized by the full width at half maximum (FWHM) of the Hβ broad emission line < 2000 km…

astro-ph.GA2017★ 67 cited

Optical Variability of Narrow and Broad line Seyfert 1 galaxies

Suvendu Rakshit, C. S. Stalin

We studied optical variability (OV) of a large sample of narrow-line Seyfert 1 (NLSy1) and broad-line Seyfert 1 (BLSy1) galaxies with z<0.8 to investigate any differences in their…

astro-ph.SR2017★ 5 cited

Science cases for a visible interferometer

Philippe Stee, France Allard, Myriam Benisty +54

High spatial resolution is the key for the understanding various astrophysical phenomena. But even with the future E-ELT, single dish instruments are limited to a spatial resolutio…

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