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S. Srinivasan

2 papers hereh-index 6790 citations12 works total

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

author position
  • middle author2

Across the 2 of 2 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
same name
  • S. Srinivasan — 37 papers, h 28
  • S. Srinivasan — 27 papers, h 30
  • S. Srinivasan — 19 papers, h 15
  • S. Srinivasan — 14 papers, h 7
  • S. Srinivasan — 12 papers, h 15
  • S. Srinivasan — 11 papers, h 20

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

most citedTowards an observationally motivated AGN dusty torus model -- II. The roles of density distribution and chemical composition of the dust

1 citations · 1 across the 2 of their papers we have counts for

collaborators

2 papers

astro-ph.GA2025★ 1 cited

Towards an observationally motivated AGN dusty torus model -- II. The roles of density distribution and chemical composition of the dust

Omar Ulises Reyes-Amador, Omaira González-Martín, Jacopo Fritz +5

Several models of nuclear dust in active galactic nuclei (AGN) have been presented in the literature to determine its physical and geometrical properties, usually assuming the dust…

astro-ph.GA2024

Towards an observationally motivated AGN dusty torus model. I. Dust chemical composition from the modeling of Spitzer spectra

Omar Ulises Reyes-Amador, Jacopo Fritz, Omaira González-Martín +7

Spectral energy distribution (SED) fitting is one of most commonly used techniques to study the dust properties in Active Galactic Nuclei (AGN). Works implementing this technique c…

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