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researcher

S. Mathur

56 papers hereh-index 4710k citations372 works total

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

author position
  • sole author3
  • first author5
  • middle author30
  • last author6

Across the 44 of 56 papers where every author was matched, so the position is known.

fields
  • astro-ph55
  • astro-ph.HE1
same name
  • S. Mathur — 29 papers, h 56
  • S. Mathur — 12 papers, h 64
  • S. Mathur — 6 papers
  • S. Mathur — 6 papers, h 18
  • S. Mathur — 5 papers, h 25
  • S. Mathur — 3 papers, h 5

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
19952009
most citedRadio-loud Narrow-Line Type 1 Quasars

337 citations · 652 across the 23 of their papers we have counts for

collaborators
Showing 2007 · astro-phShow all

4 papers · 2 filters

astro-ph2007★ 7 cited

On the nature of the z=0 X-ray absorbers: I. Clues from an external group

Smita Mathur, Gregory R. Sivakoff, Rik J. Williams +1

Absorption lines of OVII at redshift zero are observed in high quality Chandra spectra of extragalactic sightlines. The location of the absorber producing these lines, whether from…

astro-ph2007

Lost Baryons at Low Redshift

Smita Mathur, Fabrizio Nicastro, Rik J. Williams

We review our attempts to discover lost baryons at low redshift with ``X-ray forest'' of absorption lines from the warm-hot intergalactic medium. We discuss the best evidence to da…

astro-ph2007★ 10 cited

Variable X-ray Absorption toward Gravitationally-Lensed Blazar PKS1830-211

Xinyu Dai, Smita Mathur, George Chartas +2

We present X-ray spectral analysis of five Chandra and XMM-Newton observations of the gravitationally-lensed blazar PKS1830-211 from 2000 to 2004. We show that the X-ray absorption…

astro-ph2007★ 1 cited

Time-Evolving Photoionization: the Thin and Compact X-Ray Wind of NGC 4051

Fabrizio Nicastro, Yair Krongold, Martin Elvis +3

We discuss the power of time-evolving photoionization as a diagnostic tool to measure the electron density of photoionized gas. We apply this technique to a XMM-Newton observation…

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