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researcher

F. Shankar

23 papers hereh-index 121.3k citations30 works total

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

author position
  • first author1
  • middle author16
  • last author2

Across the 19 of 23 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA15
  • astro-ph.CO5
  • astro-ph.HE3
same name
  • F. Shankar — 57 papers, h 8
  • F. Shankar — 47 papers, h 12
  • F. Shankar — 45 papers, h 25
  • F. Shankar — 11 papers, h 10
  • F. Shankar — 10 papers, h 3
  • F. Shankar — 8 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
20112026
most citedBolometric luminosities and Eddington ratios of X-ray selected Active Galactic Nuclei in the XMM-COSMOS survey

417 citations · 1.8k across the 23 of their papers we have counts for

collaborators
Showing 2016Show all

3 papers · 1 filter

astro-ph.GA2016★ 76 cited

Constraining the UV emissivity of AGN throughout cosmic time via X-ray surveys

F. Ricci, S. Marchesi, F. Shankar +2

The cosmological process of hydrogen (HI) reionization in the intergalactic medium is thought to be driven by UV photons emitted by star-forming galaxies and ionizing active galact…

astro-ph.GA2016★ 25 cited

The Chandra COSMOS Legacy Survey: Clustering of X-ray selected AGN at 2.9<z<5.5 using photometric redshift Probability Distribution Functions

V. Allevato, F. Civano, A. Finoguenov +16

We present the measurement of the projected and redshift space 2-point correlation function (2pcf) of the new catalog of Chandra COSMOS-Legacy AGN at 2.9≤z≤5.5 ($\langle…

astro-ph.GA2016★ 29 cited

The optical-UV emissivity of quasars: dependence on black hole mass and radio loudness

Francesco Shankar, Giorgio Calderone, Christian Knigge +15

We analyzed a large sample of radio-loud and radio-quiet quasar spectra at redshift 1.0 < z < 1.2 to compare the inferred underlying quasar continuum slopes (after removal of the h…

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