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S. Chatterjee

148 papers hereh-index 5814.2k citations832 works total

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

author position
  • first author13
  • middle author9

Across the 22 of 148 papers where every author was matched, so the position is known.

fields
  • hep-ex102
  • nucl-ex13
  • physics.ins-det9
  • hep-ph8
  • astro-ph.CO6
  • cond-mat.mes-hall6
same name
  • S. Chatterjee — 461 papers
  • S. Chatterjee — 178 papers
  • S. Chatterjee — 109 papers, h 43
  • S. Chatterjee — 107 papers, h 53
  • S. Chatterjee — 95 papers, h 44
  • S. Chatterjee — 89 papers, h 43

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
20162026
most citedSearch for production of four top quarks in final states with same-sign or multiple leptons in proton-proton collisions at s​= 13 TeV

112 citations · 2.1k across the 144 of their papers we have counts for

collaborators
Showing 2017Show all

3 papers · 1 filter

nucl-ex2017★ 30 cited

Principal-component analysis of two-particle azimuthal correlations in PbPb and pPb collisions at CMS

CMS Collaboration

For the first time a principle-component analysis is used to separate out different orthogonal modes of the two-particle correlation matrix from heavy ion collisions. The analysis…

astro-ph.IM2017★ 13 cited

Simulated foreground predictions for HI at z = 3.35 with the Ooty Wide Field Array: I. Instrument and the foregrounds

Visweshwar Ram Marthi, Suman Chatterjee, Jayaram Chengalur +1

Foreground removal is the most important step in detecting the large-scale redshifted HI 21-cm signal. Modelling foreground spectra is challenging and is further complicated by the…

astro-ph.CO2017★ 7 cited

Simulating the z = 3.35 HI 21-cm visibility signal for the Ooty Wide Field Array(OWFA)

Suman Chatterjee, S. Bharadwaj, V. R. Marthi

The upcoming Ooty Wide Field Array (OWFA) will operate at 326.5MHz which corresponds to the redshifted 21-cm signal from neutral hydrogen (HI) at z = 3.35. We present t…

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