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researcher

S. Chatterjee

4 papers hereh-index 5317.8k citations191 works total

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

author position
  • first author1
  • middle author2

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph4
same name
  • S. Chatterjee — 2 papers, h 43
  • S. Chatterjee — 2 papers, h 2
  • S. Chatterjee — 1 paper, h 43
  • S. Chatterjee — 1 paper, h 15
  • S. Chatterjee — 1 paper, h 30

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
20022005
most citedGetting Its Kicks: A VLBA Parallax for the Hyperfast Pulsar B1508+55

180 citations · 320 across the 3 of their papers we have counts for

collaborators

4 papers

astro-ph2005★ 180 cited

Getting Its Kicks: A VLBA Parallax for the Hyperfast Pulsar B1508+55

S. Chatterjee, W. H. T. Vlemmings, W. F. Brisken +7

The highest velocity neutron stars establish stringent constraints on natal kicks, asymmetries in supernova core collapse, and the evolution of close binary systems. Here we presen…

astro-ph2005★ 1 cited

Pulsar Astrometry at the Microarcsecond Level

W. H. T. Vlemmings, S. Chatterjee, W. F. Brisken +12

Determination of pulsar parallaxes and proper motions addresses fundamental astrophysical questions. We have recently finished a VLBI astrometry project to determine the proper mot…

astro-ph2003★ 139 cited

Pulsar Parallaxes at 5 GHz with the Very Long Baseline Array

S. Chatterjee, J. M. Cordes, W. H. T. Vlemmings +3

We present the first pulsar parallaxes measured with phase-referenced pulsar VLBI observations at 5 GHz. Due to the steep spectra of pulsars, previous astrometric measurements have…

astro-ph2002

XMM-Newton sets the record straight: No X-ray emission detected from PSR J0631+1036

J. Kennea, F. Cordova, S. Chatterjee +5

The pulsar PSR J0631+1036 was discovered during a radio search of Einstein X-ray source error circles. A detection of a 288ms sinusoidal modulation in the ASCA lightcurve, the same…

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