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researcher

B. S. Sathyaprakash

65 papers here

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

author position
  • sole author1
  • last author1

Across the 2 of 65 papers where every author was matched, so the position is known.

fields
  • gr-qc39
  • astro-ph.HE18
  • astro-ph.CO3
  • astro-ph.IM3
  • astro-ph2
ORCID 0000-0003-3845-7586
same name
  • B. S. Sathyaprakash — 5 papers
  • B. S. Sathyaprakash — 3 papers, h 1
  • B. S. Sathyaprakash — 2 papers
  • B. S. Sathyaprakash — 2 papers
  • B. S. Sathyaprakash — 2 papers
  • B. S. Sathyaprakash — 1 paper

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
20032026
most citedGW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

9.8k citations · 30.6k across the 65 of their papers we have counts for

collaborators
Showing 2019Show all

3 papers · 1 filter

gr-qc2019★ 564 cited

Open data from the first and second observing runs of Advanced LIGO and Advanced Virgo

The LIGO Scientific Collaboration, the Virgo Collaboration, R. Abbott +1245

Advanced LIGO and Advanced Virgo are actively monitoring the sky and collecting gravitational-wave strain data with sufficient sensitivity to detect signals routinely. In this pape…

gr-qc2019★ 383 cited

A guide to LIGO-Virgo detector noise and extraction of transient gravitational-wave signals

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1135

The LIGO Scientific Collaboration and the Virgo Collaboration have cataloged eleven confidently detected gravitational-wave events during the first two observing runs of the advanc…

astro-ph.HE2019★ 149 cited

All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1130

We present results of an all-sky search for continuous gravitational waves (CWs), which can be produced by fast-spinning neutron stars with an asymmetry around their rotation axis,…

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