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researcher

A. Singhal

20 papers hereh-index 6125.1k citations145 works total

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

author position
  • first author4
  • middle author4
  • last author4

Across the 12 of 20 papers where every author was matched, so the position is known.

fields
  • astro-ph.IM8
  • gr-qc7
  • astro-ph.HE3
  • astro-ph.CO1
  • hep-ex1
same name
  • A. Singhal — 21 papers
  • A. Singhal — 11 papers, h 5
  • A. Singhal — 5 papers, h 9
  • A. Singhal — 2 papers, h 30
  • A. Singhal — 2 papers, h 1
  • A. Singhal — 1 paper, h 1

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 citedA standard siren measurement of the Hubble constant from GW170817 without the electromagnetic counterpart

239 citations · 1.1k across the 20 of their papers we have counts for

collaborators
Showing 2019Show all

3 papers · 1 filter

astro-ph.IM2019★ 71 cited

How effective is machine learning to detect long transient gravitational waves from neutron stars in a real search?

Andrew L. Miller, Pia Astone, Sabrina D'Antonio +12

We present a comprehensive study of the effectiveness of Convolution Neural Networks (CNNs) to detect long duration transient gravitational-wave signals lasting O(hours−days) fro…

gr-qc2019★ 98 cited

All-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1186

We present the results of a search for short-duration gravitational-wave transients in the data from the second observing run of Advanced LIGO and Advanced Virgo. We search for gra…

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.