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researcher

A. Balasubramanian

20 papers hereh-index 10872 citations25 works total

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

author position
  • first author5
  • middle author14
  • last author1

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

fields
  • astro-ph.HE17
  • astro-ph.IM2
  • physics.flu-dyn1
same name
  • A. Balasubramanian — 13 papers, h 5
  • A. Balasubramanian — 10 papers, h 5
  • A. Balasubramanian — 9 papers, h 2
  • A. Balasubramanian — 7 papers, h 25
  • A. Balasubramanian — 2 papers, h 2
  • A. Balasubramanian — 2 papers, 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
20172026
most citedIlluminating Gravitational Waves: A Concordant Picture of Photons from a Neutron Star Merger

822 citations · 1k across the 20 of their papers we have counts for

collaborators
Showing 2020Show all

3 papers · 1 filter

astro-ph.HE2020★ 13 cited

The JAGWAR Prowls LIGO/Virgo O3 Paper I: Radio Search of a Possible Multi-Messenger Counterpart of the Binary Black Hole Merger Candidate S191216ap

D. Bhakta, K. P. Mooley, A. Corsi +7

We present a sensitive search with the Karl G. Jansky Very Large Array (VLA) for the radio counterpart of the gravitational wave candidate S191216ap, classified as a binary black h…

astro-ph.HE2020★ 7 cited

Search for radio remnants of nearby off-axis Gamma-Ray Bursts in a sample of Swift/BAT events

C. Grandorf, J. McCarty, P. Rajkumar +7

The multi-messenger discovery of gravitational waves (GWs) and light from the binary neutron star (NS) merger GW170817, associated with Gamma-Ray Burst (GRB) 170817A and kilonova A…

astro-ph.HE2020★ 13 cited

The Panchromatic Afterglow of GW170817: The full uniform dataset, modeling, comparison with previous results and implications

Sphesihle Makhathini, Kunal P. Mooley, Murray Brightman +35

We present the full panchromatic afterglow light curve data of GW170817, including new radio data as well as archival optical and X-ray data, between 0.5 and 940 days post-merger.…

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