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D. Mukherjee

24 papers hereh-index 4815.3k citations164 works total

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

author position
  • first author1
  • middle author21

Across the 22 of 24 papers where every author was matched, so the position is known.

fields
  • gr-qc15
  • astro-ph.IM6
  • astro-ph.HE3
same name
  • D. Mukherjee — 42 papers, h 55
  • D. Mukherjee — 23 papers, h 48
  • D. Mukherjee — 22 papers
  • D. Mukherjee — 12 papers, h 7
  • D. Mukherjee — 10 papers, h 5
  • D. Mukherjee — 8 papers, h 3

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
20182026
most citedAll-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data

149 citations · 318 across the 19 of their papers we have counts for

collaborators
Showing 2020 · astro-ph.IMShow all

3 papers · 2 filters

astro-ph.IM2020

Automating the Inclusion of Subthreshold Signal-to-Noise Ratios for Rapid Gravitational-Wave Localization

Cody Messick, Surabhi Sachdev, Kipp Cannon +29

The accurate localization of gravitational-wave (GW) events in low-latency is a crucial element in the search for further multimessenger signals from these cataclysmic events. The…

astro-ph.IM2020

GstLAL: A software framework for gravitational wave discovery

Kipp Cannon, Sarah Caudill, Chiwai Chan +28

The GstLAL library, derived from Gstreamer and the LIGO Algorithm Library, supports a stream-based approach to gravitational-wave data processing. Although GstLAL was primarily des…

astro-ph.IM2020★ 1 cited

Improving the background estimation technique in the GstLAL inspiral pipeline with the time-reversed template bank

Chiwai Chan, Kipp Cannon, Sarah Caudill +20

Background estimation is important for determining the statistical significance of a gravitational-wave event. Currently, the background model is constructed numerically from the s…

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