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researcher

D. Chattopadhyay

39 papers hereh-index 173.8k citations43 works total

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

author position
  • sole author1
  • first author9
  • middle author18
  • last author6

Across the 34 of 39 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE27
  • astro-ph.GA5
  • astro-ph.SR3
  • gr-qc3
  • astro-ph.IM1
same name
  • D. Chattopadhyay — 4 papers, h 7
  • D. Chattopadhyay — 3 papers, h 28
  • D. Chattopadhyay — 3 papers, h 3
  • D. Chattopadhyay — 2 papers, h 1
  • D. Chattopadhyay — 1 paper, h 1
  • D. Chattopadhyay — 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
20192026
most citedGWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run

2.4k citations · 3.7k across the 39 of their papers we have counts for

collaborators
Showing 2026Show all

3 papers · 1 filter

astro-ph.HE2026

Neutron Star Mass across Binary Pulsar Subpopulations: Mass-Spin Correlation, Mass Distributions, and Moment of Inertia Effects

Debatri Chattopadhyay

We present a hierarchical Bayesian analysis of the joint mass, spin, and orbital properties of ∼50 Galactic binary radio pulsars with measured neutron star masses, classified…

astro-ph.HE2026

Transitions in the Mass-ratio and Spin Properties of Binary Black Holes in GWTC-5

Elizabeth Flanagan, Fabio Antonini, Thomas Callister +4

We analyze the mass-ratio and effective-spin (χeff​) distributions of binary black hole mergers in the latest gravitational-wave catalog, GWTC-5, as a function of primary m…

astro-ph.HE2026

Repopulating the pair-instability mass gap without sustained growth to massive IMBHs: the case of 47\,Tuc

Debatri Chattopadhyay, Daniel Marín Pina, Mark Gieles +2

We model the formation and retention of the most massive black hole (BH) in 47~Tuc using the semi-analytical code \texttt{cBHBd}, coupling cluster evolution with binary BH dynamics…

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