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researcher

S. Bhattacharya

25 papers hereh-index 12357 citations38 works total

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

author position
  • sole author1
  • first author11
  • middle author5
  • last author4

Across the 21 of 25 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA22
  • astro-ph.HE1
  • astro-ph.IM1
  • astro-ph.SR1
same name
  • S. Bhattacharya — 393 papers
  • S. Bhattacharya — 287 papers
  • S. Bhattacharya — 283 papers
  • S. Bhattacharya — 128 papers
  • S. Bhattacharya — 75 papers, h 23
  • S. Bhattacharya — 71 papers, h 28

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 citedML-MOC: Machine Learning (kNN and GMM) based Membership Determination for Open Clusters

69 citations · 387 across the 23 of their papers we have counts for

collaborators
Showing 2021Show all

3 papers · 1 filter

astro-ph.GA2021★ 33 cited

Tidal tails in the disintegrating open cluster NGC 752

Souradeep Bhattacharya, Manan Agarwal, Khushboo K. Rao +1

We utilize the robust membership determination algorithm, ML-MOC, on the precise astrometric and deep photometric data from Gaia Early Data Release 3 within a region of radius 5$^{…

astro-ph.GA2021★ 20 cited

Determination of dynamical ages of open clusters through the A+ parameter -- I

Khushboo K. Rao, Kaushar Vaidya, Manan Agarwal +1

The sedimentation level of blue straggler stars (BSS) has been shown to be a great tool to investigate the dynamical states of globular clusters (GCs). The area enclosed between th…

astro-ph.GA2021

The survey of planetary nebulae in Andromeda (M31) III. Constraints from deep planetary nebula luminosity functions on the origin of the inner halo substructures in M31

Souradeep Bhattacharya, Magda Arnaboldi, Ortwin Gerhard +4

The Andromeda (M31) galaxy displays several substructures in its inner halo whose origin as remnants of accreted satellites or perturbations of the pre-existing disc are encoded in…

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