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Tanuka Chattopadhyay

Researcher at University of Calcutta

Publications -  60
Citations -  654

Tanuka Chattopadhyay is an academic researcher from University of Calcutta. The author has contributed to research in topics: Galaxy & Elliptical galaxy. The author has an hindex of 13, co-authored 57 publications receiving 550 citations. Previous affiliations of Tanuka Chattopadhyay include Inter-University Centre for Astronomy and Astrophysics.

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Statistical Evidence for Three Classes of Gamma-Ray Bursts

TL;DR: In this article, two multivariate clustering techniques, the K-means partitioning method and the Dirichlet process of mixture modeling, have been applied to the BATSE gamma-ray burst (GRB) catalog, to obtain the optimum number of coherent groups.
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Structures in the fundamental plane of early‐type galaxies

TL;DR: In this article, a multivariate cluster and cladistic analysis of a sample of 56 low-redshift galaxy clusters containing 699 early-type galaxies, using four parameters: effective radius, velocity dispersion, surface brightness averaged over effective radius and Mg2 index, was performed.
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Study of NGC 5128 Globular Clusters Under Multivariate Statistical Paradigm

TL;DR: In this article, an objective classification of the globular clusters (GCs) of NGC 5128 has been carried out by using a model-based approach of cluster analysis.
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A six-parameter space to describe galaxy diversification

TL;DR: In this paper, a sample of 424 early-type galaxies described by 25 parameters, ten of which are Lick indices, was used to identify the most structuring parameters and determine an evolutionary classification of these objects, and four independent statistical methods were used to investigate the discriminant properties of the observables and the partitioning of the 424 galaxies.
Journal ArticleDOI

A six-parameter space to describe galaxy diversification

TL;DR: In this paper, a sample of 424 early-type galaxies described by 25 parameters, ten of which are Lick indices, was used to identify the most structuring parameters and determine an evolutionary classification of these objects, and four independent statistical methods were used to investigate the discriminant properties of the observables and the partitioning of the 424 galaxies.