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A. Dasgupta

3 papers here

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

author position
  • first author2
  • middle author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP2
  • astro-ph.SR1
same name
  • A. Dasgupta — 46 papers, h 59
  • A. Dasgupta — 31 papers, h 68
  • A. Dasgupta — 23 papers, h 21
  • A. Dasgupta — 19 papers
  • A. Dasgupta — 11 papers, h 25
  • A. Dasgupta — 9 papers, h 10

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

most citedThe Ophiuchus DIsk Survey Employing ALMA (ODISEA): A Unified Evolutionary Sequence of Planet-Driven Substructures Explaining the Diversity of Disk Morphologies

7 citations · 7 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.SR2025

VLT/ERIS observations of the V960 Mon system: a dust-embedded substellar object formed by gravitational instability?

Anuroop Dasgupta, Alice Zurlo, Philipp Weber +8

V960~Mon is an FU Orionis object that shows strong evidence of a gravitationally unstable spiral arm that is fragmenting into several dust clumps. We report the discovery of a new…

astro-ph.EP2025★ 7 cited

The Ophiuchus DIsk Survey Employing ALMA (ODISEA): A Unified Evolutionary Sequence of Planet-Driven Substructures Explaining the Diversity of Disk Morphologies

Santiago Orcajo, Lucas A. Cieza, Octavio Guilera +21

Understanding the origin of substructures in protoplanetary disks and their connection to planet formation is currently one of the main challenges in astrophysics. While some disks…

astro-ph.EP2025

The Ophiuchus DIsk Survey Employing ALMA (ODISEA): Complete Size Distributions for the 100 Brightest Disks Across Multiplicity and SED Classes

Anuroop Dasgupta, Lucas A. Cieza, Camilo I. Gonzalez Ruilova +16

The size of a protoplanetary disk is a fundamental property, yet most remain unresolved, even in nearby star-forming regions (d ∼ 140-200 pc). We present the complete continuu…

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