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researcher

D. Munshi

177 papers hereh-index 8041.5k citations338 works total

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

author position
  • sole author5
  • first author56
  • middle author27
  • last author10

Across the 98 of 177 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO105
  • astro-ph39
  • astro-ph.GA25
  • astro-ph.IM6
  • astro-ph.HE1
  • quant-ph1
same name
  • D. Munshi — 25 papers
  • D. Munshi — 4 papers
  • D. Munshi — 1 paper
  • D. Munshi — 1 paper

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
19932022
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 25.6k across the 177 of their papers we have counts for

collaborators
Showing 2004 · astro-phShow all

4 papers · 2 filters

astro-ph2004★ 6 cited

Covariance of Weak Lensing Observables

Dipak Munshi, Patrick Valageas

Analytical expressions for covariances of weak lensing statistics related to the aperture mass $\Map$ are derived for realistic survey geometries such as SNAP for a range of smooth…

astro-ph2004★ 5 cited

On Cross-correlating Weak Lensing Surveys

Dipak Munshi, Patrick Valageas

The present generation of weak lensing surveys will be superseded by surveys run from space with much better sky coverage and high level of signal to noise ratio, such as SNAP. How…

astro-ph2004★ 18 cited

Evolution of the Cosmological Density Distribution Function: A New Analytical Model

Patrick Valageas, Dipak Munshi

The one-point probability distribution function (pdf) of the large-scale density field is an important tool to follow the evolution of cosmological structures. In this paper we pre…

astro-ph2004★ 17 cited

On the estimation of gravity-induced non-Gaussianities from weak lensing surveys

Patrick Valageas, Dipak Munshi, Andrew J. Barber

We study various measures of weak lensing distortions in future surveys, taking into account the noise arising from the finite survey size and the intrinsic ellipticity of galaxies…

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