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20122026
most citedDark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

1.2k citations · 6.2k across the 88 of their papers we have counts for

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Showing 2019Show all

6 papers · 1 filter

astro-ph.CO2019★ 57 cited

Baryonic effects for weak lensing. Part II. Combination with X-ray data and extended cosmologies

Aurel Schneider, Alexandre Refregier, Sebastian Grandis +6

An accurate modelling of baryonic feedback effects is required to exploit the full potential of future weak-lensing surveys such as Euclid or LSST. In this second paper in a series…

physics.comp-ph2019★ 1 cited

Cosmological N-body simulations: a challenge for scalable generative models

Nathanaël Perraudin, Ankit Srivastava, Aurelien Lucchi +3

Deep generative models, such as Generative Adversarial Networks (GANs) or Variational Autoencoders (VAs) have been demonstrated to produce images of high visual quality. However, t…

astro-ph.CO2019★ 26 cited

Monte Carlo Control Loops for cosmic shear cosmology with DES Year 1

T. Kacprzak, J. Herbel, A. Nicola +52

Weak lensing by large-scale structure is a powerful probe of cosmology and of the dark universe. This cosmic shear technique relies on the accurate measurement of the shapes and re…

astro-ph.CO2019★ 152 cited

Cosmological constraints with deep learning from KiDS-450 weak lensing maps

Janis Fluri, Tomasz Kacprzak, Aurelien Lucchi +4

Convolutional Neural Networks (CNN) have recently been demonstrated on synthetic data to improve upon the precision of cosmological inference. In particular they have the potential…

astro-ph.CO2019★ 37 cited

Effects of baryons on weak lensing peak statistics

Andreas J. Weiss, Aurel Schneider, Raphael Sgier +3

Upcoming weak-lensing surveys have the potential to become leading cosmological probes provided all systematic effects are under control. Recently, the ejection of gas due to feedb…

cs.LG2019★ 15 cited

DeepSphere: towards an equivariant graph-based spherical CNN

Michaël Defferrard, Nathanaël Perraudin, Tomasz Kacprzak +1

Spherical data is found in many applications. By modeling the discretized sphere as a graph, we can accommodate non-uniformly distributed, partial, and changing samplings. Moreover…