activity
20162021
most citedNon-Gaussian information from weak lensing data via deep learning

128 citations · 501 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2021

Robust marginalization of baryonic effects for cosmological inference at the field level

Francisco Villaescusa-Navarro, Shy Genel, Daniel Angles-Alcazar +11

We train neural networks to perform likelihood-free inference from 2D maps containing the total mass surface density from thousands of hydrodynamic simula…

astro-ph.CO2021★ 19 cited

Multifield Cosmology with Artificial Intelligence

Francisco Villaescusa-Navarro, Daniel Anglés-Alcázar, Shy Genel +10

Astrophysical processes such as feedback from supernovae and active galactic nuclei modify the properties and spatial distribution of dark matter, gas, and galaxies in a poorly und…

astro-ph.CO2021★ 31 cited

Simultaneously constraining cosmology and baryonic physics via deep learning from weak lensing

Tianhuan Lu, Zoltán Haiman, José Manuel Zorrilla Matilla

Ongoing and planned weak lensing (WL) surveys are becoming deep enough to contain information on angular scales down to a few arcmin. To fully extract information from these small…

astro-ph.CO2021★ 12 cited

Cosmological Constraints from Weak Lensing Peaks: Can Halo Models Accurately Predict Peak Counts?

Alina Sabyr, Zoltán Haiman, José Manuel Zorrilla Matilla +1

In order to extract full cosmological information from next-generation large and high-precision weak lensing (WL) surveys (e.g. Euclid, Roman, LSST), higher-order statistics that p…

astro-ph.CO2020★ 47 cited

Interpreting deep learning models for weak lensing

José Manuel Zorrilla Matilla, Manasi Sharma, Daniel Hsu +1

Deep Neural Networks (DNNs) are powerful algorithms that have been proven capable of extracting non-Gaussian information from weak lensing (WL) data sets. Understanding which featu…

astro-ph.CO2019★ 15 cited

Optimizing simulation parameters for weak lensing analyses involving non-Gaussian observables

José Manuel Zorrilla Matilla, Stefan Waterval, Zoltán Haiman

We performed a series of numerical experiments to quantify the sensitivity of the predictions for weak lensing statistics obtained in raytracing DM-only simulations, to two hyper-p…

astro-ph.GA2019★ 13 cited

Probing gaseous galactic halos through the rotational kSZ effect

José Manuel Zorrilla Matilla, Zoltán Haiman

The rotational kinematic Sunyaev-Zeldovich (rkSZ) signal, imprinted on the cosmic microwave background (CMB) by the gaseous halos (spinning "atmospheres") of foreground galaxies, w…

astro-ph.CO2018★ 63 cited

Constraining neutrino mass with tomographic weak lensing peak counts

Zack Li, Jia Liu, José Manuel Zorrilla Matilla +1

Massive cosmic neutrinos change the structure formation history by suppressing perturbations on small scales. Weak lensing data from galaxy surveys probe the structure evolution an…

astro-ph.CO2018★ 128 cited

Non-Gaussian information from weak lensing data via deep learning

Arushi Gupta, José Manuel Zorrilla Matilla, Daniel Hsu +1

Weak lensing maps contain information beyond two-point statistics on small scales. Much recent work has tried to extract this information through a range of different observables o…

astro-ph.CO2017★ 126 cited

MassiveNuS: Cosmological Massive Neutrino Simulations

Jia Liu, Simeon Bird, José Manuel Zorrilla Matilla +5

The non-zero mass of neutrinos suppresses the growth of cosmic structure on small scales. Since the level of suppression depends on the sum of the masses of the three active neutri…

astro-ph.CO2017★ 15 cited

Geometry and growth contributions to cosmic shear observables

José Manuel Zorrilla Matilla, Zoltán Haiman, Andrea Petri +1

We explore the sensitivity of weak lensing observables to the expansion history of the universe and to the growth of cosmic structures, as well as the relative contribution of both…

astro-ph.CO2016★ 32 cited

Do dark matter halos explain lensing peaks?

José Manuel Zorrilla Matilla, Zoltán Haiman, Daniel Hsu +2

We have investigated a recently proposed halo-based model, Camelus, for predicting weak-lensing peak counts, and compared its results over a collection of 162 cosmologies with thos…