activity
20212025
most citedThe CAMELS Multifield Dataset: Learning the Universe's Fundamental Parameters with Artificial Intelligence

69 citations · 388 across the 23 of their papers we have counts for

collaborators

23 papers

astro-ph.CO2025★ 1 cited

Mitigating Model Misspecification in Simulation-Based Inference for Galaxy Clustering

Sébastien Pierre, Bruno Régaldo-Saint Blancard, ChangHoon Hahn +1

Simulation-based inference (SBI) has become an important tool in cosmology for extracting additional information from observational data using simulations. However, all cosmologica…

cs.LG2024

Contextual Counting: A Mechanistic Study of Transformers on a Quantitative Task

Siavash Golkar, Alberto Bietti, Mariel Pettee +12

Transformers have revolutionized machine learning across diverse domains, yet understanding their behavior remains crucial, particularly in high-stakes applications. This paper int…

astro-ph.CO2024★ 4 cited

{\sc SimBIG}: Cosmological Constraints using Simulation-Based Inference of Galaxy Clustering with Marked Power Spectra

Elena Massara, ChangHoon Hahn, Michael Eickenberg +7

We present the first CDM cosmological analysis performed on a galaxy survey using marked power spectra. The marked power spectrum is the two-point function of a marked field, wh…

astro-ph.CO2024★ 1 cited

: Cosmological Constraints from the Redshift-Space Galaxy Skew Spectra

Jiamin Hou, Azadeh Moradinezhad Dizgah, ChangHoon Hahn +7

Extracting the non-Gaussian information of the cosmic large-scale structure (LSS) is vital in unlocking the full potential of the rich datasets from the upcoming stage-IV galaxy su…

astro-ph.CO2023★ 1 cited

SimBIG: Field-level Simulation-Based Inference of Galaxy Clustering

Pablo Lemos, Liam Parker, ChangHoon Hahn +8

We present the first simulation-based inference (SBI) of cosmological parameters from field-level analysis of galaxy clustering. Standard galaxy clustering analyses rely on analyzi…

astro-ph.CO2023★ 6 cited

: The First Cosmological Constraints from Non-Gaussian and Non-Linear Galaxy Clustering

ChangHoon Hahn, Pablo Lemos, Liam Parker +8

The 3D distribution of galaxies encodes detailed cosmological information on the expansion and growth history of the Universe. We present the first cosmological constraints that ex…

astro-ph.CO2023★ 1 cited

: The First Cosmological Constraints from the Non-Linear Galaxy Bispectrum

ChangHoon Hahn, Michael Eickenberg, Shirley Ho +7

We present the first cosmological constraints from analyzing higher-order galaxy clustering on non-linear scales. We use , a forward modeling framework…

astro-ph.CO2023★ 33 cited

Galaxy Clustering Analysis with SimBIG and the Wavelet Scattering Transform

Bruno Régaldo-Saint Blancard, ChangHoon Hahn, Shirley Ho +8

The non-Gaussisan spatial distribution of galaxies traces the large-scale structure of the Universe and therefore constitutes a prime observable to constrain cosmological parameter…

cs.LG2023★ 16 cited

Multiple Physics Pretraining for Physical Surrogate Models

Michael McCabe, Bruno Régaldo-Saint Blancard, Liam Holden Parker +11

We introduce multiple physics pretraining (MPP), an autoregressive task-agnostic pretraining approach for physical surrogate modeling of spatiotemporal systems with transformers. I…

stat.ML2023★ 7 cited

xVal: A Continuous Numerical Tokenization for Scientific Language Models

Siavash Golkar, Mariel Pettee, Michael Eickenberg +11

Due in part to their discontinuous and discrete default encodings for numbers, Large Language Models (LLMs) have not yet been commonly used to process numerically-dense scientific…

astro-ph.IM2023★ 1 cited

Learnable wavelet neural networks for cosmological inference

Christian Pedersen, Michael Eickenberg, Shirley Ho

Convolutional neural networks (CNNs) have been shown to both extract more information than the traditional two-point statistics from cosmological fields, and marginalise over astro…

stat.ML2023★ 2 cited

Statistical Component Separation for Targeted Signal Recovery in Noisy Mixtures

Bruno Régaldo-Saint Blancard, Michael Eickenberg

Separating signals from an additive mixture may be an unnecessarily hard problem when one is only interested in specific properties of a given signal. In this work, we tackle simpl…

astro-ph.CO2022★ 6 cited

: A Forward Modeling Approach To Analyzing Galaxy Clustering

ChangHoon Hahn, Michael Eickenberg, Shirley Ho +7

We present the first-ever cosmological constraints from a simulation-based inference (SBI) analysis of galaxy clustering from the new forward modeling…

astro-ph.CO2022★ 32 cited

: Mock Challenge for a Forward Modeling Approach to Galaxy Clustering

ChangHoon Hahn, Michael Eickenberg, Shirley Ho +7

Simulation-Based Inference of Galaxies () is a forward modeling framework for analyzing galaxy clustering using simulation-based inference. In this work…

astro-ph.CO2022★ 1 cited

Towards a non-Gaussian Generative Model of large-scale Reionization Maps

Yu-Heng Lin, Sultan Hassan, Bruno Régaldo-Saint Blancard +2

High-dimensional data sets are expected from the next generation of large-scale surveys. These data sets will carry a wealth of information about the early stages of galaxy formati…

astro-ph.CO2022★ 9 cited

Generative Models of Multi-channel Data from a Single Example -- Application to Dust Emission

Bruno Régaldo-Saint Blancard, Erwan Allys, Constant Auclair +5

The quest for primordial -modes in the cosmic microwave background has emphasized the need for refined models of the Galactic dust foreground. Here, we aim at building a realist…

physics.flu-dyn2022★ 5 cited

TNT: Vision Transformer for Turbulence Simulations

Yuchen Dang, Zheyuan Hu, Miles Cranmer +2

Turbulence is notoriously difficult to model due to its multi-scale nature and sensitivity to small perturbations. Classical solvers of turbulence simulation generally operate on f…

astro-ph.CO2022★ 29 cited

Robust Simulation-Based Inference in Cosmology with Bayesian Neural Networks

Pablo Lemos, Miles Cranmer, Muntazir Abidi +5

Simulation-based inference (SBI) is rapidly establishing itself as a standard machine learning technique for analyzing data in cosmological surveys. Despite continual improvements…

astro-ph.CO2022★ 46 cited

Cosmological Information in the Marked Power Spectrum of the Galaxy Field

Elena Massara, Francisco Villaescusa-Navarro, ChangHoon Hahn +6

Marked power spectra are two-point statistics of a marked field obtained by weighting each location with a function that depends on the local density around that point. We consider…

astro-ph.CO2022★ 25 cited

Wavelet Moments for Cosmological Parameter Estimation

Michael Eickenberg, Erwan Allys, Azadeh Moradinezhad Dizgah +10

Extracting non-Gaussian information from the non-linear regime of structure formation is key to fully exploiting the rich data from upcoming cosmological surveys probing the large-…

astro-ph.CO2022★ 67 cited

The CAMELS project: public data release

Francisco Villaescusa-Navarro, Shy Genel, Daniel Anglés-Alcázar +44

The Cosmology and Astrophysics with MachinE Learning Simulations (CAMELS) project was developed to combine cosmology with astrophysics through thousands of cosmological hydrodynami…

astro-ph.CO2021★ 26 cited

HIFlow: Generating Diverse HI Maps and Inferring Cosmology while Marginalizing over Astrophysics using Normalizing Flows

Sultan Hassan, Francisco Villaescusa-Navarro, Benjamin Wandelt +11

A wealth of cosmological and astrophysical information is expected from many ongoing and upcoming large-scale surveys. It is crucial to prepare for these surveys now and develop to…

cs.LG2021★ 69 cited

The CAMELS Multifield Dataset: Learning the Universe's Fundamental Parameters with Artificial Intelligence

Francisco Villaescusa-Navarro, Shy Genel, Daniel Angles-Alcazar +25

We present the Cosmology and Astrophysics with MachinE Learning Simulations (CAMELS) Multifield Dataset, CMD, a collection of hundreds of thousands of 2D maps and 3D grids containi…