papers

Publications (32)

astro-ph.CO2025

Differentiable Cosmological Hydrodynamics for Field-Level Inference and High Dimensional Parameter Constraints

Benjamin Horowitz, Zarija Lukic

Hydrodynamical simulations are the most accurate way to model structure formation in the universe, but they often involve a large number of astrophysical parameters modeling subgri…

astro-ph.CO2024

Maximum A Posteriori Ly-alpha Estimator (MAPLE): Band-power and covariance estimation of the 3D Ly-alpha forest power spectrum

Benjamin Horowitz, Roger de Belsunce, Zarija Lukic

We present a novel maximum a posteriori estimator to jointly estimate band-powers and the covariance of the three-dimensional power spectrum (P3D) of Lyman-alpha forest flux fluctu…

astro-ph.CO2024

TensorFlow Hydrodynamics Analysis for Ly- Simulations

Jupiter Ding, Benjamin Horowitz, Zarija Lukić

We introduce the Python program THALAS (TensorFlow Hydrodynamics Analysis for Lyman-Alpha Simulations), which maps baryon fields (baryon density, temperature, and velocity) to Ly$Î…

astro-ph.CO2021

HyPhy: Deep Generative Conditional Posterior Mapping of Hydrodynamical Physics

Benjamin Horowitz, Max Dornfest, Zarija Lukić +1

Generating large volume hydrodynamical simulations for cosmological observables is a computationally demanding task necessary for next generation observations. In this work, we con…

astro-ph.CO2022

Plausible Adversarial Attacks on Direct Parameter Inference Models in Astrophysics

Benjamin Horowitz, Peter Melchior

In this abstract we explore the possibility of introducing biases in physical parameter inference models from adversarial-type attacks. In particular, we inject small amplitude sys…

astro-ph.IM2012

La Silla-QUEST Variability Survey in the Southern Hemisphere

Ellie Hadjiyska, David Rabinowitz, Charles Baltay +6

We describe the La Silla-QUEST (LSQ) Variability Survey. LSQ is a dedicated wide-field synoptic survey in the Southern Hemisphere, focussing on the discovery and study of transient…

hep-th2013

Group Theoretical Approach to the Construction of Conformal Field Theories

Benjamin Horowitz

A conformal field theory (CFT) is a quantum field theory which is invariant under conformal transformations; a group action that preserve angles but not necessarily lengths. There…

astro-ph.CO2019

Efficient Optimal Reconstruction of Linear Fields and Band-powers from Cosmological Data

Benjamin Horowitz, Uros Seljak, Grigor Aslanyan

We present an efficient implementation of Wiener filtering of real-space linear field and optimal quadratic estimator of its power spectrum Band-powers. We first recast the field r…

astro-ph.IM2025

jFoF: GPU Cluster Finding with Gradient Propagation

Benjamin Horowitz, Adrian E. Bayer

We present jFoF, a fully GPU-native Friends-of-Friends (FoF) halo finder designed for both high-performance simulation analysis and differentiable modeling. Implemented in JAX, jFo…

astro-ph.CO2023

Joint Cosmic Density Reconstruction from Photometric and Spectroscopic Samples

Benjamin Horowitz, Peter Melchior

We reconstruct the dark matter density field from spatially overlapping spectroscopic and photometric redshift catalogs through a forward modelling approach. Instead of directly in…

astro-ph.IM2023

NANCY: Next-generation All-sky Near-infrared Community surveY

Jiwon Jesse Han, Arjun Dey, Adrian M. Price-Whelan +206

The Nancy Grace Roman Space Telescope is capable of delivering an unprecedented all-sky, high-spatial resolution, multi-epoch infrared map to the astronomical community. This oppor…

astro-ph.CO2017

Cosmological constraints from thermal Sunyaev Zeldovich power spectrum revisited

Benjamin Horowitz, Uroš Seljak

Thermal Sunyaev-Zeldovich (tSZ) power spectrum is one of the most sensitive methods to constrain cosmological parameters, scaling as the amplitude . It is determined by the…

astro-ph.CO2021

Fast, high-fidelity Lyman forests with convolutional neural networks

Peter Harrington, Mustafa Mustafa, Max Dornfest +2

Full-physics cosmological simulations are powerful tools for studying the formation and evolution of structure in the universe but require extreme computational resources. Here, we…

astro-ph.CO2016

Revisiting Primordial Black Holes Constraints from Ionization History

Benjamin Horowitz

Much attention has been drawn to the recent discoveries by the Advanced Laser Interferometer Gravitational-Wave Observatory (LIGO) of merging intermediate mass black holes. Of part…

astro-ph.IM2023

Forecasting the power of Higher Order Weak Lensing Statistics with automatically differentiable simulations

Denise Lanzieri, François Lanusse, Chirag Modi +4

We present the Differentiable Lensing Lightcone (DLL), a fully differentiable physical model designed for being used as a forward model in Bayesian inference algorithms requiring a…

astro-ph.IM2025

diffhydro: Inverse Multiphysics Modeling and Embedded Machine Learning in Astrophysical Flows

Benjamin Horowitz, Zarija Lukić, Kentaro Nagamine +1

We present the extension of the differentiable hydrodynamics code, diffhydro, enabling scalable PDE-constrained inference and integrated hybrid physics-ML models for a wide range o…

astro-ph.CO2019

Reconstructing Small Scale Lenses from the Cosmic Microwave Background Temperature Fluctuations

Benjamin Horowitz, Simone Ferraro, Blake D. Sherwin

Cosmic Microwave Background (CMB) lensing is a powerful probe of the matter distribution in the Universe. The standard quadratic estimator, which is typically used to measure the l…

astro-ph.CO2022

Constraining the Fluctuating Gunn-Peterson Approximation Using Lyman- Forest Tomography at

Robin Kooistra, Khee-Gan Lee, Benjamin Horowitz

The fluctuating Gunn-Peterson approximation (FGPA) is a commonly-used method to generate mock Lyman- (Ly) forest absorption skewers at Cosmic Noon () from the m…

astro-ph.IM2026

Fast(er)PM and Moving Mesh: JAX-native Geometric Multigrid Methods

Benjamin Horowitz

The paper introduces a JAX-native geometric multigrid framework for solving Poisson equations in particle‑mesh simulations, offering a communication‑avoiding alternative to FFTs on…

#geometric multigrid#particle-mesh methods#differentiable programming#moving mesh
astro-ph.CO2026

MujicΛ: Reconstructing Initial Conditions from Incomplete Redshift Surveys with Projected Optimization

Chenze Dong, Benjamin Horowitz, Adrian E. Bayer +1

In this paper, we introduce MujicΛ (Mapping the Universe with Jax-based Initial Condition ReconstrΛction), an optimization-based framework for reconstructing initial conditions f…

astro-ph.GA2023

Observational Evidence for Large-Scale Gas Heating in a Galaxy Protocluster at z=2.30

Chenze Dong, Khee-Gan Lee, Metin Ata +2

We report a galaxy protocluster (COSTCO-I) in the COSMOS field, where the Lyman- forest as seen in the CLAMATO IGM tomography survey does not show significant absorpti…

math.LO2013

Categories within the Foundation of Mathematics

Benjamin Horowitz

The recent trend in mathematics is towards a framework of abstract mathematical objects, rather than the more concrete approach of explicitly defining elements which objects were t…

astro-ph.CO2022

Differentiable Stochastic Halo Occupation Distribution

Benjamin Horowitz, ChangHoon Hahn, Francois Lanusse +2

In this work, we demonstrate how differentiable stochastic sampling techniques developed in the context of deep Reinforcement Learning can be used to perform efficient parameter in…

astro-ph.CO2020

TARDIS Paper II: Synergistic Density Reconstruction from Lyman-alpha Forest and Spectroscopic Galaxy Surveys with Applications to Protoclusters and the Cosmic Web

Benjamin Horowitz, Benjamin Zhang, Khee-Gan Lee +1

In this work we expand upon the Tomographic Absorption Reconstruction and Density Inference Scheme (TARDIS) in order to include multiple tracers while reconstructing matter density…

cs.IT2025

Generalized Hyperderivative Reed-Solomon Codes

Mahir Bilen Can, Benjamin Horowitz

This article introduces Generalized Hyperderivative Reed-Solomon codes (GHRS codes), which generalize NRT Reed-Solomon codes. Its main results are as follows: 1) every GHRS code is…

astro-ph.CO2020

TARDIS Paper I: A Constrained Reconstruction Approach to Modeling the z~2.5 Cosmic Web Probed by Lyman-alpha Forest Tomography

Benjamin Horowitz, Khee-Gan Lee, Martin White +2

Recent Lyman- forest tomography measurements of the intergalactic medium (IGM) have revealed a wealth of cosmic structures at high redshift (). In this work, we pres…

astro-ph.CO2025

BaryonBridge: Stochastic Interpolant Model for Fast Hydrodynamical Simulations

Benjamin Horowitz, Carolina Cuesta-Lazaro, Omar Yehia

Constructing a general-purpose framework for mapping between dark matter simulations and observable hydrodynamical simulation outputs is a long-standing problem in modern astrophys…

astro-ph.CO2023

Second Data Release of the COSMOS Lyman-alpha Mapping and Tomographic Observation: The First 3D Maps of the Detailed Cosmic Web at 2.05<z<2.55

Benjamin Horowitz, Khee-Gan Lee, Metin Ata +12

We present the second data release of the COSMOS Lyman-Alpha Mapping And Tomography Observations (CLAMATO) Survey conducted with the LRIS spectrograph on the Keck-I telescope. This…

astro-ph.GA2021

Improved Lyman Alpha Tomography using Optimized Reconstruction with Constraints on Absorption (ORCA)

Zihao Li, Benjamin Horowitz, Zheng Cai

In this work, we propose an improved approach to reconstruct the three-dimensional intergalactic medium from observed Lyman- forest absorption features. We present our new meth…

astro-ph.CO2023

Alignments Between Galaxies and the Cosmic Web at in the IllustrisTNG Simulations

Benjamin Zhang, Khee-Gan Lee, Alex Krolewski +3

Galaxy formation theories predict that galaxy shapes and angular momenta have non-random alignments with the cosmic web. This leads to so-called intrinsic alignment between pairs o…

astro-ph.GA2024

Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field

Chris Byrohl, Dylan Nelson, Benjamin Horowitz +2

We introduce the new cosmological simulation project cosmosTNG, a first-of-its-kind suite of constrained galaxy formation simulations for the universe at Cosmic Noon (). c…

astro-ph.GA2024

The Dependence of Galaxy Properties on the Underlying 3D Matter Density Field at 2.0 < z < 2.5

Rieko Momose, Khee-Gan Lee, Benjamin Horowitz +2

We study the environmental effect of galaxy evolution as a function of the underlying 3D dark matter density for the first time at , in which the underlying matter density…