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pyC <sup>2</sup> Ray: A flexible and GPU-accelerated radiative transfer framework for simulating the cosmic epoch of reionization

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pyC <sup>2</sup> Ray: A flexible and GPU-accelerated radiative transfer framework for simulating the cosmic epoch of reionization

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LXXI. Simulations and nonlinearities beyond ΛCDM. 3. Constraints on f(R) models from the photometric primary probes

The AGORA High-Resolution Galaxy Simulations Comparison Project VII. Satellite quenching in zoom-in simulation of a Milky Way-mass halo

Desi 2024 Vi: Cosmological Constraints From the Measurements of Baryon Acoustic Oscillations

Analytical and EZmock covariance validation for the DESI 2024 results

Euclid preparation: XLVII. Improving cosmological constraints using a new multi-tracer method with the spectroscopic and photometric samples

Euclid preparation

Intermediate complexity atmospheric modeling in complex terrain: is it right?

Euclid preparation XXVI. The Euclid Morphology Challenge: Towards structural parameters for billions of galaxies

DESI mock challenge: constructing DESI galaxy catalogues based on FastPM simulations

Hydrogen Intensity and Real-Time Analysis Experiment: 256-element array status and overview

Euclid preparation XIX. Impact of magnification on photometric galaxy clustering

Differentiable Signed Distance Function Rendering

H I constraints from the cross-correlation of eBOSS galaxies and Green Bank Telescope intensity maps

Euclid: Covariance of weak lensing pseudo-C-l estimates Calculation, comparison to simulations, and dependence on survey geometry

Unsupervised Visual Entity Abstraction towards 2D and 3D Compositional Models

Account of the baryonic feedback effect in gamma-ray measurements of intergalactic magnetic fields

The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1

The AGORA High-resolution Galaxy Simulations Comparison Project. III. Cosmological Zoom-in Simulation of a Milky Way-mass Halo

Towards Efficient and Accurate Numerical Simulations of Galaxies using Task-based Parallelism and Application to Dwarf Galaxies

The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1