collaborators

10 papers

astro-ph.GA2026

A Pixel-by-Pixel Path to Population III Discovery with JWST

Patricia Iglesias-Navarro, Thomas Harvey, Marc Huertas-Company +11

The identification of the first generation of metal-free stars, known as Population III (Pop~III), remains a primary goal of modern observational astronomy. While JWST has discover…

astro-ph.CO2026

Simulation-based inference from the Lyman-alpha forest 1D power spectrum with CAMELS

Francesco Sinigaglia, Patricia Iglesias-Navarro, Matteo Viel

We perform for the first time full simulation-based inference on the Lyman- forest 1D power spectrum. In particular, we consider the prediction of the Lyman- forest $P_{\rm…

astro-ph.GA2026

JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: stellar population catalogue for galaxies in GOODS-N and GOODS-S

Qiao Duan, Sandro Tacchella, Benjamin D. Johnson +37

We present the galaxy stellar population catalogue from the JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5 (DR5), providing homogeneous Bayesian inference of physic…

astro-ph.GA2025

Euclid preparation: LXXXI. The impact of nonparametric star formation histories on spatially resolved galaxy property estimation using synthetic Euclid images

Euclid Collaboration, A. Nersesian, Abdurro'uf +283

We analyzed the spatially resolved and global star formation histories (SFHs) for a sample of 25 TNG50-SKIRT Atlas galaxies to assess the feasibility of reconstructing accurate SFH…

astro-ph.GA2025

Flexible Simulation Based Inference for Galaxy Photometric Fitting with Synthesizer

Thomas Harvey, Christopher C. Lovell, Sophie Newman +13

We introduce Synference, a new, flexible Python framework for galaxy SED fitting using simulation-based inference (SBI). Synference leverages the Synthesizer package for flexible f…

astro-ph.GA2025

Simulation-based inference of galaxy properties from JWST pixels

Patricia Iglesias-Navarro, Marc Huertas-Company, Pablo Pérez-González +6

We present an efficient Bayesian SED-fitting framework tailored to multiwavelength pixel photometry from the JWST Advanced Deep Extragalactic Survey (JADES). Our method employs sim…