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GalSyn I: A Forward-Modeling Code for Synthetic Galaxy Observations from Hydrodynamical Simulations and First Data Release from IllustrisTNG

Abdurro'uf et al. · 2026 · arxiv_all
arXiv (All) · Papers · 2026
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[2603.23986] GalSyn I: A Forward-Modeling Code for Synthetic Galaxy Observations from Hydrodynamical Simulations and First Data Release from IllustrisTNG Skip to main content Search Submit Donate Log in Search arXiv Press Enter to search · Advanced search Astrophysics > Astrophysics of Galaxies arXiv:2603.23986 (astro-ph) [Submitted on 25 Mar 2026 ( v1 ), last revised 15 Aug 2026 (this version, v2)] Title: GalSyn I: A Forward-Modeling Code for Synthetic Galaxy Observations from Hydrodynamical Simulations and First Data Release from IllustrisTNG Authors: Abdurro'uf , Henry C. Ferguson , Samir Salim , Kartheik G. Iyer , Larry D. Bradley , Dan Coe , Novan Saputra Haryana , Sultan Hassan , Intae Jung , Gourav Khullar , Takahiro Morishita , Lamiya Mowla View a PDF of the paper titled GalSyn I: A Forward-Modeling Code for Synthetic Galaxy Observations from Hydrodynamical Simulations and First Data Release from IllustrisTNG, by Abdurro'uf and 11 other authors View PDF HTML (experimental) Abstract: We present GalSyn (Galaxy Synthesizer), a modular and flexible Python package for generating synthetic observations from hydrodynamical galaxy simulations. GalSyn generates synthetic spectrophotometric data cubes for individual galaxies from simulation cutouts, employing a particle-by-particle spectral modeling approach that enables the rapid production of large synthetic datasets required for statistical population studies, offering a computationally efficient alternative to full radiative transfer codes. Users have full control over the spectral modeling choices, including the stellar population synthesis engine, stellar isochrones, spectral libraries, and initial mass functions. Dust attenuation is modeled at spatially resolved scales using a line-of-sight column-density method, with a comprehensive suite of fixed and adaptive attenuation laws. A decoupled kinematics model independently Doppler-shifts the stellar and nebular components, enabling realistic synthetic integral field unit data cubes. It also provides features to add observational realism, including PSF convolution and noise simulation. Beyond generating imaging and spectroscopic data cubes, GalSyn reconstructs spatially resolved physical property maps and star formation histories (SFHs) of a galaxy. Alongside this paper, we present the first data release of synthetic imaging observations and resolved SFHs generated from the IllustrisTNG simulations. This release includes four mock extragalactic survey fields together with data cubes of the individual galaxies within them, data cubes of 290 local massive galaxies and their progenitors tracked across $0<z<5$, and 259 major-merger systems. Each galaxy data cube contains imaging across 47 filters spanning HST, JWST, Euclid, Rubin/LSST, and the Roman Space Telescope. GalSyn is publicly available at this https URL . Comments: 31 pages, 20 figures, Accepted for publication in ApJS. GalSyn is publicly available at this https URL , and its documentation is available at this https URL . The first public data release is available at this https URL . Comments are welcome! Subjects: Astrophysics of Galaxies (astro-ph.GA) Cite as: arXiv:2603.23986 [astro-ph.GA] (or arXiv:2603.23986v2 [astro-ph.GA] for this version) https://doi.org/10.48550/arXiv.2603.23986 Focus to learn more arXiv-issued DOI via DataCite Submission history From: Abdurro'uf Abdurro'uf [ view email ] [v1] Wed, 25 Mar 2026 06:31:33 UTC (25,453 KB) [v2] Sat, 15 Aug 2026 02:32:58 UTC (25,456 KB) Full-text links: Access Paper: View a PDF of the paper titled GalSyn I: A Forward-Modeling Code for Synthetic Galaxy Observations from Hydrodynamical Simulations and First Data Release from IllustrisTNG, by Abdurro'uf and 11 other authors View PDF HTML (experimental) TeX Source view license Current browse context: astro-ph.GA < prev | next > new | recent | 2026-03 Change to browse by: astro-ph References & Citations NASA ADS Google Scholar Semantic Scholar export BibTeX citation Loading... BibTeX formatted citation × loading... 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