GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations

Fuente: arXiv
Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Zhou, Xingchen, Yang, Hang, Li, Nan, Xiong, Qi, Deng, Furen, Meng, Xian-Min, Ye, Renhao, Shen, Shiyin, Wei, Peng, Cui, Qifan, He, Zizhao, Ibitoye, Ayodeji, Wei, Chengliang, Fang, Yuedong
Format: Preprint
Veröffentlicht: 2025
Schlagworte:
Online-Zugang:
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
_version_ 1866916893564076032
author Zhou, Xingchen
Yang, Hang
Li, Nan
Xiong, Qi
Deng, Furen
Meng, Xian-Min
Ye, Renhao
Shen, Shiyin
Wei, Peng
Cui, Qifan
He, Zizhao
Ibitoye, Ayodeji
Wei, Chengliang
Fang, Yuedong
author_facet Zhou, Xingchen
Yang, Hang
Li, Nan
Xiong, Qi
Deng, Furen
Meng, Xian-Min
Ye, Renhao
Shen, Shiyin
Wei, Peng
Cui, Qifan
He, Zizhao
Ibitoye, Ayodeji
Wei, Chengliang
Fang, Yuedong
contents We introduce GalaxyGenius, a Python package designed to produce synthetic galaxy images tailored to different telescopes based on hydrodynamical simulations. Its implementation will support and advance research on galaxies in the era of large-scale sky surveys. The package comprises three main modules: data preprocessing, ideal data cube generation, and mock observation. Specifically, the preprocessing module extracts necessary properties of star and gas particles for a selected subhalo from hydrodynamical simulations and creates the execution file for the following radiative transfer procedure. Subsequently, building on the above information, the ideal data cube generation module executes a widely used radiative transfer project, specifically the SKIRT, to perform the SED assignment for each particle and the radiative transfer procedure to produce an IFU-like ideal data cube. Lastly, the mock observation module takes the ideal data cube and applies the throughputs of aiming telescopes, while also incorporating the relevant instrumental effects, point spread functions (PSFs), and background noise to generate the required mock observational images of galaxies. To showcase the outcomes of GalaxyGenius, we created a series of mock images of galaxies based on the IllustrisTNG and EAGLE simulations for both space and ground-based surveys, spanning ultraviolet (UV) to infrared (IR) wavelength coverage, including CSST, Euclid, HST, JWST, Roman, and HSC. GalaxyGenius offers a flexible framework to generate mock galaxy images with customizable recipes. These generated images can serve as valuable references for verifying and validating new approaches in astronomical research. They can also serve as training sets for relevant studies using deep learning in cases where real observational data are insufficient.
format Preprint
id arxiv_https___arxiv_org_abs_2506_15060
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
Zhou, Xingchen
Yang, Hang
Li, Nan
Xiong, Qi
Deng, Furen
Meng, Xian-Min
Ye, Renhao
Shen, Shiyin
Wei, Peng
Cui, Qifan
He, Zizhao
Ibitoye, Ayodeji
Wei, Chengliang
Fang, Yuedong
Instrumentation and Methods for Astrophysics
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
We introduce GalaxyGenius, a Python package designed to produce synthetic galaxy images tailored to different telescopes based on hydrodynamical simulations. Its implementation will support and advance research on galaxies in the era of large-scale sky surveys. The package comprises three main modules: data preprocessing, ideal data cube generation, and mock observation. Specifically, the preprocessing module extracts necessary properties of star and gas particles for a selected subhalo from hydrodynamical simulations and creates the execution file for the following radiative transfer procedure. Subsequently, building on the above information, the ideal data cube generation module executes a widely used radiative transfer project, specifically the SKIRT, to perform the SED assignment for each particle and the radiative transfer procedure to produce an IFU-like ideal data cube. Lastly, the mock observation module takes the ideal data cube and applies the throughputs of aiming telescopes, while also incorporating the relevant instrumental effects, point spread functions (PSFs), and background noise to generate the required mock observational images of galaxies. To showcase the outcomes of GalaxyGenius, we created a series of mock images of galaxies based on the IllustrisTNG and EAGLE simulations for both space and ground-based surveys, spanning ultraviolet (UV) to infrared (IR) wavelength coverage, including CSST, Euclid, HST, JWST, Roman, and HSC. GalaxyGenius offers a flexible framework to generate mock galaxy images with customizable recipes. These generated images can serve as valuable references for verifying and validating new approaches in astronomical research. They can also serve as training sets for relevant studies using deep learning in cases where real observational data are insufficient.
title GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
topic Instrumentation and Methods for Astrophysics
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2506.15060