High-resolution synthetic UV–submm images for simulated Milky Way-type galaxies from the Auriga project (Au 9-15)

We present redshift-zero synthetic observational data considering dust attenuation and dust emission for the thirty galaxies of the Auriga project, calculated with the SKIRT radiative transfer code. The set of thirty Auriga galaxies reproduce a wide range of present-day observables, in particular, disk-dominated galaxies with appropriate stellar masses, sizes, rotation curves, star formation rates, and metallicities. The post-processing procedure includes components for star-forming regions, stellar sources, and diffuse dust taking into account stochastic heating of dust grains. This allows us to obtain realistic high-resolution broadband images and fluxes from ultraviolet to sub-millimeter wavelengths. Please visit auriga.ugent.be for more information.

This dataset contains images/SEDs for Auriga galaxies 9-15 i.e. 7/30 galaxies.

本研究针对欧里加（Auriga）项目的30个星系，提供了考虑尘埃消光与尘埃发射的红移为零的合成观测数据，该数据通过SKIRT辐射传输代码计算得到。这30个欧里加星系能够复现现今观测到的多种天体物理特征，具体包括拥有合理恒星质量、尺度、旋转曲线、恒星形成率以及金属丰度的盘状主导星系。后处理流程涵盖恒星形成区、恒星辐射源与弥漫尘埃的相关组分，并考虑了尘埃颗粒的随机加热效应。这使得我们能够获得从紫外到亚毫米波段的高分辨率逼真宽带图像与通量。更多信息请访问 auriga.ugent.be 网站。
本数据集包含欧里加星系9至15（即7/30个星系）的图像与光谱能量分布（SEDs）数据。