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Galaxy spectra from the UV to the mid-IR

机译:来自紫外线到中外的星系光谱

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Templates and models of galaxy spectra are often essential for determining the physical properties of galaxies. Many commonly used templates have large systematic errors, which significantly impact photometric redshifts and k-corrections. We present a new library of 110 galaxy template spectra spanning from the ultraviolet to the mid-infrared. The templates combine optical, Spitzer and Akari spectra with MAGPHYS models, all normalised and verified with matched aperture photometry. Our library contains more galaxies, spans a broader range of colours and has smaller systematic errors than previous libraries of galaxy spectra.
机译:Galaxy Spectra的模板和模型通常是必不可少的,用于确定星系的物理性质。许多常用的模板具有大量的系统误差,这显着影响了光度射频和k校正。我们介绍了从紫外线到中红外线的110个星系模板谱的新图书馆。模板将光学,Spitzer和Akari Spectra与Magphys模型相结合,全部归一化并用匹配的孔径光度测定验证。我们的图书馆包含更多的星系,跨越更广泛的颜色,并且具有比以前的Galaxy Spectra图书馆更小的系统误差。

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