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首页> 外文期刊>Astronomy and astrophysics >CALIFA, the Calar Alto Legacy Integral Field Area survey - IV. Third public data release
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CALIFA, the Calar Alto Legacy Integral Field Area survey - IV. Third public data release

机译:CALIFA,Calar Alto旧式整体实地调查-IV。第三次公开数据发布

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This paper describes the third public data release (DR3) of the Calar Alto Legacy Integral Field Area (CALIFA) survey. Science-grade quality data for 667 galaxies are made public, including the 200 galaxies of the second public data release (DR2). Data were obtained with the integral-field spectrograph PMAS/PPak mounted on the 3.5 m telescope at the Calar Alto Observatory. Three different spectral setups are available: i) a low-resolution V500 setup covering the wavelength range 3745–7500 ? (4240–7140 ? unvignetted) with a spectral resolution of 6.0 ? (FWHM) for 646 galaxies, ii) a medium-resolution V1200 setup covering the wavelength range 3650–4840 ? (3650–4620 ? unvignetted) with a spectral resolution of 2.3 ? (FWHM) for 484 galaxies, and iii) the combination of the cubes from both setups (called COMBO) with a spectral resolution of 6.0 ? and a wavelength range between 3700–7500 ? (3700–7140 ? unvignetted) for 446 galaxies. The Main Sample, selected and observed according to the CALIFA survey strategy covers a redshift range between 0.005 and 0.03, spans the color-magnitude diagram and probes a wide range of stellar masses, ionization conditions, and morphological types. The Extension Sample covers several types of galaxies that are rare in the overall galaxy population and are therefore not numerous or absent in the CALIFA Main Sample. All the cubes in the data release were processed using the latest pipeline, which includes improved versions of the calibration frames and an even further improved image reconstruction quality. In total, the third data release contains 1576 datacubes, including ~1.5 million independent spectra.
机译:本文介绍了Calal Alto旧式整体野外区域(CALIFA)调查的第三次公开数据发布(DR3)。公开了667个星系的科学级质量数据,包括第二次公开数据发布(DR2)的200个星系。数据是通过安装在Calar Alto天文台3.5 m望远镜上的积分场光谱仪PMAS / PPak获得的。提供三种不同的光谱设置:i)覆盖波长范围3745–7500的低分辨率V500设置? (4240–7140?未渐晕),光谱分辨率为6.0? (FWHM)适用于646个星系,ii)中分辨率V1200设置,覆盖3650–4840波长范围? (3650–4620?未渐晕),光谱分辨率为2.3? (FWHM)用于484个星系,以及iii)两种设置的立方体的组合(称为COMBO),其光谱分辨率为6.0?波长范围在3700–7500之间? (3700–7140?未消失)446个星系。根据CALIFA调查策略选择和观察的主样本覆盖了0.005至0.03之间的红移范围,跨越了色度图,并探查了广泛的恒星质量,电离条件和形态类型。扩展样本涵盖了几种类型的星系,这些星系在整个银河系人口中很少见,因此在CALIFA主样本中并不很多或不存在。数据发布中的所有多维数据集均使用最新的流水线进行了处理,其中包括改进版本的校准框架以及甚至进一步提高了图像重建质量。总共,第三次数据发布包含1576个数据立方体,包括约150万个独立光谱。

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