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The ESO UVES advanced data products quasar sample - I. Dataset and new NH?I measurements of damped absorbers

机译:ESO UVES先进的数据产品类星体样本-I.阻尼器的数据集和新的NH?I测量值

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We present here a dataset of quasars observed with the Ultraviolet Visual Echelle Spectrograph (UVES) on the Very Large Telescope and available in the European Southern Observatory UVES Advanced Data Products archive. The sample is made up of a total of?250?high resolution quasar spectra with emission redshifts ranging from 0.191?≤?zem?≤?6.311. The total UVES exposure time of this dataset is 1560 h. Thanks to the high resolution of UVES spectra, it is possible to unambiguously measure the column density of absorbers with damping wings, down to NH???I???1019 cm-2, which constitutes the sub-damped Lyα absorber (sub-DLA) threshold. Within the wavelength coverage of our UVES data, we find 150 damped Lyα systems (DLAs)/sub-DLAs in the range 1.5?
机译:我们在这里介绍在超大型望远镜上用紫外视觉埃歇尔光谱仪(UVES)观测到的类星体数据集,该数据集可从欧洲南方天文台UVES高级数据产品档案中获得。样品由总共250个高分辨率类星体光谱组成,发射红移范围为0.191≤≤zem≤≤6.311。该数据集的总UVES暴露时间为1560小时。得益于UVES光谱的高分辨率,可以毫无疑问地测量带有阻尼翼的吸收器的柱密度,低至NH 3 I≈1019 cm-2,这构成了亚阻尼的Lyα吸收器(亚DLA)阈值。在我们的UVES数据的波长范围内,我们发现150个阻尼Lya系统(DLA)/ sub-DLA的范围为1.5≤

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