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The Great Observatories Origins Deep Survey VLT/FORS2 spectroscopy in the GOODS-South Field

机译:伟大的天文台起源于GOODs-south油田的深度测量VLT / FORs2光谱

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摘要

We present the first results of the ESO/ GOODS program of spectroscopy of faint galaxies in the Chandra Deep Field South ( CDF- S). 399 spectra of 303 unique targets have been obtained in service mode with the FORS2 spectrograph at the ESO/ VLT, providing 234 redshift determinations ( the median of the redshift distribution is at 1.04). The typical redshift uncertainty is estimated to be sigma(z) similar or equal to 0.001. Galaxies have been color selected in a way that the resulting redshift distribution typically spans from z = 0.5 to 2. The reduced spectra and the derived redshifts are released to the community through the ESO web page http:// www. eso. org/ science/ goods/. Large scale structure is clearly detected at z similar or equal to 0.67, 0.73, 1.10 and 1.61. Three Lyman- break galaxies have also been included as targets and are confirmed to have redshifts z = 4.800, 4.882 and 5.828. In a few cases, we observe clear [ OII] 3727 rotation curves, even at the relatively low resolution ( R = 860) of the present observations. Assuming that the observed velocity structure is due to dynamically- relaxed rotation, this is an indication of large galactic masses ( few times 10(11) M.) at z similar to 1.
机译:我们介绍了钱德拉深场南(CDF-S)中微弱星系光谱的ESO / GOODS计划的初步结果。使用ESO / VLT上的FORS2光谱仪,在维修模式下已获得303个唯一目标的399个光谱,提供234个红移测定值(红移分布的中位数为1.04)。典型的红移不确定度估计为sigma(z)相似或等于0.001。已对银河系进行了颜色选择,其结果是红移分布的典型范围是z = 0.5到2。减少的光谱和派生的红移将通过ESO网页http:// www发布到社区。 eso。组织/科学/商品/。在z处近似或等于0.67、0.73、1.10和1.61清楚地检测到大型结构。三个莱曼断裂星系也已包括在内,并已确认其红移z = 4.800、4.882和5.828。在少数情况下,即使在当前观察值的相对较低分辨率(R = 860)下,我们也观察到了清晰的[OII] 3727旋转曲线。假定观测到的速度结构是由于动态松弛旋转引起的,这表明在大的银河系质量(几倍于10(11)M.),其z与1相似。

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