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The Canada-France-Hawaii Telescope Optical PDCS Survey (COP). I. The Data

机译:加拿大-法国-夏威夷望远镜光学PDCS调查(COP)。一,数据

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This paper presents the COP (CFHT optical PDCS; CFHT: Canada-France-Hawaii Telescope, PDCS: Palomar Distant Cluster Survey) survey data. We describe our photometric and spectroscopic observations with the multiobject spectrograph (MOS) at the CFHT. A comparison of the photometry from the PDCS catalogs and from the new images we have obtained at the CFHT shows that the different magnitude systems can be cross-calibrated. After identification between the PDCS catalogs and our new images, we built catalogs with redshift, coordinates, and VPDCS, IPDCS, and RCOP magnitudes. We have classified the galaxies along the lines of sight into field and structure galaxies using a gap technique from Katgert et al. In total we have observed 18 significant structures along the 10 lines of sight.
机译:本文介绍了COP(CFHT光学PDCS; CFHT:加拿大-法国-夏威夷望远镜,PDCS:帕洛玛远程聚类调查)调查数据。我们用CFHT上的多目标光谱仪(MOS)描述了我们的光度学和光谱学观察。从PDCS目录和我们在CFHT获得的新图像进行的光度学比较表明,可以对不同幅度的系统进行交叉校准。在PDCS目录和我们的新图像之间进行识别之后,我们使用redshift,坐标以及VPDCS,IPDCS和RCOP量级构建了目录。我们使用Katgert等人的间隙技术将星系沿视线分类为野外星系和结构星系。总共我们沿着10条视线观察到18个重要结构。

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