The Canada-France-Hawaii telescope optical PDCS survey (COP). I. The data

被引：8

作者：

Adami, C

Holden, BP

Castander, FJ

Nichol, RC

Mazure, A

Ulmer, MP

Postman, M

Lubin, LM

机构：

[1] Northwestern Univ, Dearborn Observ, Dept Phys & Astron, Evanston, IL 60208 USA

[2] IGRAP, Astron Spatiale Lab, F-13012 Marseille, France

[3] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA

[4] Observ Midi Pyrenees, F-31400 Toulouse, France

[5] Carnegie Mellon Univ, Dept Phys, Pittsburgh, PA 15213 USA

[6] Space Telescope Sci Inst, Baltimore, MD 21218 USA

[7] CALTECH, Palomar Observ, Pasadena, CA 91125 USA

来源：

ASTRONOMICAL JOURNAL | 2000年 / 120卷 / 01期

基金：

美国国家科学基金会;

关键词：

cosmology : observations; galaxies : clusters : general; large-scale structure of universe;

D O I：

10.1086/301445

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 V-PDSC, I-PDSC, and R-COP magnitudes. We have classified the galaxies along the lines of sight into field and structure galaxies using a gap technique from Katgert ct al. In total we have observed 18 significant structures along the 10 lines of sight.

引用

页码：1 / 22

页数：22

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[2]

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[3]

Adami C, 1998, ASTRON ASTROPHYS, V334, P765

[4]

BAHCALL NA, 1997, APJ, V485, P53