The CFH Optical PDCS survey (COP) I: The Data

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dc.creatorAdami, C.
dc.creatorHolden, B.
dc.creatorCastander, F. J.
dc.creatorNichol, R. C.
dc.creatorMazure, A.
dc.creatorUlmer, M. P.
dc.creatorPostman, M.
dc.creatorLubin, L.
dc.date2000-03-09
dc.date.accessioned2026-07-07T01:52:41Z
dc.date.available2026-07-07T01:52:41Z
dc.descriptionThis paper presents and gives the COP (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 MOS multi-slit spectrograph at the CFH telescope. A comparison of the photometry from the PDCS (Postman et al. 1996) catalogs and from the new images we have obtained at the CFH telescope shows that the different magnitude systems can be cross-calibrated. After identification between the PDCS catalogues and our new images, we built catalogues with redshift, coordinates and V, I and Rmagnitudes. We have classified the galaxies along the lines of sight into field and structure galaxies using a gap technique (Katgert et al. 1996). In total we have observed 18 significant structures along the 10 lines of sight.
dc.description40 pages, 13 figures, accepted in AJ
dc.identifierhttps://arxiv.org/abs/astro-ph/0003137
dc.identifierhttp://arxiv.org/abs/astro-ph/0003137
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/700
dc.subjectAstrophysics
dc.titleThe CFH Optical PDCS survey (COP) I: The Data
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