Sign on

SAO/NASA ADS Astronomy Abstract Service


· Find Similar Abstracts (with default settings below)
· Electronic Refereed Journal Article (HTML)
· Full Refereed Journal Article (PDF/Postscript)
· arXiv e-print (arXiv:0802.0149)
· On-line Data
· References in the article
· Citations to the Article (8) (Citation History)
· Refereed Citations to the Article
· SIMBAD Objects (5)
· Associated Articles
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
Spectroscopy of clusters in the ESO distant cluster survey (EDisCS). II.. Redshifts, velocity dispersions, and substructure for clusters in the last 15 fields
Authors:
Milvang-Jensen, B.; Noll, S.; Halliday, C.; Poggianti, B. M.; Jablonka, P.; Aragón-Salamanca, A.; Saglia, R. P.; Nowak, N.; von der Linden, A.; De Lucia, G.; Pelló, R.; Moustakas, J.; Poirier, S.; Bamford, S. P.; Clowe, D. I.; Dalcanton, J. J.; Rudnick, G. H.; Simard, L.; White, S. D. M.; Zaritsky, D.
Affiliation:
AA(Max-Planck-Institut für extraterrestrische Physik, Giessenbachstraße, 85748 Garching bei München, Germany ; Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen Ø, Denmark ; The Royal Library / Copenhagen University Library, Research Dept., Box 2149, 1016 Copenhagen K, Denmark), AB(Max-Planck-Institut für extraterrestrische Physik, Giessenbachstraße, 85748 Garching bei München, Germany ; Observatoire Astronomique Marseille Provence, Laboratoire d'Astrophysique de Marseille, Traverse du Siphon, 13376 Marseille Cedex 12, France), AC(Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy), AD(Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, 35122 Padova, Italy), AE(Université de Genève, Laboratoire d'Astrophysique de l'École Polytechnique Fédérale de Lausanne (EPFL), Observatoire, 1290Â Sauverny, Switzerland), AF(School of Physics and Astronomy, University of Nottingham, University Park, Nottingham NG7 2RD, UK), AG(Max-Planck-Institut für extraterrestrische Physik, Giessenbachstraße, 85748 Garching bei München, Germany), AH(Max-Planck-Institut für extraterrestrische Physik, Giessenbachstraße, 85748 Garching bei München, Germany), AI(Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Straße 1, 85748 Garching bei München, Germany), AJ(Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Straße 1, 85748 Garching bei München, Germany), AK(Laboratoire d'Astrophysique de Toulouse-Tarbes, CNRS, Université de Toulouse, 14 avenue Édouard Belin, 31400 Toulouse, France), AL(New York University, 4 Washington Place, New York, NY 10003, USA), AM(GEPI, CNRS-UMR8111, Observatoire de Paris, section de Meudon, 5 place Jules Janssen, 92195 Meudon Cedex, France), AN(ICG, University of Portsmouth, Mercantile House, Hampshire Terrace, Portsmouth, PO1 2EG, UK), AO(Ohio University, Department of Physics and Astronomy, Clippinger Labs 251B, Athens, OH 45701, USA), AP(Department of Astronomy, University of Washington, Box 351580, Seattle WA 98195-1580, USA), AQ(NOAO, 950 North Cherry Avenue, Tucson AZ 85719, USA), AR(Herzberg Institute of Astrophysics, National Research Council of Canada, 5071 West Saanich Road, Victoria, BC V9E 2E7, Canada), AS(Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Straße 1, 85748 Garching bei München, Germany), AT(Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA)
Publication:
Astronomy and Astrophysics, Volume 482, Issue 2, 2008, pp.419-449 (A&A Homepage)
Publication Date:
05/2008
Origin:
EDP
Keywords:
galaxies: clusters: general, galaxies: distances and redshifts, galaxies: evolution
DOI:
10.1051/0004-6361:20079148
Bibliographic Code:
2008A&A...482..419M

Abstract

Aims. We present spectroscopic observations of galaxies in 15 survey fields as part of the ESO Distant Cluster Survey (EDisCS). We determine the redshifts and velocity dispersions of the galaxy clusters located in these fields, and we test for possible substructure in the clusters. Methods: We obtained multi-object mask spectroscopy using the FORS2 instrument at the VLT. We reduced the data with particular attention to the sky subtraction. We implemented the method of Kelson for performing sky subtraction prior to any rebinning/interpolation of the data. From the measured galaxy redshifts, we determine cluster velocity dispersions using the biweight estimator and test for possible substructure in the clusters using the Dressler-Shectman test. Results: The method of subtracting the sky prior to any rebinning/interpolation of the data delivers photon-noise-limited results, whereas the traditional method of subtracting the sky after the data have been rebinned/interpolated results in substantially larger noise for spectra from tilted slits. Redshifts for individual galaxies are presented and redshifts and velocity dispersions are presented for 21 galaxy clusters. For the 9 clusters with at least 20 spectroscopically confirmed members, we present the statistical significance of the presence of substructure obtained from the Dressler-Shectman test, and substructure is detected in two of the clusters. Conclusions: Together with data from our previous paper, spectroscopy and spectroscopic velocity dispersions are now available for 26 EDisCS clusters with redshifts in the range 0.40-0.96 and velocity dispersions in the range 166 km s-1-1080 km s-1.

Based on observations collected at the European Southern Observatory, Chile, as part of large programme 166.A-0162 (the ESO Distant Cluster Survey). Full Table 4 is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/482/419


Associated Articles

Part 1     Part  2     Catalog Description    


Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)

   

Find Similar Abstracts:

Use: Authors
Title
Keywords (in text query field)
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints
    



SAO/NASA ADS Homepage | ADS Sitemap | Query Form | Basic Search | Preferences | HELP | FAQ