Astron. Astrophys. Suppl. Ser.
Volume 122, Number 3, May I 1997
|Page(s)||409 - 414|
|Published online||15 May 1997|
Institut d'Astrophysique de Paris, CNRS, Université Pierre et Marie Curie, 98bis Bd Arago, F-75014 Paris, France
2 Centro de Astrofísica da Universidade do Porto, Rua do Campo Alegre 823, P-4150 Porto, Portugal
3 Istituto T.E.S.R.E., Area della Ricerca del CNR, via Gobetti 101, I-40129, Bologna, Italy
4 ESA Villafranca Satellite Tracking Station, Apto. 50727, CAM IDT, E-28080 Madrid, Spain
5 DAEC, Observatoire de Paris, Université Paris VII, CNRS (UA 173), F-92195 Meudon Cedex, France
6 IGRAP, LAS, Traverse du Siphon, Les Trois Lucs, B.P. 8, F-13376 Marseille Cedex, France
7 Observatoire de la Côte d'Azur, B.P. 229, F-06304 Nice Cedex 4, France
Corresponding author: Send offprint request to: C. Lobo, e-mail: firstname.lastname@example.org
Accepted: 2 August 1996
We have obtained a mosaic of CCD images of the Coma cluster in the V-band covering a region of approximately 0.4 degrees2 around both central cluster galaxies NGC 4889 and NGC 4874. An additional frame of was taken of the south-west region around NGC 4839. We derived a catalogue of 7023 galaxies and 4096 stars containing positions, central surface brightnesses and isophotal V26.5 magnitudes. We estimate that data is complete up to and the surface brightness limiting detection value is . In this paper we present the catalogue (available in electronic form alone), along with a detailed description of the steps concerning the data reduction and quality of the computed parameters.
Key words: galaxies: clusters: individual: Coma / galaxies: photometry / galaxies: luminosity function
Based on observations collected at the Canada-France-Hawaii telescope, operated by the National Research Council of Canada, the Centre National de la Recherche Scientifique of France, and the University of Hawaii.
© European Southern Observatory (ESO), 1997