A& A Supplement series, Vol. 122, May I 1997, 409-414
Received June 29; accepted August 2, 1996
C. Lobo
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A. Biviano
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F. Durret
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D. Gerbal
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O. Le Fèvre
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A. Mazure
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E. Slezak
Send offprint request: C. Lobo, lobo@iap.fr
Institut d'Astrophysique de Paris, CNRS, Université Pierre et
Marie Curie, 98bis Bd Arago, F-75014 Paris, France
Centro de Astrofísica da Universidade do Porto, Rua do Campo
Alegre 823, P-4150 Porto, Portugal
Istituto T.E.S.R.E., Area della Ricerca del CNR, via Gobetti 101,
I-40129, Bologna, Italy
ESA Villafranca Satellite Tracking Station, Apto. 50727, CAM IDT,
E-28080 Madrid, Spain
DAEC, Observatoire de Paris, Université Paris VII, CNRS (UA 173),
F-92195 Meudon Cedex, France
IGRAP, LAS, Traverse du Siphon, Les Trois Lucs, B.P. 8, F-13376
Marseille Cedex, France
Observatoire de la Côte d'Azur, B.P. 229, F-06304 Nice Cedex 4,
France
We have obtained a mosaic of CCD images of the Coma cluster in the V-band
covering a region of approximately 0.4 degrees 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
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.
keywords: galaxies: clusters: individual: Coma -- galaxies: photometry -- galaxies: luminosity function