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DOI: 10.1051/aas:1999477
Astron. Astrophys. Suppl. Ser. 137, 83-92
ESO Imaging Survey
VII. Distant cluster candidates over 12 square degrees
M. Scodeggio1 - L.F. Olsen1,2 - L. da Costa1 - R. Slijkhuis1,3 - C. Benoist1 - E. Deul1,3 - T. Erben1,4 - R. Hook5 - M. Nonino1,6 - A. Wicenec1 - S. Zaggia 1,7
Send offprint request: M. Scodeggio
1 - European Southern Observatory, Karl-Schwarzschild-Str. 2,
D-85748 Garching b. München, Germany
2 -
Astronomisk Observatorium, Juliane Maries Vej 30, DK-2100 Copenhagen,
Denmark
3 -
Leiden Observatory, P.O. Box 9513, 2300 RA Leiden, The Netherlands
4 -
Max-Planck Institut für Astrophysik, Postfach 1523, D-85748 Garching b.
München, Germany
5 -
Space Telescope - European Coordinating Facility, Karl-Schwarzschild-Str.
2, D-85748 Garching b. München, Germany
6 -
Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, I-31144
Trieste, Italy
7 -
Osservatorio Astronomico di Capodimonte, via Moiariello 15, I-80131 Napoli,
Italy
Received August 5; accepted December 21, 1998
Abstract:
In this paper the list of candidate clusters identified from the
I-band images of the ESO Imaging Survey (EIS) is completed using the
data obtained over a total area of about 12 square degrees (EIS
Patches C and D). 248 new cluster candidates are presented.
Together with the data reported earlier the total
I-band coverage of EIS is 17 square degrees, which has yielded a
sample of 302 cluster candidates with estimated redshift in the range
and a median redshift of z=0.5. This is the
largest optically-selected sample currently available in the Southern
Hemisphere. It is also well distributed in the sky thus providing
targets for a variety of VLT programs nearly year round.
Key words: galaxies: clusters: general -- large-scale structure of the Universe -- Cosmology: observations -- surveys
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