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A Redshift Survey in the South Galactic Pole Region

Published online by Cambridge University Press:  26 July 2016

G. Vettolani ,
E. Zucca ,
A. Cappi ,
R. Merighi ,
M. Mignoli ,
G. Stirpe ,
G. Zamorani ,
C. Collins ,
H. Macgillivray  and
C. Balkowski
...Show all authors
G. Vettolani
Affiliation:
Istituto di Radioastronomia del CNR, Bologna, Italy
E. Zucca
Affiliation:
Istituto di Radioastronomia del CNR, Bologna, Italy
A. Cappi
Affiliation:
Osservatorio Astronomico di Bologna, Bologna, Italy
R. Merighi
Affiliation:
Osservatorio Astronomico di Bologna, Bologna, Italy
M. Mignoli
Affiliation:
Osservatorio Astronomico di Bologna, Bologna, Italy
G. Stirpe
Affiliation:
Osservatorio Astronomico di Bologna, Bologna, Italy
G. Zamorani
Affiliation:
Osservatorio Astronomico di Bologna, Bologna, Italy
C. Collins
Affiliation:
Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK
H. Macgillivray
Affiliation:
Royal Observatory, Blackford Hill, Edinburgh EH9 3HJ, UK
C. Balkowski
Affiliation:
DAEC, Observatoire de Meudon, France
J.M. Alimi
Affiliation:
DAEC, Observatoire de Meudon, France
A. Blanchard
Affiliation:
DAEC, Observatoire de Meudon, France
V. Cayatte
Affiliation:
DAEC, Observatoire de Meudon, France
P. Felenbok
Affiliation:
DAEC, Observatoire de Meudon, France
S. Maurogordato
Affiliation:
DAEC, Observatoire de Meudon, France
D. Proust
Affiliation:
DAEC, Observatoire de Meudon, France
G. Chincarini
Affiliation:
Osservatorio Astronomico di Brera, Milano, Italy
L. Guzzo
Affiliation:
Osservatorio Astronomico di Brera, Milano, Italy
D. Maccagni
Affiliation:
Istituto di Fisica Cosmica e Tecnologie Relative, Milano, Italy
R. Scaramella
Affiliation:
Osservatorio Astronomico di Roma, Monteporzio Catone, Italy
M. Ramella
Affiliation:
Osservatorio Astronomico di Trieste, Trieste, Italy

Abstract

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We present preliminary results of a galaxy redshift survey we are accomplishing as an ESO Key Project over about 40 square degrees in a region near the South Galactic Pole, to a limiting magnitude bJ = 19.4. Up to now ∼ 50% of the survey has been completed, providing about 2000 galaxy redshifts.

Type
Part Fourteen: Mapping the Large-Scale Structure
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 687 - 691
Copyright
Copyright © Kluwer 1994 

References

Heydon-Dumbleton, N.H., Collins, C.A. and MacGillivray, H.T., 1988. In ‘Large-Scale Structures in the Universe’, eds. Seitter, W., Duerbeck, H.W. and Tacke, M., Springer-Verlag, p. 71.Google Scholar
Loveday, J., Peterson, B.A., Efstathiou, G. and Maddox, S.J., 1992. Astrophys. J, 390, 338.CrossRefGoogle Scholar
Lynden-Bell, D., 1971. Mon. Not. R. astron. Soc., 155, 95.CrossRefGoogle Scholar
Sandage, A., Tamman, G. and Yahil, A., 1979. Astrophys. J, 232, 252.Google Scholar