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Projected Clustering Around 1 < Z < 2 Radiogalaxies

Published online by Cambridge University Press:  25 May 2016

E. Martínez-González ,
N. Benítez ,
J. I. González-Serrano  and
L. Cayón
E. Martínez-González
Affiliation:
Dpto. de Física Moderna, Universidad de Cantabria and Instituto de Física de Cantabria, CSIC–Universidad de Cantabria, Facultad de Ciencias, Avda. de Los Castros s/n, 39005 Santander, Spain
N. Benítez
Affiliation:
Dpto. de Física Moderna, Universidad de Cantabria and Instituto de Física de Cantabria, CSIC–Universidad de Cantabria, Facultad de Ciencias, Avda. de Los Castros s/n, 39005 Santander, Spain
J. I. González-Serrano
Affiliation:
Dpto. de Física Moderna, Universidad de Cantabria and Instituto de Física de Cantabria, CSIC–Universidad de Cantabria, Facultad de Ciencias, Avda. de Los Castros s/n, 39005 Santander, Spain
L. Cayón
Affiliation:
Lawrence Berkeley Laboratory and Center for Particle Astrophysics, Berkeley, CA 94720, USA

Abstract

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We have taken deep R-band images of fields around five radiogalaxies: 0956+47, 1217+36, 3C256, 3C324 and 3C294 with 1 < z < 2. We found a statistically significant excess of bright (19.5 < R < 22) galaxies on scales of 2 arcmin around the radiogalaxies. The excess has been determined empirically to be at ≳99.5% level. It is remarkable that this excess is not present for 22 < R < 23.75 galaxies within the same area, suggesting that the excess is not physically associated to the galaxies but due to intervening groups and then related to gravitational lensing.

Type
Part II: Contributed Papers
Information
Symposium - International Astronomical Union , Volume 168: Examining the Big Bang and the Diffuse Background Radiations , 1996 , pp. 493 - 496
Copyright
Copyright © Kluwer 1996 

References

Bartelmann, M. and Schneider, P. 1993, preprint.Google Scholar
Bartelmann, M., Schneider, P. and Hasinger, G., 1994, Astron. Astrophys., in press.Google Scholar
Boyle, B.J. and Couch, W.J. 1993, Mon. Not. R. astr. Soc., 264, 604.Google Scholar
Draper, P.W. and Eaton, N. 1992, Starlink Project User Note 109.5, Rutherford Appleton Laboratory.Google Scholar
Dickinson, M. 1994, private communication.Google Scholar
Ellingson, E., Yee, H.K.C. and Green, R.F. 1991, Ap. J., 371, 49.Google Scholar
Fried, J.W., Stickel, M. and Kühr, H. 1993, Astron. Astrophys., 268, 53.Google Scholar
Hammer, F., and Le Fevre, O. 1990, Ap. J., 357, 38.CrossRefGoogle Scholar
Hill, G.J. and Lilly, S.J. 1991, Ap. J., 367, 1.CrossRefGoogle Scholar
Hintzen, P., Romanishin, W. and Valdés, F. 1991, Ap. J., 366, 7.CrossRefGoogle Scholar
Lilly, S.J. and Prestage, R.M. 1987, Mon. Not. R. astr. Soc., 225, 531.Google Scholar
Seitz, S. and Schneider, P. 1994, preprint.Google Scholar
Wu, X.P., Hammer, F. 1994, to appear in Astron. Astrophys.,.Google Scholar
Yee, H.C. and Green, R.F. 1987, Ap. J., 319, 28.Google Scholar