- ... results
- The catalogue is only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr
(130.79.128.5) or via
http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/374/861
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...
- The Appendix is only available in electronic form at http://www.edpsciences.orig
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...
- Present address: ASTRON, PO Box 2, 7990 AA Dwingeloo, The Netherlands.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... 1 Mpc
- We use H0 =
50 kms-1Mpc-1 and q0 = 0.5 throughout this paper.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ... 1 Jy
-
From a recent paper by Lara et al. (2001), however, it was noted that
three genuine candidate sources
were missed after a first selection round from WENSS (B1838+658,
B1919+741, B0603+612). The source B1838+658 has a
redshift of 0.23 (NED) and is as such a GRG; for B1919+741 the
redshift is 0.194 and for B0603+612 it is 0.227 (Lara
et al. 2001).
Also, the source B1855+310 was not further observed.
Further, high resolution observations by Lara et al. show that some
sources, whose size was estimated to be less than
on basis of
the WENSS maps, actually have angular sizes
and should
thus be included in our candidate sample.
The implication of these findings is that the earlier made claim that we
have observed a complete flux-density limited sample of GRGs (Paper II, Schoenmakers et al. 2000b), must be recalled.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.