All Tables

Table 1: 36 X-ray sources (plus two additional structures) in the survey. We give the coordinates (from the SHARC wavelet analysis, see Adami et al. 2000), the optical imaging data origin and characteristics (exposure time ET in minutes), the X-ray data (ROSAT PSPC, XMM or Chandra and radial offset in arcmin), the optical spectroscopy data origin (S for SDSS, CA for Calar Alto or V for the VIMOS IFU), the source status (Single: X-ray point source, Cluster: galaxy structure, Pending: to be determined), an estimated redshift (if a galaxy structure), the ROSAT PSPC count rates (CR in units of 10^-3/s in the [0.5-2] keV range), except for Cl J1202+4439 where it is an XMM count rate in the [0.5-10] keV band; all the luminosities given are based on the assumption of the maximum estimated redshift, in units of 10⁴⁴ erg cm^-2 s^-1, and $n_{\rm H}$ in units of 10²² cm^-2. The two additional sources are not detected in the original SHARC analysis and we therefore do not give X-ray properties for them.