- Table 1:
Fit parameters for a
model centred on M1 and M2: S0 is the central surface brightness,
is the core radius, and
is the slope parameter.
- Table 2:
List of point sources detected in the field covered by MOS CCD.
Columns 1-3 give the source identification number, and its coordinates (J2000). In Cols. 4 and 5 the source count rate (in counts per second) and the radius (in arcseconds) out to which the source can be detected, respectively, are listed.
- Table 3:
Results of the spectral fits for the whole cluster. Column 1: line number. Column 2: detectors in use. In Cols. 3-6 the fit parameters (temperature in keV, metallicity in solar units, redshift and HI column density in
are listed. In Col. 7 is the fit reduced .
- Table 4:
Results of the spectral fits for the three subregions using a MeKaL model. HI column density and redshift are fixed to the average values for the whole cluster. Column 1: region analyzed. In Cols. 2 and 3 the fit parameters (temperature in keV and metal abundance, respectively) are listed. In Col. 4 is the reduced
of the fit.
- Table 5:
Numerical values for the mass determination in the two subclusters M1 and M2.
- Table 6:
Numerical values for the mass determination in cluster CL 0939+4713 for two specific radii; the masses are computed using the fit parameters for the profile centred on subcluster M2.