All Tables

Table 1: Cosmological and gas physics parameters used in the simulations. Densities relative to critical density are labelled $\Omega$ . $\Omega _{\rm tot}$ is the density of universe, all components included, $\Omega _{\rm b}$ is the baryon density, $\Omega _{\Lambda }$ the vacuum energy density, $\Omega _{\rm DM}$ the dark matter density. h is the reduced Hubble constant, $n_{\rm s}$ the spectral index of primordial density power spectrum, $\sigma _8$ the rms density fluctuations in spheres of $8~\rm MPc$ diameter, $f_{\rm Mass}$ the mass function used in cluster abundance computations, $T_{\star }$ the cluster mass-temperature normalisation factor, and $f_{\rm g}$ the cluster gas mass fraction. The double vertical line destinguishes the primordial cosmological parameters, from the ingredients of the structure formation semi-analytic model.
Table 2: Foreseen experimental features of the Olimpo balloon bolometer project.
Table 3: Selection function versus redshift. Value entered correspond to 90% efficiency.