All Tables

Table 1: Observational information of the galaxies.
Table 2: Total integrated MIR (4.5 $\mu {\rm m}$ , 6.7 $\mu {\rm m}$ and 15 $\mu {\rm m}$ ) fluxes inside the field of view for the galaxies in the sample.
Table 3: Model parameters. The age and metallicity as calculated from the PÉGASE stellar evolutionary model, and the dust mass and dust temperature as derived from black-body fits, assuming an emissivity index of $\beta = 1$ .
Table 4: The MIR excess at $6.7~\mu {\rm m}$ and $15~\mu {\rm m}$ for each galaxy. The excess is quantified as the excess beyond the stellar component which is modelled using the stellar evolutionary synthesis model PÉGASE.