Fig. 2
Distribution of the stellar masses derived using the average M/L ratios described in Bell & de Jong (2001) and the B- and V-band photometry (Y axis in all panels) along the stellar masses derived using other procedures (X axis in all panels): top-left panel: stellar masses derived using the entire five-bands SDSS photometry and the M/L ratio provided by the SED analysis performed using PARADISE; top-right panel: stellar masses derived using the 2MASS K-band photometry and the M/L ratio provided in Longhetti & Saracco (2009); bottom-left panel: stellar masses derived using the CALIFA datacube spectrophotometry and the M/L ratio provided by PyCASSO/Starlight; and bottom-right panel: stellar Masses derived from CALIFA datacube spectrophotometry and the M/L ratio provided by FIT3D.
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