The PCCS completeness level outside the Galactic plane (see Table 1) is shown relative to other wide area surveys. The ERCSC completeness levels have been obtained from Planck Collaboration XIII (2011) up to 70 GHz and Planck Collaboration Int. VII (2013) for the other channels, while the WMAP ones are from González-Nuevo et al. (2008) up to 41 GHz and Lanz et al. (2013) for 61 and 94 GHz. The sensitivity levels for Herschel SPIRE and PACS instruments are from Clements et al. (2010) and Rigby et al. (2011), respectively. The other wide area surveys shown as a comparison are: GB6 (Gregory et al. 1996), CRATES (Healey et al. 2007), AT20G (Murphy et al. 2010), PACO (Bonavera et al. 2011), SPT (Mocanu et al. 2013), ACT (Marsden et al. 2014) and IRAS (Beichman et al. 1988).