Comparison of the properties of the SNe II and their hosts in our sample to the SNe II presented in A14/G17 and G18. The top and middle panels show, respectively, the distribution of the apparent (m_V) and absolute (M_V) magnitudes in V band at peak brightness for the transients. Apparent magnitudes for the A14/G17 sample are estimated using values of M_V, distance modulus, host and Milky Way extinction provided by the authors, while for the G18 sample apparent magnitudes are estimated using the M_V and Milky Way extinction values provided in the paper. The bottom panel shows the distribution of the SN host galaxy redshift as a function of the host absolute magnitude in B band, M_B. For A14/G17 and G18, the host redshift is estimated using the recession velocity, while for the ASAS-SN sample we use the host z_CMB reported in Table 2.