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Table 1.

Sample studies of SNe IIn based on optical observations.

Reference Sample Lowest z Median z Maximum z Mode of sample Main area
size in sample in sample in sample source survey(s) of study
Li et al. (2002) 7 0.0022 0.0047 0.018 Targeted Late-time photometry
Richardson et al. (2002) 9 0.0028 0.0082 0.043 Targeted Luminosity function
Li et al. (2011) 7 0.0024 0.0088 0.012 Targeted Luminosity function
Kiewe et al. (2012) 4 0.015 0.024 0.031 Targeted Light-curves and spectra
Taddia et al. (2013) 7 0.0071 0.017 0.029 Mainly targeted Light-curves and spectra
Ofek et al. (2014c) 19 0.031 0.073 0.28 Untargeted Rise times
Ofek et al. (2014a) 16 0.004 0.031 0.14 Mainly untargeted Precursor outbursts
Richardson et al. (2014) 31 0.0021 0.016 0.35 Mainly targeted Luminosity function
Bilinski et al. (2015) 6 0.0061 0.0095 0.011 Targeted Precursor outbursts
de la Rosa et al. (2016) 8 0.004 0.01 0.017 Mainly targeted Light-curves

This work 42 0.014 0.078 0.313 Untargeted Light-curves

Notes. The works included in the table all discuss photometric properties of SNe IIn. For the sample size counts, the SNe labelled as SNe IIn by the respective authors were used. If available, the redshifts (z) of the SNe in each sample were taken from the respective papers. Otherwise, distance moduli or luminosity distances given in the papers were converted to redshifts using cosmological parameters from Sect. 3 without infall correction. Li et al. (2002) gives no distance information for their sample SNe; here, NED redshifts for their respective SN host galaxies were used.

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