Fig. 10.
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Luminosity functions of ccSNe. The solid red distribution shows the V-band LF considering all the ccSNe in our sample, while the dashed blue, orange, and green lines show the V-band LFs for SNe II, SESNe, and Interacting SNe, respectively. We also show the ASAS-SN V-band LF for SNe Ia from D24, and the r-band ZTF-BTS ccSN LF from P20. The LFs are corrected for Galactic but not for host galaxy extinction.
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