Compilation of literature values for dust mass determinations based on mid-IR SED analyses in several individual CCSNe. The orange stars mark the dust masses of SN 1993J determined during this work. Other blue labels mark the cases of SNe IIP 2004et, 2017eaw (Shahbandeh et al. 2023), and SN IIL 1980K (Zsíros et al. 2024), where the estimated dust masses are also based on the recent analyses of JWST/MIRI SEDs. Dashed lines show examples of rapid (turquoise line, Sarangi & Cherchneff 2015) and steady continuous (pink line, Wesson et al. 2015) dust-formation theories. The source of the original interactive diagram is Roger Wesson’s homepage (https://nebulousresearch.org/dustmasses/).