Synthetic magnitudes of spectra. B_max is taken to have been 18 days after explosion. The spectra are NOT corrected for extinction or heliocentric redshift and so these should be observed magnitudes. I also havn't corrected to make the early spectra agree with a fit to Bruno's template. The zdaya spectra have have the correction for extinction, redshift, and Bruno's template fit. The day 732 spectrum was obtained by scanning from Kirshner & Oke (1975) and so the value for day 732 are especially suspect which is too bad because they are vitally important. Note none of the U magnitudes are from good coverage of the U band. Thus these U's are probably pretty poor. Omit altogether 34.0 .000 1 .000 1 12.192 1 9.666 1 9.392 0 No. t(days) U B V R I END: 22.0 8.904 1 8.981 0 8.828 0 8.838 0 9.186 0 23.0 8.637 1 8.721 0 8.593 0 8.691 0 9.106 0 24.0 8.499 1 8.633 0 8.545 0 8.701 0 9.119 0 27.0 9.132 1 9.085 0 8.870 0 9.053 0 9.413 0 29.0 9.561 1 9.402 0 9.279 0 9.433 0 9.522 0 30.0 9.830 1 9.642 0 9.230 0 9.416 0 9.595 0 38.0 10.547 1 10.285 0 9.474 0 9.354 0 9.343 0 41.0 10.395 1 10.142 0 9.261 0 9.200 0 9.223 0 44.0 10.811 1 10.637 0 9.694 0 9.423 0 9.262 0 53.0 11.626 1 11.365 0 10.351 0 10.198 0 9.878 0 62.0 12.081 1 11.681 0 10.755 0 10.610 0 10.489 0 73.0 11.707 1 11.309 0 10.480 0 10.281 0 10.250 0 76.0 11.995 1 11.727 0 11.033 0 10.880 0 10.896 0 98.0 13.489 1 12.321 1 11.659 0 11.571 0 11.656 0 222.0 18.653 1 13.998 1 13.730 0 14.509 0 14.587 0 253.0 15.740 1 14.480 0 14.347 0 15.153 0 15.120 0 365.0 17.677 1 16.207 0 16.107 0 16.886 0 16.104 0 434.0 17.527 1 17.276 0 17.168 0 17.775 0 16.661 1 732.0 23.653 1 20.837 1 22.091 1 .000 1 .000 1 0 means everything is OK. 1 means the spectrum did not cover the whole passband.