OBJ:  Normal SN Ia 1972E in NGC 5253.
DATE: JD2442163.  Bmax by Bruno is JD2441449.
      Therefore assuming an 18 d rise time the explosion was on
      JD2441431.
      Thus, this is day 732.
OBS:  Kirshner et al.
REP:  F_lambda (cgs-A) vs. lambda (ang)
COR:  not deredshifted??? (heliocentric velocity 403. from Asiago),
      not dereddened (foregroud E(B-V)=.0475),
      photometrically corrected ???? (Kirshner asserts that these
      spectra have an absolute energy distribution), not smoothed???
REF: \refpaper Kirshner, R.~P., \&~Oke, J.~B. 1975, ApJ, 200, 574.
          % nebular epoch spectra of Type~Ia SN~1972E
          % and analysis up to $\sim 700$ days after explosion.
          % The 72E spectrum set from day 253 with a claim to
          % photometric accuracy equal to photometry.
COMMET:  I scanned this from Kirshner & Oke 1975.

DAY:
    732.


END:
   3897.810     .12711E-16
   3961.145     .18038E-16
   4044.089     .82828E-17
   4119.274     .21736E-16
   4205.530     .45413E-16
   4293.591     .40568E-16
   4363.357     .42090E-16
   4444.477     .30987E-16
   4527.106     .36828E-16
   4611.272     .35009E-16
   4686.199     .44277E-16
   4784.325     .92083E-17
   4850.882     .48885E-16
   5009.804     .24899E-16
   5091.206     .25129E-16
   5173.932     .12308E-16
   5245.908     .70013E-17