SN 1988L Ib in NGC 5480 (Sc)
OBJ: SN 1988L Ib in NGC 5480 (Sc). See
NGC 5480.
DISCOVERY: 1988apr30 by Berkeley Automated supernova search (Perlmutter & Pennypacker)
CfA Supernova List.
MAX: 1988apr30 which is just the discovery date {matheson2001}.
This day of the year 120.
SUPERNOVA of the YEAR: 12.
HEADER: D. J. Jeffery (2006jan01).
REF:
{matheson2001}
\bibitem[Matheson et al.(2001)]{matheson2001} Matheson, T.,
Filippenko, A. V., Li, W., Leonard, D. C., \& Shields, J. C.
2001, \aj, 121, 1648
%
% ADS Reference
% optical spectroscopy of type Ib/c supernovae
% The observational paper with all kinds of spectra reported.
% They derive R maximum and maxima for some supernovae.
REP: F_lambda (erg/cm2/s/A) ??? vs. lambda (ang) (iformat = -1)
COR: not deredshifted ??? (heliocentric velocity 1851 +/- 8 km/s and
v_hel corrected for CMB radiation 1991 km/s from
NGC 5480.
But {matheson2001} gives 2050 km/s from a superimposed H II region.
not dereddened ??? (Galactic foreground .08/4... =.02
Schlegel et al. (1998).
not smoothed ????, not photometric ????
Derived maximum in some band is (see above).
OBS: ??? David Branch got these from Alex Filippenko and/or Tom Matheson.
Date: 1988 () with 1988apr30 (121 which is just the discovery date in a leap year) for visible maximum gives:
day = - 121 =
&specnamelist
aname='sn1988l Ib 1988_'
ebv=.0475
epoch= ! This parameter needs to updated for the particular spectrum.
iformat=1 ! This is my first guess, but I'll have to check the spectra against the figures.
! Comparison to the figures shows that the data is f_lambda and it is not redshifted.
itick=2
itickln=4
t_rise=20.d0 ! Just the default rise time.
v_helio=2050. ! The redshift suggested by \citet{matheson2001}
ymin2=.1
ymax2=10.
ymin3=.3
ymax3=3.
wlammin1=
wlammax1=
wlammin2=
wlammax2=
wlammin3=
wlammax3=
/
Postscript plot of the spectrum.
Postscript plot of the spectrum with local normalization.
Information from somewhere.
These spectra are from /home/branch/synow/flipIbc/sn1988l
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