SN 1997ef Ic in UGC 4107 (Sc)

OBJ:  SN 1997ef Ic in UGC 4107 (Sc).  See
          UGC 4107.
DISCOVERY: 1997nov25 by Sano.  See CfA Supernova List.
MAX:  1997dec10 in V and UVOIR bolometric {mazzali2002}.  
           This day of the year 344.
SUPERNOVA of the YEAR:  136.

HEADER:  D. J. Jeffery (2006jan01).

REF:

    {deaton1998}
\bibitem[Deaton et al.(1998)]{deaton1998}
        Deaton, J., Branch, D., Baron, E., Fisher, A., Kirshner, R., \&~Garnavich, P. 1998,
        American Astronomical Society, 192nd AAS Meeting, \#06.10;
        Bulletin of the American Astronomical Society, Vol. 30, p.824
%
        % ADS Reference
        % Spectral Analysis of the Peculiar Type IC Supernova 1997ef in UGC 4107.

    {mazzali2000}
\bibitem[Mazzali et al.(2000)]{mazzali2000}
        Mazzali, P. A., Iwamoto, K., Nomoto, K. 2000, \apj 545, 407
%
        % ADS Reference
        % A Spectroscopic Analysis of the Energetic Type Ic Hypernova SN 1997EF.
        % Paolo calls it a hypernovae and gives V max as 1997dec10 which is nearly UVOIR bolometric max.
        % He finds a rise time of about 18 days.



REP:  F_lambda (erg/cm2/s/A) ??? vs. lambda (ang)  (iformat = -1)
COR:  deredshifted ??? (heliocentric velocity 3506 +/- 10 km/s and 
        v_hel corrected for CMB radiation 3626 km/s from
          UGC 4107.
      not dereddened ??? (Galactic foreground .19/4... =.0475
     Schlegel et al. (1998).
      not smoothed ????, not photometric ????
      Derived maximum in some band is  (see above).

OBS:  ??? I got these from Peter Garnavich.

Date: 1997 () with 1997dec10 (344) for visible maximum gives:
      day = - 344 = 



&specnamelist
   aname='sn1997ef Ic hyp 1997_'
   ebv=.0475
   epoch=              ! This parameter needs to updated for the particular spectrum.
   iformat=-1
   itick=2
   itickln=4
   t_rise=18.d0         ! Based on \citet{mazzali2000} 
   v_helio=3506.        ! The Garnavich spectra have been deredshifted.  The v_helio=3506 +/- 10 km/s.  iformat < 0 means no further correction.
   ymin2=1.d-17
   ymax2=1.d-12
   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. 

From: Peter Garnavich 
Message-Id: <199901141951.OAA10375@mars.harvard.edu>
Subject: Re: 97ef
To: jeffery@beauty.physics.unlv.edu (David Jeffery)
Date: Thu, 14 Jan 1999 14:51:54 -0500 (EST)

David,

  Thanks for the reminder. I've put all the spectra I have
on 97ef at my anonymous ftp site. You can get them by:

ftp cfa0.harvard.edu

username: anonymous
password: your-email-address

cd outgoing/peterg/sn97ef
mget *.dat
bye

They are all ASCII two column spectra with the header
at the top (which may or may not help). The spectra have
been reduce in the usual way plus the spectra *** have been shifted to the rest frame ***
and narrow emission lines removed.
Let me know if you have any problems.

Peter

(Where I got all the 97ef spectra from.
Note according to Iwamoto et al. (1999, astro-ph/9807060)
the heliocentric velocity is 3400 km/s.
This has been removed from the spectra according to Peter above.)