OBJ: SN Ibc 2005bf in MCG +00-27-5 (SB galaxy) (which Leda
calls PGC030473).
DISCOVERY: 2005apr06 by L. A. G. Monard at Bronberg Observatory;
M. Moore and W. Li at Lick Observatory.
MAX: 2005may09 UT (JD 2453499.8) in bolometric from \citet{folatelli2006}.
See the US Navy Observatory Julian Date Converter.
This day of the year 129.
SUPERNOVA of the YEAR: M = 58.
HEADER: D. J. Jeffery (2006jan01).
REF:
{anupama2005}
% The Peculiar Type Ib Supernova SN 2005bf: Explosion of a Massive He Star with a Thin Hydrogen Envelope?
% A very long rise 2-maximum Ibc SN.
% Just a letter.
{branch2007} SYNOW Synthetic spectrum analysis.
{folatelli2006}
% 25 coauthors
% SN 2005bf: A Possible Transition Event between Type Ib/c Supernovae and Gamma-Ray Bursts
% A very long rise 2-maximum Ibc SN.
{tominaga2005}
% about 25 coauthors
% The Unique Type Ib Supernova 2005bf: A WN Star Explosion Model for Peculiar Light Curves and Spectra
% A very long rise 2-maximum Ibc SN.
% Just a letter.
REP: F_lambda (erg/cm2/s/A) vs. lambda (ang) (iformat = 1)
COR: not deredshifted (heliocentric velocity 5656 +/- 7 and
v_hel corrected for CMB radiation 6006 km/s from
Leda: PGC030473 (MCG+00-27-005)
\bibitem[folatelli et al.(2006)]{follatelli2006} give 5670 km/s).
not dereddened (Galactic foreground .19/4... =.0475
Schlegel et al. (1998)
not smoothed ????, not photometric ????
Derived bolometric maximum is 2005may09 (see above).
OBS:
\bibitem[folatelli et al.(2006)]{follatelli2006}
Date: 2005 () with 2005may09 (JD 2453499.8) for bolometric maximum gives:
day = - 499.8 = (See JD in FITS information below).
&specnamelist
aname='sn2005bf Ibc 2005_'
ebv=.0475d0
epoch= ! This parameter needs to updated for the particular spectrum.
iformat=1
itick=2
itickln=4
t_rise=41.8d0 ! {follatelli2006}, p. 1049.
v_helio=5656.d0
ymin2=.2d-16
ymax2=4.5d-16
ymin3=.3
ymax3=3.
wlammin1=3800.d0
wlammax1=
wlammin2=3800.d0
wlammax2=
wlammin3=3800.d0
wlammax3=
/
Postscript plot of the spectrum.
Postscript plot of the spectrum with local normalization.
FITS: Fits format information from the observers.