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.