SN 1972E Ia in NGC 5253
OBJ: SN 1972E Ia in NGC 5253 (S? according to Leda) which in
Leda is
Leda: NGC 5253.
DISCOVERY: 1972may? UT by Kowal (1972).
MAX: 1972may11.5 (JD 2441449) in B according to a private communication long ago from Bruno Leibundgut.
Since the observations began post-Bmax, this is somewhat uncertain.
See the US Navy Observatory
Julian Date Converter.
Sometimes USNO is unavailable: try
OnlineConversion.com: Julian Converter
which is a modified version of USNO.
This day 132 of the year recalling that 1972 was
a leap year.
SUPERNOVA of the YEAR: M = 5.
Those were the good old days when there were only 10 to 20 SNe per year and we never
ran out of the alphabet.
COMMENT: This is a core normal SN Ia I guess.
Spectrum Date Phase relative to Bmax Observed Wavelength Range
kirshner1973b 1972may15.5 4. 3247.06--10644.78
kirshner1973b 1972may16.5 5. 3290.231--10659.75741
kirshner1973b 1972may17.5 6. 3282.95--10616.63
kirshner1973b 1972may20.5 9. 3281.47--10686.21
kirshner1973b 1972may22.5 11. 3402.255--9994.62
kirshner1973b 1972may23.5 12. 3423.316--10011.3086
kirshner1973b 1972may27.5 16. 6070.831--9981.905
kirshner1973b 1972may31.5 20. 3306.50--10565.328
REF:
CfA List of Supernovae.
\citet{conley2006} General value
of 19.4 days for Ia rise time in B.
\citet{kirshner1973a} They
give early photometry and narrow band photometry that approximates spectra.
\citet{kirshner1973b} They
give spectra from day +4 to day +235 relative to B max.
\citet{kirshner1975} They
give spectra from day +235 to day +714 relative to B max.
HEADER: Header Common header information for this supernovae.
The common header may (or may not) be updated relative to the header information above
(D. J. Jeffery (2007jan01)).
REP: F_lambda (erg/cm2/s/A) vs. lambda (ang) (iformat = 1)
COR: not deredshifted (heliocentric velocity 409 +/- 2 km/s from
Leda: NGC 5253
not dereddened (Galactic foreground 0.24/4=.06 reddening from
Leda: NGC 5253
but derived from
Schlegel et al. (1998)
not smoothed ????, not photometric ????
Derived bolometric maximum is ??? (see above).
OBS: One of
{kirshner1973b}
{kirshner1975}
But I seem to have scarfed all these SN 1972E spectra from Mark Philips's
anonymous ftp pub site when I was just poking around looking for goodies.
I think Mark must have just scanned them from {kirshner1973b} and {kirshner1975}.
They arn't at the
CfA Supernova Archive,
and so Bob Kirshner may have lost track of his versions.
That was 1997sep07 or so when I was in Oak Ridge, Tennessee.
Date: 1972may31 with 1972may11.5 (JD 2441449) for B maximum gives:
day = 2441469 - 2441449 = 20
&specnamelist
aname='sn1972e Ia 1972_05_31'
ebv=.06 !
epoch=20. ! This parameter needs to updated for the particular spectrum.
iformat=1 ! Not deredshifted as far as I know, but that's not very far.
ismooth=0
itick=2
itickln=4
t_rise=19.4d0 ! \citep{conley2006}, Just an average rise time.
v_helio=409.
ymin2=.6d-13
ymax2=9.d-13
ymin3=.3
ymax3=2.1
wlammin1=3306.50
wlammax1=10565.328
wlammin2=3306.50
wlammax2=10565.328
wlammin3=3600. ! As far as I trust to the blue.
wlammax3=9000. ! As far as I trust to the red.
/
Postscript plot of the spectrum.
Postscript plot of the spectrum with local normalization.
Information from somewhere:
BITPIX = 8 / 8-bit ASCII characters
NAXIS = 1 / Number of Image Dimensions
NAXIS1 = 500 / Length of axis
ORIGIN = 'NOAO-IRAF: WTEXTIMAGE' /
IRAF-MAX= 0. / Max image pixel (out of date)
IRAF-MIN= 0. / Min image pixel (out of date)
IRAF-B/P= 32 / Image bits per pixel
IRAFTYPE= 'REAL FLOATING ' / Image datatype
OBJECT = ' ' /
FILENAME= 'SN72E.469.IMH ' / IRAF filename
FORMAT = '5G14.7 ' / Text line format
W0 = 3306.5
WPC = 14.54675
CRVAL1 = 3306.5
CDELT1 = 14.54675
$END
OBJ: Normal SN Ia 1972E in NGC 5253.
DATE: JD2441469. Bmax by Bruno is JD2441449.
Therefore assuming an 18 d rise time the explosion was on
JD2441431.
Thus, this is day 38.
OBS: Kirshner et al.
REP: F_lambda (cgs-A) vs. lambda (ang)
COR: not deredshifted??? (heliocentric velocity 1804 from Asiago),
not dereddened (foregroud E(B-V)=???),
photometrically corrected ???? (Kirshner asserts that these
spectra have an absolute energy distribution), not smoothed???
REF: \refpaper Kirshner, R.~P., Oke, J.~B., Penston, M.~V., \&~Searle, L.
1973, ApJ, 185, 303.
% a study of supernova spectra, both I and II, with
% emphasis on Type~Ia SN~1972E. The full SN~1972E
% spectrum set with a claim (p. 307) for absolute
% flux calibration.
COMMNET: I scarfed up the 72E spectra from Mark Phillips anonymous ftp
pub site when I was just poking around looking for goodies.
The IRFLUX style for specmon.f is 12.
DAY:
38.
END:
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