Table 10.2 has the result of the adjustments of the lightcurves of Nos three supernovæ.
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The magnitudes are each time expressed in the filters U and B Johnson-Cousins in the reference frame of the supernova. Absorptions are expressed in magnitude in the filters of observation of the supernovæ V and R for 2000fr and I and Z for 2001gn and 2001hb. Enfin, the K-corrections make it possible to pass from the observant filters to the filters in the reference frame of the supernova.
The value of the color of 2001gn ( knop2003).
This supernova thus has either a very atypical color, or there is a problem in the evaluation magnitude to the maximum of the curves of light in Z or out of I the lightcurves of 2001gn are presented in the appendix B . We point out that only one measurement in Z was taken, it thus exists can be a problem with this single point. Moreover, we based our construction of the lightcurves by using the items zero of camera ACS which are not yet very well-known.
Lastly, the
magnitude to the maximum of 2001gn out of I seems to be in agreement
with the flux awaited of a supernova of the Ia type to a shift towards
the red of 1.1 for standard cosmology. We will thus build our
estimators of distance by using an analysis identical to that of
perlmutter1999, i.e. , by considering only the corrections of factor of stretching and by selecting the nonextinct close supernovæ (with around -0.4 to the maximum), that is to say 12 supernovæ among the 15 previously selected.