Cards of identities of the supernovæ

This appendix shows the characteristics of the close supernovæ used during this analysis. They are for the majority exits of the three batches resulting from from Calàn-Tololo Supernova Survey (hamuy1996c) and from two research of CFA between 1993 and 1998 (riess1999) and between 1997 and 2000 jha2002.

C.1 table gives the principal observational characteristics of these supernovæ:

• their name and that of their galaxy host
• their position on the sky
• the number of observations per filter
• their redshift observed, that corrected for our movement compared to the CMB (this value was given by using astronomical waiter NED ).
• The value of the Galactic excess of color ($E(b-v)$) calculated starting from the charts of dust determined by schlegel1998.