Astronomy & Astrophysics

Table 1: List of SNe discovered by the Mount Stromlo Abell cluster SN search . * indicate those SNe which occurred within the targeted cluster. $^{\dagger }$ indicates those SNe which were spectroscopically classified. The SNIa? (i.e. those without the $^{\dagger }$ ) were classified through the goodness of fit of the template light curves (Sect. 4.4.2) and hence could be SNe of another type that have been misclassified. Those SNe designated nIa were deemed not to be SNIa through the template fits and were not investigated further.
Table 2: Averaged colour terms for the CTIO data.
Table 3: The $\Delta m_{15}$ , $B_{\max}$ , $V_{\max}$ , $R_{\max}$ , $I_{\max}$ , z and the distance modulus for each of the SNe determined to be SNIa. Also included are the values we derived for the SNe listed in Phillips et al. (1999). The errors are listed in parentheses in units of $0.01^{\rm m}$ .
Table 4: Cepheid Calibration of SNIa for Measuring H₀.