Table 5: Supernova observation summary.
SN^a Archive id.^b UT date z^c Phase^d

2002bo 2002bo 06 Dec. 2002 0.0042 +258

2002gr sloan9 11 Oct. 2002 0.091 +14 $^{\dag }$

2002go sloan5 11 Oct. 2002 0.236 +2 $^{\dag }$

^a IAU designation.
^b Target name for search in the ESO archive.
^c Redshift determined from nebular lines in the host galaxy.
^d SN phase in rest-frame days from B-band maximum. Phases marked with $^{\dag }$ have been determined from cross-correlations
with local SN Ia templates using the SuperNova IDentification (SNID) code (Tonry et al. 2005).

**Table 5:** Supernova observation summary.
SN^a	Archive id.^b	UT date	z^c	Phase^d
2002bo	2002bo	06 Dec. 2002	0.0042	+258
2002gr	sloan9	11 Oct. 2002	0.091	+14 $^{\dag }$
2002go	sloan5	11 Oct. 2002	0.236	+2 $^{\dag }$

Source LaTeX | All tables | In the text

	1 Introduction
	2 The algorithm and its implementation
	3 The importance of the slit spread function
	4 The spatial resolution kernel
	5 Testing the algorithm on simulated data
	6 Testing the algorithm on real data
	7 Comparison with other methods
	8 Conclusion
	References