Table 4: Specinholucy parameters.
SN^a $\sigma _{\rm kernel}$ FWHM SN+bg^c SN/bg^d

[pixels] DIMM SSF

2002bo_1 4.0 6.25 6.93 63.6 4.8

2002bo_2 4.0 7.95 6.57 62.5 4.6

2002gr
2.2 5.85 3.46 9.0 1.4

2002go
3.5 5.75 3.97 5.2 2.1

^a IAU designation. Note that two spectra were taken of SN 2002bo.
^b Mean FWHM in pixels of the Gaussian seeing corresponding to the DIMM station measurement or to the SSF used to extract the spectrum.
^c Mean number of counts (ADU) in the dispersion direction of the input 2D spectrum at the location of the SN.
^d Ratio of the integrated SN flux and that of the underlying background. One can calculate the mean signal-to-noise per pixel using ${\rm SNR\ pix}^{-1} = {\rm SN/bg}+1$ .

**Table 4:** *Specinholucy* parameters.
SN^a	$\sigma _{\rm kernel}$	FWHM	SN+bg^c	SN/bg^d
	[pixels]	DIMM	SSF
2002bo_1	4.0	6.25	6.93	63.6	4.8
2002bo_2	4.0	7.95	6.57	62.5	4.6
2002gr	2.2	5.85	3.46	9.0	1.4
2002go	3.5	5.75	3.97	5.2	2.1

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