Table 1: SSF FWHM data.
SSF pixelsa arcsecondsa
SN 2002go $3.83^{4.74}_{3.48} \pm 0.41$ $0.77^{0.95}_{0.70} \pm 0.08$
star on slit $4.71^{5.44}_{4.18} \pm 0.39$ $0.94^{1.10}_{0.84} \pm 0.08$
standard star $4.17^{4.64}_{3.93} \pm 0.23$ $0.83^{0.93}_{0.79} \pm 0.05$

a The quoted values are read as $\langle{\rm mean}\rangle^{\max}_{\min} \pm 1\sigma$ error.

Source LaTeX | All tables | In the text

Article Contents
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
List of tables
List of figures