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Table 6
Mean spectral resolving power and number of pixels per optical resolution element for each detector and each field of view.
Telescope 1 | Telescope 2 | ||||
Row | Strip | Resolving power | Resolution element (pix) | Resolving power | Resolution element (pix) |
4 | 15 | 12 587 | 2.798 ± 0.009 | 12 065 | 2.923 ± 0.009 |
4 | 16 | 12 361 | 2.849 ± 0.009 | 12 106 | 2.912 ± 0.008 |
4 | 17 | 12 240 | 2.876 ± 0.009 | 11 954 | 2.948 ± 0.009 |
5 | 15 | 12 159 | 2.891 ± 0.008 | 11 600 | 3.032 ± 0.010 |
5 | 16 | 12 430 | 2.827 ± 0.007 | 11 809 | 2.978 ± 0.009 |
5 | 17 | 12 085 | 2.908 ± 0.008 | 11 861 | 2.965 ± 0.009 |
6 | 15 | 12 021 | 2.919 ± 0.007 | 11 523 | 3.045 ± 0.010 |
6 | 16 | 12 132 | 2.891 ± 0.007 | 11 447 | 3.066 ± 0.011 |
6 | 17 | 12 148 | 2.888 ± 0.006 | 11 901 | 2.948 ± 0.009 |
7 | 15 | 12 117 | 2.890 ± 0.007 | 11 078 | 3.160 ± 0.010 |
7 | 16 | 11 885 | 2.946 ± 0.007 | 10 983 | 3.188 ± 0.010 |
7 | 17 | 11 525 | 3.038 ± 0.008 | 11 377 | 3.077 ± 0.009 |
Notes.From Panuzzo et al. (2015).
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