Table 1.
CRISP prefilters installed 2018.
Main diagnostic [nm] | Part # | CWL [nm] | FWHM [nm] | Tpeak | PC | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Mg I | 517.2 | 1 | (7) | 517.24 | (517.23) | 0.32 | (0.32) | 0.83 | (0.83) | ||||||
He D3 | 587.6 | 9 | 587.66 | 0.54 | 0.90 | ✓ | |||||||||
Fe I | 617.3 | (6) | 9 | (617.36) | 617.43 | (0.49) | 0.50 | (0.92) | 0.91 | ✓ | |||||
Fe I | 630.2 | (9) | 10 | (630.21) | 630.19 | (0.50) | 0.50 | (0.97) | 0.97 | ✓ | |||||
H-α | 656.3 | (1) | 10 | (656.30) | 656.40 | (0.52) | 0.53 | (0.89) | 0.89 | ||||||
Ca II | 854.2 | (7) | 10 | (854.22) | 854.23 | (0.84) | 0.83 | (0.96) | 0.97 | ✓ |
Notes. The CWL (center wavelength at normal incidence), Tpeak (peak transmission), and FWHM values are measured from the profiles plotted in Fig. 3. Part numbers were assigned by the manufacturer. PC: Calibrated telescope polarization model exists. The numbers in parentheses correspond to filters not currently installed in the CRISP filter wheel. Compare with Table A.1 in the CRISPRED paper.
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