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Table 1

Input parameters for the seven dual FPI systems discussed.

Parameter/FPI system CRISP CRISPm CRISP2 CHROMIS EST-B EST-V EST-R
Telescope SST SST SST SST EST EST EST
FPI system status Obsolete Operational In progress Operational Proposal Proposal Proposal
Telescope diameter (m) 0.98 0.98 0.98 0.98 4.2 4.2 4.2
Input focal ratio 46 46 46 46 50 50 50
FOV diameter (arc min) Max Max Max Max 1.0 1.0 1.0
Etalon clear aperture (mm) 75 75 98 75 Min Min Min
Camera pixel size (μm) 16 6.5 6.5 5.48 5-12 6-12 6-12
Wavelength range (nm) 500-860 500-860 520-860 390-500 380-500 500-680 680-1000
Reference wavelength(s) (nm) 630 630 630 390 380 396 500 630 680 854
Required rms cavity error (nm) 2 2 2 2 2 2 2
Target Strehl intensity (%) 90 90 90 90 90 90 90
Spectral FWHM at ref. wavel. (pm) 6 6 7 8 7.9 6.3 11
Peak transmission (%) 90 90 90 90 90 90 90
Parasitic light level (%) 1.0 1.0 1.0 1.0 1.0 1.0 1.0
Prefilter type 2-cavity 2-cavity 2-cavity 2-cavity 2-cavity 2-cavity 2-cavity

Notes. CRISP and CRISPm are identical except for their camera lenses. The three designs of the FPI systems for EST were proposed by (Scharmer & Lindberg 2025), based on requirements decided by the EST Science Advisory Group, but have not been reviewed by the EST project. The first reference wavelength for EST FPI systems refers to the requirement on Strehl, the second to the requirement on spectral resolution. The Strehl intensities required refer to a combination of apodisation effects and optical design limitations.

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