Table 2: rms WFE, image rms width (for the two reference spectral types), and chromaticity at different field angle locations over the focal plane.
  X position Y position rms WFE Image rms width Image rms width Chromaticity
  [degrees] [degrees] [nm] for a B3V star [mas] for a M8V star [mas] [ $\rm {\mu as}$]
F1 0.53 0.00 22.03 39.27 42.85 0.00
F2 0.86 0.33 208.73 41.80 43.89 -3071.23
F3 0.86 -0.33 208.73 41.81 43.89 3070.16
F4 0.20 0.33 39.77 41.93 44.92 2077.02
F5 0.20 -0.33 39.77 41.93 44.92 -2077.02
F6 0.70 0.17 24.32 38.51 42.54 124.94
F7 0.70 -0.17 24.32 38.51 42.54 -124.94
F8 0.36 0.17 28.82 40.30 43.34 2545.20
F9 0.36 -0.17 28.83 40.30 43.34 -2545.20
F10 0.86 0.00 71.09 38.95 42.76 0.00
F11 0.53 -0.33 41.81 40.07 43.77 -389.84
F12 0.53 0.33 41.81 40.07 43.77 389.84
F13 0.20 0.00 18.59 39.28 43.02 0.00


Source LaTeX | All tables | In the text