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STIS Instrument Handbook
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The F25CIII filter with the NUV-MAMA provides narrow band imaging of the C III] 1907 + 1909 Å feature.
Pivot λ (Å)
FWHM (Å)
AB mag zero point
Speak
Bλ
R80 (arcsec)
Table 14.12: F25CIII NUV-MAMA Sensitivity & Throughput
Figure 14.60: Point Source S/N vs. V+ABν for the F25CIII NUV-MAMA mode. Curves are labeled by required exposure time (seconds).
Figure 14.61: Extended Source S/N vs. V+ABν for the F25CIII NUV-MAMA mode. Top curves are for an area of 0.2 arcsec2; bottom curves are for 1 arcsec2. Average sky assumed. Curves are labeled by required exposure time (seconds).
Fraction of Energy Encircled
Figure 14.62: Point Source PSF for F25CIII NUV-MAMA, 7."5 square (at pixel 741,402, log scaled, B-V=-0.04). Note PSF ghost ~45 pixels left of peak pixel and a few 10-3 of the peak

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