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STIS Instrument Handbook
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The 50CCD mode is very sensitive for broad-band optical imaging. For a fixed exposure time, it can detect point sources roughly 0.8 mag fainter than with WFPC2 with the F606W filter. However, the ACS WFC with the F606W or F814W will be a better choice for most users.
Recommended for deep imaging where detailed color information is not needed. In most cases the ACS WFC will be a better choice.
Pivot λ (Å)
FWHM (Å)
AB mag zero point
Speak
Bλ
R80 (arcsec)
Figure 14.4: Throughput for 50CCD
Figure 14.5: Point Source S/N vs. V+ABν for the 50CCD filter. Top curves are for low sky; bottom curves are for average sky. Curves are labeled by required exposure time (seconds).
Figure 14.6: Extended Source S/N vs. V+ABν for the 50CCD filter for gain=1. Top curves are for a source 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 14.7: Point Source PSF for 50CCD, 7."5 square (at pixel 518,517, log scaled, B-V=-0.25).

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