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STIS Instrument Handbook
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The 25MAMA mode with the FUV-MAMA detector provides high-throughput broad-band far-ultraviolet (FUV) imaging with the highest available throughput at ~1500 Å and the highest possible spatial resolution. The field of view is 25x25 arcsec.
Recommended for broad-band NUV imaging of sources where sky background is not a consideration.
For long exposures of faint targets, sky background is likely to be a limiting factor. Observers should consider the use of DARKTIME or (preferably) use the F25QTZ filter, which has nearly the same throughput but rejects geocoronal Lyman-α and [O I] 1302 + 1306 Å air glow.
Users may also want to consider whether the ACS SBC detector might be better for their observing program.
Pivot λ (Å)
FWHM (Å)
AB mag zero point
Speak
Bλ
R80 (arcsec)
Table 14.1: 25MAMA FUV-MAMA Sensitivity & Throughput
Figure 14.72: Point Source S/N vs. V+ABν for the 25MAMA FUV-MAMA mode. Curves are labeled by required exposure time (seconds).
Figure 14.73: Extended Source S/N vs. V+ABν for the 25MAMA FUV-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

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