25MAMA-FUV-MAMA Clear
Description
The 25MAMA mode with the FUV-MAMA detector provides high-throughput broad-band far-UV imaging with the highest available throughput at ~1500 Å and the highest possible spatial resolution. The field of view is 25x25 arcsec.
Recommended Uses
Recommended for broad-band near-UV imaging of sources where sky background is not a consideration.
Special Considerations
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-
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 (Å)
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FWHM (Å)
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AB mag zero point
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Speak
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B
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R80 (arcsec)
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Flux in central pixel
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Figure 14.66: 25MAMA FUV-MAMA Integrated System Throughput and Redleak

Table 14.26: 25MAMA FUV-MAMA Sensitivity & Throughput
Figure 14.67: Point Source S/N vs. V+AB
for the 25MAMA FUV-MAMA mode. Curves are labeled by required exposure time (sec).

Figure 14.68: Extended Source S/N vs. V+AB
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 (sec).

Table 14.27: Radial Profile for 25MAMA*
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Radius
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Fraction of Energy Encircled
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Pixels
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Arcsec
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Intensity
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* See STIS ISR 2003-01.
Figure 14.69: Point Source Encircled Energy for 25MAMA FUV-MAMA

Figure 14.70: Point Source Intensity vs. Radius for 25MAMA FUV-MAMA
