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Sensitivity is limited by geocoronal Lyman-α. Observers can limit the background (with some cost to the total amount of observing time per orbit) by using the DARKTIME special requirement.
Pivot λ (Å) Speak Bλ R80 (arcsec) Figure 14.88: F25LYA FUV-MAMA Integrated System Throughput and RedleakTable 14.36: F25LYA FUV-MAMA Sensitivity & Throughput
Figure 14.89: Point Source S/N vs. flux for the F25LYA FUV-MAMA mode. Curves are labeled by required exposure time (seconds).Figure 14.90: Extended Source S/N vs. flux for the F25LYA 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).Table 14.37: Radial Profile for F25LYA*
Figure 14.91: Point Source PSF for F25LYA FUV-MAMA, 7."5 square (at pixel 739, 368, log scaled, B-V=-0.04)Figure 14.92: Point Source Encircled Energy for F25LYA FUV-MAMAFigure 14.93: Point Source Intensity vs. Radius for F25LYA FUV-MAMA