| Space Telescope Imaging Spectrograph Instrument Handbook for Cycle 14 | |||||
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F25QTZ-FUV-MAMA, Longpass
Description
The
F25QTZfilter with the FUV-MAMA provides high-throughput broad-band far-UV imaging with better rejection of geocoronal emission than theF25MAMAorF25SRF2modes and the same field of view and spatial resolution.Recommended Uses
Recommended filter for broad-band far-UV imaging of faint targets.
Special Considerations
With this filter the background is dominated by detector dark current. The dark current is not constant across the detector and not constant in time. This could limit the sensitivity for very extended faint targets, however, note that the FUV-MAMA dark is extremely low.
Users may also want to consider whether the ACS SBC detector might be better for their observing program.
Figure 14.78: F25QTZ FUV-MAMA Integrated System Throughput and Redleak
Table 14.32: Throughput and Sensitivity for F25QTZ FUV-MAMA
Figure 14.79: Point source S/N vs. V+ABfor the F25QTZ FUV-MAMA mode. Curves are labeled by required exposure time (sec).
Figure 14.80: Extended source S/N vs. V+ABfor the F25QTZ 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 14.33: Radial Profile for F25QTZ*
* See
Figure 14.81: Point Source Encircled Energy for F25QTZ FUV-MAMASTIS ISR 2003-01.
Figure 14.82: Point Source Intensity vs. Radius for F25QTZ FUV-MAMA
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Space Telescope Science Institute http://www.stsci.edu Voice: (410) 338-1082 help@stsci.edu |