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Space Telescope Imaging Spectrograph Instrument Handbook for Cycle 22 > Chapter 14: ImagingReference Material > F25SRF2—NUV-MAMA, Longpass

F25SRF2—NUV-MAMA, Longpass
Description
The F25SRF2 filter with the NUV-MAMA provides high-throughput broad-band NUV imaging with better rejection of geocoronal emission than the F25MAMA but worse than or F25QTZ modes. It provides the same field of view and high spatial resolution.
Recommended Uses
This filter has slightly higher throughput than F25QTZ, but lets in geocoronal [O I] 1302 + 1306 . In most cases the sky background will still be lower than the detector background.
Special Considerations
Sky background on the day side of the orbit contains a significant contributions from [OII] air glow emission at 2471 and [O I] air glow at 1302 + 1306 . In high-background conditions, the sky background can dominate the detector background. In average day-side observing conditions about half the background will be from the sky and half from detector dark current. Also, the background through F25SRF2 will be about 10% higher than through F25QTZ. Observers can limit the background by using the DARKTIME special requirement.
Users should also consider whether the ACS HRC with the F220W or the F250W filter might be a better choice for their science goals.
 
Pivot λ ()
Speak
Bλ
R80 (arcsec)
Figure 14.41: F25SRF2 NUV-MAMA Integrated System Throughput and Redleak
Table 14.17: F25SRF2 NUV-MAMA Sensitivity & Throughput
Figure 14.42: Point Source S/N vs. V+ABν for the F25SRF2 NUV-MAMA mode. Top curves are for DARKTIME. Bottom curves are for average sky. Curves are labeled by required exposure time (seconds).
Figure 14.43: Extended Source S/N vs. V+ABν for the F25SRF2 NUV-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).

Space Telescope Imaging Spectrograph Instrument Handbook for Cycle 22 > Chapter 14: ImagingReference Material > F25SRF2—NUV-MAMA, Longpass

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