| Space Telescope Imaging Spectrograph Instrument Handbook for Cycle 14 | |||||
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F25MGII-NUV-MAMA
Description
The
F25MGIIfilter with the NUV-MAMA provides narrow-band imaging centered on the 2798 Å Mg II feature.Recommended Uses
Special Considerations
There is a substantial redleak in this filter. Sources with a red underlying continuum may be difficult to observe. Users should be careful to take into account the underlying continuum in estimating whether the observation will fall within the bright-object protection limits. This filter also has a complex PSF and exhibits several ghosts.
Figure 14.44: Point Source PSF for F25MGII NUV-MAMA 7."5 square (at pixel 316,658, log scaled, B-V=-0.04). Note psf ghost ~45 pixels left of peak pixel and a few 10-3 of the peak, as well as the much more complex ghost about 10 pixels to the right of the central pixel.
Figure 14.45: F25MGII NUV-MAMA Integrated System Throughput and Redleak
Table 14.18: Throughput and Sensitivity for F25MGII NUV-MAMA
Figure 14.46: Point Source S/N vs. V+ABfor the F25MGII NUV-MAMA mode. Curves are labeled by required exposure time (sec).
Figure 14.47: Extended Source S/N vs. V+ABfor the F25MGII 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 (sec).
Table 14.19: Radial Profile for F25MGII*
* See
Figure 14.48: Point Source Encircled Energy for F25MGII NUV-MAMASTIS ISR 2003-01.
Figure 14.49: Point Source Intensity vs. Radius for F25MGII NUV-MAMA
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Space Telescope Science Institute http://www.stsci.edu Voice: (410) 338-1082 help@stsci.edu |