The F25ND5
mode with the FUV-MAMA detector provides broad band imaging with an attenuation of 7 x 10-7. The field of view is 25 x 25 arcsec. The R80 and central pixel flux are unmeasured but assumed to be approximately the same as produced by the F25QTZ
filter.
Recommended for broad-band imaging of objects too bright by about a factor of 106 to meet FUV-MAMA BOP limits.
At FUV wavelengths the attenuation is closer to a factor of 106 rather than the nominal 105, but the throughput relative to the unfiltered FUV-MAMA is much larger at longer wavelengths, so special care should be taken for red sources. To make an accurate prediction of the expected count rate, observers should use a good approximation of the source spectrum as input for the STIS ETC.
Pivot ![]() |
FWHM (Å) |
AB mag zeropoint |
Speak |
B ![]() |
R80 (arcsec) |
Flux in central pixel |
---|---|---|---|---|---|---|
1385.1 |
333.6 |
8.188 |
8.81e7 |
377.2 |
0.28 |
10% |
Space Telescope Science Institute http://www.stsci.edu Voice: (410) 338-1082 help@stsci.edu |