Space Telescope Science Institute  F25ND3-FUV-MAMA F25NDQ - FUV-MAMA

F25ND5-FUV-MAMA


Description

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 Uses

Recommended for broad-band imaging of objects too bright by about a factor of 106 to meet FUV-MAMA BOP limits.

Special Considerations

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 (Å)
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%

Figure 14.74: F25ND5 FUV-MAMA Integrated System Throughput and Redleak

 

Table 14.29: Throughput and Sensitivity for F25ND5 FUV-MAMA
l
Sensitivity
Throughput %
1150.
7.19E6
2.75e-7
1175.
3.23E7
1.21e-6
1200.
5.90E7
2.16e-6
1225.
8.03E7
2.88e-6
1250.
8.69E7
3.05e-6
1300.
8.51E7
2.87e-6
1350.
7.89E7
2.56e-6
1375.
7.51E7
2.40e-6
1400.
7.12E7
2.23e-6
1425.
6.66E7
2.05e-6
1450.
6.23E7
1.88e-6
1475.
5.83E7
1.74e-6
1500.
5.43E7
1.59e-6
1550.
4.65E7
1.32e-6
1600.
3.73E7
1.02e-6
1650.
2.91E7
7.75e-7
1700.
2.01E7
5.19e-7
1750.
1.32E7
3.31e-7
1800.
8.07E6
1.97e-7
1850.
2.67E6
6.34e-7
1875.
1.16E6
2.71e-8
Figure 14.75: Point Source S/N vs. V+AB for the F25ND5 FUV-MAMA mode.

 
Figure 14.76: Extended Source S/N vs. V+AB for the F25ND5 FUV-MAMA mode. Top curves are for an area of 0.2 arcsec2; bottom curves are for 1 arcsec2. Average sky assumed.

 

F25ND3-FUV-MAMA F25NDQ - FUV-MAMA
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