Space Telescope Science Institute  25MAMAD1-FUV-MAMA Pseudo-aperture F25ND5-FUV-MAMA

F25ND3-FUV-MAMA

Description

The F25ND3mode with the FUV-MAMA detector provides broad band imaging with an attenuation of 10-3. The field of view is 25x25 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 bright objects requiring 10-3 attenuation to meet FUV-MAMA bright-object protection limits.

Pivot (Å)
FWHM (Å)
AB mag zeropoint
Speak
B
R80 (arcsec)
Flux in central pixel
1376.0
316.2
16.070
1.26e+11
368.9
0.28
10%

Figure 14.71: F25ND3 FUV-MAMA Integrated System Throughput and Redleak

 

Table 14.28: Throughput and Sensitivity for F25ND3 FUV-MAMA
l
Sensitivity
Throughput %
1150.
1.07E10
0.41e-3
1175.
4.69E10
1.75e-3
1200.
8.42E10
3.08e-3
1225.
1.14E11
4.08e-3
1250.
1.24E11
4.35e-3
1300.
1.25E11
4.22e-3
1350.
1.20E11
3.91e-3
1375.
1.16E11
3.71e-3
1400.
1.10E11
3.46e-3
1425.
1.03E11
3.16e-3
1450.
9.37E10
2.84e-3
1475.
8.49E10
2.53e-3
1500.
7.59E10
2.22e-3
1550.
5.93E10
1.68e-3
1600.
4.37E10
1.20e-3
1650.
3.20E10
0.85e-3
1700.
2.16E10
0.56e-3
1750.
1.45E10
0.36e-3
1800.
9.53E9
0.23e-3
1850.
3.53E9
0.08e-3
1875.
1.64E9
0.04e-3
Figure 14.72: Point Source S/N vs. V+AB for the F25ND3 FUV-MAMA mode. Curves are labeled by required exposure time (sec).

 
Figure 14.73: Extended Source S/N vs. V+AB for the F25ND3 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).

 
25MAMAD1-FUV-MAMA Pseudo-aperture F25ND5-FUV-MAMA
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