Space Telescope Science Institute  25MAMA-FUV-MAMA Clear 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 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 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.

 
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.

 

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