Space Telescope Science Institute  25MAMA-NUV-MAMA, Clear F25ND5-NUV-MAMA

F25ND3-NUV-MAMA

Description

The F25ND3mode with the NUV-MAMA 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 near-UV imaging of objects too bright by 103for clear mode.

Pivot (Å)
FWHM (Å)
AB mag zeropoint
Speak
B
R80 (arcsec)
Flux in central pixel
2343.7
1344.5
16.62
2.38e+11
942.0
0.32
8%

Figure 14.28: F25ND3 NUV-MAMA Integrated System Throughput and Redleak

 

Table 14.12: Throughput and Sensitivity for F25ND3 NUV-MAMA
l
Sensitivity
Throughput %
1200.
9.75E9
4.0e-4
1300.
2.74E10
9.0e-4
1400.
3.77E10
1.2e-3
1500.
4.09E10
1.2e-3
1600.
3.80E10
1.0e-3
1700.
3.57E10
9.0e-4
1800.
3.81E10
9.0e-4
1900.
4.65E10
1.1e-3
2000.
6.27E10
1.4e-3
2100.
8.56E10
1.8e-3
2200.
1.13E11
2.3e-3
2300.
1.41E11
2.7e-3
2400.
1.70E11
3.1e-3
2500.
1.97E11
3.5e-3
2600.
2.19E11
3.7e-3
2700.
2.30E11
3.7e-3
2800.
2.33E11
3.7e-3
2900.
2.05E11
3.1e-3
3000.
1.61E11
2.4e-3
3100.
7.87E10
1.1e-3
Figure 14.29: Point Source S/N vs. V+AB for the F25ND3 NUV-MAMA mode. Top curves are for DARKTIME. Bottom curves are for average sky. Top curves are for DARKTIME. Bottom curves are for average sky.

 
Figure 14.30: Extended Source S/N vs. V+AB for the F25ND3 NUV-MAMA mode. Top curves are for an area of 0.2 arcsec2; bottom curves are for 1 arcsec2. Average sky assumed.

 
25MAMA-NUV-MAMA, Clear F25ND5-NUV-MAMA
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