Space Telescope Science Institute  F25CN270-NUV-MAMA F25CN182-NUV-MAMA

F25CIII-NUV-MAMA


Description

The F25CIII filter with the NUV-MAMA provides narrow band imaging of the 1909 Å C III] feature.

Recommended Uses

C III] imaging.

Pivot (Å)
FWHM (Å)
AB mag zeropoint
Speak
B
R80 (arcsec)
Flux in central pixel
2013.3
375.0
19.417
1.05e+13
207.6
0.23
10%

Figure 14.55: F25CIII NUV-MAMA Integrated System Throughput and Redleak

 

Table 14.22: Throughput and Sensitivity for F25CIII NUV-MAMA
l
Sensitivity
Throughput %
1750.
1.74E11
0.00
1800.
3.68E11
0.01
1850.
1.27E12
0.03
1900.
4.84E12
0.11
1950.
9.54E13
0.21
2000.
9.94E13
0.22
2050.
7.36E12
0.16
2100.
4.14E12
0.09
2150.
1.96E12
0.04
2200.
8.65E11
0.02
2250.
4.25E11
0.01
Figure 14.56: Point Source S/N vs. V+AB for the F25CIII NUV-MAMA mode.

 
Figure 14.57: Extended Source S/N vs. V+AB for the F25CIII NUV-MAMA mode. Top curves are for an area of 0.2 arcsec2; bottom curves are for 1 arcsec2. Average sky assumed.

 

Table 14.23: Radial Profile for F25CIII
Radius

Fraction of Energy Encircled
Pixels
Arcsec
intensity
1
0.024
4.859e-02
0.173
2
0.037
3.660e-02
0.284
2
0.049
2.557e-02
0.392
3
0.073
9.899e-03
0.528
4
0.098
3.609e-03
0.598
5
0.122
1.832e-03
0.649
10
0.245
2.759e-04
0.753
15
0.367
1.339e-04
0.822
20
0.490
7.056e-05
0.873
25
0.613
4.358e-05
0.911
30
0.735
3.353e-05
0.944
40
0.980
1.002e-05
0.981
Figure 14.58: Point Source PSF for F25CIII NUV-MAMA, 7."5 square (at pixel 741,402, log scaled, B-V=-0.04). Note PSF ghost ~45 pixels left of peak pixel and a few 10-3 of the peak

 
Figure 14.59: Point Source Encircled Energy for F25CIII NUV-MAMA

 
Figure 14.60: Point Source Intensity vs. Radius for F25CIII NUV-MAMA

 

F25CN270-NUV-MAMA F25CN182-NUV-MAMA
Space Telescope Science Institute
http://www.stsci.edu
Voice: (410) 338-1082
help@stsci.edu