Space Telescope Science Institute  F28X50OIII-CCD 50CORON-Clear CCD

F28X50OII-CCD


Description

The F28X50OII mode is useful for narrow-band imaging of OII 3727 Å. The high throughput and high spatial resolution provide a significant advantage over WFPC2 imaging with the F375N filter for some purposes. The narrow bandpass may offer some advantage over ACS and either the HRC or WFC with the [O II] ramp filter.

Recommended Uses

Recommended for deep high-resolution O II imaging.

Special Considerations

This filter does not have a significant red leak. Flat field images taken through this filter show scattered light at the top and bottom of the frame. This is not expected to be a problem for astronomical targets

.
Pivot (Å)
FWHM (Å)
AB mag zeropoint
Speak
B
R80 (arcsec)
Flux in central pixel
3737.3
62.0
20.534
3.47e+14
60.5
0.12
17%

Figure 14.18: Throughput for F28x50OII

 

Table 14.8: Throughput and Sensitivity for F28X50OII
l
Sensitivity
Throughput %
3675.
6.32E12
0.08
3685.
3.35E13
0.40
3695.
9.91E13
1.18
3705.
1.65E14
1.95
3715.
2.25E14
2.66
3725.
2.73E14
3.22
3735.
2.49E14
2.92
3745.
2.68E14
3.14
3755.
3.15E14
3.68
3765.
2.93E14
3.41
3775.
1.44E14
1.67
3785.
2.81E13
0.33
Figure 14.19: Point Source S/N vs. Line Flux for the F28X50OII filter. Top curves are for low sky; bottom curves are for average sky.

 
Figure 14.20: Extended Source S/N vs. V+AB for the F28X50OII for gain =1.Top curves are for an area of 0.2 arcsec2; bottom curves are for 1 arcsec2. Average sky assumed.

 

Table 14.9: Radial Profile for F28X50OII
Radius

Fraction of Energy Encircled
Pixels
Arcsec
Intensity
1
0.050
1.945e-02
0.405
2
0.075
9.266e-03
0.622
2
0.100
3.589e-03
0.750
3
0.150
7.742e-04
0.849
4
0.200
3.628e-04
0.895
5
0.250
1.826e-04
0.924
10
0.500
1.966e-05
0.982
15
0.750
4.876e-06
0.997
20
1.000
5.800e-07
1.000
Figure 14.21: Point Source Encircled Energy for F28X50OII

 
Figure 14.22: Point Source Intensity vs. Radius for F28X50OII

 

F28X50OIII-CCD 50CORON-Clear CCD
Space Telescope Science Institute
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