CCD Long-Pass Imaging F28X50LP

Description

The F28X50LP mode is useful for deep imaging longward of 5500 Å. For a fixed exposure time it can detect point sources roughly as faint as with WFPC2 with the F606W filter, but with higher spatial resolution. The field of view is 28x50". The ACS/WFC with the F814W filter will be more appropriate for most programs.

Recommended Uses

Recommended for deep high-resolution imaging between 5500 Å and 10,000 Å. Default aperture for target acquisitions.

Special Considerations

Very red sources may show significant wings from detector halo (see Section 7.1.7).

Pivot (Å)	FWHM (Å)	AB mag zeropoint	Speak	B	R80 (arcsec)	Flux in central pixel
7228.5	2721.6	25.191	1.64e+15	3495.7	0.15	14%

Figure 14.7: Throughput for F28x50LP

Table 14.4: Throughputs and Sensitivities for F28X50LP

	Sensitivity	Throughput %
5400.	1.54E14	1.25
5600.	1.24E15	9.69
5800.	1.49E15	11.27
6000.	1.70E15	12.39
6200.	1.70E15	12.04
6400.	1.75E15	11.98
6600.	1.75E15	11.66
6800.	1.65E15	10.64
7000.	1.70E15	10.66
7200.	1.63E15	9.95
7400.	1.61E15	9.55
7600.	1.42E15	8.22
7800.	1.39E15	7.82
8000.	1.27E15	6.97
8400	1.11E15	5.78
8800.	1.01E15	5.03
9200.	9.68E14	4.61
9400.	9.42E14	4.39
9600.	8.75E14	4.00
9800.	7.18E14	3.21
10000.	5.20E14	2.28

Figure 14.8: Point Source S/N vs. V+AB for the F28X50LP filter. Top curves are for low sky; bottom curves are for average sky. Curves are labeled by required exposure time (sec).

Figure 14.9: Extended Source S/N vs. V+AB for the F28X50LP filter for gain=1. Top curves are for a source area of 0.2 arcsec2; bottom curves are for 1 arcsec2. Average sky assumed. Curves are labeled by required exposure time (sec).

Figure 14.10: Point Source Encircled Energy for F28X50LP

Figure 14.11: Point Source Intensity vs. Radius for F28X50LP