Reason
The purpose of this document is to provide a simple check on the sensitivity of the four CCDs that comprise the WFC. The check involves taking a flatfield and determining the number of counts that appear in each CCD image.
Procedure
This is an example of the expected output :
ing> wfc_disp r443886
Displaying image of CCD4 in frame 4 ....
z1=12641.33 z2=15143.
# IMAGE MIDPT STDDEV MIN MAX
r443886[4] 14010. 3258. 1369. 65535.
Displaying image of CCD3 in frame 3 ....
z1=11783.5 z2=16474.
# IMAGE MIDPT STDDEV MIN MAX
r443886[3] 15593. 3931. 1276. 65535.
Displaying image of CCD2 in frame 2 ....
z1=9037.232 z2=13360.
# IMAGE MIDPT STDDEV MIN MAX
r443886[2] 12245. 2823. 1263. 65535.
Displaying image of CCD1 in frame 1 ....
z1=10839.54 z2=13612.
# IMAGE MIDPT STDDEV MIN MAX
r443886[1] 12799. 2949. 1269. 43344.
Table 1
| Filter | Telescope Position | Integration Time | Counts |
| Ha | Access Park | 6 seconds | 30 000 |
Rev 0.1 Draft issue: Nov 27th 2006 Don Carlos Abrams
Rev 1.0 Release issue: Nov 28th 2006 Don Carlos Abrams
This file: http://www.ing.iac.es/~eng/ops/int/wfc_sensitivity.html