![]() |
EFOSC2ESO Faint Object Spectrograph and Camera |
|---|
CCD#40 CosmeticsBad Pixel Map |
High intensity normalised flatfields in each of the UBVRi bands (binned 2x2) were filtered to distinguish 2 groups of pixels
It may be noted that the above procedure exagerrates the extent and hence improves the visibility of each bad pixel cluster. This was needed to make them visible on a compressed plot. The number of bad pixels in any single filter will be less than in the above combined plot. Further, a rather conservative limit has been chosen to define "good pixels" (within 15% of unity gain).
The Point is: CCD#40 has (but is not just) a pretty face! Apart from a sprinkling of bad pixel clusters, most of which are just 1-5 pixels in size, all the others are concentrated either on 3 (and a quarter) columns or are on the margins.
A more detailed view in each individual filter may be had by downloading the following files :
However the above files are between 2 and 3 MB in size. Listed below is a filtered version of the same (to change real numbers into a small set of integers to reduce the size drastically) which are between 10 and 45 KB in size. The intensity code in the images is as follows :| Intensity range on the flatfield | Corresponding value on the Filtered Image |
| < 0.55 |
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
|
| > 1.45 | 15 |
| Send comments to : ls-spectro
Last modified: Tue Jan 15 20:06:39 CLST 2002 |