Modification in the CFH12K Focal Plane - May 25, 2000
(New Output Geometry)
To improve noise characteristics of CCD03, the output B (right) is
now being used. The following table provides an update on the
mosaic performance.
Mosaic geometry
---------------
Hi Rho parts = HZ
B---------- B--------- B--------- B--------- B--------- B---------
| | | | | | |
| CCD06 | CCD07 | CCD08 | CCD09 | CCD10 | CCD11 |
| | | | | | |
------------------------------------------------------------------------ East
| | | | | | |
| CCD00 | CCD01 | CCD02 | CCD03 | CCD04 | CCD05 |
| | | | HZ | HZ | HZ |
A--------- A--------- ----------B ---------B A--------- A---------
North
Gain/noise
----------
The CCDs are linear within 1% over the indicated dynamic (less than 65K
for those whose full well is reached before the digital saturation).
The pixel time is 7 microseconds (145 Kpixels per second per channel, to
be multiplied by 12 for the global data flow, say 1.8Mpixels per second).
Gain (e-/ADU): 1.8 1.7 1.4 1.5 1.8 1.5
1.5 1.5 1.6 1.5 1.3 1.7
Noise (e-): 5.0 5.1 3.4 3.9 3.4 5.2
4.2 3.0 5.4 5.1 10.5 3.4
Noise (ADU): 2.8 3.0 2.4 2.6 2.2 3.5
2.8 2.0 3.4 3.4 8.1 2.0
Linearity range (ADU): 52000 53000 65000 54000 51000 65000
62000 65000 51000 65000 60000 65000
Jean-Charles Cuillandre
Canada-France-Hawaii Telescope Corporation, 1999
E-mail: jcc@cfht.hawaii.edu