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Main CCD Camera: SBIG Research 1001E

     This is the new research line of large format, dual head triple sensor, self-guiding CCD cameras from SBIG. The Research-1001XE utilizes the megapixel KAF-1001E "Blue-Plus" Enhanced CCD from Kodak. The CCD array is nearly 1” square with 1024 x 1024 pixels at 24 microns square and has the highest quantum efficiency of any KAF enhanced detector.

Figure 1: The camera CCD chips and electronics (SBIG)

 

Figure 2: The physical appearance of the camera (SBIG)

 

     This high QE is not only in the blue but particularly in the red and near infrared. In addition to high QE, the low dark current characteristic of Kodak sensors and large pixel size means that the sensitivity and field of view of this detector compares very well to similar sized backlit sensors in cameras costing more than twice as much. The imaging area of this CCD array (24.5 mm x 24.5 mm) is nearly as large as a 35mm film frame.

 

 

   Figure 3: CCD Chip KAF 1001E (Kodak)

CCD                       :        KAF-1001E
Total Pixels            :        1.0 million
Array                      :        1024 x 1024 pixels
Pixel Size                :        24 microns
Antiblooming          :        No
Class                      :        1,2,3
Peak QE                 :        72%
Image Area            :        24.6 mm x 24.6 mm
Focal Length at 1 arcsecond  per pixel  :        195 inches
FOV at 1 arcsecond per pixel                 :        0.3 x 0.3 degrees

 

 

 

Figure 4: Quantum Efficiency of KAF 1001E (SBIG)
    

     At 2.54m focal length the detector has a field of view greater than 1/2 degree while each 24 micron pixel sees less than 2 arc seconds. This camera is ideal for supernova searches, minor planet searches, and general imaging using 10" F/10 and longer focal length telescopes. The imaging camera includes an electro-mechanical shutter, 16 bit analog to digital (A/D) converter, new design two-stage TE cooling with regulated temperature control and optional water assist, and all of the electronics are integrated into the CCD head. Communication to the PC is through the USB.

     This camera is employed the internal TC-237 tracking CCD for guiding sensor.
Figure 5 : 2" internal filter wheel with RGB filters (SBIG)


     An internal 5 position 2" filter carousel is integrated into the front cover of the camera body.  For color, UBVRI, or narrow band imaging simply add filters to the camera's carousel.   The filter carousel accepts both 50mm diameter flats and 48mm threaded filter cells.  The front cover of the camera is easily removed for changing filters.  Since the CCD is in a separate sealed chamber, removal of the front cover to change filters does not expose the CCD to dust or air and the desiccant does not need to be recharged after replacing the cover.  A shutter mechanism is also located inside the camera body, between the filter wheel and the sealed CCD chamber.

     The standard cooling design utilizes a very efficient two-stage TE cooler for maximum performance with large format detectors.  Each camera is also liquid assist ready so that additional cooling in warm climates may be achieved by circulating water if needed. Preliminary tests indicate that cooling -50 Degrees C below ambient will be achieved with this system.   
    
     This CCD will be the main instrument for Photometry and CCD Imaging.