Tests with the 2nd engineering grade array


Variance plot from pairs of flat field exposures at different illumination levels. Different symbols are used for each quadrant.
This yields: Gain = 2.4e-/ADU, RON = 9 to 13e-, full well 120Ke-, linearity ok.


25 sec dark exposure, with the detector at LN2 temperature.


Pupil image. As can be seen, the wheel zero point of the filter, grism and pupil wheels have been adjusted. The image was made with a pinhole in the aperture wheel. This turns out to be the preferred way to make flat fields, as flat fields looking into a room temperature wall immediately saturates.


Pinhole image with the wide field camera. Focus position Z=0. Image diameter = 68 pixels.


Pinhole image with the high resolution camera. Focus position Z=0. Image diameter = 91 pixels. At Z=6150, diameter has only decreased to 72 pixels. Note the symmetric illumination due to proper placement of the pupil wheel.


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Last updated April 6, 2001 by norup@astro.ku.dk