Testing the Array
The script begins by taking, displaying, and plotting a one-second dark. If Vista's own image and control windows do not already exist, a few moments will be required for their creation. The dark-frame should appear in the image display window as a more or less uniform square composed of four quadrants, resembling Figure 10. Note the positions of the few blemishes.
A black plot window will appear with a row plot which should look something like Figure 11. Values should vary about 100 DN peak to peak. The level should be in the neighborhood of 2,000 DN, representing the bias level. (Remember that if you've enabled baseline subtraction, the level should be much lower--about 100 DN--but the peak to peak variation should be the same.) If your image is markedly different, you may have a light leak or a baseline problem. Make sure that all wheels are in their `Dark' positions. Have a technician check your baseline setting.
The procedure will have paused at this point to allow you to examine the image and plot. To resume, type `continue' (or just `c', as it is often aliased) in the Vista window. A second dark frame will be taken and subtracted from the first. The remainder is then displayed and plotted. The plot should resemble Figure 12, with levels of about 30 DN peak to peak. This number, divided by six and multiplied by 12e- DN-1, will yield the approximate read-noise level in terms of e- pixel-1.
If it's not already running, open a Vista window and
start Lirctop.
From the main menu, select `Tests', from the submenu select
`Stability'. This procedure automates the stability test by taking the
requested
number of exposures, calculating the mean DN within one or more user-defined
boxes, and finally plotting mean DN against exposure number.
The response test is only as accurate as the illumination is constant.
A good, stable thermal source, over periods of time during which the
dome temperature
does not change significantly, is the backside of the TUB diagonal mirror or
the inside of the primary mirror cover.
The appropriate exposure time will
depend strongly on air temperature and other local conditions, varying by as
much as a factor of three or four between summer and winter. The 45-second
exposure shown in Figure 14 was made with the intermediate field of
view, at 39° Farenheit, under a clear, moonless sky. The same exposure
level is
reached in about half the time at 55°. See the
`Times to Saturation' table.
Stability
The constancy of the systems response can be measured by examining flux
levels in repeated exposures, or the stability of the baseline can be
checked by
looking at a series of darks. Such tests measure the stability of the
array and its
associated electronics, including exposure timing.
Sky Test
This check must be performed after dark. From the motor control program,
select the K' filter and the intermediate field of view.
Take an exposure of the
evening sky, long enough to bring the average pixel to about 15,000 DN, and
make a rowplot. It should resemble Figure 14.