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In order to test the CCD, you should first confirm that the system has
been configured to use the correct camera. This is usually done by
the Palomar staff, but it should be checked as follows:
The cameras command controls other CCD options as well,
including the binning pattern. A notable option within the
cameras command is the configuration for dewar #0. This is an
engineering setup with which you may want to experiment, for example,
to extend the overscan region (which is almost non-existent in the
default configurations for CCDs #15 and #16). However the default
configurations will often be sufficient.
Once the camera is configured, check the temperature indicators on the
monitor to verify that the dewar is cold (T ~ -100 K). Then test
the CCD by taking a 0-second test exposure:
After the readout interval, this exposure should appear on the monitor
and resemble a bias image, i.e., random noise with a mean level of a
couple thousand counts. If the image appears suspicious in any way,
notify the Palomar crew to make sure the camera is functioning
properly.
You will probably next want to test the camera with a slightly longer
exposure, i.e., 2-10 seconds. There are a few telescope-specific
issues to consider for this test:
- 60-inch
Make sure you have removed the telescope cover and extinguished the
lights in the dome. Light leaking in through the dome shutter and/or
the calibration lamp emission should be sufficient for tests at this
stage.
- 200-inch
If the dome lights are still on for some reason (e.g., it is
earlier than 4:00 p.m.), the exposure should be kept very short,
and the mirror cover should be left closed. If the dome lights can be
extinguished, do so, and then ask the Palomar crew for help opening
the mirror cover. This procedure is easily done from the control
room, but the crew should be notified, since certain operations are
prohibited when the mirror cover is open (e.g., ascending to prime
focus). If the calibration lamp has been installed, you may want to
turn it on, although light leaking in through the dome shutter will
probably be sufficient.
Then set the filter wheel to an empty slot and try a short (e.g.,
3-second) exposure:
The image should show light illuminating most of the field, possibly
with a vignetting pattern around the edge indicating the extent of the
filter cell. If this is not the case, consult the Troubleshooting
section (3.9.5) below. If the image is saturated, i.e.,
pixel values greater than 216-1 = 32767, you may want to reduce
the exposure time and try again.
Next: Verify Fabry-Perot operation
Up: Verify instrument operation
Previous: Verify filter wheel operation
Patrick Shopbell
4/23/2001