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14

QUIRC User Guide

dither subtract on/off This option, when turned on, will subtract the previous image
from the current one and store the result in a file with a “chop" added to the normal
data file name instead of the file number. The name is the same as the chop mode
described above. This is often useful when dithering on a faint source that cannot
be seen without subtracting the sky/array background from the image.

For experienced users: note that if you want to use auto from a script, you can specify
the complete set of parameters, in the order above, as numeric arguments. Be careful not
to skip any, and use 1 for on and 0 for off.

>

clear

h[

num

]i

Clear (reset) array

clear resets the detector

num

times, default 1. If you have CTRL-C’d out of an

integration, you should do a clear to reset the device and qcdcom. If you do not use
clear after CTRL-C, on typing the next

go

qcdcom will assume you want to continue the

previous exposure.

>

comment

h

text

i

Adds a comment to the obs.log file, and to the FITS header of the

image file. This is added only to the next observation header, then it is cleared.

>

et

h

seconds

i

Set exposure time

et sets the exposure time. Any floating point value is accepted; the accuracy of the

exposure timing is somewhat better than 0.01 second, but it is ultimately limited by the
mechanics of the shutter. et uses Unix to compute the exposure time, and an exposure
which is based on Unix timing can be interrupted. Some care is taken to make sure that
the unix timed exposures are correct, but the machine running qcdcom is heavily loaded
it is possible for the shutter to stay open slightly longer. The exposure time recorded in
the header, however, will reflect the true amount of time the shutter was open.

>

filter

h

num command

i

Set filter

This command selects the filter setting. If no filter setting number is given, the list

of installed filters and the current setting is given. To specify a filter setting, its number
is given. If it is different than the current filter setting, the wheels are moved to the new
position. Note that for a filter wheel setting, both wheel positions are specified and the
movements are done simultaneously. See the

fw

command description below if other

filter wheel motions are required. To reinitialize the filter wheels, the command

fi

home

is used. One can use

fi home1

or

fi home2

to reinitialize only one particular

wheel. To use the polarizer (wheel 2 position 8) with one of the filters in wheel 1, one
adds the word “pol" after the number requested, e.g.

fi 1 pol

will select filter setting

1 and the polarizer instead of the OPEN position in wheel 2. Since the polarizer is in the
second wheel, it can only be used with filters that are in wheel #1 (filter settings 1-7).

The command

fi DARK

will move the filter 1/2 filter step backward between filters

to aid in taking a dark frame if necessary. Note that there is now a LOWFLUX filter
setting which should give a reasonable dark frame. The command

fi BACK

inverts the

DARK command and restores the wheel to its previous position. Be very careful to issue
BACK when finished taking dark frames, otherwise the filter wheel position will be lost.
If this happens, more than one DARK or BACK command in a row or not in pairs are
issued, or the filter wheel motion fails for any reason, issue a

filter home

command

to re-calibrate the filter wheel positions. It is well worth the extra time.

Summary of Contents for QUick Infrared Camera

Page 1: ...Observer s Guide for QUIRC K W Hodapp J L Hora M R Metzger University of Hawaii October 30 1997...

Page 2: ......

Page 3: ...ith QUIRC The qcdcom program controls taking exposures and writing data in FITS format to disk operates the moving parts of the instrument such as the shutter filter wheel and pupil mask communicates...

Page 4: ...ation differences for integration times less than 1 second Therefore short exposures should be avoided particularly when exposing dome flats it is far better to dim the lights with the domelight dimme...

Page 5: ...elow assume a PSF of 0 5 arcsec FWHM Table 2 QUIRC Sensitivity UH 2 2m Telescope Filter Point SRC Mag Mag arcsec2 Jy ADU 1 sec J 18 6 17 9 1 052e 6 H 17 8 17 1 8 295e 7 K 16 2 15 5 9 622e 7 H K 18 6 1...

Page 6: ...ted image display capability A separate program should be used to display the data One option is to use the viewfits program vf This is a display program developed by Tony Denault at the IRTF that dis...

Page 7: ...ode is running The command to download the current standard DSP code is the following df quirc Occasionally the download will fail if the camera is in some undetermined state and a reset will need to...

Page 8: ...rash for any reason the parameters it reads in may be old and you may need to set them again Typically only resetting the file number is necessary 3 3 Taking exposures For each object you are observin...

Page 9: ...telescope and guide probe and turns the guider back on On the 88 this communicates with Atlas and MiniOtto over the ethernet to perform the guider movements and on CFHT commands are sent over a seria...

Page 10: ...6 H K dual 1 8 m 2 794 20 6 6 1 7 H2BP23 2 12 m 0 914 2 1 7 1 8 2260BP60 2 260 m 2 794 20 6 8 2 1 1560BP120 1 56 m 9 2 2 1710BP120 1 71 m 10 2 3 1 989BP50 1 989 m 11 2 4 1 506 60 1 506 m 12 2 6 1 107...

Page 11: ...th auto or the shutter will not open Also note that you should always do only one filter DARK followed by exactly one filter BACK always in pairs otherwise the filter wheel will get lost and require a...

Page 12: ...chop image and displayed in vf Therefore the observer can take focus frames acquire and center the object etc without saving all the images as separate data files This avoids filling the disk with use...

Page 13: ...P initialization commands In general you will need to initialize the DSP processor in the Leach electronics after power up or after a DSP reset because its cold reset state is not appropriate for runn...

Page 14: ...rform first data read of double correlation pair store image in memory 4 Turn off output amplifiers 5 Open the shutter and wait for a predetermined exposure time 6 Close the shutter 7 Turn on output a...

Page 15: ...e double correlated read on off Controls whether the device is read out before and after the shutter opening or only after If reading before and after the difference between the two are taken and this...

Page 16: ...o stay open slightly longer The exposure time recorded in the header however will reflect the true amount of time the shutter was open filter hnum commandi Set filter This command selects the filter s...

Page 17: ...fp q940811 go h num i Start exposure Go is the command to take an exposure As described above according to the param eters which are set go may reset the chip open the shutter and close it a predeterm...

Page 18: ...resulting image to a disk file set hparami n Set parameter Certain program parameters can be set or unset with this command To set a param eter for example save one issues the command set save To uns...

Page 19: ...direct access to the DSP computer hall hnloopi Read Hall sensors read the Hall effect sensors nloop times The filter wheel 1 sensor is displayed and depending on the position of the switch either the...

Page 20: ...en data is used as a seed for a random number generator and 65536 words of random data are sent per loop diag l3 hcnt fr cg data i Timing board loopback test Loopback test with timing board in place M...

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