MOSTWEAK (Sep2005) Nordic_Optical_Telescope MOSTWEAK (Sep2005)
NAME
mostweak -- find telescope tweak parameters from two images taken
with a mask and of the object field.
USAGE
mostweak maskimage objectimage maskdefinitionfile holesize
PARAMETERS
maskimage
Name of the image taken WITH a mask of a calibration lamp.
objectimage
Name of the image taken WITHOUT a mask of the target field.
maskdefinitionfile
Name of the MOS mask definition file (.ap file).
holesize
The diameter of the fiducial holes in arcsec. In this task,
this parameter affects the centroid algorithm.
DESCRIPTION
This task determines the centroid positions of the fiducial stars
and the fiducial holes on an image of the mask and an image of the
target object field. To measure the pixel coordinates on the image
the interactive task imexamine is used.
The differences in the measured positions of the stars and the holes
are then transformed into telescope tweak parameters: offsets and
rotation. Ask somebody who knows about it (maybe yourself) to apply
this tweak, which should bring the fiducial stars closer to the
centre of the fiducial holes of the mask.
EXAMPLES
Take an image of the target astronomical field at the required
telescope position and rotator angle, and an image of a calibration
lamp (i.e. halogen) with the mask, and do
mostweak /data/alfosc/jc240012.fits /data/alfosc/jc240011.fits MOS0006.ap
Ask yourself to apply the recommended tweak (first the offset, then
the rotation). This tweak should bring your fiducial stars closer
to the centre of the mask holes.
Iterate the tweak by using the task finetweak until the stars are
properly positioned in the holes.
THE INTERACTIVE PART OF THE TASK
This task will first display the mask image which contains the
fiducial-star slits/holes; the slits are marked by a circle. The
user is advised to adjust the colour scale of the image display
tool such that the fiducial stars AND the fiducial holes are
clearly visible. Then the object field image will be displayed
with the fiducial stars marked as described above.
The user has to point the cursor at the fiducial stars (slits)
marked by a YELLOW circle, and has to press key -a- to activate the
centroid algorithm. If key -a- is pressed more than once, the
final press will be evaluated. Each press will be acknowledged by
statistics appearing on the terminal that runs IRAF. To advance to
the next star (slit), press -q-.
On the image display the centroid positions of the slits and stars
will be marked by a RED circle.
When all fiducial slits and fiducial stars have been marked by the
user, the tweak will be computed. Check the distances between slits
and stars as output in the IRAF window. Check that the suggested XY
and rotational offsets make sense, before applying the tweak with
mosmove.
If one of the centroid positions of the stars or holes seems wrong
(judging from the RED circles and/or the computed distances), the
task can be run again with the user discarding the star in the way
described above.
A good tweak fit needs no less than 3 stars. Nevertheless, a tweak
can be computed on only 2 stars.
TIME REQUIREMENTS
A lot less than doing it by hand.
BUGS
email Jacob W. Clasen (jclasen@not.iac.es),
for bug reports and constructive remarks
SEE ALSO
mosmove, mosstrong
|