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This is a variation on the initialization procedure above. It is the most
precise method and essential for objects which are not visible in panoramic mode. It does have a significant overhead associated with it, however. Quicker
methods are described later.
- 1.
- Image the slit using the IRS, e.g.: ap to .35mm; mirror; go
- 2.
- Measure the pixel position of the slit center on display.
- 3.
- Image the field around the slit: ap to open_hole; go
Hopefully you see a star at this point.
- 4.
- Set up guiding either of the
object itself or another object. Turn follow on if it isn't already.
- 5.
- Use offsets to center infrared star on previously measured slit position
(0.32 arcsec/pixel); in effect using guider encoders for precision. The
command recenter <xposition> <yposition> takes the current position
in pixels and makes the required offsets. It is designed to work at an
arbitrary rotation of the rotator.
- 6.
- Now replace slit; disperse light and expose: ap to .35mm;
lambda 2 2.2; go
Next: Centering on bright objects
Up: Object Centering
Previous: Initialization of tip-tilt camera
robert blum x297
1998-04-25