WHITE GUIDER USER'S MANUAL
Last update: 04/05/2005 MF
The McDonald White Guider is an offset guider similar to the McDonald
photometry offset guiders. Here are some basic points for its use:
1) Be sure the offsets are near 0,0 on the vernier by the eyepiece for
pointing to an object (if you intend to look through the eyepiece).
2) Focus values for the CCD and WHT guider is ~1500 to 1950 at the 30"
depending on the temperature. Anywhere else, a good rule of thumb is to
focus the telescope to the eyepiece. It is usually in or near focus.
3) If the mirror knob (right side of guider) is in, the light from the
telescope comes out the eyepiece. To move it out, turn the knob
counterclockwise until it stops to take it out of locked position,
pull the knob away from the guider as far as it will go, then lock it
again by turning the knob slightly clockwise. In this position, the light
all goes down through the filters to the CCD. This guider has an unused
second channel option. If you see no light at all in the eyepiece
(other than the reticle), flip the knurled knob at the left of the
eyepiece at its base. This flip mirror allows the light to be sent
down the non-existent second channel as well as the eyepiece.
4) The filter wheel is reached by removing the four knurled screws on the
right side of the guider below the mirror plunger. You'll have to
disconnect the filter motor cable. The filter wheel is attached to the
plate you've just loosened. Gently pull the filter wheel out. It is a
tight fit. The filter wheel that is normally left in the guider has
eight 1x1" holes. The filters normally resident in it are B, V, R, I
and BVR (a thin clear filter useful for finding faint objects). Other
filter wheels are available; some have two 1x1" holes and two 2x2" holes.
Adapters are available for other sizes and shapes. There is an allen
screw holding the filter wheel to its holder. Loosen this to change the
wheel (it is a captive screw). Make sure the wheel is tight before you
put it back into the guider. It is possible for telescope motion to
loosen it. Reconnect the filter motor cable. With the filter motor off,
set the filter wheel to position 1. Be sure the wheel is solidly in the
detent. Turn the filter motor on. ICE assumes that you start in filter
position 1. Be sure to home the filter wheel in ICE any time you restart
ICE or IRAF or if you have hit CTRL-C or if you have had the filter motors
turned off. Check from time to time as you observe that the filter
locations seem to be correct, i.e, ON the filter number and not between
numbers. The motor occasionally gets out of synch. If you notice
non-repeatable flat fields, you may wish to operate without the filter
motor and turn the wheel by hand.
5) To offset guide, first set up on your object, positioning it as desired
on the chip. Then loosen the two black knurled knobs on the front left
of the guider. This will give full motion of the eyepiece around your
object. Move the eyepiece physically around the field, being careful
not to shove the telescope off of your object. When you find a guide star,
lock down the black knurled knobs with the object near the center of
the crosshair. You can then use the brass knurled knobs at upper and
lower left to adjust the fine positioning of your object on the crosshair.
If you run out of travel on the fine motion, turn the knob several
full turns the other way, then move the guider using the coarse
adjustments (not the telescope) back to center your object. Then do the
fine adjustment with the knobs. Once you've centered on your guide star,
doublecheck to make sure the black knurled knobs are tight. This will
prevent any slippage of the guider while the telescope is tracking.
Some Suggestions:
1) If you don't want to have to focus separately with each filter, do your
focus on the thickest filter you'll be using. The focus for the rest
will probably be pretty good. If you focus using a thin one, the
reverse does not always hold true.
2) To help save time, focus the telescope to the CCD, then focus the
eyepiece to your eye. Then, if the focus changes during a long
integration, you can do a rough focus by eye. The focus WILL change
with change in temperature, particularly at the 82" and the 30". When
doing a focus at the 36", try to pick stars close to the the center of
the field. Objects away from the center will show a lot of coma.
3) If you want to make a quick test integration to find and center your
object, use the BVR filter. It is a clear-looking thin filter supplied
with each guider. If the filters you are using are very thick, doing a
test integration with no filter can produce a very out of focus image.
BVR lets most of the light through, but the focus will be better. This
will save you time if you are trying to locate faint objects to be
observed with thick or narrow-band filters.