Sky & Telescope - June 2019 - 67

COLLIM ATION: SE A N WA LK ER / S&T

causes a slight oscillation of the ﬁeld. This
often is represented in the technical speciﬁcations of your mount as, for example,
a PE of +/- 3 arcseconds. Some high-end
mounts reduce this error to near-imperceptible levels below one arcsecond, which
permits long, unguided exposures at moderately long focal lengths. For most of us,
though, long-exposure imaging requires
guiding on a ﬁeld star near your target and
correcting these small periodic errors.
Guiding used to be performed manually using a reticle eyepiece, your own
eye, and copious amounts of both time
and patience. Thankfully, technology eliminated the need for
manual guiding almost three decades ago. Autoguiders are
small, inexpensive CCD or CMOS cameras that you use to
monitor a star and make the corrections necessary during a
long exposure.
You can use an autoguider in either of two conﬁgurations:
through the imaging telescope equipped with an off-axis
guider, or attached to a separate telescope mounted on the
side of your imaging scope. The autoguider checks the position of a single star (the guide star) every few seconds and
sends pointing corrections to the mount as needed to keep
the guide star centered.
Most camera-control software has autoguiding capabilities, including TheSkyX's camera control add-on (bisque.
com), MaxIm DL (diffractionlimited.com), and PHD2 (starklabs.com, reviewed in S&T: Dec. 2017, p. 64). Lots of good
documentation can be found online explaining how to use
autoguiding software and how to troubleshoot any issues.
One common problem encountered when autoguiding
through a guidescope is known as differential ﬂexure. This
generally occurs when the guidescope isn't attached securely
enough to prevent slight differences in movement between
the guidescope and imaging scope. A device called an off-axis
guider, or OAG, can mitigate this problem by eliminating
the guidescope entirely. Placed between the telescope and
main camera, an OAG contains a small pick-off prism that
directs light from the telescope to the guide camera's sensor. When correctly positioned, this prism protrudes only
far enough into the light path to capture star images for
guiding and should not cast a shadow on the main camera's
sensor. The small ﬁeld provided by the prism should contain
an adequately bright guide star. If not, the position of the
telescope can be adjusted slightly to bring a suitable star into
the autoguider's ﬁeld of view.
An OAG takes up some of the physical space between your
camera and any ﬁeld ﬂattener or coma corrector in your optical path, so check that you have adequate room between the
two before using one.
While autoguiding can help immensely, it isn't always
sufﬁcient to produce round stars. I recommend that you consider autoguiding only after optimizing the mechanical and

t SENSOR COLLIMATION Cameras with large
CCD and CMOS detectors are highly sensitive
to having the sensor square to the telescope's
optical axis. Some (such as the Starlight Xpress
camera at left) include a push/pull adjustment
plate at the front of the camera that allows users
to fine-tune the squareness of the detector.

optical aspects of your setup. If you have
an excellent mount, or if you're shooting
at short focal lengths or limiting your
exposures to only how long your mount
can go before PE becomes noticeable, you
may not need to autoguide at all.

Balance
Another consideration for improving tracking is making sure
the weight on your mount is evenly distributed. This minimizes the load that the motors need to bear, reducing wear
and tear on one of the most crucial parts of an imaging rig.
Having the payload and counterweights balanced well can go
a long way toward reducing tracking errors.
To balance equipment on a German equatorial mount,
start by balancing the declination axis ﬁrst. Throughout this
process, be sure to hold the equipment steady to prevent sudden rotation due to extreme imbalance. Orient the mount
so that the counterweight shaft is horizontal, and the scope
with all the gear you intend to use (include any anti-dew
straps, and remember to remove any lens caps) is also pointed
horizontally. Loosen the clutch on the declination axis and
gently nudge the scope up and down. If it moves easily in
q FIELD ROTATION This photo of the Double Cluster (NGC 869 and
NGC 884) suffers from field rotation, where all the stars appear to arc
around a point outside the top-left side of the image frame. The cause
may be either inaccurate polar alignment or differential flexure between
the imaging telescope and guidescope.

sk yandtele scope.com * J U N E 2 019

http://www.bisque.com http://www.diffractionlimited.com http://www.bisque.com http://www.starklabs.com http://www.labs.com http://www.skyandtelescope.com

Sky & Telescope - June 2019

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