You had one of your favorite pictures printed and it just has been delivered! Full of excitement, you unbox the image and contemplate your work in large format. So many details you didn't even notice during the post-processing! Such a breath-taking result. Faint nebulae, dark background, vivid colors, oval stars!
Wait, what? Oval stars? OVAL STARS?
It... it can only be a printing mistake... or maybe it is... it must be one of those...
Congratulation! You have just unlocked the new astrophotography secret: the art of autoguiding.
And just because you paid a special attention to the roundness of the stars, you realized that your guiding is far from perfect. No worry, some astronomers say that guiding is one of the hardest obstacle.
Possible causes are multiple and diverse:
Bad polar alignment (but you nailed it already!)
Cheap mount mechanics (but come on, you invested 2000€ in a new mount!)
A wrong telescope balancing (but you always spend 30 minutes on it! how can it be?)
Unfortunately, less obvious causes can create guiding troubles too:
Wind gust (the seasonal one)
Bad seeing (the unavoidable one)
System flexture (the underrated one)
Cables snag (the classical one)
The camera timeout (the nasty one)
Let's have a look together
Let's first demystify one point: A not-so-good polar alignment shouldn't have a massive influence on the autoguiding quality. However, a bad polar alignment can create strange banana-like pattern. The further the field is from the guide star, the more visible the phenomenon is.
Trick: always try to align your guide scope and your telescope. By doing this, the alignment error shouldn't be detectable, unless your misalignment is huge (several arcmin)
Here, no secret: A good mount combined with a careful maintenance is key for success.
Trick: Turn both axles and ensure there are no "sticky" spots
This point look easy to solve, but it's not. Most of the astronomers balance the telescope in horizontal position only and it's a mistake. In the example below, the telescope is properly balanced in horizontal position, but the center of gravity is below the DEC axis. Consequently, the telescope is unbalanced in vertical position. Even worse, it seems to be balanced at 180°, but in an unstable position.
Sliding and rotating the optical tube is important, but not enough. A perfect balancing can only be done with off-axis counterweights. For the Newton F/4, we use small Gimbal off-axis counterweights usually used for smart phones, combined with 6x 10g weights. It's usually sufficient for most of the telescope positions.
Without off-axis counterweight
With off-axis counterweight
Gusts can make the guiding deviate by more than 20 arcsec. Those are rapid errors, practically impossible to control with software. The best way is still to protect your gear from the wind and avoid any equipment that can make your scope move. For this reason, we decided not to install any automated dust cover on the tube, frequently amplifying the wind effects. The optical tube is kept as simple as possible.
And please, please! Remove this Telrad you haven't used since you started doing exclusively astrophotgraphy! :-)
Under our dark Austrian sky and during a clear night, our standard FWHM is close to 1,5 arcsec. This mean that the star size is approximately 3 arcsec. For this reason, our guiding limit is set at 3 arcsec. Whenever the guiding star deviates by more than this limit, the image is stopped and a new one starts.
Surprisingly, a concrete floor or any other thermal inertia can affect your seeing dramatically, by creating thermal disturbances in the air. Very large concrete blocks look very professional and steady, but in our case, 300kg of concrete were more than enough. However, if you poured 2 tons of concrete, it is recommended to paint it white.
I can't repeat it more: stiffness is the key. One of the usual mistake is to install the finder scope and its camera on the original finder shoe. Frequently, this part is made of plastic and far too weak. Instead, you can use CNC-machined adapters. Believe me, you won't regret the invest.
Some people pay a fortune for CNC-made telescope clamps. Personally, I would rather invest in a carbon tube instead, combined with a very, very rigid dovetail.
Unless you have a costly direct-driven one, most of the mounts are driven by gears or belt.
The reason I prefer the belt is described in the page "The right mount", exactly for its ability to perform a good autoguiding. Still, this type of mount isn't backlash-free and needs to be tensioned regularly, ideally twice a year (hmm. OK, let say every year).
Now, let's combine a loose belt, with an unbalanced telescope previously described, and let see with an example how it performs
In this example, we try to stabilize the orange mass on the green cross. First, the gears turn CCW and the upper side of the belt is tensioned. The driver pulley starts turning in the opposite direction (2), release the tension and starts to tension the lower part of the belt (3). Due to the resulting overshoot, the orange mass misses the green spot and continues its movement
And now you get it: it is not just about the proper balancing, but also how well the entire transmission is tuned.
This phenomenon easy to identify: it usually happens close to the meridian flip or after a dithering, and usually affects one axis only (for our mount: usually the DEC axis).
When I started doing astrophotography, I don't know how many times I have red: "Take care of your cable management".
Until I understood it the hard way. At that time, we used a Skywatcher 80 without any guiding issue. We purchased a 120ED and only when we were close to the horizon, we started to have massive guiding issues, even leading to a fatal guiding error.
We investigated the issue rapidly and it turned out that the guiding pulses were becoming longer and longer, the closer we were from the horizon. We looked at the refractor carefully and understood what was wrong: The cabling was the same, but the overhang was longer and pulled the camera down.
That being said: let's optimize the cable management
Bring the cables as close as possible to the axes of rotation
Don't let cables drag
Use cable clamps
Can I use cable wraps instead?
Rather not, and here is the reason. We used a big cable wrap for 6 or 7 cables between the mount and the telescope, and rapidly experienced guiding issues on the DEC axis. Why? Because the cabling was simply to rigid and disturbed the DEC movement. We still have a few wraps, but as less as possible, and this is why our cable management look... crap!
Here my only piece of advice is: slow and steady!
We usually reuse the same guiding calibration during one or two months, and it seems it's good enough. Ekos calculates normalized RA and DEC calibrating values in ms/arcsec, therefore, no need to start to new calibration for each object.