Re: Mach2 Unguided testing continues


Roland Christen
 


So, when using the keypad quick method, what happens after a meridian flip?
You would need a model for the path that the object takes, one on either side of the meridian.

For some objects you may be able to start the scope under the mount and image all night long without ever flipping. It depends on the amount of clearance you have at the back of the scope before it hits the pier or tripod legs. With my short scope (130EDF) i can start under the mount for any object that's just south of the zenith. With the long 160 refractor it clears the tripod legs about 18 degrees south of the zenith.

Starting under the mount I can image the same object from dusk to dawn without flipping. I would then do a model of 8 points every 1.5 hours or so along the path.

Otherwise, if you flip, you will do a separate model on each side. Of course, doing the entire sky manually would take a lot of time. So if that's the goal, I would just let APCC Pro do it automatically.

Rolando


-----Original Message-----
From: Dean Jacobsen <deanjacobsen@...>
To: main@ap-gto.groups.io
Sent: Thu, May 28, 2020 12:12 pm
Subject: Re: [ap-gto] Mach2 Unguided testing continues

On Thu, May 28, 2020 at 09:35 AM, uncarollo2 <chris1011@...> wrote:
Right now we have not integrated plate solving, but this may be added in the future to make the cycle faster. Remember, this is just a quick way to achieve unguided imaging for an object that you wish to image all night long. Doesn't require super perfect polar alignment, although you want to be close to prevent field rotation.
Assume that the mount will be taken down and then set up for each use.

So, when using the keypad quick method, what happens after a meridian flip?

Will I need to re-do it again? ... or would doing the automated APCC full sky model be the best approach?
 
--
Dean Jacobsen
http://astrophoto.net/wp/ 
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