I want to give you my qualifications before I make any statements about the process.
I have no formal training in any aspect of astronomy. I have been recording occultations under the guidance of IOTA for about 15 years. I get great satisfaction in being able to contribute to the efforts of "the big guys" in this way. My recording period usually about 2 min before and after the predicted event time.. In that interval I capture about 800 FITS images. I process these files with Tangra. As the images are processed I can see on the monitor screen the target star bouncing around, probably due to atmospheric turbulence, but Tangra's astrometric aperture bounces with it. I assume AstroimageJ does much the same. So not as accurate as a GEM but adequate for asteroidal occultations. So the only problem source I see between a GEM and a DOB is field rotation. I have no idea if AstroimageJ can handle that through image alignment?
So I want to give it a shot. I have two scopes: a 25" DOB and an
8" RC on a Mach 1 GEM. If the DOB won't due perhaps the RC will?
Hi NedS,
The reason I mention in my Guide that DOBs are the least desirable type of instrument for conducting exoplanet observations is for the following reason. Exoplanet transits typically require a total continuous observing time of 4-6 hours, with ideally very minimal image movement during that time. Although computerized DOB GO-TO mounts with tracking have only recently come on the market, I am not aware that their tracking accuracy can satisfy this requirement. If you or other users have experience with such accurate tracking DOB mounts, I'd be most interested in hearing about your experience. I will be attending NEAF this year and will certainly query the DOB vendors there as to their mount's tracking accuracy.
Thanks for the question.
Dennis Conti
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