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  2. Planetary Nebulae are worth the effort of finding as they look very impressive with a big Newtonian. Here's one of my favourites, the Eskimo Nebula (NGC2392), observed in early March with an 8" Newtonian with x1.7 Barlow, x400 gain (50%), 77 x 15s frames.
  3. Thanks Ian. I will try again tonight with the clutches. I found a replacement motor with encoder etc, new, but I don't want to fork £100 if I am missing something with the clutch etc.
  4. So I succumbed to temptation and purchased the Martin Pugh 27 hr LHaRGB dataset from Chile taken with a Planewave CDK 17. I'm not sure whether I should have done this, but for added effect I added in the 8.5 hrs of Starbase RGB data to give 35 hrs total integration. I think I have sated my appetite for this galaxy, at least as far as using third party data goes.
  5. I can connect my CPC 800 XLT to CPWI without any problems, however if I connect my celestron auto focuser the focuser is recommended but the mount no longer communicated with CPWI.
  6. Downloaded and tried Graxpert for the first time today. The noise reduction and everything else works very well for me (standalone Windows version). Why not add sharpening and star reduction as well? You know you want to 😃
  7. What he said ^ 🙂 It matters most how the telescope supplied to you works and that there is sufficient redress if it does not work as expected. Steve
  8. Apologies, I was thinking catadioptric was another term for a spherical mirror If I find a very cheap one locally I know what to look out for now ty
  9. I had intended to have a go at the Owl Nebula this session, however rather embarassingly after half an hour's searching I was unable to find it in the eyepiece.🤣 Instead I tried to improve on my previous attempt at M82. This is 800 x 400ms exposures, at 60% gain. And here's a bonus pic of procyon and its spectacular diffraction spikes:
  10. Catadioptric has refractive glass element in optical train next to mirrors - usually as front aperture corrector - making tube closed. Sometimes this element sits inside focuser or in front of secondary - but then you'd have very short tube (Bird-Jones design) or Ruten Maksutov type (but you have newtonian, so it's not that). If it's a longer tube - greater chance that it's spherical mirror. Fast telescopes and spherical mirrors don't get along. If it's F/8 or slower - then it might be spherical.
  11. Thats fine, however I think over companies offer a minimum value (tolerance), instead of offering an actual value.
  12. Today
  13. The tilt adapter would sit between the camera and diagonal. Typically the camera screws into one side of the tilt adapter and a 1.25” nose piece would screw into the other. The nose piece is then inserted into the diagonal. You have two potential issues. 1) the asi120 is prone to newton rings. Even with a tilt adapter there are comments on other forums where even the maximum tilt in the adapter wasn’t enough to remove them. 2) I haven’t seen a tilt adapter that fits a mini version of the asi cameras. That’s not to say there isn’t one, I just haven’t seen one. Like Elp, I am of the opinion that flats will not calibrate out Newton Rings this is because they appear in the flats too. To capture flats I would point the Lunt towards the centre of the Sun, remain in focus and put an opaque plastic bag over the front of the scope secured by an elastic band. Something like a crumpled sandwich or freezer bag works but it needs to be clear/whiteish. Pull the bag tight. Then adjust your exposure time so that the histogram peaks around the 50% mark and capture your frames, say 100 in SER format. In Autostakkert you can create a master flat and open the SER file. Autostakkert will then stack and produce a master flat in tiff format which you can then load into Autostakkert to calibrate your images. Hope that helps. John
  14. Hi Elp, yes filters in the B600 diagonal.
  15. This is the Gassendi crater and the Mare Humorum. Taken with my TAL 2M, ASI120MC-S ( 1 x 2 minute video using ASICAP ) and processed with PIPP, AutoStakkert and Registax with some tweaking in GIMP. I had hoped to use a 2x Barlow to get a more detailed view but the seeing was very "wobbly" and I didn't think that the image would be as good. I also like the composition of this one with the view of the whole Mare and the transition from bright sunlight at the top right to dark shadow at the bottom left.
  16. Ty for this. I meant more how would I know from looking at it? Big aperture shorter tube length would suggest not spherical/catadioptric? Or the opposite? Or neither me trying to collimate it would be something I'd only try on a non spherical newt? Only for the possibility of imaging with it.
  17. I've used 4 and the best one to avoid the most frustration and have a pleasant PA experience is the WO one bar none. If you're patient they do come up for sale used quite often. Second would be the ioptron one.
  18. Does anyone have an (Excel) example for accurately calculating the equation of time value through a whole year? Less accurate example attacheed. Thanks! Anton (www.astronomy-morsels.ch) Equation of Time V1.0.xlsx
  19. Hi all. Just a quick question. I have a skywatcher AZ-GTi that I have converted for use in EQ mode using the Skywatcher wedge. However it really isn’t great. Any suggestions on a decent replacement without spending a vast amount. Looked at the WO but costs the same as the mount so that’s out. Any advice would be appreciated.
  20. Hi Dave. It's difficult to do a direct comparison between Paramount's and 10 Micron regarding reliability because the service model for Software Bisque provides support only via the user forum, it's virtually impossible to get support for Paramount problems that are away from the public gaze. For 10 Micron mounts the user forum is primarily a talking space for users and a repository for information and software etc. Support for hardware problems is direct via email to Baader, or eventually 10u themselves if Baader can't resolve the problem, so you will not be able to compare reliability as we don't know the failure rate for 10u products. There is also a volume bias. There must be thousands of Paramounts sold and in use around the world while the large price differential that previously existed between Paramounts and 10u means the volume of 10 Micron mounts in use worldwide will be much smaller. 10u has only recently gained a foothold in the US market which has been dominated by Software Bisque and Astro-Physics for premium mounts for many years. Now that Software Bisque products have seen a large price hike over the last year we might expect to see many more 10u mounts sold worldwide. While not going into boring detail I did spend almost half as much again on spares and repairs for my Paramount MX Classic over the ten+ years that I owned it as the mount cost me when I bought it new in 2012. HTH William.
  21. Many people are asking why I didn't post photos of iOptron mounts. I intended to, but iOptron didn't have a stall at NEAIC, and the two times I visited their stall at NEAF, they were busy. Next year, I'll contact them beforehand to arrange a time. Sorry ☺️
  22. Would you say you prefer your apm to the morpheus 12.5?
  23. Most of those videos reveal a lot that was announced at NEAF (SW HD mount details, ioptron new mounts, ZWO new products etc), worth watching. ZWO also announced the 2600MM Duo and a square sensor planetary camera the 676MC.
  24. Probably best that I do not comment on another retailer's sales spiel 😇 Some manufacturers include a Strehl report, but I wish they wouldn't. I don't like the way they are used for marketing. A Zygo is intended for use during the manufacturing process. And, let's face it, you don't have to search far on this or any other large astronomy forum to find telescopes that don't match their included report. FWIW, we have two optical benches and a Shack Hartmann. We use them when appropriate. HTH, Steve
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