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Shibby

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Posts posted by Shibby

  1. Thanks all - much appreciated! :)

    I realise everything looks a little soft, which is down to my poor processing of the stars (the luminance layer looked fine before final tweaks).

    17 hours ago, carastro said:

    Very nice Shibby from another Atik460EX owner.

    Could do with your skies though (I'm SE London) 

    They're Bortle 5, so don't be too jealous! :)

     

    12 hours ago, bomberbaz said:

    I am having a go at it myself but my gear is far lower spec than yours so if I manage a quarter the detail I will be happy. 

    You should definitely try it, it's a nice target for all sorts of equipment. I managed to dig out this old image I took (11 years ago!) with a Canon 450D and unguided exposures:

    image.jpeg.582a0eb7d086030a65062c38daa8974c.jpeg

     

    • Like 1
  2. First image of the season!

    I really struggled with this one, so I'm not too pleased with the result. I think a new set of flats might help - although they are recent, I may have nudged the camera assembly around when fitting a new auto-focuser.

    Once combining channels, I found I had awkward colour gradients to try and sort out. I'm thinking it might help matters if I were to rotate the filters between each exposure rather than capturing a full set of each in turn? Then they might match up better?

    Anyway, the details:

    • MN190
    • Atik 460ex
    • L: 20x600s
    • RGB: 3x18x300s

    image.thumb.png.3288f799478c5dcbdddb41fa8239b494.png

    • Like 13
  3. 16 hours ago, wimvb said:

    Essentially, focuser tube, outer edge of secondary, and reflection of primary should be centered.

    Let me clarify my question/situation. Sorry for not being clear enough, or (more likely) still not understanding properly.

    So, my scope has its secondary offset towards the primary mirror (as well as away from the focuser). My understanding is that this is a "classical offset" and is common on a Mak-Newt. Therefore, the outer edge of the secondary is NOT centred under the focuser. Please see green circle in my images.

    Is that wrong? I would want to be 100% certain before moving the secondary up/down the OTA. If it's not wrong, and I should leave it where it is, my question is: should the primary reflection (red circle) still be centred under focuser.

  4. Thanks for you comments @wimvb

    I was aware of the dangers of moving the secondary offset, so I have *not* done that! Having read several threads, I still can't quite figure out if my collimation as shown above is even theoretically correct. I'm thinking that, given a secondary is a flat mirror, the offset should not be affect the primary reflection, therefore that primary reflection should indeed be centred under the focuser, same as it is with an ordinary secondary. 

    Anyway, I will try a star test the next chance I get.

  5. On 28/07/2022 at 17:55, Dave scutt said:

    How do you get the blue, green and red circles overlaying 

    Yep, it's in the OCAL software.

    You align the outer circle yourself with respect to the focuser, then the inner circles remain concentric to help you collimate those elements.

    Can anyone answer the question: Should the primary be centred to the focuser OR the secondary??

  6. My MN190 hadn't been collimated for a long time - it's a somewhat daunting task, so I recently bought an OCAL to help out.

    The collimation, as far as I can tell, was actually still pretty good but I did end up making a small tweak. However, I may have made it worse - my star shapes aren't as round as they used to be, however I can't 100% rule out my tracking/guiding as the cause.

    With the help of some screenshots, can someone tell me if I have done this OK?

    In image 1, you can see the initial collimation. You can see that the secondary is not centred under the focuser. My understanding is that is by design on the MN190 and you should not move it up/down the OTA.

    collimation1.PNG.8ad66fe23ac00d89bdefdc28115b5df7.PNG

    In the above, you can see that the reflection of the primary is not quite centred either. This is where I made the (possibly incorrect) decision to tilt the secondary slightly to re-centre it. However, I can't quite get my head around whether it should actually be centred or not based on the fact that the secondary isn't centred??

    collimation2.PNG.81c28c8cb5f38a7c8a4ac06021548d2f.PNG

    Below, you can see the final collimation. [Note: The circles appear to expand a little as I change the focus]

    collimation3.PNG.5e2073dd5cbd9588e5b0b83dc53e2913.PNG

     

  7. 15 hours ago, wimvb said:

    Excellent! Once again, a 190MN delivers.

    Thanks very much! Yeah I've been very happy with the 190MN ever since I got it. It's difficult to imagine ever swapping it for anything else (unless I come across a massive windfall!) I decided to re-collimate it recently, though, using an OCAL and think I've had a negative effect. I'll post a separate thread about that.

    • Like 1
  8. It took me several nights to pull together enough data for this one. I've still had to push the luminance quite hard to reveal the fainter parts, but a fresh set of flats helped a lot. I'm a little disappointed I haven't revealed a bit more structure in the outer arms.

    I went looking for interesting facts about this galaxy. Couldn't really find any so here a couple of mildly notable facts :)

    • It is not part of a group, which is relatively uncommon.
    • It has an unsually high number of globular clusters - 300 or so.
    • Although arguably flying, it's not unidentified. It was discovered by Herschel in 1788, although of course nobody knew what "spiral nebulae" were for sure until Hubble figured it out in the 1920s!

    Image details

    • 190MN
    • Atik 460ex
    • L: 22x600s
    • RGB: 3x17x300s
    • Total: ~8 hours
    • Processing: DSS, Photoshop
    • Scale ~1.4 arcsec/pixel

    Thanks for looking

    1310735091_UFOGalaxy-NGC2683.thumb.png.763a4ef0c36de13d0e051ea0f71678b7.png

    • Like 18
  9. 11 hours ago, almcl said:

    They look like hot pixels.  

    If you are not tracking, the stars progressively move across the frame and when each frame is aligned the hot pixel appears to move.

    You might be able to eliminate them with a Kappa-Sigma clip stacking algorithm, but if you're using DSS you will probably need a good deal more than 20 frames for this to be effective.

    I believe 16 is the "magic" number, so stacking 20 should work OK with a sigma clip stack.

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