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ampleamp

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ampleamp last won the day on November 16 2014

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  1. Instead of renewing my pc, I’ve kept my 5yr old machine but recently upgraded to the extent the motherboard could take. This has meant two new m.2 drives (one as c drive and one as swop and storage). I’ve maxed out the RAM (very cheaply as it is now deemed old) and I also swopped out the video card for a second hand NVIDIA cuda card (RTX4000). The speed of general processes and scripts like WBPP which use processor and RAM have noticably improved, but the current whizzkids BlurX, StarX and NoiseX are transformed from minutes to seconds with the NVIDIA. I was going down the rabbit hole of chasing PI benchmark numbers, but as the ££££ mounted I decided upgrading a known machine would keep me going a while yet. Benchmarking the renewed machine suggests it is decidedly average according to their lists but I don’t care. One day maybe I will transfer to PI on a Linux computer, maybe even this one 😁
  2. As Fegato says, this all depends on location as well as fl, camera etc, determining pixel scale and field of view. Using 650mm and a scale of 1.44", I took this image the other night using 60 seconds subs and running through RGBRGBRGB.... in 15 minute blocks before moving the scope to push the comet back to where i wanted it on the screen. Its not the best and i hope to improve next time, but remember the comet is moving fast across the screen so give plenty margin around the comet so that when you align stars, and then the comet, there is enough surrounding sky (unlike here).
  3. Adam Block has had a lot to do with the development of WBPP and has a really good set of videos that he has made available on his Youtube channel https://www.youtube.com/c/AdamBlock/videos both mono and OSC, and includes cosmetic correction, normalisation, integration etc. Well worth as look. Coming from an entirely manual approach with individual PI modules, i have now swopped entirely to WBPP, just press 'run' and walk away for an hour (usually around 200 frames of 12Mb)
  4. Thanks Rodd. I admit having to go in close to see what you meant 😃 but I see it now. Something to remember for the future when checking images 👍🏼
  5. Below is my SHO version of the Cygnus Wall in the North American Nebula. This was my setting up image at PixelSkies and was taken between 24-30th July with an APM650/105 and an SX H694 camera. The image comprises 51x600" Ha, 28x600" O111 and 21x600" S11, entirely processed in Pixinsight barring a final tweak in Gigapixel. Obviously the region is commonly imaged though this is my first attempt at this specific area. I made the conscious decision to retain a little of the green and not go too blue purely because i preferred the final result. Thanks for looking.
  6. I have had two goes at this very feint object over the last few months, once from home in limited skies, and once from my remote imaging setup at PixelSkies. I'm sure you can guess which image came from which location. Home - four hours of Ha and O111 data, plus some lum, all form a widefield setup PixelSkies - eighteen hours of Ha and O111, from a medium focal length setup, plus consistently darker skies 😉 The home image was challenging in that despite being at a much higher altitude, my sky was just never good enough for such a dim object and whatever the rights and wrongs of processing, there really is no substitute for dark skies and time. thanks for looking
  7. this is light years ahead of my effort! great result for your dedication
  8. That's quite an effort from sun-kissed Grimsby, and dedication to a long term project! 👍
  9. I would be spending some time in the classified section here, or at https://www.astrobuysell.com/uk/browse.php In my experience the vast vast majority of second hand kit is of very good quality and the vast majority of people who sell would declare any imperfections anyway; i would be more cautious about placing a 'wanted' ad and always try and speak to someone on the phone before parting with any money but this may well be your fastest way to find what you want with some longer nights being more apparent now
  10. With clear nights still forecast, you can still take your subs while you figure out what has gone wrong; then you will have lots of processing during the next lot of clouds 😁 This does look like an over-correction and to me looks like an overcorrection of the flats, at least with the above that’s where I would start, temperature differences??. When I struggled once with calibration I used the trial version of APP; changing software made me rethink what I was doing. What I liked about APP was you just throw everything into the same folder, let it sort everything out while you enjoy the sunshine before you pick up the result. At least you will know if you can get a result with your existing data before you spend ages taking more. If you use the old calibration files first and then compare with a new stack recalibrated with the new calibration files you can start to tie things down with existing files, swoping different old/new groups in and out etc. I often create a raw uncalibrated stack, ie a baseline right out of the camera. Sure there will be vignetting etc but assuming it is better than above, you have removed the camera from the list of possibilities. If things were working, why did you update the calibration files? Unfortunately I dint think there are shortcuts here.
  11. A very big thank you to all involved in StarGazine as the work, hassle and time involved must be significant. This has been a very successful series with many of the talks ranking as excellent, including some topics I never knew I didn't know 😀. For me though, this has been via the YouTube followups as Sunday evenings are no use to me. If there is a desire to keep going and live attendance is the main driver, moving the day or reducing the frequency might work. However I suspect the YT option, being the most convenient, will always be best for most. Maybe then the question becomes, do you want to commit to a wider YT channel and how to stand out? Specific talks have a lot more interest than general 'society' aob, but that's just mho.
  12. Not yet. Voyager really is the complete package, though I have found it takes some learning. The focus routine is so much better but for me the real seller is the fully integrated array system. Mosaics are probably easier in SGP as it is within the programme whereas the only way I have found to work this in V is via their web access tool which drops the mosaic settings into Roboclip (in V) though that may be my lack of practice. You get 45 days full use as a trial, which for you in Spain should be plenty time to find the functionality you need
  13. Hi Peter, if a computer numpty like me can make it work I'm sure you will have no trouble. Like everything, it is the initial setup that makes everything else happen and Voyager is no exception. The array aspect needs both scopes/cameras etc setting up individually in their respective Voyager programmes and then the primary system (the one that controls the mount) has additional settings that directs the array to the secondary system. I have them on different computers but I believe that isn't necessary (though certainly simpler). The primary system is put into array mode and is linked to the secondary. From there, nearly everything you do in the primary system is mimicked in the secondary though the two sequences can be different. In answer to your question, yes, the secondary/slave stops imaging and the primary takes over, pushes the mount to flip, plate solves, and re-initiates the imaging again. I am still baby sitting this manually at the moment but am getting braver about using dragscript which will mean once I ask it to go, everything should work on its own from there; except my roof motor still does not work so I have to be available for manual closure. The attached picture is from the widefield array but you get the idea. So far I am really impressed with this programme, and the backup, and since I am more or less out of astro dark now, I intend to learn what I can over the summer especially developing and using dragscript for all functions.
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