Well That’s Really Put the Cat Amongst the Pigeons

It’s actually quite hard to know where to start on this one. We’re at the beginning of a new imaging season and I thought I would take a good look at past data in an attempt to see what the best sub-exposures were for the various bits of kit, with and without duo-narrowband filters, from my Bortle 4.5 location. Whilst I’m in the middle of doing this I come across this YouTube video which I am only half-watching at the time https://www.youtube.com/watch?v=eXdv86sH6co 

I was going to immediately reply to the bloke that I thought what he was saying was a pile of rubbish when something in the subconscious said don’t be so quick and check out what he’s saying against your own data, after all you’re looking at it right now for similar reasons. I am so glad I didn’t write him a snotty reply as of course he’s quite right and this has completely upset my plans for this season’s imaging. But at least they’ve been upset for the better.

So what does this guy say that I immediately poo-pooed as rubbish? He’s basically saying that narrowband filters are not magic nebula revealers and that the same, if not better data is present in the UV/IR cut filtered full RGB images. Sounds like nonsense at first, but it is very easily checked with data I already have, in spades.

Looking at the images above, the first one is a full RGB image (UV/IR cut filter) of the Crescent nebula region, 20 subs at 15-minutes per sub, and let’s be honest, the nebulosity is pretty crap. Now take a look at the next image taken with an Optolong dual-band L-Enhance filter 11 subs at 20 minutes per sub. Now that’s much more like it, clear nebulosity looking way better than the nebulosity in the full RGB image – or is it? Take a really close look at the filtered image. Does the nebulosity only appear to be better than the unfiltered image because all the detracting stars have been suppressed? Well that’s dead easy to check. Take the full RGB image and reduce the stars using Russ Croman’s StarXterminator with Noel Carboni’s Photoshop action which gives you a slider to control the amount of star reduction. The result of simple star reduction on the full RGB image is seen in the third image down, Oh-oh. What’s this? The brighter nebulosity actually appears a bit better in the star reduced image than it does in the narrowband filtered image. The narrowband filtered image better shows some of the faint nebulosity, but that’s simply because the star reducing process has taken out that faint nebulosity, and better processing on my part would have retained it. Oh dear, what do we make of this?

Well for me it has completely put the kaibosh on the plans I had for the kit over this season, and I need to think it all out again. Fortunately it changes nothing on my plans for the Hyperstar as it doesn’t use any narrowband filters.

I should point out that the filtered data was 11 subs at 20-minutes and the full RGB data was 20 subs at 15-minutes so that’s not like for like in that we have 220-minutes total imaging time versus 300-minutes, but I know from experience that the difference is not that hugely significant in this case where I am trying to prove there is no real advantage in using the duo-band filters. If pushed I would say that the slightly better bright nebulosity in the star reduced full RGB data might well be down to the longer exposure time, but if I had used similar exposure times for both I expect the narrowband filtered data to be no better than the full RGB data, and that’s the real point to be made here. What a turn up for the books.

Well, the final nail in the coffin, as far as I’m concerned, would be to take a full RGB image, with a long total exposure time, that I was unhappy with due to poor nebulosity, and knock the stars right back and see what happens. That is the purpose of the 4th image above. Here we have 32 subs at 20-minutes per sub on the IC410/405 region in Auriga. That is a huge amount of data totalling nearly 11 hours!!! My standard processing gave me a result I was very dissapointed in given the amount of time I had spent on the thing. But just now I really whacked the image with the star reducing app, and this is the result. I am much more happy with that, and although it could still do with another 18 subs (at least) for a very nice image, it has at least shown me the way forward. 

Thank you Sky Story on YouTube for supplying a most amazing piece of astro-imaging work.

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Arcturus and Napoleon’s Hat Asterism

I am looking at old data from all the rigs to calculate the best sub-exposures to use from my Bortle 4.5 skies. This is a stack of 4-minute subs on Arcturus using the 200mm lenses and 2600MC Pro CMOS cameras.

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Micro-Dragonfly Array Online

Last night was the most productive I’ve ever had in the observatories. Managed to get all 3 of the Canon EF 200mm prime lenses aligned and running. But this was not without having to overcome 5 or 6 major issues. I will only recount the last one. The 3rd lens was not autofocusing using FocusMax. I checked the lens was on auto (not manual) and I checked that the Astrometrics focuser was connected under FocusMax, and FocusMax said it was. Traced it down to the focuser USB cable not being connected to the computer, yet FocusMax said it was. Go figure. That took just over half an hour to sort out, made more difficult by brain shutdown at midnight, but once the USB cable was connected, the MicroDragonfly array was up and running – hooray!!!

I should point out that with 3 Canon lenses on the top plate, and the position of the guide scope in the mount head, there is now zero adjustment between the position of the mount head and the aperture, it needs to be spot on all the time. This would be totally impossible if it were not for Tom How’s superb Dome Rotator system. Thank you Tom!!!

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Picture of the Week

The “Pillars of Creation” – a composite between Hubble and Webb data with stars removed.

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Affinity Photo 2

Up until the present, I have been using Photoshop with various actions/plugins to do all my astro-image processing. This has only been possible due to the generosity of Noel Carboni who has provided me with yearly subscriptions. Unfortunately that has now come to an end as Noel has moved on from Adobe, so I only have one more year’s use of Photoshop. Oh dear, what to do. Last year my son persuaded me to buy the Affinity suite of apps which included Affinity Photo 2, image processing software, and yesterday I took my first look at AP2 to see if it could possibly replace PS as my main image processing software. A huge bonus was that it claimed to be able to incorporate PS plugins which would be a huge bonus,  if true. So I tried for an hour to get Rogelio’s Hasta la Vista Green into AP2 with zero success. It would have helped if I’d have read the label. To get a plugin into AP2 you have to specify the FOLDER that holds the .8bf file, not point directly to the file itself! Once I’d followed instructions HLVG went straight in and ran! Perfect. So gaining confidence (always a bad thing) I tried the same procedure with Noel Carboni’s Astroflat Pro plugin. Again straight in and running with no issues. This is getting too good to be true. But there was a final plugin that I was a bit concerned about, Russ Croman’s StarXterminator plugin. Now although Russ says that this is compatible with AP2 I did have my doubts. So I gave it a go – and – in it went, and it ran perfectly. Well now that’s changed the landscape somewhat. I have got the main plugins up and running in AP2, so now I’d better look and see if I can actually process a stacked image. The running of AP2 is a little different to the procedure in PS, but it is so similar that if you are less of a dinosaur than me I think you would find no issues at all. I had Dave Eagle’s book “Guide to Affinity Photo Astrophotography Image Processing – 2nd Edition” to hand, and its clear description of the procedure to follow for image processing was a great confidence-booster. So I opened an old Sky90 array calibrated image and went at it. Half an hour later I had a processed image that (to me) was indistinguishable from my PS effort. So that made my decision very easy indeed. Over the next year I will slowly wean myself off PS and move over entirely to AP2. A looming problem that I have been panicking over has now been sorted. I can hear you all shouting “Why didn’t you go to Pixinsight?” I am too old, and it looks way too complicated for my dinosaur brain, and the move from PS to AP2 was so painless, I’ll stick with what I’ve got. You will see over the coming months the difference between my PS and AP2 processing of my images.

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The Last and Final Iteration

Is this the final iteration of the MiniWASP/MicroDragonfly imaging arrays? Who knows. But as you can’t see round the back you can’t see that I have yet to swap out the 3 x Trius M26C OSC CCDs for ASI 2600MC Pro CMOS cameras, so I’m not quite done yet. However, you can see from the image that I now have 3 x Canon EF 200mm prime lenses on the top plate, and in the main-frame there are 3 x Sky90s (with 405mm focal reducer-correctors) plus a refractor guide scope. The finder scope has had to be moved onto the side plate as it has now lost its position on the top plate to that central 200mm lens. I suppose even with the swap out of the Sky90 cameras, it’s still not the end of the story. I will soon have to swap out 5 Win10 computers for beefier Win11 Pro computers as the current computers are struggling, especially with the huge data volumes coming down from the CMOS cameras. So it will still be a while yet before things settle down. Maybe that’s our main incentive to keep going.

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North Dome Imaging Array Statrep

In between gales and pouring rain (continuing today and for the next few days) I have managed to fit the third 200mm Canon lens and 2600MC Pro CMOS camera to the top plate, in between the other two 200mm lenses.

The third Sky90 has gone back into its old slot in the main support frame.

I haven’t yet replaced any of the Trius M26C CCDs on the Sky90s with the 2600MCs yet, and I’m waiting to see if the M26C on Sky90(1) is working OK or not as it was swapped out for a spare as it looked like the head amplifier had gone. If the replacement M26C is no good, then Sky90(1) will be the first Sky90 to receive a 2600MC.

The next clear sky will be used to set up the third 200mm lens. This will mean aligning, collimating and taking a 30-minute sub (the maximum for the 2600MC Pro) to check for flexure.

Also, in parallel, I am getting all the necessary software loaded and tested on a DELL Optiflex 3090 which I will use to run the third 200mm lens.

I have also decided, with the Sky90s, that I will not purchase a 52mm duo-narrowband filter for Sky90(3), but instead I will put the Optolong L-Enhance filters in the filter-wheels on Sky90(1) and Sky90(2) and will take straight RGB data at the same time on Sky90(3). This is perhaps not ideal for maximising data, but for overall time expediency it is probably the best for me.

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Picture of the Week

The Gamma Cass/Pacman region captured with the 200mm lens array. This needs a lot more exposure time to bring out more of the Gamma Cass nebulosity.

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Picture of the Week

From Sadr to the crescent nebula. A 200mm lens image incorporating RGB and dual narrowband data.

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Vega From Last Night

Managed to get 14 x 3-minute subs with the 200mm lenses on Vega last night after a LONG and weary battle setting up. Realised that the head amplifier has probably given up in M26(1) camera and that led to all the grief. Just as well I just bought 3 x ASI 2600MC Pro CMOS cameras from First Light Optics (with a good discount for 3-off, thank you very much FLO) as it looks like the M26Cs have had their day.

So the next long upgrade on the array will be to fit the 3 x 2600MC Pro cameras to the 3 x Sky90s, get the lot aligned and collimated, and then to fit the 3rd 200mm lens rig to the top plate to join the other 2 lenses. This is likely to take some time, but I will do it in bits, so that I always have a set of imagers ready to go.

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