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Equipment and Techniques |
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Written by Dave Grennan
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An look at some of the equipment and techniques used to take some of the images presented on our website.
Dave Grennan's Astro Imaging Setup.
I have been asked by a few people for some details on the equipment I use for astrophotography. This article is my effort to describe my equipment and answer many of the most frequently asked questions with regard to it. It is, of course, by no means comprehensive but hopefully it will explain a bit about why things are done as they are and more importantly help guide (pardon the pun!) a few people who are new to astrophotography.
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 | My equipment is centered around a Celestron C9.25 XLT SGT telescope. Essentially it is a 9 1/4" Classical Schmidt Cassegrain. It's an f/10 telescope (focal lenght is 2350mm, diameter 235mm). I really love this telescope. I have found the optical quality to be second to none. On nights of good seeing this scope produces textbook star images. Even close to the edge of the field of view of the supplied 25mm plossl eyepiece the coma is not very apparent. I do have one major complaint though. The focus mechanism! Image shift during focussing is very noticable, depending on circumstances this can be enough to even throw an object off the frame of a smaller imaging camera. This, of course, is most problematic when imaging at f/10. Focus shift can occur even during the course of an exposure. At the time of writing I am looking at adding a crayford style focusser which screws onto the back of the scope and then implenting a mirror locking mechanism to reslove these issues. The XLT part of the description refers to Celestrons enhanced coatings nown as Starbright XLT. According to Celestron's information, this enhanced coating increases light transmission by 16% the end result is a 9.25" telescope with the light gathering power of around a 10" scope with normal coatings. Without having a non XLT 9.25" to compare with its hard to say if the claims are well founded. The scope comes with a CG5 Advanced Series mount. When I purchased the scope, I had serious reservations about this mount, particularly after reading a review in Sky and Telescope (Aug 2005). In his article the reviewer indicates that the mount is not capable of being autoguided. I felt that the mount itself would be a stopgap which I would eventually have to sell on when I could afford a better mount like the Losmandy G11 or Celestron CGE mount. Boy was I wrong, the mount has exceeded all of my expectations and proved wholly adequate as a platform for my astro imaging. That being said its important to remember that this is a budget mount and does have limitations. The main issue I have is backlash (slop) in the declination axis. This has been problematic sometimes, however since my setup is not permanent and I set up each session, less than perfect polar alignment means that
| | Celestron C.9.25XLT SGT with 127mm Maksutov Cassegrain mounted piggyback. |
| declination drift is almost always in one direction only. So once the backlash is taken up the autoguider has no issues making declination corrections. The other point of note with the mount is its carrying capability. The spec says the load is 35lbs however my rig is much heavier than that. The mount doesnt have any problems moving the extra weight, including the extra counterweight I need to balance the whole thing. | | Guide Scope and Mounting
The guidescope shown adjacent is a 127mm Maksutov Cassegrain by Skywatcher. It has a focal lenght of 1500mm. In itself this makes for a lovely imaging scope however I have yet to exploit its capabilities in that regard and for the moment it serves an excellent guidescope for the SCT. Its probably a little overkill to use such a decent scope for autoguiding but it makes no sense to buy another scope when I have this one.
On other occassions I mount a Celestron 80ED refractor where the 127mm Mak is shown. The C80ED is a delightful little scope and particularly good value for money. It is a semi-apo (ED doublet) with a focal lenght of 600mm. This makes it ideal for wide angle imaging of nebulae and larger clusters.
|  | | The mounting rings and plate are by losmandy. This piece of kit is fantastic and another investment I'm glad I made. Ok they are not cheap (considering I'm in europe and had to pay shipping and import tax on top of what losmandy charged me). I do not regret a single cent of that outlay. The tube rings clamp rigidly to the mounting plate and by loosening the two thumb nuts on the bottom the guidescope can be attached or removed in < 10 seconds. In order to achieve decent guiding the guidescope must be fixed TOTALLY rigidly to the main scope. Initally I used a camera mounting bracket which proved to be totally inadequate. I could only move the guidescope in one axis (left right) and flexure was a big problem. Since taking delivery of the losmandy gear all of those problems evaporated. I can now move the scope in any direction easily by adjusting the six thumbwheels and flexure is non-existant. To anyone beginning astrophotography, I urge you to consider investing in a decent mounting arrangement for you guidescope. Failure to do so will result in endless frustration and poorly guided shots. Don't think that some flimsy arrangement of nuts and bolts will do, it WILL NOT work.
| | Auto Guiding
This was the single biggest challenge I faced when putting the rig together. Initial tests showed that I could acheive around 2 minutes unguided exposure with the CG5 AS mount. Thats a pretty good result for a budget mount. However this is not consistently repeatable (maybe works 2 in 5 times). It became clear that guiding was going to be necessary. My good friend Jed Glover, gave me a 'Celestron radial guider' which I could use along with my Meade 12.5mm illuminated reticle eyepeice for manual guiding. I was pleased with my initial efforts however it was patently clear to me that manual guiding could still be a hit-and-miss affair and was definitely a right pain in the neck!! I was going to have to autoguide the only question was how.
From some research I arrived at two options.
- Purchase a stand alone autoguider, like the SBIG ST4
- Make uses of freely available software to autoguide using a webcam
Having been given a loan of an SBIG ST4, it was clear that this would work well with my setup. The only drawback was cost. I already had a webcam so I decided to pursue this and see if I could do autoguiding "on the cheap". The results were very satisfying and is worthy of an article in its own right.
|  |  | | Close up, showing my modified webcam at the prime focus of the guidescope | The GP-INT from shoestringastronomy allows a single parallel port to communicate with the modified webcam and also send guiding signals to the mount via the RJ-22 (6pin) cable at right. A USB version is now available but has limited software support at present | The webcam is based on a Toucam II Pro from Philips. Using a procedure developed by Steve Chambers it is possible to modify the circuitry to make the camera capable of infinitely long exposures. This modification allows the camera to see extremely faint guide-stars. So faint, in fact, that I have never failed to find a suitable guidestar in any field of view of the guidescope. So I must modify the webcam to autoguide? Well actually no, you dont. Even a non-modified webcam is capable of autoguiding however you will endure significant frustration trying to find a guidestar bright enough for a non-modified webcam to see it. Even when you do the scintillations caused by atmospheric seeing will give the software flase readings effectively. My webcam is further enhance by replacing the standard CCD chip, a Sony ICX098AQ with its monochrome sibling the Sony ICX098AL Basically the autoguiding setup works as follows. The camera is repeatedly taking exposures of the field of view of the guidescope (typically 1-3 seconds long). The camera send its images to the laptop where they are received by the free autoguiding software ( Guide Dog v1.0.6 by Steve Barkes). The software then compares a stars position in the frame to it's last known position and sends corrections to the mount to counter the drift). Simply in theory but it does take a bit of practice to get right. Interestingly the laptop I use is just an old IBM Thinkpad (233Mhz, 32MB RAM) but it works very well for autoguiding.
My Imaging Camera
My camera is a Canon 300D digital SLR. At the time I purchased it, I was looking for a decent camera for regular photography which would also be useful for astro-imaging. The 300D (BTW now superceded by the 350D) again outperformed my expectations no-end! The camera has a 6 megapixel CMOS sensor (22 x 15mm). My first shots with the camera showed that this was going to be an extremely capable astro imager. Best results are acheived by taking several exposures of the same target and averaging these afterwards in software. This has the effect of bumping up the signal/noise ratio resulting in sharper and less grainy images. After using the camera for a while I came upon probably its major limitation. Due to the UV/IR cut filter built in just above the sensor blocking some important wavelenghts of light, the camera is not as sensitive to astro targets as it might be. To correct this I surgically removed the filter and replaced it with clear glass. Further details can be found here.
Focus
I mentioned earlier some of the woes which image shift causes during astroimaging. However achieving critical focus in the first place can be a daunting task. Focussing by eye through the viewfinder of the camera is just not good enough. You may get lucky but you really dont want to be relying on luck. A repeatable method which can quantify focus numerically and allow you to acheive the best possible focus is required. The solution I chose was a piece of software called DSLR focus. This works by measuring the width and height of a star in a short exposure and allowing you to correct the focus until the star image is as small as possible. I found this method to be highly effective at achieving the very best focus. This software also allows an automated sequence of shots to be taken, thus allowing for a more 'hands off' approach.
Light Pollution, Filters and Local issues
Oh that dreaded subject!! How I long for pristine inky black skies, so many others seem to take for granted. I'm located in suburban, Dublin, Ireland. For those outside Ireland, Dublin is a major city with over 1 million people living there. Though I live about 4 miles from the city center, I'm luckier than some as I live very close to the coast. Light pollution is always evident but not nearly as bad as other cities I have visited. On a decent night the milky way is easily seen overhead. However on a moist night the sky glows bright orange and presents major difficulties.
Most of my astro-imaging is taken through a 1.25" Parks Optical Broadband LPR Filter. I bought this a couple of years back and its proven very useful. Its performance offers a decent ratio of dimming light pollution to dimming astro objects, much better than other general LPRs, I have seen. This works well for imaging nebulae but galaxies present a different problem. LPRs dim light from galaxies appreciably meaning much longer exposures are required to get decent results. This is a problem I have been wrestling with for sometime and have not yet come up with a satisfactory solution. I use a baader 1.25" UV/IR now that the stock UV/IR has been removed from my imaging camera.
Another problem I have is a busy commuter train line running alongside my house. As trains pass the ground shakes noticeably. I have found however that as long as the gear is well secured and everything is locked down, the couple of seconds it takes a train to pass doesnt affect the overall image quality too much. In any case the trains stop running shortly after midnight.
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Latest Images |
 Description: NGC 281 The Pacman Nebula exposures was 112 X 5Mins - 9Hrs 30Mins in H Alpha on the11th &12th of November 2008 through a William Optics FLT-110 Triplet APO refractor Atik 16Hr cdd camera. Guided with a Celestron 80ED And Sac 4.2 CCD camera with PhD guiding software On a CGE mount. Processed in Images Plus V3.5 and Photoshop CS2 |
 Description: IC 1396 The Elephant Trunk Nebula in Cepheus HA (R+HA G,B) 240:240:120:120 image from the 07th October through to 27th October 2008 through a William Optics FLT-110 Triplet APO refractor Atik 16Hr cdd camera. Guided with a Celestron 80ED And Sac 4.2 CCD camera with PhD guiding software On a CGE mount. Processed in Images Plus V3.5 and Photoshop CS2 |
 Description: NGC2024 The HorseHead Nebula B33 HA (R+HA G,B) 240:240:90:120 28th of October through to 1st of November 2008 through a William Optics FLT-110 Triplet APO refractor Atik 16Hr cdd camera. Guided with a Celestron 80ED And Sac 4.2 ccd camera with phd guiding software On a CGE mount. Processed by Carl O'Beirnes & Dave Grennan in ImagesPlus V3.5 and Photoshop CS2 |
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