Astro ImageNP127is

NP127is: Imaging the Skies Over Upstate New York!

We noticed some great Tele Vue-NP127is images on Instagram tagged with our #RPTVO (repost hashtag). They were all taken by Greg Thompson in Tele Vue’s home region of the Hudson Valley, NY. Due to the weather, one has to be persistent to be an astro-imager in these parts. So, we contacted him and that resulted in this guest blog post in two parts. The first part describes his journey into astrophotography and experience imaging with the Tele Vue-NP127is and the second part is a step-by-step guide for image acquisition and processing.

 
Reprocess of The Pillars of Creation by Instagram user Gregory Thompson. All rights reserved. Used by permission. The Eagle Nebula (Messier 16 or NGC-6611) is a diffuse emission nebula and open cluster that is home to the finger-like “Pillars of Creation” star-forming region. Ultraviolet light emitted by the young, giant blue stars in the nebula causes the gasses in the nebula to glow. The “Pillars” are actually cold accumulations of dust and gas that are silhouetted by the background glow.
Exposures at ISO 800 and 1600, 174 x 60″/45″ because of wind and low elevation.
Tele Vue-NP127is APO refractor with Canon EOS 7D Mark II DSLR riding on iOptron CEM60EC mount. Software: BackyardEOS, DeepSkyStacker, StarTools, and Corel Photo-Paint X5.

When I saw the first image of the Orion Nebula on the camera’s LED screen ─ WOW, I was hooked!

As a child, I would always look up at the night sky in hopes of seeing a “shooting star.” I loved the night sky but was never interested in astronomy or cosmology as a young man. I began a photography business in 2011 and had to take early retirement from my day job of 25+ years. My photography led me down many roads, from portraiture and landscapes, birds and wildlife, and many other genres. I had heard of astrophotography but was not interested as I thought it was beyond my reach. Then the television series “How the Universe Works” came to my television in 2016 and could not get enough of it. Soon after, I was browsing a photography forum that I was a member of, and saw some photographs (Deep Sky Objects’s) that a well-known scientist and photometrist had posted using a camera that I already had, and a lens very similar to one of my lenses. That opened my eyes wide and I then began to research everything about astrophotography. Three months later I bought my first camera tracker (Fornax LighTrack II) and accessories to begin my new hobby. That was in the fall of 2016. When I saw the first image of the Orion Nebula on the camera’s LED screen ─ WOW, I was hooked!

Fireworks Galaxy by Instagram user Gregory Thompson. All rights reserved. Used by permission. Shown are the “Fireworks Galaxy” (NGC 6946 and Caldwell 12) at center and open cluster NGC 6939 in upper-left. The arms of this face-on spiral galaxy is home to many supernovae including some of the oldest detected. It owes its name to the ten supernovae observed in the galaxy over the last 100-years.
Exposures at ISO 1600, 120″, 90″, and 60″ in bright Moonlight for a total exposure time of 3h:8m.
 Tele Vue-NP127is APO refractor with Canon EOS 7D Mark II DSLR riding on iOptron CEM60EC mount. Software: BackyardEOS, PHD2, DeepSkyStacker, StarTools, ON1, and Corel Photo-Paint X5.

I averaged only 1 image per month because of bad weather!

With physical limitations, I am confined to my home property in upstate New York in the Mid-Hudson Valley for astrophotography. My viewing is limited as well because of trees and many power and telephone cables along my property and neighboring properties. I have limited views in the south and virtually no views from southwest to northwest. So I am constantly moving the small tracker rig around to capture objects that might come into view. With the new mount, I am limited to just my driveway at the moment. I will put in a stable brick platform soon for the backyard. I also do not have a lot of time to capture because of these obstacles. Most nights only allow for 1 to 3 hours of imaging time. At Bortle 4, the sky here is quite good in that regard, however, the seeing is usually just fair. Living in a river valley, we have to deal with clouds all the time. In the summer, heavy dew, heat, and humidity (sometimes reaching 95-100%) can be off the charts. During my first two years of doing this, I averaged only 1 image per month because of bad weather!

First Light (Markarian’s Chain crop) by Instagram user Gregory Thompson. All rights reserved. Used by permission. Markarian’s Chain is part of the Virgo Supercluster of galaxies of which our own Milky Way is a member. Seven members of the chain are moving together through space.
“The first imaging test with the new Tele Vue-NP127is and iOptron CEM60EC mount was a success. Amazed by the amount of data I did receive with only 1 hour.”
Exposures at ISO 800 and 400, 30 x 120″ lights.
 Tele Vue-NP127is APO refractor with Canon EOS 7D Mark II DSLR riding on iOptron CEM60EC mount. Software: BackyardEOS, DeepSkyStacker, StarTools, and Corel Photo-Paint X5.

I decided on the Tele Vue-NP127is. It just fit into everything that I was looking for. Fast, light, outstanding optics, a focal length I was looking for, and the images I was seeing on Astrobin just had a different look to them that set them apart. I was sold!

Even with these limitations, I decided to get my first scope and heavy-duty mount. Being a heavy researcher with anything, I looked long and hard at many scopes. I needed something with fast optics because of the time restraints around my property. I wanted a refractor for my first scope that was light enough for me to handle. I also wanted superior optics and the ability to use it for visual use too. The popular astrophotography hosting site “Astrobin” is probably the best site to look for images created, with the ability to look them up via specific gear. After looking at many, many images, taken by many, many different telescopes, I decided on the Tele Vue-NP127is. It just fit into everything that I was looking for. Fast, light, outstanding optics, a focal length I was looking for, and the images I was seeing on Astrobin just had a different look to them that set them apart. I was sold!

Western Veil by SmugMug user Gregory Thompson. All rights reserved. Used by permission. The Western Veil (Caldwell 34 or “Witch’s Broom”) has the bright foreground star 52 Cygni (magnitude 4.22) at center. It is part of the greater Veil Nebula supernova remnant that spans the width of 6 full-Moons. Shockwaves from the supernova formed a shell as it scooped together gas as it rushed outward. The filament-like structure we see in the photo is the edge-on view of this shell of gas.
Exposure at ISO 1600 over two nights: 89 x 90″ and 76 x 60″ for a total integration time of 3h:29m:30s.
 Tele Vue-NP127is APO refractor with Canon EOS 7D Mark II DSLR riding on iOptron CEM60EC mount. Software: BackyardEOS, DeepSkyStacker, StarTools, and Corel Photo-Paint X5.

The data was so clean and the beautiful galaxies were so clear.

First light with the scope and new mount (iOptron CEM60-EC ) was March 15th of this year after a month of waiting for clear skies (and a 400 pound Black Bear that began showing up at night to leave!). Using the Tele Vue-NP127is visually is just a dream. Looking through the two eyepieces I have (Tele Vue DeLite 18.2mm and Nagler 3.5mm) produced crisp, clear, and clean images of the Moon and larger planets and the Coathanger star cluster was just brilliant! Being pressed for time, I decided to get to imaging and slewed to M 84 which is part of Markarian’s Chain of galaxies. I could only get about an hour of data before trees became an issue but WOW. The data was so clean and the beautiful galaxies were so clear. The data was just so easy to work with. I was totally impressed and continue to be so today.

Tele Vue-NP127is Imaging System / Visual APO Refractor
Ready to image! by Instagram user Gregory Thompson. All rights reserved. Used by permission. The basic imaging setup consists of the Tele Vue-NP127is APO (Nagler-Petzval) Refractor (Elements/Groups: 4/2) telescope with a Canon EOS 7D Mark II DSLR (APS-C sized 20.2 Megapixel CMOS) camera riding on an iOptron CEM60EC (Center-Balanced Equatorial) Mount. In the background is a laptop running BackyardEOS.
The largest and fastest scope on offer by Tele Vue is the 5-inch, f/5.2, flat-field Tele Vue-NP127is. It is the ultimate incarnation of the Nagler-Petzval design (4-elements in 2-groups) which continues our 40-year heritage of making exemplary multi-purpose refractors. The “Imaging System” scopes come with additional features to make imaging easier and more flexible without any compromise to visual observing. Imaging System features include: large rear group elements to maximize illumination, a 2.4″ focuser to allow those additional light rays to illuminate across 52-mm diagonal chips, a lockable, tilting end-ring to square the camera to the image plane if necessary, and 10:1 FocusMate dual-speed focuser for fine-focus . The focuser accepts the optional motorized FDF-2004 Focusmate Driver for vibration-free, variable-speed, electronic motor control. For automated focusing, it is compatible with Starlight Instruments Focus Boss II system.
 
Sky & Telescope’s review of this versatile photo/visual scope raves that “if you expect better from a 5-inch, f/5 refractor, you probably haven’t been living on this planet.” They also reported, “no focus shift when switching between standard red, green, and blue filters used for conventional tricolor imaging — a tribute to the TV-NP127is’s superb color correction.”
 
The focuser is built to carry 12-lbs / 5.4-kg of payload, so it can handle most any filter-wheel / camera combinations or the heaviest Tele Vue eyepiece with ease. With a 4° maximum visual field of view, using our optional 55mm Plössl or 41mm Panoptic, this scope can act as its own finder. The OTA has a captive, sliding, metal dew shield, and screw-on metal lens cover. It comes in a custom-designed hard-shell carry case with room for all standard accessories.
 
“There’s no such thing as an all-purpose optical system for astrophotography, but if you’re looking for a 5-inch f/5.2 refractor that can cover today’s 37-mm-square CCDs, then you’ll be hard-pressed to do better than the TV-NP127is,” is how Sky & Telescope concluded their review.
 

There are so many wonderful things about this scope that it is hard to say what I like best about it.

There are so many wonderful things about this scope that it is hard to say what I like best about it. But if I had to give just one answer, I would have to say it is the quality of the images it produces. I only wish the weather here would be more cooperative to allow me to get out with it more often. Oh, one more thing. To see this scope mounted up is a sight to behold. It is quite an impressive sight to see. Well, that’s what my friends and family tells me!

Cocoon Nebula (crop) by SmugMug user Gregory Thompson. All rights reserved. Used by permission. (See the next section to learn how this image was made.) The Cocoon (IC 5146 or Caldwell 19 or Sh 2-125) is an emission / reflection nebula with a cluster of new stars. The tell-tail red glow is hydrogen gas ionized by ultraviolet light from new stars in this stellar nursery. The blue color around the edges of the “Cocoon” is light reflecting off dust formed by supernovae explosions. The dark lanes crossing through the nebula are cold gas and dust.
Exposures at ISO 1600, daylight white balance, over two nights. 60″ subframes for a total exposure of 3hr:6m.
 Tele Vue-NP127is APO refractor with Canon EOS 7D Mark II DSLR riding on iOptron CEM60EC mount. Software: BackyardEOS, DeepSkyStacker, StarTools, and Corel Photo-Paint X5.
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Tele Vue-NP127is Image Capture and Processing
Greg explains his image capture and processing steps.
 

I am currently using Canon Cameras, mostly the Canon 7D Mark II. I also have a Canon 5D Mark III. At some point, I am going to invest in a dedicated cooled astro-camera which will require me to get some new capturing software. For now, the Canons do a fine job. They do produce heavy sensor noise in hot weather, and that is really a big reason wanting to get a cooled camera. That “noise” is really tough to remove in post-processing.

Single sub-frame from BackyardEOS. Even at full-size, the nebula is barely visible in this 60″ exposure.
Credit: Gregory Thompson. All rights reserved. Used by permission

I use BackyardEOS for acquisition. It is a really great tool for controlling Canon Cameras and has the ability to control two cameras at the same time which I have done this year. The software just works very well! I save the images to the camera’s CF card. This is much faster (read/write) than saving to the laptop. Remember, time is precious where I am located.

After a night of imaging, the next day is processing time. Images are loaded into a folder on my desktop workhorse, and I use Canon’s own RAW converter/processing/viewing software “Digital Photo Professional” (DPP) to view each RAW frame. Any frames that show any problems like elongated stars, clouds that have wandered in, or the odd tree branch, are deleted. Since obtaining the new mount, those star issues are practically ZERO! But I will admit, I am not the best at processing astro images. It takes years to become “good” at it and I am still learning! The next step is to stack the images.

TIF file produced after all the sub-frames (3hr:6m total exposure) are stacked in Deep Sky Stacker. The nebula is not apparent at this stage in processing.
Credit: Gregory Thompson. All rights reserved. Used by permission

I use Deep Sky Stacker (DSS) to stack the RAW images. It does a nice job of registering, calibrating, aligning, and stacking the images. I almost never use dark, flat, or bias frames as the Canon 7D MII has onboard dark current suppression built into it. I have found that adding dark frames to the stacking process with this camera actually ADDS noise to the stacked images. The Tele Vue-NP127is works so well with the 7D MII, that I do not need to take flats as the scope’s images are well illuminated right up to the edge of the field. There is only a tiny bit of cropping that may have to be done, but that can also be avoided in post-processing with the next step.

Automatic histogram stretch in StarTools. The nebula appears.
Credit: Gregory Thompson. All rights reserved. Used by permission

The next step is to bring in the DSS “tiff” or “fits” file created, and bring that file into StarTools for “stretching” and other dedicated processing. There are so many different types of objects in astrophotography that each one requires a different approach in processing them. I generally do an Auto Develop “stretch” first. This is a histogram stretch. Then a gradient wipe is usually done. Next a manual re-stretch. After these steps, you will have an image that is ready for the finer processing of details of the main object and surrounding stars. Some objects such as Globular Star Clusters require little work while other objects such as Galaxies or Large nebulae may require very long intensive processing. I think the longest processing image to date took me about 18-hours of actual processing time!

The second histogram stretch is done manually. The nebula stands out from the blackness of space.
Credit: Gregory Thompson. All rights reserved. Used by permission

The stretches shown here are in black and white because StarTools starts you off working with “luminance” (brightness) of the linear data. As long as you have not changed that data in stacking software (a big no-no), then the astro-specific software can work with that data to recreate colors that are scientifically or artistically reproduced.

Cocoon Nebula final image.
Credit: SmugMug user Gregory Thompson. All rights reserved. Used by permission.

Any astrophotographer will tell you that whatever software you use, StarTools, PixInsight, Astro Pixel Processor, etc., you should take the image from that software to a final step. That step is using a photo processing package that has “curves and levels” such as Photoshop, Gimp, PS Elements, or the program I have been using for many years Corel. I currently use Corel Photo-Paint X5 for final touches to bring the image to what I think it should look like. These are very fine adjustments because I firmly believe that one should take the image as far as possible in the dedicated astro-program before exporting it to the final post-processing software.

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