Orion Nebula (M42) in the SHO Hubble Palette

September 29, 2019 - Reading time: 5 minutes

I have been thinking about how to represent false-color imaging for deep sky objects, and I've been keeping more of that abundant hydrogen green in the mix when doing SHO Hubble Palette images, where we map Sulfur, Hydrogen, and Oxygen bandpasses to Red Green Blue (RGB). Because hydrogen is--by a wide margin--the most abundant element in the universe, and many of these nebulae are HII Regions (vast expanses of interstellar ionized hydrogen), there ought to be more green in SHO images than we normally see. It's become standard to go heavy on a rust red and deep blue, with most of the green removed. All of these color choices are esthetic choices. The images I'm posting come from the data from three separate filters, Ha, OIII, and SII, so in a sense there are no incorrect color levels--within reason. 

You do see a lot of color (LRGB) imaging with a target like M42, and with corresponding heavy reds and browns of bandpasses on the red end of the spectrum--and heading off into infrared. Most of my shots of Orion Nebula from past years has been in RGB with a luminance layer.

In the first set I toned the hydrogen green way down--actually all the colors are lower--until I'm just getting a nice green cast over everything. 

I expanded on this in an Astrobin comment, dropping it here:

I'm going to reprocess data for some recent targets, see how they turn out. I think the reasoning is sound--that we should see more green with SHO, but we'll have to see how the images look. I know many handle this already by going with HSO to map Ha to Red, which makes a lot of sense, closer to where Ha is on the EM spectrum, even if we put sulfur in Green with this pattern. At the end of the day, though, it's still about how beautiful these images of nebulae look, and how each of us measures that beauty. It could also be that dozens of others have gone through this exact cycle with color levels and patterns and ended up back where we are today, simply because the stronger blues and reds are more appealing! I think one of the best things about this hobby/obsession is that it's data driven, and when I get new data and I try new techniques--and I like what I see, I can go back and reprocess data and try these techniques on other targets. There's something very powerful about this.

M42 Orion Nebula with the stars removed. I used the star removal in Annie's Astro Actions in Photoshop, which gets you 90% there, with some cleanup around the remnants of larger stars. Okay, this looks like H.R. Giger's version of the Orion Nebula.

To show you what I mean by "no incorrect color levels", this is the same imaging data, from the same stacked Ha, OIII, and SII frames. I just went in a different direction with which bandpass to stress--oxygen in this case, with stronger blues. It's strange how the "running man" shape in Sh2-279 Running Man Nebula, the brightish cloud above Orion, only appears faintly in narrowband. And in Orion, on the bottom right side, there's the weird chicken leg of hydrogen that now stands out behind the wispy pale clouds that ring the nebula.

And here's the same data set in HSO, with hydrogen-alpha mapped to red in RGB, sulfur green, and oxygen blue. You could argue that this is slightly more natural, as the hydrogen-alpha line is off the red end of the visible spectrum at 656nm, just this side of infrared. Mapping Ha to red makes sense, but mapping sulfur to green doesn't. The sulfur line is also on the red end of the spectrum, which is why normal RGB images of most deep sky objects taken with a DSLR or OSC camera are usually very red. 

Imaging notes: William Optics GT81 at f/4.7 with WO 0.8x Flat6A II, Astronomik Ha, OIII, SII 6nm filters, Moonlite focuser, ZWO ASI120MM OAG, Imaging camera: ZWO ASI1600MM Pro cooled mono on an Orion Atlas EQ-G mount. Stacked in DSS, processed in PS CC 2019. 40 x 120 second exposures for each filter.


Hanging out on the border between Cepheus and Cassiopeia

September 28, 2019 - Reading time: ~1 minute

NGC 7822, Sharpless 171, Ced 214 region, along with the star cluster, Berkeley 59 at the top left. The bright core on the right is a massive star-forming complex that lights up most of the surrounding clouds of interstellar hydrogen and oxygen between Cepheus and Cassiopeia. 

Imaging notes: William Optics GT81 at f/4.7 with WO 0.8x Flat6A II, Astronomik Ha, OIII filters, Moonlite focuser, ZWO ASI120MM OAG, Imaging camera: ZWO ASI1600MM Pro cooled mono on an Orion Atlas EQ-G mount. Stacked in DSS, processed in PS CC 2019. Bi-color Ha and OIII, 13 x 300 second exposures for each filter.


Night sky--get out and see it once in a while

September 28, 2019 - Reading time: 2 minutes

Sure, automating your astro systems is a wonderful thing--computers, programmable controllers, sensors tied to cameras, motorized telescope mounts, and other hardware were made for this. Bringing them all under a single application, or a set of applications and protocols, makes the process of scheduling imaging runs relatively easy--slewing to targets, focusing, plate solving, image capture sequences, auto-guiding--everything machines do very well. It's what they're good at. And yes, there's a lot of preparation, configuration, even tinkering involved in getting these systems to run smoothly through the night--and that goes for all of them. I don't know of an astronomical equipment or observatory control suite that just works out of the box. That doesn't exist yet. 

Back to "Sure, automating your astro systems is a wonderful thing..." because you know there's going to be a "but", or in this case, a "just".

Just don't forget to get out there and look at the sky--if you can. If you're shooting narrowband targets in a red zone, maybe there isn't much to look at above you but the pale glow of street lights. Sorry to hear that, but it's awesome to see you're persevering anyway. I've seen some kick-ass narrowband DSO images on Astrobin shot from the middle of LA. Technology will find a way--or rather, people will reconfigure or refine the technology to find a way. That's what we're good at. 

Anyway, I happen to be out in the backyard at 3 in the morning with my Nikon D750 and 24mm lens on a tripod. You know, like you do. I only took one shot--this one of the constellation Orion from a low angle with some of my equipment in the foreground. I spent the rest of the time just looking up, doing some honest to goodness stargazing. The universe really is awesome. I mean that in the true sense of the word, not the cool California sense, which it also is, of course.  

If you don't have clear skies tonight, I hope you will be blessed with several in a row very soon!


High-gain Test - Gathering Narrowband Data

September 26, 2019 - Reading time: 3 minutes

Autumn is officially here, and this is the season of the Pleiades, Orion, the nebulae in the constellations of Perseus, Monoceros, Auriga, Taurus, and Gemini. Now, M42 isn't in view until 2am, so that had to be the last in the sequence. And, yes, you can tell I was just dorking around with filters with our galactic neighbor, Andromeda M31, in near IR and hydrogen-alpha. I know M31 is a decent Ha target, and you can see some wonderful images in Ha-RGB out there in the world, but I had never tried shooting 2-minute subs of M31 with a 685nm long pass filter.  

I ran the ZWO ASI1600MM-Pro mono CMOS camera at a gain of 200 and offset of 65 in the following shots. And no calibration frames for any of these. Higher gain reduces dynamic range, but you're also reducing read noise and gaining (ha ha) resolution and the ability to shoot shorter exposures--and more of them, and if you take enough subs, this should balance things out.  There are miles of discussion on gain and offset in astro-imaging, but I was recently reading Jon Rista's comments in an astrobin forum thread and that got me to test out higher gain/offset. 

M31 in Near-IR + Ha

I moved over to Cassiopeia and shot 40 x 4-minute subs each of IC 1805 (Heart Nebula) and IC 1848 (Soul Nebula) in Hydrogen-alpha. Here's the stitched together pair:

Still waiting for Orion to get above 30°, I spent some time on NGC 1499 "California Nebula"

And Orion is back in the sky! Sure, you have to get up at 3 in the freakin' morning to see it with your own eyes. Or you can program your astro imaging system to stay up all night and take pictures without you. Here's M42, Orion Nebula, along with M43, De Mairan's Nebula--that's the spherical-looking cloud formation with the big bite taken out of it. And above that, shining brightly, Sh2-279 Running Man Nebula--although the famous running man shape isn't clear in hydrogen alpha. I'm not sure how well it comes out with oxygen III and sulfur II, but I'll come back another night to capture the OIII and SII frames. Notes: 31 x 240 second exposures in Ha + 20x 10 second subs just for the Trapezium (the super bright core of the Orion Nebula--so bright I have to take separate short exposure shots and merge it back in processing). William Optics GT81 APO refractor, ZWO ASI1600MM-Pro mono camera, Astronomik 6nm Ha filter.


Very wide-angle view of the sky

August 31, 2019 - Reading time: ~1 minute

Here's my first night out with the Irix 15mm f/2.4 Blackstone (the heavier, more durable, aluminum and magnesium alloy housing version of this lens).  And I'm impressed with just a few shots, wide-open aperture, and single 15 - 20 second exposures--no tripod, although I rested the Nikon on the deck railing.


iOptron SkyGuider Pro Test 2

August 25, 2019 - Reading time: ~1 minute

Cygnus region of the Milky Way, with NGC 7000 North America nebula at the bottom left, the Sadr Region in the center, and it's crazy how much of the Veil Nebula showed up--that's the ring of wispy, mostly white nebulosity on the right toward the bottom. The reddish/pinkish areas are mostly clouds of hydrogen gas, while the pale cloudy areas are mostly stars--so many stars. Our galaxy contains somewhere between 150 and 250 BILLION stars. 3 x 120 sec exposures, Nikon D750 85mm f/5.6, on an iOptron SkyGuider Pro tracker.

The SkyGuider Pro has iOptron's standard polar scope and reticle, and by "standard" I mean so much easier to use than just about any other polar scope on the market--that I've used anyway. With just a simple alignment, using the SkyGuider's polar scope, I was shooting 2 and 3 minute exposures. This little tracker is amazingly simple and powerful. At some point I will start testing my color wide-field rig with the William Optics ZS61 and ZWO ASI071MC camera, but for now I want to get used to the SkyGuider, and I'm using my good old Nikon D750 full frame DSLR (unmodified). And you can see this setup produced some decent images to stack.


Ultra-portable astro rig

August 24, 2019 - Reading time: ~1 minute

Last month I picked up an iOptron SkyGuider Pro, because, well who doesn't have one of these best-in-class star trackers? I felt left out. It also gave me an excuse to get the Stronghold Tangent Alt-Az base from AstroShop on AliExpress (https://www.aliexpress.com/item/32822479423.html). I've been looking at images of this one for a while, and in reality it doesn't disappoint. It's a nicely machined piece of equipment, very sturdy, with a 10kg/22lb carrying capacity! I'm using this instead of the very compact light-weight version that comes with the SkyGuider Pro. 

Here's my ultra-portable astro setup, with the William Optics ZS61 APO, ZWO ASI071MC cooled color, ZWO ASI120MM-S guide cam, DeepSkyDad AF1 focuser, homemade powerbox (2 x 12v out, 1 x 5v 4 amp out, 1 x dew control out), controlled by a Raspberry Pi 4 4GB running Stellarmate 1.4.2 beta. The SkyGuider Pro has it's own battery for power, and the scope, cameras, focuser only require a single 12v 7-10 amp input. All other cabling and control functions are mounted on the ZS61. I'm using an old Celestron tripod--I tightened the bolts on the legs, and it's definitely sturdy and stable enough for any payload the iOptron can handle.


Color Wide-field test with the new Raspberry Pi 4 4GB and Stellarmate

August 24, 2019 - Reading time: 2 minutes

I'm testing out my color widefield setup with the William Optics ZS61 APO, ZWO ASI071MC cooled color, ZWO ASI120MM-S guide cam, DeepSkyDad AF1 focuser, homemade powerbox (2 x 12v out, 1 x 5v 4 amp out, 1 x dew control out), controlled by a Raspberry Pi 4 4GB running Stellarmate 1.4.2 beta. I ran some test sequences in Ekos and everything appeared to function normally. I am getting an error for the focuser ("...temperature value (!100)"), but the AF1 doesn't support temperature controlled focus adjustment, so not sure if this affects anything. It focuses properly, so I'm choosing to ignore the error for now. And I'm not absolutely sure this is a Raspberry Pi 4 thing, instead of an INDI/Ekos thing on any hardware.  And you may have noticed that I'm testing this out (remotely, using Jump Desktop) from my brand new Apple iMac 5k 27" i9/8core with... yes, I ordered it with 8 GB RAM, but I have 64GB on order, and I'll add that myself. (No sense paying $1000 to have someone at Apple do that for me).

What's funny is Dylan O'Donnell on his Star Stuff channel posted about upgrading his iMac and the giant performance improvement with PixInsight--same iMac I just bought, but I haven't used PixInsight processing software. I'm a Photoshop guy from way back in the 90s and version 4. https://youtu.be/J_EsH54XqjE