First steps
Fifteen years after high school, in the late 1990s, I toyed with the idea of taking my own pictures of space, albeit with limited funds. With what little I knew at the time, I started taking pictures of aurorae with a film camera. Then I took pictures of the Milky Way. Later, I graduated to my backyard setup: a homemade equatorial platform with my film camera duct-taped to the eyepiece of a Dobsonian telescope. It did the trick at the time. I still remember seeing the first image of the bands of color in Jupiter’s atmosphere. Next were the rings of Saturn. I was hooked.
Around that time, I learned about our local astronomy club, the Madison Astronomical Society (MAS). MAS had a dark-sky site — Yanna Research Station (YRS) — and permanent telescopes. There I met the late Richard A. Greiner (“Doc”), and my life changed. Doc was a retired engineering professor from the University of Wisconsin-Madison and already well known in the astronomy community. He saw my passion for learning and began to teach me the mechanics of telescopes, mounts, cameras, and roof controllers. There were many nights when I served as his telescope mechanic out at YRS while he gave me instructions over the phone.
My passion became an obsession under Doc’s guidance. As a beginner, there was so much to learn. In 2003, I took my first trip to New Mexico Skies in Mayhill, New Mexico, where I met Mike and Lynn Rice. I was so excited about having the site’s 6-inch refractor all to myself, and Mike let me put my DSLR on it. While I was on the trip, Lynn showed me my own photograph of the Witch Head Nebula (IC 2118) in the August 2003 issue of Astronomy. I couldn’t believe it.
Science, too?
Amateur astronomers can definitely contribute to science. After all, you never know what will end up in your images.
In 2014, I was approached by David Martinez-Delgado, a Spanish astrophysicist working on the Stellar Tidal Stream Survey at the Max Planck Institute for Astronomy in Heidelberg, Germany. He saw something in my data that he hadn’t seen before and asked if I would share it with him. It was a newly discovered stellar stream in a nearby spiral galaxy, NGC 3628. Now I collaborate with him regularly by receiving specific targets to image so that data can be included in his group’s research papers.
I have really started to enjoy this aspect of imaging. Whenever I image a new stream target, I have a hard time sleeping until I get those first 10 frames back and can take a peek at them.
While I image from DSNM, I am also a part of Sierra Remote Observatories in San Jose, California, and Star Shadows Remote Observatory in Chile. You can never have too much data, and imaging new targets from the Southern Hemisphere has been fascinating.
I’ve embraced the constant change and growth in this field and try to keep current with videos, books, online information, and trial and error. My current programs of choice for processing are CCDStack, Photoshop, and, more recently, PixInsight. For many years, I’ve used CCDStack to do my image calibration. For research purposes, the images are complete at this point, but for me this is just the beginning. Adding my own creative take on the final product is what I love the most, and I can spend tens of hours working on one image to get it just right. My goal is to keep the images as real as possible, while adding my own artistic influence along the way.
M27, or the Dumbbell Nebula, is shown here imaged with a 14.5-inch RCOS telescope on a Paramount ME II Mount and an SBIG STX 16803 camera. The author also recently added data from a 24-inch PlaneWave telescope. This Hα/OIII/S2/LRGB image has exposures of 6, 10, 6, 4, 2.7, 2.7, and 2.7 hours, respectively. Unless noted, all data were calibrated, aligned, and combined in CCDStack, with all other processing done using CC Photoshop and PixInsight.
This obscure part of the Veil Nebula is sometimes called the Leaping Leopard Nebula. Simeis 3-210 is a long, thin filament at the extreme southern end of the Veil Nebula and is virtually unknown. To the author’s knowledge, it has never before been imaged at this resolution, which was achieved with a 24-inch PlaneWave telescope on a PlaneWave Ascension 200HR German Equatorial Mount, using an SBIG STX 16803 camera. This Hα/OIII/LRGB image contains exposures of 10, 11, 3.75, 3.75, 3.75, and 3.75 hours, respectively.
These galaxies, NGC 4438 and NGC 4435, are nicknamed The Eyes. This is an LGRB image with exposures of 8, 4, 4, and 4 hours, respectively.
A seldom-imaged area in Orion, this region features a beautiful full field of wispy blues and dynamic reds. The LGRB image contains exposures of 3.75, 2.5, 2.5, and 2.5 hours, respectively.
NGC 4725 is a spiral galaxy much like our Milky Way. Mark captured this image, which has been inverted for added contrast, using Stellar Winds Observatory’s 24-inch PlaneWave CDK24. He used an SBIG STX 16803 camera with an SBIG AOx adaptive optics unit and an Astrodon filter wheel. This LGRB image has exposures of 5.75, 3.25, 3.25, and 3.5 hours, respectively.
NGC 1275 (also known as Perseus A or Caldwell 24), visible at center, houses an actively feeding central supermassive black hole. This shot of the active galaxy was taken with a PlaneWave 24-inch f/6.7 telescope on a PlaneWave Ascension 200HR German Equatorial Mount, using an SBIG STX 16803 camera. It is an LGRB image with exposures of 8.3, 3.25, 3.25, and 3.25 hours, respectively.
This two-panel mosaic shows the well-known Whirlpool Galaxy (M51a or NGC 5194) and its companion (M51b or NGC 5195) at the top, with the rarely imaged NGC 5198 south of the pair. Mark took this photo using a PlaneWave 17-inch f/6.7 on a PlaneWave Ascension 200HR German Equatorial Mount, with an SBIG STX 16803 camera. The Hα/LRGB image has exposures of 7, 16.7, 5, 5, and 5 hours, respectively, for M51, and LRGB exposures of 7.5, 4, 4, and 4 hours, respectively, for NGC 5198.
This exceptionally deep color view of the Cocoon Nebula (IC 5146) traces tantalizing features within and surrounding the dusty stellar nursery. It was taken with a 20-inch Officina Stellare Pro RC telescope on a Paramount ME II Mount.
Near the Crescent Nebula lies PN G75.5+1.7, also called the Soap Bubble Nebula. Mark captured it with a PlaneWave 24-inch f/6.7 telescope, using an SBIG 16803 camera. This Hα/OIII/LRGB image contains exposures of 10.5, 12, 3.5, 3.5, 3.5, and 3.5 hours, respectively.
As one of the more dynamic and colorful areas in the southern sky, this beautiful star-forming region in the constellation Corona Australis has much to offer. This image was taken using an FLI 16803 camera on a 16-inch RCOS telescope with a PlaneWave Ascension 200HR German Equatorial Mount. It is an LGRB image with exposures of 21, 14.5, 13.5, and 13.5 hours, respectively.
NGC 3718 is an interesting galaxy with a warped structure; NGC 3729 is the smaller spiral galaxy in this image, showing remarkable detail as well. Mark shot the pair over two nights with excellent transparency and seeing, using a 14.5-inch RCOS f/8 telescope and an Apogee Alta U16M camera running at –31 F (–35 C). He spent several weeks processing this deep LGRB image, which contains exposures of 8, 4.3, 3.3, and 4.3 hours, respectively.
IC 10 is a starburst galaxy within the northern constellation Cassiopeia. Mark took this image using a 20-inch Officina Stellare Pro RC telescope and an Apogee Alta U16M camera.
Mark frequently uses the 24-inch telescope at Stellar Winds Observatory in New Mexico to take his stunning images.