Updated version of my test image of the Lagoon Nebula (M8) with the first light of the ZWO ASI1600MM Pro camera and broad-band filters.
This image combines:
39 x 120s H-alpha (Baader 3.5nm ultra-narrow filter), in red. Darks and flats included.
40 x 15s OPTOLONG L-Pro filter, in green. No flat or darks.
28 x 300s [O III] 3 nm ultra-narrow Antlia filter, in green. Includes darks and flat (this image is the new addition).
56 x 6s ZWO B filter, in blue, no flat or dark.
H-alpha data taken on 21st Aug 2020, L-Pro and B data taken on 23rd Aug 2020, from my backyard at home, 15 km North from Sydney’s city center.
Telescope: Skywatcher Black Diamond 80, f=600mm (f/7.5)
Equipment: I used the ZWO ASIAir to control the camera, the mount (Skywatcher AZ-EQ6) and the guiding system (ASI120MM + Orion 50mm finderscope). ZWO filter drawer for changing filter.
The [O III] data taken on 18 August 2021, including the Orion 0.75x focal reducer and the ZWO 7×2″ filter wheel.
Processing: Data processed with Siril software. FITS converted on TIFF using NASA’s Fits Liberator considering a logarithmic function. Color / saturation / levels / contrast / smart sharpen with Photoshop.
Article originally written for the AAO’s Newsletter published on 29th June 2021.
During the last year I’ve been setting up my telescope in the backyard to do astrophotography as an amateur astronomer. This has been possible thanks to getting a good mount (Skywatcher AZ-EQ6-Pro) that allows me to do auto-guiding, and using a little but very clever device (it’s a modified Raspberri Pi manufactured by ZWO called “ASIAir”) that allows me to connect mount and cameras (the main camera for astrophotography and the auxiliary camera for auto-guiding) together, being everything controlled using my son’s iPad (who, with only 8 years, has been also helping me with all of this). In the last months I’ve been able to get a process so smooth that I only need 10 minutes for setup (checking polar alignment, guiding, focus) and then the telescope is observing all the night (it will automatically move to a parked position at the end of the run).
I must confess this has been a lot of fun for me, also for keeping extra busy and awake during the many meetings / workshops in the middle of the night we all are having lately. I’m getting some nice photos, particularly of nebulae, as I’m using some ultra-narrow (3.5nm thickness) H-alpha and [O III] filters. One of my favourite images is the Cat’s Paw nebula, who would have told me just some few years ago I will be able to get such an image with all these details using a 80mm refractor telescope in Sydney!
Hence, when last May, I was starting to use TAIPAN and observing with this new instrument, I couldn’t help myself…
While Tayyaba and Anthony helped me to get trained for TAIPAN observing, I decided to check if the instrument could be used for observing HII regions in the outskirts of the nearby spiral galaxy M 83, as well as observing the dwarf galaxies in the neighbourhood. Unfortunately this has been hard for the 1.2m UKST because of the faintness of the targets, but at least I got some test data from the central parts of M83 and some dwarf galaxies, including beautiful starburst NGC 5253.
However, I was thrilled to be using TAIPAN to observe M83 while, at the same time, in my backyard, my small telescope was also observing M 83 to get a new color-image of this galaxy. It was quite exciting and rewarding!
This image is still work in process, because we need to take usually hundreds of frames in each filter to get a good astronomical image to mitigate the light pollution plus reducing the background noise as much as we can. And, of course, dealing later with the processing of the data (it’s not that hard as it sounds, there is actually some software already available for amateur astronomers that does this very quickly in a very efficient way, even considering darks, flats, offsets and median stacking with different options). Also, I still need to add the H-alpha data in this image to emphasise the star-forming regions in the spiral disk of M 83. Unfortunately, the weather over Sydney during the last weeks has not being very good for astrophotography, but I hope to get the rest of the data soon.
Additionally, on Wednesday 26th May we enjoyed a total lunar eclipse. I took almost 2000 images of the event while I was participating in an online live event with many schools in Spain (8000+ views during the day). The telescope setup in this case was different, as I used my CANON 5D Mark III DSLR as main camera attached to my telescope. But, even though the totality of this lunar eclipse was short (only around 15 minutes), I got a very nice image of the eclipsed moon. For this image I combined the same data independently for getting the stars and the moon, and merged them together later.
The Trifid Nebula (M20), with its pink (left) and blue (right) colours, is at the center. The Lagoon Nebula (M 8) is at its left. Very close to M20 is the open cluster M21, almost in the very center of the image. The faint nebula IC 4685 is also seen over M 8. The open cluster M23 is located at the bottom right corner (this cluster has a similar size to the full moon in the sky). The diffuse nebula IC 1283 is located at the top right, in the middle of a dark cloud.
CANON EOS 5D Mark III with a Tamrom 200mm lens, 15 x 5 minutes exposure at f/2.8 and ISO 800.
Piggyback using my old mount, battery powered but very well polar-aligned, no autoguiding.
Full processed with Photoshop.
Siding Spring Observatory, Coonabarabran (NSW, Australia), 19 September 2017.
Deep H-alpha image of the Cat’s Paw Nebula (NGC 6334) in Scorpius obtained from my backyard, 15 km from Sydney’s city centre.
This image combines 40 frames I got during some few nights during late September and early October 2020 using the ZWO ASI1600MM Pro and the H-alpha Baader 3.5nm ultra-narrow filter.
All frames had an exposition time of 900s (15 minutes), hence this image combines a total of 10 hours of telescope time!
Telescope: Skywatcher Black Diamond 80, f=600mm (f/7.5)
Equipment: I used the ZWO ASIAir to control the camera, the mount (Skywatcher AZ-EQ6) and the guiding system (ASI120MM + Orion 50mm finderscope). The H-alpha filter was in the ZWO filter drawer.
Processing: Data processed with Siril software. FITS converted on TIFF using NASA’s Fits Liberator considering a logarithmic function. Color / saturation / levels / contrast / smart sharpen with Photoshop.
For this image I decided to give some false colour instead of just the greyscale image, I used Photoshop to get the kind of “fire” aspect to the gas in the nebulae.
I would love to get some data in broad-band filters to get the colours, but I’m afraid this will have to wait till next year, as Scorpius is already a bit too low over the western horizon, and some palm tress block the view from my backyard.
This image combines 60 x 20s light frames, and 21 x 20s dark frames. Aligned and stacked with SiriL, stretching, colour contrast, saturation, levels, and luminosity with Photoshop.