Thursday, February 24, 2022
4K zoom in the Milky Way
I made a 4K video out of my massive 145 degree Milky Way panorama. In the video you can see the actual resolution of this massive image when it zoom in to IC 1396 in constellation Cepheus
Super Zoom to IC 1396
Best seen as full screen and 4K display, direct link to the YouTube:
https://youtu.be/weeA-jEzezA
Info about the large panorama of Milky Way:
https://youtu.be/weeA-jEzezA
Info about the large panorama of Milky Way:
Wednesday, February 23, 2022
Super Zoom to my photo, the Grand Mosaic of the Milky Way Revision 2
4K Super Zoom to my photo
Grand Mosaic of the Milky Way Revision 2
Super Zoom to the Milky Way, note, best to see in full screen
It took over 12 years to finalize this massive photo of Milky Way
Blog post with a zoomable image, please, have a look here: https://astroanarchy.blogspot.com/2021/10/grand-mosaic-of-milky-way-is-now-large.html
IMAGE SPECS
- Panorama spans 145 x 22 degrees of sky (Full Moon covers 0,5 degrees of sky)
- Resolution 120.000 x 18.000 pixels
- Photos has 2.2 gigapixels in it, the spatial resolution is equal to 8.8 gigapixel image from color camera since all the channels are in native resolution.
- There are least nine confirmed supernova remnants in this panorama
- About 25 million stars are visible in the photo
- Distance to the nebulae in the image between 350 to 20.000 light years
- Exposure time over 1500 hours between 2009 - 2021
- 301 individual images are stitched together seamlessly
- It took about 12 years to finalize this photo
- Narrowband image from light of ionized elements, hydrogen = green, sulfur = red and oxygen = blue
- Processing time for the whole panorama, way too large part of my life
Monday, February 14, 2022
Supernova remnant HB3 and the cosmic heart
I have shot this target originally at January 14 2020 and it was the second light to my modified Tokina lens. Now I have reprocessed the data and I do like this result much better.
new imaging system based on Tokina AT-x 300mm f2.8 camera lens.
The Heart Nebula, IC 1805
Please, click for a large image
Going very deep just in two hours! Image is in visual color palette from emission of an ionized hydrogen and oxygen. R=hydrogen, G=Oxygen and B=oxygen. I have made a starless version out of this image, it can be seen here, https://astroanarchy.blogspot.com/2020/01/an-animated-heart-nebula-ic1805805-with.html
SUPERNOVA REMNANT 132.7+1.3 (HB3)
IC 1805 in visual palette
Please, click for a large image
Supernova remnant
In this photo there is a large supernova remnant, marked as a white circle. I haven't seen any photos of it before. I must take more O-III exposures to see, if I'm able to pick up any signal from this supernova remnant.
Radio image of the area shows mostly signal from OB6
Technical details
Processing workflow
Image acquisition, MaxiDL v5.07.
Stacked and calibrated in CCDStack2.
Deconvolution with a CCDStack2 Positive Constraint, 33 iterations, added at 50% weight
Color combine in PS CS3
Levels and curves in PS CS3.
Imaging optics
Tokina AT-x 300mm f2.8 camera lens
Mount
10-micron 1000
Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and an old spotting scope of Meade LX200
Astrodon filters,
5nm H-alpha 3nm S-II and 3nm O-III
5nm H-alpha 3nm S-II and 3nm O-III
Total exposure time
H-alpha, 12 x 600 s, binned 1x1 = 2 h
O-III, 3x 600 s, binned 1x1 = 30 min..
S-II, 2x1200 s, binned 2x2 = 40 min.
O-III, 3x 600 s, binned 1x1 = 30 min..
S-II, 2x1200 s, binned 2x2 = 40 min.
INFO About undersampling etc
The CCD I'm using has kind of large pixels, 9 microns, so I'm undersampled, the image scale is almost 5 arc seconds / pixel. Undersampling is not a bad thing when my targets are large and dim nebula complexes. This system collects photons very fast!
I selected the Heart Nebula as a target since I have plenty of reference material for it. Another reason is interesting and rarely imaged area after the bright tip of the heart. There are some remnants of a supernova explosion. I was really thrilled, when I saw the final stack of 12 600s H-alpha light frames. (Equal to 2h of exposures) I never have seen so much background nebulae and details from this popular target.
Beside 2h of H-alpha (Light from an ionized hydrogen) I shot 30 min of O-IIII (Light from an ionized Oxygen) To be able to make an image in visual palette.
Wednesday, January 5, 2022
Cygnus Mosaic in Visual Colors
Three Musketeers of Swan
Deepest and most detailed image showing the whole constellation Cygnus ever taken
There are three large supernova remnants visible in this image. The Veil nebula is the most bright of them, other two are really dim and diffused. I spent about 200 exposure hours for those two alone to show them well. I call this trio to the Three musketeers.
I like the new composition, it's very dynamic and shows the whole constellation Cygnus first time ever at this detail level and deepness. I haven't seen anything like this before. Image spans now 31 x 23 degrees of sky and has 118 individual frames in it. total exposure time is now around 700 hours and the resolution 20.000 x 25.500 pixels. Image it took over a decade to finalize this photo between 2010 and 2021.
The mapped color version of this mosaic can be seen here, https://astroanarchy.blogspot.com/2021/12/cygnus-mosaic-gets-large.html
Bang, Bang & Bang
Three large supernova remnants in the same field of view
Click for a large image
Click for a large image
ZOOMABLE VERSION
Three Large Supernova Remnants
Click for a large image
Click for a large image
INFO
Three supernova remnants, two Wolf Rayet stars and a black hole
In the orientation image above, there are three large supernova remnants visible, first the Cygnus Shell W63 , bluish ring at middle left, secondly the large SNR G65.3+5.7 at upper right and the third is a brighter SNR, the Veil nebula at right edge of the image.
Beside three supernova remnants there are two Wolf Rayet stars with outer shell formations. NGC 6888, the Crescent Nebula at center of the image and the WR 134, it can be seen as a blue arch just right from the Crescent Nebula, near the Tulip nebula.
Next to the Tulip Nebula lays a Black hole Cygnus X-1
Constellation Cygnus is an endless source of celestial wonders, both scientifically and aesthetically. For me, as an visual artist, this are of night sky is very inspiring There are endless amount of amazing shapes and structures, I can spend rest of my life just shooting images from this treasury.
Equipments used
Monday, December 20, 2021
Cygnus mosaic gets large
Three Musketeers of Swan
Deepest and most detailed image showing the whole constellation Cygnus ever taken
The new composition is designed so that the Veil Nebula supernova remnant fits within the field of view.
In this image, three large supernova remnants are visible. The Veil Nebula is the brightest among them, while the other two are extremely faint and diffuse. I dedicated approximately 200 hours of exposure time to capturing these two remnants alone to make them more visible. I like to call this trio The Three Musketeers.
I really like the new composition—it’s dynamic and, for the first time, showcases the entire Cygnus constellation at this level of detail and depth. At least, I haven’t seen anything like this before. The image now spans 31 × 23 degrees of the sky and consists of 118 individual frames. The total exposure time is around 700 hours, and the final resolution is 20,000 × 25,500 pixels. It took over a decade to complete this photograph, from 2010 to 2021.
The previous version of this mosaic can be seen here: Great Mosaic of Cygnus.
Bang, bang & bang
Three large supernova remnants in the same field of view
Click for a large image
Three large supernova remnants in the same field of view
Click for a large image
This is a large area of sky, it spans 31 x 23 degrees of sky. Image is in mapped colors, from the emission of ionized elements, R=Sulphur, G=Hydrogen and B=Oxygen.
ZOOMABLE VERSION
ZOOMABLE VERSION
Image is reduced to 6000 x 7700 pixels size from the original 20.000 x 25.500 pixels.
118 Mosaic Panels
Click for a large image
Click for a large image
All the 112 frames used are shown in this image. Since many of the frames are originally shot as independent artworks, panel structure is very complex. Also different instruments has a different field of view and resolution, so mosaic panels are at three different size.
DETAILS
Click for a large image
Three large supernova remnants in constellation Cygnus, the Swan, are in image as colored circles
NOTE, there is an apparent size of the Moon as a scale at lower right corner in a grayscale image.
INFO
Three Supernova Remnants, Two Wolf-Rayet Stars, and a Black Hole
In the orientation image above, three large supernova remnants are visible. The first is the Cygnus Shell (W63), a bluish ring located in the middle left. The second is the large supernova remnant (SNR) G65.3+5.7, seen at the upper right. The third is the brighter SNR, the Veil Nebula, positioned at the right edge of the image.
Besides these three supernova remnants, there are two Wolf-Rayet stars with outer shell formations. The first is NGC 6888, the Crescent Nebula, located at the center of the image. The second is WR 134, which appears as a blue arc just to the right of the Crescent Nebula, near the Tulip Nebula.
Next to the Tulip Nebula lies the black hole Cygnus X-1. It is marked in a small close-up image of the Tulip Nebula, positioned at the center-right of the orientation image above.
The constellation Cygnus is an endless source of celestial wonders, both scientifically and aesthetically. As a visual artist, I find this region of the night sky incredibly inspiring. The intricate shapes and structures are mesmerizing—I could spend the rest of my life capturing images of this cosmic treasury.
Equipment Used
I have used several optical configurations for this mosaic image over the years. Until 2014, I used an old Meade LX200 GPS 12" telescope, a QHY9 astro camera, Canon EF 200mm f/1.8 camera optics, and a Baader narrowband filter set.
Since 2014, I have used a 10Micron 1000 equatorial mount, an Apogee Alta U16 astro camera, a Tokina AT-X 200mm f/2.8 camera lens, and an Astrodon 50mm square narrowband filter set.
Additionally, I have captured many detailed images using longer focal lengths. Before 2014, I used the Meade 12" scope with a reducer, and after 2014, I used a Celestron EDGE 11" with a reducer. My guiding camera has been a Lodestar and later a Lodestar II.
Monday, December 13, 2021
The Pelican Nebula with new data
I originally publish this nebula image at December 2016. After that, I have shot some very high resolution material from the same area of sky and I decided to upgrade my old image with better data. I'm kind of happy with the result, especially the details in dark nebulae are much sharper now and shows the complex structures of unionized gas and dust. Main reason is the long exposure time used, for H-alpha alone, there are 30 hours of exposures. Total exposure time is around 60 hours.
The dark nebula in the upper part of the photo is the gas bridge splitting visually the Pelican Nebula and the North America nebula so that the they look like two separate nebula. In reality they are actually a one large emission area.
Pelican Nebula, constellation Cygnus, the Swan
Click for a large image
The older version of this image can be seen here: https://astroanarchy.blogspot.com/2016/12/pelican-nebula-two-frame-mosaic.html
Zoomable Image
Zoomable Image
Orientation in large context
Subscribe to:
Posts (Atom)
