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Sunday, February 16, 2020
Panorama mosaic, Cederblad 214, Sharpless 170 and supernova remnant CTB1
his morning I published the photo of supernova remnant CTB1 (Abell 85). Photos are overlapping, so I was able to build a mosaic image out of them. image spans about ten degrees of sky vertically, that's as large as twenty full Moons side by side.! (The CTB1 at lower center has a same angular diameter as our Moon.) Photo is taken with the Tokina AT-x 300mm f2.8 camera lens, Apogee Alta U16 astro camera and Astrodon narrowband filters. Info about my current setup here, https://astroanarchy.blogspot.com/2020/01/the-frankenstein-monster-my-current.html
A two frame mosaic panorama from constellation Cassiopeia
Click for a large image, it's worth it!
mage is in mapped colours, from the emission of ionized elements, R=Sulphur, G=Hydrogen and B=Oxygen.
Upper part of the mosaic image
Click for a large image
Image details here, https://astroanarchy.blogspot.com/2020/02/new-photo-of-cederblad-214-cosmic.html
Lower part of the mosaic image Click for a large image
Image details here, https://astroanarchy.blogspot.com/2020/02/ctb1-supernova-remnant-in-cassiopeia.html
Upper part of the mosaic image
Click for a large image
Image details here, https://astroanarchy.blogspot.com/2020/02/new-photo-of-cederblad-214-cosmic.html
Lower part of the mosaic image Click for a large image
Technical details
Click for a large image
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 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
Total exposure time for both panels
H-alpha, 21 x 1200 s, binned 1x1 = 7 h
O-III, 2x 1200 s, binned 2x2 = 40 min.
S-II, 2 x 1200 s. binned 2x2 = 40 min.
Click for a large image
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 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
Total exposure time for both panels
H-alpha, 21 x 1200 s, binned 1x1 = 7 h
O-III, 2x 1200 s, binned 2x2 = 40 min.
S-II, 2 x 1200 s. binned 2x2 = 40 min.
An older longer focal length image of CTB1 from 2016
Please, click for a large image
Please, click for a large image
More info about this photo here, https://astroanarchy.blogspot.com/2016/01/abell-85-ctb1-dim-galactic-supernova.html
An older longer focal length image of Cederblad 214 from 2016
Please, click for a large image
An older longer focal length image of Cederblad 214 from 2016
Please, click for a large image
A detail shot from the bright central region of the image at the top. This photo was taken with my new setup, Celestron Edge HD 1100 f7, Apogee Alta U16 astro camera and the Astrodon narrowband filters, Spring 2014. The original blog post from 2012, with technical details, can be seen HERE
Labels:
Narrowband color images,
nebula
CTB1, a supernova remnant in Cassiopeia
CTB1 (Abell 85)
Please, click for a large image, it's worth it.
Image is in mapped colours, from the emission of ionized elements, R=Sulphur, G=Hydrogen and B=Oxygen.
A closer look
Please, click for a large image
An older longer focal length image back from 2016
Please, click for a large image
More info about this photo here, https://astroanarchy.blogspot.com/2016/01/abell-85-ctb1-dim-galactic-supernova.html
INFO
Abell 85 is a very faint supernova remnant in constellation Cassiopeia. It's difficult to image with any details due to extremely low surface brightness. Abell 85 has a largish diameter, about half a degree, it has a same apparent diameter as a full Moon. The physical diameter is about 98 light years across. This SNR locates about 9800 light years from the Earth. CTB1 was originally thought to be a planetary nebula and it was included the Abell catalog of planetary nebulae under a name Abell 85. It was confirmed to be a supernova remnant by Willis & Dickel at 1971.
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 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
Total exposure time
H-alpha, 9 x 1200 s, binned 1x1 = 3 h
O-III, 1x 1200 s, binned 2x2 = 20 min.
S-II, 1 x 1200 s. binned 2x2 = 20 min.
INFO
Abell 85 is a very faint supernova remnant in constellation Cassiopeia. It's difficult to image with any details due to extremely low surface brightness. Abell 85 has a largish diameter, about half a degree, it has a same apparent diameter as a full Moon. The physical diameter is about 98 light years across. This SNR locates about 9800 light years from the Earth. CTB1 was originally thought to be a planetary nebula and it was included the Abell catalog of planetary nebulae under a name Abell 85. It was confirmed to be a supernova remnant by Willis & Dickel at 1971.
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 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
Total exposure time
H-alpha, 9 x 1200 s, binned 1x1 = 3 h
O-III, 1x 1200 s, binned 2x2 = 20 min.
S-II, 1 x 1200 s. binned 2x2 = 20 min.
Labels:
Narrowband color images,
nebula
Friday, February 14, 2020
Cosmic heart beats for the Valentine's Day
The Heart nebula
Technical info about the photo, https://astroanarchy.blogspot.com/2020/01/deep-in-to-my-heart-ic-1805-in-mapped.html
Labels:
Narrowband color images,
nebula
Monday, February 10, 2020
Cederblad 214, the Cosmic Question mark, in visual colors
This photo was taken with my "new" imaging system. I managed to mate an old Tokina AT-x 300mm f2.8 camera optics with the Apogee Alta U16 astro camera and filter wheel. Some angle grinder was needed to have enough back focus... More info here, https://astroanarchy.blogspot.com/2020/01/the-frankenstein-monster-my-current.html
This photo of Cosmic Question Mark has a great symbolic value for me. The cosmic curiosity is the very reason I'm doing this difficult, and sometimes frustrating, form of nature photographing.
" ? "
Cederblad 214 and Sharpless 170,
Please, click for a full size image
Visual palette combined from emissions of ionized elements. Red = hydrogen + 33% sulfur, Green = oxygen and Blue = oxygen + 20% hydrogen to compensate missing h-beta emission.
INFO
This cosmic question mark, in constellation Cepheus, contains following objects; At top, Cederblad 214(Ced 214) surrounded by NGC 7822, a dot like nebula at the bottom is known as Sharpless 170,(Sh2-170). Image spans over Five degrees vertically. Distance from my observatory, is ~2750 light years and it spans about 40 light years.
Orientation in the sky
Cederblad 214 can be seen at upper left corner. Image shows its location related to constellation Cepheus.
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 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 1200 s, binned 1x1 = 4 h
O-III, 1x 1200 s, binned 2x2 = 20 min.
S-II, 1 x 1200 s. binned 2x2 = 20 min.
Labels:
Narrowband color images,
nebula
Sunday, February 9, 2020
New photo of Cederblad 214, the Cosmic Question mark
This photo was taken with my "new" imaging system. I managed to mate an old Tokina AT-x 300mm f2.8 camera optics with the Apogee Alta U16 astro camera and filter wheel. Some angle grinder was needed to have enough back focus... More info here, https://astroanarchy.blogspot.com/2020/01/the-frankenstein-monster-my-current.html
This new photo of Cosmic Question Mark has a great symbolic value for me. The cosmic curiosity is the very reason I'm doing this difficult, and sometimes frustrating, form of nature photographing.
Cederblad 214 and Sharpless 170, " ? "
Please, click for a full size image
Image is in mapped colours, from the emission of ionized elements, R=Sulphur, G=Hydrogen and B=Oxygen.
Closeup from the center (An older, long focal length image)
Please, click for a full size image
A detail shot from the bright central region of the image at the top. This photo was taken with my new setup, Celestron Edge HD 1100 f7, Apogee Alta U16 astro camera and the Astrodon narrowband filters, Spring 2014. The original blog post from 2012, with technical details, can be seen HERE
INFO
This cosmic question mark, in constellation Cepheus, contains following objects; At top, Cederblad 214(Ced 214) surrounded by NGC 7822, a dot like nebula at the bottom is known as Sharpless 170,(Sh2-170). Image spans over Five degrees vertically. Distance from my observatory, is ~2750 light years and it spans about 40 light years.
Orientation in the sky
Cederblad 214 can be seen at upper left corner. Image shows its location related to constellation Cepheus.
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 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 1200 s, binned 1x1 = 4 h
O-III, 1x 1200 s, binned 2x2 = 20 min.
S-II, 1 x 1200 s. binned 2x2 = 20 min.
Tuesday, February 4, 2020
Astro Anarchy gets published!
AAPOD2
My photo of IC 1396, the Elephant's Trunk Nebula get selected as an Amateur Astronomy Image of the Day, -AAPOD2
My photo of IC 1396, the Elephant's Trunk Nebula get selected as an Amateur Astronomy Image of the Day, -AAPOD2
Please, click for a large image
Labels:
publications
Tuesday, January 28, 2020
IC 1396 wide field, reprocessed
This was my first light image for my "new" imaging system and first light for the whole winter season 2019 -2020.
Image is now "deeper" and stars are much better resolved. I'm really happy, how well this old second hand Tokina AT-x 300mm f2.8 lens performs. Even the CCD-shell in Apogee Alta U16 camera is very large, over 36x36mm, image from the lens can cover the whole CCD. There are some coma at out most corners of the full frame image but nothing serious.
The imaging system is undersampled, it has a spatial resolution of 6 arc seconds / pixel. This makes the optical system very fast. The same Tokina lens with a small pixel CCD and spatial resolution of 1 arc second / pixel, is 36 times slower to capture light. That's a lot! One hour exposure with my current system is equal to 36 hours exposure with one that has tiny pixels.The lost of resolution is not really an issue, when I want to capture very faint and diffused nebula structures.
Info about my current imaging system can be seen here, https://astroanarchy.blogspot.com/2020/01/the-frankenstein-monster-my-current.html
IC 1396
Please, click for a full size photo it's worth it!
Image is in mapped colours, from the emission of ionized elements, R=Sulphur, G=Hydrogen and B=Oxygen. The signal for ionized oxygen. Note, at lower right corner shows a small part of Sharpless 129, Sh2-129. Some images of Sharpless 129 can be seen here, https://astroanarchy.blogspot.com/2018/11/a-giant-squid-ou4-imaging-project.html
An experimental starless version
Please, click for a full size photo
The planetary nebula candidate at middle left stands out well in this starless photo of IC 1396 area.
Planetary Nebula?
Please, click for a full size photo
Just left from the IC 1396 seems to be a circular formation with some weak O-III emission. Could this be a planetary nebula? My friend, Sabik Rasool, a planetary nebula enthusiast, Find out that this formation is a HII area discovered in 2015. This doesn't rule out, that this could be an ancient planetary nebula?
Please, click for a full size photo
IC 1396 spans hundreds of light years at distance of about 3000 light years in constellation Cepheus. The famous formation of glowing gases, the "Elephant's Trunk Nebula" can be seen at four o'clock position.
This is an active star formation region and it has several massive young stars inside it, coursing the ionization of elements of this emission nebula.
The Garnet Star and the suspected planetary nebula PM 1-333. When I published the first version of this image in Facebook, an other friend of mine, Jussi Kantola, pointed out, that near the Garnet Star lays the PM 1-333. More info about this interesting region can be seen here, https://massimo-cosmicjourney.blogspot.com/2009/09/garnet-star-and-suspected-planetary.html?fbclid=IwAR2dmttg1Q2NmualjjwEPYI1wY8jlUJLClbcHwXkk9xnm7Tvi0YFcaHVwT4
H-alpha, 12 x 600 s, binned 1x1 = 2 h
O-III, 6x 600 s, binned 2x2 = 1 h.
S-II, 3 x 600 s. binned 2x2 = 0,5 h
The Garnet Star and the suspected planetary nebula PM 1-333. When I published the first version of this image in Facebook, an other friend of mine, Jussi Kantola, pointed out, that near the Garnet Star lays the PM 1-333. More info about this interesting region can be seen here, https://massimo-cosmicjourney.blogspot.com/2009/09/garnet-star-and-suspected-planetary.html?fbclid=IwAR2dmttg1Q2NmualjjwEPYI1wY8jlUJLClbcHwXkk9xnm7Tvi0YFcaHVwT4
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 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, 6x 600 s, binned 2x2 = 1 h.
S-II, 3 x 600 s. binned 2x2 = 0,5 h
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