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Wednesday, December 13, 2017

Sharpless 119 in Cygnus, visual spectrum version


Since beginning of September we have had three clear nights. This Autumn season has been the worst in twenty years.

I made a visual color version out of my two frame mosaics of Sharpless 119 (Sh2-119). You can find a mapped color version from HERE. My aim is to make a six panel mosaic of the whole area of the Sharpless 119. At the moment it's not possible due to weather up here.


Sharpless 119 as a two frame mosaic
Please, click for a full size photo

Image is in Natural color palette from the emission of ionized elements, R=Hydrogen + Sulphur, G=Oxygen and B=Oxygen + 10% Hydrogen to compensate the missing H-beta emission. A mapped color version can be seen HERE.


An experimental starless version
Please, click for a full size photo

In this starless version the shapes in gas and dust are much easier to see.


INFO

Sh2-119, Sharpless 119, is a large complex of emission nebulosity in Cygnus constellation, about 2 degrees east of the North American Nebula. It is located just around 68 Cygni, a quite bright star of magnitude 5. (The most bright star in the photo)



A wider field image of the area, Canon 200mm f1.8 lens
Please, click for a full size image

Sharpless 119 can be seen at lower left corner. The white rectangle shows the location of the new photo. It spans about a square degree of sky. (The full Moon spans about 0,5 degrees of sky.)
This photo was taken with the Canon EF 200mm f1.8 lens and the QHY9 astrocam, Baader narrowband filter set at 2012.



An other wide field shot, Tokina AT 300mm f2.8 lens
Please, click for a full size image

Area of the two frame mossaic is marked as a white rectangle. More info about this photo HERE


Technical details

Processing work flow

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
Celestron Edge HD 1100 @ f10 with 0,7 focal reducer for Edge HD 1100 telescope

Mount
10-micron 1000

Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and SXV-AOL

Astrodon filter, 5nm H-alpha

Exposure times

H-alpha, 30x 1200s, binned 2x2 = 10h
O-III and S-II channels are borrowed form my older wide field photos.


Wednesday, November 22, 2017

Sharpless 119 in Cygnus, project continues



I have published first photo out of Sharpless 119 at 8.11. 2017, since then we have had a full cloud cover. Yesterdat we had about three hours of clear skies and I was able to shoot an other frame next to first one. My target is to make a six panel mosaic image out of the whole Sharpless 119.


Sharpless 119 as a two frame mosaic
Please, click for a full size photo

Image is in mapped colours, from the emission of ionized elements, R=Sulphur, G=Hydrogen and B=Oxygen. The photo covers about two square degrees of sky. (The full Moon spans about 0,5 degrees of sky.)


An experimental starless version
Please, click for a full size photo


In this starless version the shapes in gas and dust are much easier to see.


INFO

Sh2-119, Sharpless 119, is a large complex of emission nebulosity in Cygnus constellation, about 2 degrees east of the North American Nebula. It is located just around 68 Cygni, a quite bright star of magnitude 5. (The most bright star in the photo)



A wider field image of the area, Canon 200mm f1.8 lens
Please, click for a full size image

Sharpless 119 can be seen at lower left corner. The white rectangle shows the location of the new photo. It spans about a square degree of sky. (The full Moon spans about 0,5 degrees of sky.)
This photo was taken with the Canon EF 200mm f1.8 lens and the QHY9 astrocam, Baader narrowband filter set at 2012.


An other wide field shot, Tokina AT 300mm f2.8 lens

More info about this photo HERE



Technical details

Processing work flow

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
Celestron Edge HD 1100 @ f10 with 0,7 focal reducer for Edge HD 1100 telescope

Mount
10-micron 1000

Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and SXV-AOL

Astrodon filter, 5nm H-alpha

Exposure times

H-alpha, 30x 1200s, binned 2x2 = 10h
O-III and S-II channels are borrowed form my older wide field photos.











Tuesday, November 14, 2017

An other detail from the Southern Cygnus


This has been the most cloudy Autumn season in twenty years.
I'm still processing material from couple of clear nights we had this Autumn. I made another individual image out of the material, I shot for the WR 134 mosaic image.


An other nameless detail from the Southern Cygnus
Please, click for a full size photo

Image is in mapped colours, from the emission of ionized elements, R=Sulphur, G=Hydrogen and B=Oxygen.


Image in visual spectrum
Please, click for a full size photo

Image is in Natural color palette from the emission of ionized elements, R=Hydrogen + Sulphur, G=Oxygen and B=Oxygen + 10% Hydrogen to compensate the missing H-beta emission.


The mosaic image
Please, click for a full size photo


The area of interest can be seen at bottom left.


The location in Cygnus
Please, click for a full size photo


The area of the mosaic image above is marked as a white rectangle.
Info about this large mosaic image can be seen HERE


Technical details

Processing work flow

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
Celestron Edge HD 1100 @ f10 with 0,7 focal reducer for Edge HD 1100 telescope

Mount
10-micron 1000

Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and SXV-AOL

Astrodon filter, 5nm H-alpha
Astrodon filter, 3nm O-III
Astrodon filter, 3nm S-II

Exposure times

H-alpha, 21 x 1200s, binned 2x2 = 7h
O-III, 6 x 1200s binned 4x4 = 2h 
S-II,  6 x 1200s binned 4x4 = 2h 
Total 11h


Monday, November 13, 2017

A miss shot



Now and then something goes wrong... Especially when the target is very dim, it's very easy to miss the whole target while aiming to it.
I was shooting my first light for the Autumn season 2017 and I thought that my telescope was centred to the WR 134. It was not, instead I shot some dim filaments of gas and lots of stars next to actual target.

Not much a photo but I didn't want to waste three hours of exposures so I made this image out of them. Color data is borrowed from my older mosaic image of the area.


A miss shot
Please, click for a full resolution photo



A large image of the area
Please, click for a full resolution photo

The area in the small photo above is marked with a white rectangle.



Sunday, November 12, 2017

WR 134, Ring Nebula in visual colors


I have published a mapped color version of WR 134 in Cygnus. Now I have made a visual color composition out of the narrow band channels, H-alpha, O-III and S-II. This composition is very close to a visual spectrum. The most powerful emission is from ionzed hydrogen, H-alpha. It emits light at red wavelength as well as ionized sulfur, S-II. Ionized oxygen, O-III, can be seen as blue color. There are very few photos out of this object. There are total 33 hours of exposures in this composition.


A mosaic image of WR 134 area in Cygnus
Please, click for a large image.


Image is in Natural color palette from the emission of ionized elements, R=Hydrogen + Sulphur, G=Oxygen and B=Oxygen + 10% Hydrogen to compensate the missing H-beta emission.


A closer look
Please, click for a large image.




A vertical composition
Please, click for a large image.




INFO

This image shows a ring-like nebula traced by the glow of ionized hydrogen and oxygen gas. Embedded in the region's interstellar clouds of gas and dust, the complex, glowing arcs are sections of bubbles or shells of material swept up by the wind from Wolf-Rayet star WR 134, brightest star near the center of the frame. Distance estimates put WR 134 about 6,000 light-years away, making the frame over 100 light-years across. Shedding their outer envelopes in powerful stellar winds, massive Wolf-Rayet stars have burned through their nuclear fuel at a prodigious rate and end this final phase of massive star evolution in a spectacular supernova explosion. The stellar winds and final supernovae enrich the interstellar material with heavy elements to be incorporated in future generations of stars. (Source, NASA APOD, https://apod.nasa.gov/apod/ap120621.html )


Technical details

Processing work flow

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
Celestron Edge HD 1100 @ f10 with 0,7 focal reducer for Edge HD 1100 telescope

Mount
10-micron 1000

Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and SXV-AOL

Astrodon filter, 5nm H-alpha
Astrodon filter, 3nm O-III
Astrodon filter, 3nm S-II

Exposure times

H-alpha, 51x 1200s, binned 2x2 = 17h
O-III, 9 x 1200s binned 4x4 = 8h 
S-II,  9 x 1200s binned 4x4 = 8h 
Total 33h


Wednesday, November 8, 2017

Sharpless 119 (Sh2-119) in Cygnus




This is my second light for the Autumn season 2017. This is a detail of the large emission area just couple of degrees from the North America nebula. It's very overlooked due to its low surface brightness and a close proximity of brighter and more famous emission targets.
I have plans to shoot the whole nebula as a mosaic of six image panels, when ever the weather permits.


Sharpless 119 in Cygnus (Sh2-119)
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. The photo spans about a square degree of sky. (The full Moon spans about 0,5 degrees of sky.)


An experimental starless version

In this starless version the shapes in gas and dust are easier to see.


Image in visual spectrum
Please, click for a full size photo

Image is in Natural color palette from the emission of ionized elements, R=Hydrogen + Sulphur, G=Oxygen and B=Oxygen + 10% Hydrogen to compensate the missing H-beta emission.



A wider field image of the area, Canon 200mm f1.8 lens
Please, click for a full size image

Sharpless 119 can be seen at lower left corner. The white rectangle shows the location of the new photo. It spans about a square degree of sky. (The full Moon spans about 0,5 degrees of sky.)
This photo was taken with the Canon EF 200mm f1.8 lens and the QHY9 astrocam, Baader narrowband filter set at 2012.


An other wide field shot, Tokina AT 300mm f2.8 lens

More info about this photo HERE


INFO

Sh2-119, Sharpless 119, is a large complex of emission nebulosity in Cygnus constellation, about 2 degrees east of the North American Nebula. It is located just around 68 Cygni, a quite bright star of magnitude 5. (The most bright star in the photo)


Technical details

Processing work flow

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
Celestron Edge HD 1100 @ f10 with 0,7 focal reducer for Edge HD 1100 telescope

Mount
10-micron 1000

Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and SXV-AOL

Astrodon filter, 5nm H-alpha

Exposure times

H-alpha, 21x 1200s, binned 2x2 = 7h
O-III and S-II channels are borrowed form my older wide field photos.









Friday, November 3, 2017

WR 134, Ring Nebula area as a mosaic image.



While shooting  my first light photo for the Autumn season 2017, I shot some frames frames around it for a mosaic image. 



A mosaic image of WR 134 area in Cygnus
Click for a large image.

The Wolf-Rayet shell, WR 134, can be seen as an oval shape at center up. There is a strong emission from ionized oxygen, O-III, it can be seen as blue color. 
Image is in mapped colours, from the emission of ionized elements, R=Sulphur, G=Hydrogen and B=Oxygen.


A large six panel version of the mosaic image

Lots of is coining on in this area in Cygnus.

Orientation in Cygnus
Click for a large image.


The area of WR 134 is marked as a white rectangle.
Info about this large mosaic image can be seen HERE

INFO

This image shows a ring-like nebula traced by the glow of ionized hydrogen and oxygen gas. Embedded in the region's interstellar clouds of gas and dust, the complex, glowing arcs are sections of bubbles or shells of material swept up by the wind from Wolf-Rayet star WR 134, brightest star near the center of the frame. Distance estimates put WR 134 about 6,000 light-years away, making the frame over 100 light-years across. Shedding their outer envelopes in powerful stellar winds, massive Wolf-Rayet stars have burned through their nuclear fuel at a prodigious rate and end this final phase of massive star evolution in a spectacular supernova explosion. The stellar winds and final supernovae enrich the interstellar material with heavy elements to be incorporated in future generations of stars. (Source, NASA APOD, https://apod.nasa.gov/apod/ap120621.html )


Technical details

Processing work flow

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
Celestron Edge HD 1100 @ f10 with 0,7 focal reducer for Edge HD 1100 telescope

Mount
10-micron 1000

Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and SXV-AOL

Astrodon filter, 5nm H-alpha
Astrodon filter, 3nm O-III
Astrodon filter, 3nm S-II

Exposure times

H-alpha, 51x 1200s, binned 2x2 = 17h
O-III, 9 x 1200s binned 4x4 = 8h 
S-II,  9 x 1200s binned 4x4 = 8h 
Total 33h


Thursday, November 2, 2017

First light for the Autumn season 2017, finally!


This Autumn season has been the most cloudy one, I have never publish my first light so late.
We have had only one clear night plus two nights with opening at clouds for few hours.  

My first light for the Autumn season 2017  shows a rare and exotic target at Cygnus. It's a largely unknown Wolf-Rayet shell around the star WR 134.
I noticed this formation at first time in my large 18-panels mosaic of Cygnus. It's clearly visible, specially at Ionised oxygen channel (O-III)


A three frame mosaic of WR 134
 Click for a large image.

The Wolf-Rayet shell can be seen as an oval shape at center up. There is a strong emission from ionized oxygen, O-III, it can be seen as blue color. 
Image is in mapped colours, from the emission of ionized elements, R=Sulphur, G=Hydrogen and B=Oxygen.


WR 134
Wolf-Rayet shell around WR 134 in Cygnus, click for a large image.


A starless version
Click for a large image.


The structure and shapes in ionized gas are easier to see in this experimental starless version.
(Note. the straight line at  seven o'clock is not an artefact but a real shape.)

Orientation in Cygnus
Click for a large image.

The area of WR 134 is marked as a white rectangle at middle right.
Info about this large mosaic image can be seen HERE

INFO

This image covers a field of view about one square degree in the constellation Cygnus. It highlights the bright edge of a ring-like nebula traced by the glow of ionized hydrogen and oxygen gas. Embedded in the region's interstellar clouds of gas and dust, the complex, glowing arcs are sections of bubbles or shells of material swept up by the wind from Wolf-Rayet star WR 134, brightest star near the center of the frame. Distance estimates put WR 134 about 6,000 light-years away, making the frame over 100 light-years across. Shedding their outer envelopes in powerful stellar winds, massive Wolf-Rayet stars have burned through their nuclear fuel at a prodigious rate and end this final phase of massive star evolution in a spectacular supernova explosion. The stellar winds and final supernovae enrich the interstellar material with heavy elements to be incorporated in future generations of stars. (Source, NASA APOD, https://apod.nasa.gov/apod/ap120621.html )


Technical details

Processing work flow

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
Celestron Edge HD 1100 @ f10 with 0,7 focal reducer for Edge HD 1100 telescope

Mount
10-micron 1000

Cameras and filters
Imaging camera Apogee Alta U16 and Apogee seven slot filter wheel
Guider camera, Lodestar x 2 and SXV-AOL

Astrodon filter, 5nm H-alpha
Astrodon filter, 3nm O-III
Astrodon filter, 3nm S-II

Exposure times

H-alpha, 21x 1200s, binned 2x2 = 7h
O-III, 9 x 1200s binned 4x4 = 3h 
S-II,  9 x 1200s binned 4x4 = 3h 
Total 13h


Uncropped, calibrated and stretched single 20 min. H-alpha frame as it comes from the camera



Uncropped, calibrated and stretched single 20 min. O-III frame as it comes from the camera






Friday, March 3, 2017

The central Cygnus as a cinemascope format image set


I have worked with a cinemascope format movie from my photos for a movie theatre presentation. This is an extra wide ~21:9 format used in theatres. The actual film is not ready yet but I have some of my images converted to this ultra wide format. I think they will look great at a large movie screen! I'll publish some of individual panoramic format photos here,


Central Cygnus image set
Be sure to click for a full resolution image, ~2600 x 1200 pixels

Image details can be seen HERE



Image details can be seen HERE



Image details can be seen HERE


Orientation in Cygnus
Please, click for a large image

Image details can be seen HERE



Previously published sets of my cinemascope format astro images












Thursday, February 9, 2017

B&W universe, part IV


As I'm using a cooled Gray scale astronomical CCD camera, I have a Black and White images from all of my photos. (For a color image, colors are made by shooting each color channel trough a filter, in my case mostly a narrow band filters.)

I will publish few posts out of my B&W images. Sometimes I like them better as a color ones.
B&W universe part I can be found HERE, Part II  HERE and Part III from HERE


Nebulae of the Central Cygnus, a mosaic image project
Please, click for a large image

Eleven panels ( 2200 x 1000 pixels)

Photo shows the emission of hydrogen alone. (H-alpha) You'll find a color version and the technical details from HERE


Five panels ( 2200 x 1000 pixels)

You'll find a color version and the technical details from HERE


One panel

You'll find a color version and the technical details from HERE


For technical details and a color versions, please, use a link under the images above.


Wednesday, February 8, 2017

B&W universe, part III

As I'm using a cooled Gray scale astronomical CCD camera, I have a Black and White images from all of my photos. (For a color image, colors are made by shooting each color channel trough a filter, in my case mostly a narrow band filters.)

I will publish few posts out of my B&W images. Sometimes I like them better as a color ones.
B&W universe part I can be found HERE and Part II from HERE


Dark filaments of the Pelican nebula
Please, click for a large image

Photo shows the emission of hydrogen alone. (H-alpha) You'll find a color version and  the technical details from HERE


A two panel mosaic
Please, click for a large image

You'll find a color version and  the technical details from HERE


For technical details and a color versions, please, use a link under the images above.