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Thursday, October 1, 2015

A new image, the Witch's Broom Nebula



This is my second photo for this season from my observatory. It's a detail of the veil nebula supernova remnant, as was my first light photo for this Autumn season, the Pickering's Triangle. This is a two frames mosaic image, exposed on several nights between September 10. - 27. 2015. Total exposure time is about 11h.

NGC 6960, the Witch's Broom Nebula
Click for a large image, 2200 x 1500 pixels and 2,3MB

A two frame mosaic of the Veil Nebula supernova remnant, the Witch's Broom Nebula in mapped colors. Colors are from the emission of the ionized elements, Hydrogen, Sulfur and Oxygen. 
S-II = Red, H-alpha = Green and O-III = Blue. 


Close up images
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A starless image
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An experimental starless version to show the structure of the filaments better. 


Visual colors
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Natural color composition from the emission of ionized elements. 
This composition is very close to a visual spectrum. 


Witch's broom in light of an ionized oxygen only
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This image shows the Witch's Broom in Light of an ionized oxygen, O-III, alone.


A wide field photo of the Veil Nebula supernova remnant

The Witch's Broom Nebula can be see at three o'clock position.
My blog post about this older wide field shot 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, 21 iterations, added at 25% weight
Color combine in PS CS3
Levels and curves in PS CS3.

Imaging optics
Celestron Edge HD 1100 @ f7 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 x2 and SXV-AOL

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

Exposure times
H-alpha, 15 x 1200s = 5h
O-III, 36 x 1200s binned = 5h (Autumn 2014)
S-II,  from my older wide field photo of the Veil Nebula = 1h 
Total 11h



Friday, September 25, 2015

Astro Anarchy gets published



The Cnet published an article about Messier 31, the Great galaxy  of Andromeda, photo.
Photo of Messier 31 is produced by collaboration between David Lane and me.

You can read the Cnet article by Michelle Starr from 




The Wired noticed us too
Ten must-read articles for 25 September
Our photo is number five on the list


Thursday, September 24, 2015

Messier galaxies, M81-M82, with integrated flux nebula


A new collaboration image with David Lane. Beside beeing a deep sky astrophotographer he is also a master of landscape astrophotographing, please, have a look at his homepage: http://www.davelaneastrophotography.com/

Image acquisition is made by David Lane. He sent a massive amount of data to me to process and here is the result, Messier galaxies 81 and 82 with a large amount of  dim integrated flux nebula at front of them.
Total exposure time is around 40 hours with the William Optics GT81 telescope and SBIG STL-1100 3 CCD-camera. 



Messier 81 and 82 with an integrated flux nebula
Click for a large photo

So dusty, don't they ever clean up there...


An experimental starless photo
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Brighter dots in this starless image are more distant galaxies


 A horizontal composition
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A better resolution photo

Technical details

Data acquisition, David Lane
Image processing, J-P Metsavainio

Processing workflow

Deconvolution with a CCDStack2 Positive Constraint, 27 iterations, added at 33% weight
Color combine in PS CS3
Levels and curves in PS CS3.

Imaging optics
 William Optics GT81

Camera
SBIG STL-1100 3 CCD

Exposure times
Total ~40h






Wednesday, September 23, 2015

Messier 31, M31, the Great Galaxy of Andromeda


Another collaboration image, this time with David Lane. He is also a master of landscape astrophotographing, please, have a look at his homepage: http://www.davelaneastrophotography.com/ 

Image acquisition is made by David Lane. He sent a massive amount of data to me to process and here is the first result, the Great Galaxy of Andromeda with 37 hours of exposure time.


Messier 31, M31, the Galaxy of Andromeda 
Click for a large image

A deep H-alpha boosted LRGB exposure of the Galaxy of Andromeda


Large resolution detail from the image above
Click for a large image

Dust lanes of Andromeda


A starless view
Click for a large image

This photo shows the M31 as it was seen just outside of our home galaxy, the Milky way. All the stars in the first photo are located in Our galaxy at maximum distance of few tens of thousands light years. M31 lies at distance of about 2.5 million light years. There is 2.5 million light years of nothing between us and Messier 31. Dim dots at the starless image are more distant galaxies and some hundred of globular cluster associated to M31 galaxy .


A vertical composition of M31

A poster format view to the M31


INFO

The Andromeda Galaxy, also known as Messier 31, M31, or NGC 224, is a spiral galaxy approximately 2.5 million light years from Earth. It is the nearest major galaxy to the Milky Way.

The Milky Way and Andromeda are expected to collide in 3.75 billion years, eventually merging to form a giant elliptical galaxy or perhaps a large disk galaxy.

At 3.4, the apparent magnitude of the Andromeda Galaxy is one of the brightest of any of the Messier objects, making it visible to the naked eye on moonless nights even when viewed from areas with moderate light pollution. It has an apparent diameter of six times as wide as the full Moon


An experimental test

This funny looking image is just stretched vertically to try to show the actual round shape of the galaxy.
It looks like a barred spiral to me.


Technical details

Data acquisition, David Lane
Image processing, J-P Metsavainio

Processing workflow

Deconvolution with a CCDStack2 Positive Constraint, 27 iterations, added at 33% weight
Color combine in PS CS3
Levels and curves in PS CS3.

Imaging optics
 William Optics GT81

Camera
SBIG STL-1100 3 CCD

Exposure times
Luminance, 18h
H-alpha, 1h
Red = ~6h
Green = ~6h
Blue = ~6h
Total 37h