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Sunday, November 1, 2020

A supernova remnant in Cygnus, G65.3+5.7 SNR

 This is a rarely imaged target, this is also one of the most difficult targets, I have ever shot. Due to a very dense star field, large angular dimension and a very diffused structure this is even more difficult target, than a Simeis 147 supernova remnant in Taurus. Total exposure time of 10h was needed to have this image. The imaging system is very fast since it's undersampled and that's good when I want capture a very large, dim and diffused targets like this one. My current imaging system, https://astroanarchy.blogspot.com/2020/01/the-frankenstein-monster-my-current.html


G65.3+5.7 SNR has about the same angular dimensions, than brighter and more famous remnant in Cygnus, the Veil Nebula The angular dimensions are about 3x4 degrees. This is a very difficult target it has a very low surface brightness and the starfield is extremely dense in this part of the Milky Way.


NOTE, the "noise" in the photos is not a noise at all, it's glow from countless stars,
it can be seen best in full size photo!

G65.3+5.7 SNR
Please, click for a large image, it's worth it!

There are very few images out of this dim and diffused supernova remnant around. Image is in mapped colours, from the emission of ionized elements, R=Sulphur, G=Hydrogen and B=Oxygen. 
Note! An apparent size of the Moon in a same scale can be seen at lower left corner.


A closeup
click for a large image

This is a full resolution close up from the photo to show, how dense the star field really is!


O-III light alone
click for a large image


H-alpha and S-II light Only
click for a large image



Orientation in Cygnus
click for a large image

This super nova remnant can be seen at bottom of the image above. It's partly overlapping with my large mosaic image of Cygnus nebula complex. I have some plans to shoot more frames to the mosaic to it to fully cover both supernova remnants visible in image. 

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, 12 x 1200 s, binned 1x1 = 4 h
O-III, 12 x 1200 s, binned 1x1 = 4 h
S-II, 6 x 1200 s, binned 2x2 = 2 h






Sunday, October 25, 2020

Exhibition, Oulu, Finland 28.10 - 15.11. 2020

 EXHIBITION



KUTSU SINULLE JA YSTÄVILLESI
            
     

J-P METSÄVAINIO
PER ASPERA AD ASTRA
28.10.-15.11.2020
 
J-P Metsävainio kuvaa yöllisen taivaan kauneutta tieteen työmenetelmiä ja välineitä hyödyntäen. Per aspera ad astra -näyttely esittelee hänen uusimpia astronomisia luontokuviaan. Vaikka itse kuvausprosessi on teknisesti raskas, Metsävainion valokuvat soivat sfäärien musiikkia luonnollisesti ja tekniikan kahleista vapautuneena. Katsojalle avautuu yhä uusia näkymiä ympäröivään todellisuuteen taiteilijan raottaessa salaisuuksien verhoa ympärillämme. 

Järjestämme näyttelyn aikana taiteilijatapaamisia ryhmille ja työporukoille. Jos olet kiinnostunut tapaamaan taiteilija näyttelyn aikana, niin soita galleristi Hanna Manniselle 040 1780 980 järjestääksesi taiteilijatapaamisen.

Juhlimme näyttelyn avajaisia tiistaina 27.10.2020 klo 18-20!  Taiteilija on paikalla avajaisissa. Tervetuloa!

 
Lisätietoja näyttelystä ja teoskuvia: https://mabd.fi/nayttely/j-p-metsavainio/

Friday, October 9, 2020

New photo, Sharpless 126 in lacerta

 


I haven't seen many pictures about this large and diffused nebula before. 
This is a very good target for my photon hungry wider field setup, https://astroanarchy.blogspot.com/2020/01/the-frankenstein-monster-my-current.html

'

Sharpless 126, Sh2-126
Click for a large image

A bicolor image from the light from ionized elements hydrogen (H-alpha) and oxygen (O-III)


INFO

Sharpless 126 (Sh2-126) is a large emission nebula in Lacerta. The source of its ionization is the ultraviolet radiation from the star 10 Lacertae.

This region with its weak nebulous filaments is part of a huge star forming region, 1200 light years away from earth.

H-alpha alone
Click for a large image



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 300 mm 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, 1 x 1200 s, binned 1x1= 20 min.

Wednesday, October 7, 2020

The Tulip nebula area in cygnus, Sh2-101, in natural colors

 


In my previous blog post this image can be seen in mapped colors, https://astroanarchy.blogspot.com/2020/10/the-tulip-nebula-in-cygnus-sh2-101.html

Photo is taken with my temporary imaging system, at the moment I'm out of the actual telescope : (
Mor info about this tool set can be seen here, https://astroanarchy.blogspot.com/2020/01/the-frankenstein-monster-my-current.html

The tulip Nebula area 
Please, click for a large image, it's worth it!¨

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


An experimental starless view
click for a large image


Info

I have shot the actual Tulip Nebula with a large 11" telescope, images and info about the Tulip nebula can be seen HERE. An other interesting detail, a blue crescent like shape at center left. It's a Wolf Rayet shell around a star WR 134. I have shot this also with a large telescope, more info and images can be found HERE  

A closeup photo of the Wolf Rayet Shell around the star WR 134

This feature can be found from the new wide field photo at center left.



Nebula in light of an ionized hydrogen alone (H-alpha)
click for a large image

Nine twenty minute 5 nm H-alpha exposures are calibrated with bias corrected flats and stacked to this cumulative three hour exposure. 


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, from my older photo of the area
S-II, from my older photo of the area
Older photo can be seen here, https://astroanarchy.blogspot.com/2011/12/cygnus-mosaic-18-panels-and-22-x-14.html