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Sunday, February 9, 2020

New photo of Cederblad 214, the Cosmic Question mark

So far this has been the most cloudy winter up here for twenty years. I'm trying to use every single clear moment to have something to publish. beside the weather problems, the light pollution is increasing every moment due to LED-lightning. We have now more light pollution than ever and it's Broadband, multi spectral light. Old high pressure sodium and mercury lights are easy to filter out since the light from them is yellowish narrowband emission. LED light is impossible to filter out, it's like a Sunlight, very broad band from IR to UV and everything between. Imaging is getting more difficult and soon it'll be impossible from my current location.

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

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.







www.tips-fb.com Posted by J-P Metsavainio at 12:23 PM 0 comments
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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

Please, click for a large image

Image info and technical details can be seen HERE





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Tuesday, January 28, 2020

IC 1396 wide field, reprocessed

I reproceed the material for IC 1396 since I noticed a small flaw in the calibration file used.
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?


A close up and some info
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


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 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


www.tips-fb.com Posted by J-P Metsavainio at 5:27 PM 0 comments
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Sunday, January 26, 2020

Deep in to my heart, IC 1805 in mapped colors

I have published this image in visual colors at January 14. Since then, I have shot the emission of sulfur, S-II, and now I'm able to publish a version in mapped colors.
HST-palette separates emission areas nicely and it's visually pleasing. In visual palette emission from sulfur and hydrogen are both at red part of the spectrum. Emission from oxygen is greenish blue.

I made some testing with my new imaging system based on Tokina AT-x 300mm f2.8 camera lens.
The CCD I'm using has kind of large pixels, 9 microns, so I'm undersampled, the image scale is just over 6 arcseconds / 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.


The Heart Nebula, IC 1805
Please, click for a large image

C 1805 in mapped colors, from the emission of ionized elements,
R=Sulfur, G=Hydrogen and B=Oxygen. (Hubble Palette)



SUPERNOVA REMNANT 132.7+1.3 (HB3)
IC 1805 in visual palette
Please, click for a large image

Red emission of an ionized hydrogen (H-alpha) is dominating the scene. Image is in visual color palette from emission of an ionized hydrogen and oxygen. R=hydrogen, G=Oxygen and B=oxygen. 
SNR
 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
SNR 132.7+1.3 at upper right. Source and more information, http://galaxymap.org/drupal/node/103

IC 1805 H-alpha emission alone
Please, click for a large image

H-alpha emission, only two hours of exposures is enough for a very deep image. The combination of 300mm f2.8 camera optics and large 9 micron pixels makes this imaging system extremely hungry for photons. Image scale is just over 6 arcseconds / pixel. By using the drizzle stacking method with well dithered subframes I can avoid any square stars. 
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

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.


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