Mike Lewis
Staff Member
So I have always wanted to go back and redo the California Nebula (NGC1499) since my last effort, where I neglected to take Oiii data, and therefore ended up with just Hα and Sii, which made for some mixing options I did not like. I ended up with 2 mixes on that image (which was a 2 panel mosaic) and did not much like either of them. So I decided to give this target another go from my remote location in dark sky TX. I did once again notice how faint the Oiii signal was compared to the other channels but this time, taking longer subs and taking twice as much Oiii seemed to help that out, and in fact, the mixing of the channels this time was really easy, with both SHO palette and a Foraxx palette results just falling out in a pleasing fashion with very little fiddling involved. This time, I like both results, although after many comparisons I think I do have a favorite. But I am VERY interested to hear what the group might think as far as picking a favorite color mix, as they are certainly quite different. In both cases I did not accentuate the colors to any real degree - I wish I knew why some 'mixes' come out with great color and contrast immediately where other data sets require hours of yanking and tweaking to get a result I like.
I have not yet posted these on Astrobin as I want to wait a little longer to make sure the one I mark as the final version over there is the choice I am happy with. Thanks for looking and any input you care to share.
For comparison's sake, here are the previous versions:
https://www.focalworld.com/media/lrcc_srgb_fw_caneb_withstars_pscc-jpg.6977/
https://www.focalworld.com/media/lrcc_srgb_fw_srgb_caneb_nb_mix7_withstars_pscc-jpg.6982/
A quick little bit on this target from Wikipedia:
The California Nebula (Also known NGC 1499 or Sh2-220) is an emission nebula located in the constellation Perseus. Its name comes from its resemblance to the outline of the U.S. State of California in long exposure photographs. NGC 1499 is almost 2.5° long on the sky and, because of its very low surface brightness, it is extremely difficult to observe visually. It lies at a distance of about 1,000 light years from Earth. Its fluorescence is due to excitation of the Hβ line in the nebula by the nearby prodigiously energetic O7 star, Xi Persei (also known as Menkib).
The SHO version:
The Foraxx version:
Collection details:
Equipment:
Poseidon-M Camera @ -5C and
Gain:125 Offset:25
Astro-Physics Mach2 Mount
Williams Optics Cat 91 Refractor, 448mm @ f/4.9
Antlia Pro Filters (3nm narrowband plus RGB)
Askar FMA180 Guide scope with ASI290MM
Software:
Pixinsight Commercial Version 1.9
Lightroom CC
Photoshop CC
N.I.N.A. Control Software
BlurXTerminator (Russell Croman)
StarXTerminator (Russell Croman)
NoiseXTerminator (Russell Croman)
Astro-Physics APCC and APPM
Light Frames:
Gain 125 / Offset 25
Hα: 12 x 900 secs 3 hrs)
Oiii: 28 x 900 secs (7 hrs)
Sii: 14 x 900 secs (3 hrs 30 mins)
Red: 23 x 120 secs (46 mins)
Green: 24 x 120 secs (48 mins)
Blue: 31 x 120 secs (1 hr 2 mins)
16 hrs 06 mins total
Dark Frames:
10 x 120 secs (20 mins)
10 x 900 secs (2 hrs 30 mins)
I have not yet posted these on Astrobin as I want to wait a little longer to make sure the one I mark as the final version over there is the choice I am happy with. Thanks for looking and any input you care to share.
For comparison's sake, here are the previous versions:
https://www.focalworld.com/media/lrcc_srgb_fw_caneb_withstars_pscc-jpg.6977/
https://www.focalworld.com/media/lrcc_srgb_fw_srgb_caneb_nb_mix7_withstars_pscc-jpg.6982/
A quick little bit on this target from Wikipedia:
The California Nebula (Also known NGC 1499 or Sh2-220) is an emission nebula located in the constellation Perseus. Its name comes from its resemblance to the outline of the U.S. State of California in long exposure photographs. NGC 1499 is almost 2.5° long on the sky and, because of its very low surface brightness, it is extremely difficult to observe visually. It lies at a distance of about 1,000 light years from Earth. Its fluorescence is due to excitation of the Hβ line in the nebula by the nearby prodigiously energetic O7 star, Xi Persei (also known as Menkib).
The SHO version:
The Foraxx version:
Collection details:
Equipment:
Poseidon-M Camera @ -5C and
Gain:125 Offset:25
Astro-Physics Mach2 Mount
Williams Optics Cat 91 Refractor, 448mm @ f/4.9
Antlia Pro Filters (3nm narrowband plus RGB)
Askar FMA180 Guide scope with ASI290MM
Software:
Pixinsight Commercial Version 1.9
Lightroom CC
Photoshop CC
N.I.N.A. Control Software
BlurXTerminator (Russell Croman)
StarXTerminator (Russell Croman)
NoiseXTerminator (Russell Croman)
Astro-Physics APCC and APPM
Light Frames:
Gain 125 / Offset 25
Hα: 12 x 900 secs 3 hrs)
Oiii: 28 x 900 secs (7 hrs)
Sii: 14 x 900 secs (3 hrs 30 mins)
Red: 23 x 120 secs (46 mins)
Green: 24 x 120 secs (48 mins)
Blue: 31 x 120 secs (1 hr 2 mins)
16 hrs 06 mins total
Dark Frames:
10 x 120 secs (20 mins)
10 x 900 secs (2 hrs 30 mins)