AstroBin saves small pieces of text information (cookies) on your device in order to deliver better content and for statistical purposes. You can disable the usage of cookies by changing the settings of your browser. By browsing AstroBin without changing the browser settings, you grant us permission to store that information on your device.
I agreeImaging telescopes or lenses:Orion Optics UK AG12, Tele Vue NP127is
Imaging cameras:ZWO ASI1600MM-Cool, ZWO ASI 183 MM pro
Mount:Paramount MEII with Absolute Encoders
Guiding telescope or lens:Orion Optics UK AG12
Guiding camera:Starlight Xpress Lodestar X2 Mono
Software:Sequence Generator Pro, PixInsight 1.8, PHD Guiding 2
Accessory:Gerd Neumann Flat Panel
Resolution: 4220x3180
Dates:Jan. 27, 2019, Jan. 31, 2019
Frames:
AstroDon 5nm Ha filter: 98x300" (gain: 99.00) -20C bin 1x1
AstroDon 5nm Oiii filter: 95x300" (gain: 99.00) -20C bin 1x1
Integration: 16.1 hours
Avg. Moon age: 23.67 days
Avg. Moon phase: 35.43%
Bortle Dark-Sky Scale: 4.00
Temperature: -5.00
Astrometry.net job: 2523343
RA center: 44.144 degrees
DEC center: 60.671 degrees
Pixel scale: 0.701 arcsec/pixel
Orientation: 177.297 degrees
Field radius: 0.514 degrees
Locations: Dark Star Observatory, Taos, New Mexico, United States
Data source: Own remote observatory
Remote source: Non-commercial independent facility
Images from the following two scopes (piggybacked) contributed to this image:
AG12+ASI1600MM at .70 asec/pix
TV127is+ASI183MM at .75 asec/pix.
They were all registered to the best Ha image taken on the AG12.
Imaged on nights of 2018/1/27, 28, 29, 30, 31.
I am quite pleased with how the star colors came out. They are reasonably close to RGB colors, but no RBG was used. I have Barry Wilson to thank for that. His excellent tutorial on processing NB images taught me a wonderful way to handle the pink stars, which I have struggled with for ages. Just Invert the image, then remove the green. Magic, and so easy. Thanks Barry. Another tip I like was to leave some of the green tones in. Adds a lot of depth to the image. Go to https://barrywilson.smugmug.com/PixInsight-Tutorials
This image looks deep inside the Soul Nebula. The dark and brooding dust clouds outlined by bright ridges of glowing gas are cataloged as IC 1871, and are commonly referred to as the Whirling Dervish. About 25 light-years across, the telescopic field of view spans only a small part of the much larger Heart and Soul nebulae. At an estimated distance of 6,500 light-years the star-forming complex lies within the Perseus spiral arm of the Milky Way, seen in planet Earth's skies toward the constellation Cassiopeia. An example of triggered star formation, the dense star-forming clouds of IC 1871 are themselves sculpted by the intense winds and radiation of the region's massive young stars. This color image adopts a palette made popular in Hubble images of star-forming regions.
(Starship Asterisk)
You have no new notifications. |
This page or operation is not available at the moment, because AstroBin is in READ ONLY mode. For more information, please check out our Twitter feed: https://twitter.com/AstroBin_com
If this image is the result of your processing of a public data pool, you can send it the pool so it's displayed there.
Use this form to select an existing public data pool.
If this image is the result of your processing of a private shared folder, you can send it the folder so it's displayed there.
Such limitation improves the website as a whole by discouraging people from creating fake accounts to like their own images. Thank you for understanding!
Currently, your AstroBin index is 0.00.
Comments