Imaging telescope or lens: Takahashi FSQ-106 ED
Imaging camera: Starlight Xpress SX-814 Trius Monochrome CCD
Mount: Sky-Watcher EZ-EQ6 GT
Guiding camera: Starlight-XPress Lodestar Autoguider
Dates: Aug. 19, 2016
Integration: 89.9 hours
Avg. Moon age: 15.41 days
Avg. Moon phase: 99.53%
Astrometry.net job: 1637828
RA center: 314.096 degrees
DEC center: 43.706 degrees
Pixel scale: 1.435 arcsec/pixel
Orientation: 179.665 degrees
Field radius: 1.851 degrees
Locations: The Hills Observatory, Manchester, United Kingdom
The project started in Sept 2014, imaged again in 2015 July to October and again in 2016 July to Aug. It has taken a long time to process as it was my first mosaic and I was still learning. This is built up from Ha, OIII, SII, Red, Green & Blue filtered data totalling 89.92 hrs
The main aim of this image is to show the detail in the dust covering this region. The central area of dust is designated L935 a large dark molecular cloud which divides NGC 7000 & IC 5070.
The basic colour pallet is based on the initial Pixelmath:
R = (ha*0.5)+(sii*0.5)
G = (oiii*0.85)+(ha*0.15)
B = (oiii*1)
But was then adapted to personal taste during processing. The RGB data was only used for the stars.
There are a variety of sub exposures and bin settings used, so I have averaged out the exposure lengths in the technical card.
I have also posted a crop of the wall area here which is at twice the resolution.
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.