NGC1499, also known as the California Nebula (it resembles the outline of this US state), is a large emission nebula with a low surface brightness, which makes it difficult to observe.
The nebula is most likely to be illuminated by Xi Persei (the brightest star in the image).

The nebula lies at a distance of about 1.000 light years, is about 100 light years long (spans about 2.5° of sky) and can be found in the constellation Perseus.

Previous/older images:

Nov 14, 2012 – ST-8300M (80mm TMB-2h 51m)
Oct 15, 2009 – Canon 350D (80mm TMB-2h 30m)

Image data

Object info
Name NGC1499 – The California Nebula
Type Emission nebula
Constellation Perseus
Right ascension 04h 03m 18s
Declination +36° 25′ 18″
Distance 1.000 ly
Other designations Sharpless 220
Image info
Image date Nov. 26, 2016
Light frames 16x 10 min. 7nm Ha unbinned (Luminance) added to the 2012 RGB color image
Total integration 5h 31m
Dark frames info n/a
Flat frames info n/a
Bias frames info n/a
Software used SGPro, PHD2 Guiding, DeepSkyStacker, Registar, Photoshop CS6
Processing Focusing and image acquisition was done using Sequence Generator Pro.
All separate frames were calibrated, aligned and stacked in DeepSkyStacker.
Images were aligned in Registar prior to combining into RGB.
Photoshop CS6 was used for further processing – curves adjustment, levels adjustment, etc.
Noel Carboni’s toolset was used as well (Local Contrast Enhancement, Deep Space Noise Reduction)
Equipment info
Telescope TMB/LOMO 80/480
Corrector Televue 2″ TRF 2008 flattener/reducer (FL: 384mm f/4.8)
Mount Losmandy G-11 Gemini
Camera SBIG ST-8300M
Guide camera Astrolumina ALccd5-II (Mono)
Guide scope Starwave 50mm f/4.1 Guide Scope
Autoguide software PHD2 Guiding
Filters Baader 2″ 7nm Ha, Baader 2″ RGB + IDAS LPS-P2
Location Landgraaf, The Netherlands
Image comments

16 x 10 minutes of H-alpha data was blended into the color RGB image from 2012.