This page presents false-color images of emission lines [OIII] (500.7 nm, mapped to red), Hα (656.3 nm, mapped to green), and [SII] (671.7 nm and 673.0 nm, mapped to blue).
The brightest stars are added to visualize the regions contaminated by strong continuum light. (Aside from that, the image does not contain continuum light.)
Click on the images below to load them in full resolution using a JavaScript viewer.
Overview image showing a 212° stereographic projection of the entire surveyed region. This projection type was used because it preserves shapes. Maximum image resolution in the JavaScript viewer (click on the image)
is 30″ at the center (δ=90°) and about 11″ at the boundary (δ=-16°).
Tile images
The tiles are arranged in four rows centered at declinations 76.125°, 50.375°, 24.625°, and -1.125°. The size of each tile is 31° × 31°, with an overlap of at least 5.3°.
Click on the preview images below to load them in maximum resolution of 10″ using a JavaScript viewer.
The angle α below the preview images describes the right ascension of the image center. (The declination angle is found in the heading above the images. The ICRS coordinate system is used.)
Declination δ=76.125°
α=22:17 h
α=18:51 h
α=15:26 h
α=12:00 h
α=8:34 h
α=5:09 h
α=1:43 h
Declination δ=50.375°
α=23:00 h
α=21:00 h
α=19:00 h
α=17:00 h
α=15:00 h
α=13:00 h
α=11:00 h
α=9:00 h
α=7:00 h
α=5:00 h
α=3:00 h
α=1:00 h
Declination δ=24.625°
α=23:09 h
α=21:26 h
α=19:43 h
α=18:00 h
α=16:17 h
α=14:34 h
α=12:51 h
α=11:09 h
α=9:26 h
α=7:43 h
α=6:00 h
α=4:17 h
α=2:34 h
α=0:51 h
Declination δ=-1.125°
α=23:09 h
α=21:26 h
α=19:43 h
α=18:00 h
α=16:17 h
α=14:34 h
α=12:51 h
α=11:09 h
α=9:26 h
α=7:43 h
α=6:00 h
α=4:17 h
α=2:34 h
α=0:51 h
Monitor calibration
For optimal display, the monitor should be calibrated so that as many shades of the grayscale shown below are distinguishable.
At least the 4% steps should be separated by every monitor. The 2% steps are visible on better monitors. To distinguish the 1% steps, a HDR monitor is required.
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