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Substrates | Optical imaging glass |
Surface Quality | 60-40 |
Spectrum | OIII 3nm Ha 3nm |
FWHM | Narrowband 3nm |
Size | 2" |
Transmitted Wavefront RMS | λ/4 |
Parallelism | 30s |
Feature1 | Maximizes the transmission of the main emission lines of the nebula in OIII (496nm and 500nm) and H-alpha (656nm). Used with DSLR,color/MONO CMOS and CCD, however, this filter is not suitable for fast ratio systems. |
Feature2 | The sky background of the image is darker, and the contrast between the nebulae and the signal-to-noise ratio are improved to the greatest extent. In heavy light pollution areas, the product can also selectively filter light pollution and clutter signals through the emission lines of nebulae, and finally avoid the impact of light pollution on astrophotography. |
Feature3 | You will get a darker sky background, more contrast of the image and the suppression on stars. L-Ultimate has also been optimized in terms of halo performance, so that there is no obvious halo when shooting on a bright star object. |




















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