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Product details
- SKU OPTO-LQUAD2
The Optolong L-Quad Enhance Broadband Filter is designed for light pollution suppression with color cameras. The L-QEF is a quad bandpass filter lowers the light generated by mercury and sodium lamps as well as natural skylight. When used with a color CMOS camera, contrast is enhanced and objects are more distinct. The filter provides better color balance while improving resistance to light pollution. This 2" L-Quad filter can be used for wide field astrophotography and deep-sky objects like nebulae, galaxies, star clusters and more. It maximizes the color balance of nebulae, galaxies and other broadband spectral targets.
Major Emission Lines of Nebulae:
H-a - 656.3nm
H-b -486.1nm
OIII - 495.9nm
OIII - 500.7nm
Major Emission Lines of Artificial Light Pollution
Hg - 435.8nm, 546.1nm, 577nm, 578.1nm
Na - 598nm, 589.6nm, 615.4nm, 616.1nm
Features of the L-Quad Enhance 2" Filter
- Cuts out light pollution from mercury and sodium lamps and produces a nice broadband image with minimal color cast;
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Signal-to-noise ratio (SNR);
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Near IR cut-off to 1000nm, reducing the effects of IR noise;
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L-QEF has more than 90% transmittance of the nebula emission lines at H-Beta/OIII/H-Alpha/SII, with cut-off depth from OD2 to OD4, thus providing a significant increase in resistance to light pollution. L-QEF is good for night sky from Bortel 1 to Bortel 7 levels; (Bortel 8, Bortel 9 environments are not recommended);
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Suitable for wide range of deep sky targets: it covers most nebulae, galaxies, star clusters, reflected and emitted line signals astronomical objects with higher contrast and rich details while maintaining excellent color balance.
Technical Data
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Substrate: Optical glass
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Thickness: 1.85 mm
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Surface Quality: 60/40 (Refer to MIL-O-13830)
- Fine-optically polished to ensure accurate 1/4 wavefront and < 30 seconds parallelism over the both surfaces
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Blocking Range: 300 nm - 1000 nm
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Blocking Depth: OD2 - OD4
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Parallelism: 30s
- Multi-layers of anti-reflection coating
- FWHM: Quad bandpass filter