Narrowband Filters
Narrowband imaging is what makes deep-sky astrophotography possible from a Canadian city. By passing only a few nanometres around a specific emission line, these filters reject almost all artificial light and most moonlight, so a nebula that is invisible visually from a suburban driveway becomes a viable multi-hour imaging target. David Astro stocks narrowband filters in Canada, held in Canadian inventory.
Bandwidth choice interacts with your telescope's focal ratio in ways that catch people out. Tell us your optic and camera and we will recommend a bandwidth that will actually perform in your system.
Filters
Chroma OIII Filter - 3nm
Isolates the 500.7 nm OIII emission line 3 nm bandpass for high contrast Designed for f/4.0 or slower optical systems 3.0 mm thick, single-substra...
View full detailsChroma OIII Filter - 5nm
Isolates the 500.7nm OIII emission line 5nm bandwidth (FWHM) 3.0mm thick single substrate for parfocal use Transmitted wavefront better than 0.25 ...
View full detailsChroma OIII Filter - 8nm
Isolates the 500.7nm OIII emission line 8nm bandpass for high signal throughput Designed for f/4.0 or slower; measured 99.7% peak transmission at ...
View full detailsChroma OIII Filter Optimized for f/3 - 3nm
Isolates the 500.7 nm OIII emission line 3 nm bandpass for high-contrast imaging Optimized for f/2.8 to f/3.6 optical systems Measured 99.2% peak ...
View full detailsChroma SII Filter - 3nm
Central Wavelength: 672.4 nm (Sulfur-II) Bandwidth (FWHM): 3 nm Substrate Thickness: 3.0 mm Parfocal: Yes, with other Chroma astronomy filters...
View full detailsChroma SII Filter - 5nm
Bandwidth: 5 nm Central Wavelength: 672.4 nm Target Emission: Sulfur-II Doublet (671.6 nm / 673.1 nm) Substrate Thickness: 3.0 mm Parfocal: Y...
View full detailsChroma SII Filter - 8nm
Isolates the 672.4 nm SII doublet emission lines 8 nm bandpass optimized for high signal throughput Designed for f/4.0 or slower; measured 98.2% p...
View full detailsChroma SII Filter Optimized for f/3 - 3nm
Isolates the 672.4 nm SII emission line doublet 3 nm bandpass for high contrast Optimized for f/2.8 to f/3.6 optical systems Maintains 98.6% peak ...
View full detailsExplore Scientific Nebula Filter H-Alpha 1.25-inch 12nm
Targets Hydrogen-Alpha emission nebulae 12nm bandpass for astrophotography 1.25-inch standard filter size Drastically improves contrast under ligh...
View full detailsExplore Scientific Nebula Filter H-Alpha 2-inch 12nm
Isolates the Hydrogen-alpha emission line at a 12nm bandpass Standard 2-inch filter format for modern focusers and filter wheels Dramatically incr...
View full detailsExplore Scientific Nebula Filter H-Alpha 2-inch 7nm
7nm H-Alpha Bandpass 2-inch Filter Format Isolates Hydrogen Emission Nebulae Blocks Urban Light Pollution Includes Individual Test Report Descr...
View full detailsExplore Scientific Nebula Filter S-II 1.25-inch 12nm
Isolates the ionized sulfur (S-II) emission line at 672nm Features a 12nm bandpass to increase contrast Standard 1.25-inch filter format Ideal for...
View full detailsExplore Scientific Nebula Filter S-II 1.25-inch 6.5nm
Isolates the ionized sulfur (S-II) emission line at 672nm Ultra-narrow 6.5nm bandpass for maximum contrast Standard 1.25-inch barrel size fits mos...
View full detailsExplore Scientific Nebula Filter S-II 2-inch 12nm
Isolates the 672nm Sulfur-II (S-II) emission line 12nm bandpass for high-contrast views 2-inch filter size with standard threads Blocks light poll...
View full detailsExplore Scientific Nebula Filter S-II 2-inch 6.5nm
6.5nm Narrow Bandpass Targets the 672nm Ionized Sulfur (S-II) Emission Line 2-inch Barrel Diameter for Larger Focusers Drastically Increases Contr...
View full detailsIDAS OL7.5 Low-Profile Filter for Celestron RASA 8 (M42 / M54)
Engineered to consume exactly 7.5mm of optical path Solves the Celestron RASA 8 25.0mm backfocus requirement with 17.5mm cameras Available in M42 ...
View full detailsOptolong H-alpha 3nm Narrowband Filter
3nm Bandpass at 656nm Wavelength Maximizes Contrast for Emission Nebulae Extreme Rejection of Light Pollution and Skyglow Ion-Assisted, Anti-Refle...
View full detailsOptolong H-Alpha 7nm Narrowband Filter
Isolates the 656nm Hydrogen-alpha emission line 7nm bandpass for maximum contrast Blocks mercury vapor, sodium vapor, and natural skyglow Ideal fo...
View full detailsOptolong Ha 7nm, OIII 6.5nm & SII 6.5nm Filter Set
H-alpha Filter: 7nm Bandpass centered at 656nm Oxygen-III Filter: 6.5nm Bandpass centered at 500nm Sulphur-II Filter: 6.5nm Bandpass Hubble Pa...
View full detailsOptolong Ha, OIII & SII 3nm Narrowband Filter Set
Complete SHO set includes H-alpha, OIII, and SII filters Ultra-narrow 3nm bandpass for maximum contrast Isolates 656nm Ha and 500nm OIII emission ...
View full detailsOptolong LRGB + H-Alpha 7nm Filter Set
Complete 5-Filter LRGB and H-Alpha Set 7nm H-Alpha Filter Centered at 656.3nm Blocks 589nm Sodium Light Pollution Line High Transmission for Natur...
View full detailsOptolong LRGB, Ha, OIII & SII Filter Set
Complete 7-filter set for monochrome astrophotography Includes Luminance, Red, Green, and Blue broadband filters Includes 7nm Hydrogen-alpha, 6.5n...
View full detailsOptolong OIII 3nm Narrowband Filter
3nm Spectral Bandpass 500nm Central Wavelength (OIII) Ion-Assisted Multi-Layer Coatings Optimized for Monochrome Cameras Available in 2" Mounted o...
View full detailsOptolong OIII 6.5nm Narrowband Filter
6.5nm Narrowband OIII Filter Centered on 500nm Wavelength Passes the 500.7nm OIII Emission Line Blocks Light Pollution and Skyglow Ideal for SHO H...
View full detailsEmission Lines, Bandwidth and Focal Ratio
Narrowband filters isolate the specific wavelengths that ionized gas emits. Narrower is not always better, because the passband shifts in a fast light cone and the exposure requirement rises.
- Hydrogen-alpha at 656.3 nm: The strongest and most widely used emission line, showing nebulosity in extraordinary detail and working well even under a bright Moon.
- Oxygen III at 500.7 nm: Reveals planetary nebulae, supernova remnants and the outer shells of emission nebulae; typically the weakest signal of the three and needs the most integration.
- Sulphur II at 672.4 nm: The third channel of the Hubble palette, adding structural differentiation in bright nebulae.
- 3 to 5 nm bandwidth: Maximum contrast under light pollution, best suited to f/5 and slower systems and to accurate, temperature-compensated focus.
- 6 to 12 nm bandwidth: More forgiving of fast optics and shorter exposures, and a better match for one-shot colour cameras and systems faster than f/4.
- Dual and multi-band filters: Pass two or more lines simultaneously for one-shot colour cameras, giving narrowband-like contrast without a filter wheel.
Why Choose David Astro for Narrowband Filters
A filter that is wrong for your focal ratio will underperform in a way that looks like a quality problem but is a specification problem.
- Focal ratio matched: Below roughly f/4 the incident cone shifts a narrow passband off the emission line. We recommend bandwidths or fast-optic designs that account for this.
- Sizing to sensor and wheel geometry: We calculate the filter size needed to avoid vignetting given your sensor diagonal and filter-to-sensor distance.
- Focus offsets explained: Narrowband channels often need per-filter focus offsets, and we help set them up so you are not refocusing manually every filter change.
- Authorized dealer: Genuine filters with verified coatings and full manufacturer warranty, in Canadian stock.
Narrowband Filters in Canada: Frequently Asked Questions
Can I use narrowband with a colour camera?
Yes, most effectively with a dual-band filter that passes Ha and OIII together, since a colour sensor's Bayer array can separate them. Single-line filters work but waste three quarters of the pixels.
Is a 3 nm filter always better than 7 nm?
Not in fast systems. Below about f/4 the steep light cone shifts the passband and a 3 nm filter can lose signal. In an f/6 system under city skies, 3 nm gives noticeably better contrast.
Can I image through a full Moon?
With Ha, largely yes. Moonlight is broadband scattered sunlight, and a narrow Ha filter rejects nearly all of it. OIII suffers more because its wavelength sits closer to the peak of scattered light.
How long should narrowband exposures be?
Longer than broadband, typically 300 to 600 seconds per sub, depending on focal ratio and camera read noise. Total integration for a good narrowband image is usually measured in tens of hours.
Imaging from a light-polluted site?
Tell us your telescope, camera and focal ratio and we will recommend the right bandwidths. Ships from Canada.