Imaging Filters
Not every imaging filter is narrowband or LRGB. Ultraviolet and infrared cut filters, luminance filters, methane band filters for planetary work and dedicated infrared pass filters each solve a specific problem, and several of them are more useful than their obscurity suggests. David Astro carries imaging filters in Canada, in Canadian inventory and shipped domestically.
These filters address particular situations rather than general imaging. Tell us what problem you are seeing and we will say whether one of them fixes it.
Filters
Baader Planetarium O-III Super-G Filter (9nm) – CMOS-optimized
9nm O-III Narrowband Passband Functions as a "Super-G" Green Filter Replacement CMOS-Optimized Coatings for High Contrast Reduces Impact of Atmosp...
View full detailsBaader Planetarium RGB B-Filter – CMOS-optimized
Available in 1.25" & 2" Mounted, Round Unmounted and Square Sizes Blue (B) Channel for LRGB Imaging Optimized for Modern CMOS Sensors Designed...
View full detailsBaader Planetarium RGB Filter Set – CMOS-optimized
Set of three Red, Green, and Blue (RGB) filters Optimized for modern CMOS sensors to eliminate reflections Available in 1.25" & 2" mounted, 31...
View full detailsBaader Planetarium RGB G-Filter – CMOS-optimized
Green (G) Component for LRGB Color Imaging Available in 1.25" & 2" Mounted, Round Unmounted and Square Sizes Optimized for Modern CMOS Sensors...
View full detailsBaader Planetarium RGB R-Filter – CMOS-optimized
Red (R) filter for LRGB astrophotography Available in 1.25" & 2" mounted, round unmounted and square sizes Optimized for modern CMOS sensors H...
View full detailsBaader Planetarium S-II f/2 Highspeed-Filter (6.5nm) – CMOS-optimized
6.5nm Sulfur-II Narrowband Filter Optimized for f/2 High-Speed Optical Systems Available in 1.25" & 2" Mounted, 31mm, 36mm, 50.4mm & 2" FC...
View full detailsBaader Planetarium S-II f/2 Ultra-Highspeed-Filter (4nm) – CMOS-optimized
4nm FWHM Bandpass for Sulfur-II (S-II) Engineered for f/2 Ultra-Highspeed Optical Systems Available in 1.25" & 2" Mounted, 31mm, 36mm, 50.4mm ...
View full detailsBaader Planetarium S-II f/3 Ultra-Highspeed-Filter (4nm) – CMOS-optimized
4nm Bandwidth (FWHM) Pre-Shifted for Fast f/3 Optical Systems Available in 1.25" & 2" Mounted, 31mm, 36mm & 50.4mm Unmounted Round, and 50...
View full detailsBaader Planetarium S-II Ultra-Narrowband-Filter (4nm) – CMOS-optimized
4nm Full-Width Half-Maximum (FWHM) Bandpass Optimized for Modern CMOS Sensors Available in 1.25" (M28.5 x 0.6) & 2" Mounted, 31mm, 36mm & ...
View full detailsBaader Planetarium UHC-L / Ultra-L-Booster Filter 65x65mm
65x65mm Unmounted Square Format Optimized for LED Light Pollution Rejection High-Contrast Views of Emission Nebulae Ideal Complement to Narrowband...
View full detailsBaader Planetarium UV/IR-Cut / L-Filter – CMOS-optimized
Serves as a high-transmission Luminance (L) filter Provides complete Ultraviolet (UV) and Infrared (IR) blocking Engineered with CMOS-optimized an...
View full detailsBaader Semi-APO Filter
Reduces chromatic aberration in achromatic refractors Enhances contrast on the Moon, planets, and bright stars Improves star sharpness by tighteni...
View full detailsBaader UHC-S/L-Booster Filter - CMOS-Optimized
Targets modern LED and broadband light pollution Optimized blue transmission to reject artificial skyglow Serves as a "pre-filter" for finding obj...
View full detailsBaader UV/IR-CUT / L-Filter CMOS Optimized
Blocks unwanted UV and IR wavelengths for sharper stars Optimized for modern CMOS sensors to prevent star bloat Serves as a high-transmission Lumi...
View full detailsCelestron UHC/LPR Filter - 1.25"
Selectively blocks mercury vapor, sodium vapor, and natural sky glow Achieves over 97% transmission of critical nebula emission lines Features a m...
View full detailsCelestron UHC/LPR Filter - 2"
Selectively blocks light pollution from mercury and sodium vapor lights Achieves over 97% light transmission for maximum brightness 60nm bandpass ...
View full detailsChroma B-Bessel Filter
Blue photometric filter in UVBRI series Filters designed for use with CCD and for f/4.0 or slower No reflections leading to image distortions or ""...
View full detailsChroma Blue Filter
Blue filter for color rendering with RGB set Filters designed for use with CCD and for f/4.0 or slower No reflections leading to image distortions ...
View full detailsChroma Clear Filter
Filters designed for use with CCD and for f/4.0 or slower No reflections leading to image distortions or "back reflections" Transmitted wavefront ...
View full detailsChroma Green Filter
Green filter for color rendering with RGB set Filters designed for use with CCD and for f/4.0 or slower No reflections leading to image distortions...
View full detailsChroma H-alpha Filter - 3nm
H-alpha filters are essential for imaging nebulae and other objects which are rich in ionized hydrogen. At 656.3nm, a narrow-band emission filter i...
View full detailsChroma H-alpha Filter - 5nm
H-alpha filters are essential for imaging nebulae and other objects which are rich in ionized hydrogen. At 656.3nm, a narrow-band emission filter i...
View full detailsChroma H-alpha Filter - 8nm
H-alpha filters are essential for imaging nebulae and other objects which are rich in ionized hydrogen. At 656.3nm, a narrow-band emission filter i...
View full detailsChroma H-alpha Filter Optimized for f/3 - 3nm
H-alpha filters are essential for imaging nebulae and other objects which are rich in ionized hydrogen. At 656.3nm, a narrow-band emission filter i...
View full detailsSpecialist Imaging Filters
Each of these targets a specific defect or a specific wavelength range that general-purpose filters do not address.
- UV and IR cut filters: Essential with refractors, which do not focus infrared at the same point as visible light. Without one, stars are bloated and soft in a way that looks like poor optics.
- Luminance filters: A broad visible-range filter with UV and IR blocking, used as the detail-carrying channel in LRGB imaging.
- Infrared pass filters: Pass only infrared, which cuts through atmospheric turbulence better than visible light and can sharpen planetary detail in poor seeing.
- Methane band filters: Very narrow filters at 889 nm revealing atmospheric structure on Jupiter, Saturn and the ice giants that is invisible in visible light.
- Continuum filters: Narrow green-band filters used for lunar and planetary imaging, reducing the effect of atmospheric dispersion.
- Anti-halation and reflection considerations: Coating quality matters here too, since a filter close to the sensor can produce reflection artifacts around bright objects.
Why Choose David Astro for Imaging Filters
These are problem-specific purchases, and the first question is whether you have the problem.
- Diagnosis before recommendation: Send us a sample image and we will tell you whether bloated stars are an infrared problem, a spacing problem or a focus problem.
- Refractor advice: If you image with a doublet and have no UV/IR cut filter, that is very often the cause of soft bright stars, and it is the cheapest fix in imaging.
- Seeing-based advice: We will explain when an infrared pass filter genuinely helps planetary work and when it simply costs you resolution.
- Authorized dealer: Genuine filters with verified coatings and manufacturer warranty, in Canadian stock.
- Ships from Canada: No duties or brokerage fees for Canadian buyers.
Imaging Filters in Canada — Frequently Asked Questions
- Do I need a UV/IR cut filter?
- With any refractor, yes. ED doublets and even triplets do not bring infrared to the same focus as visible light, and an unfiltered sensor records that as bloated, soft stars.
- Does an infrared filter help with bad seeing?
- For planetary imaging, often yes. Longer wavelengths are less affected by atmospheric turbulence, so an IR pass filter can produce sharper results on a poor night, at the cost of some resolution.
- What is a methane band filter for?
- It isolates a methane absorption band at 889 nm, revealing cloud structure on the gas giants that is invisible in visible light. It is a specialist filter needing substantial aperture and long exposures.
- Why are my bright stars bloated?
- Most commonly unblocked infrared in a refractor, sometimes filter reflections, sometimes back-focus error. Send us a crop and we will tell you which.
Diagnosing an imaging problem?
Send us a sample crop and we will tell you what will actually fix it. Held in Canada, shipped fast.