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Antlia ALP-T Dual Band Ha&OIII 3nm + SII&Hb 3.5nm 2" Filter Set

by Antlia
SKU ANT-ALP-T-3NM-KIT
Original price CA$1,008.00 - Original price CA$1,008.00
Original price
CA$1,008.00
CA$1,008.00 - CA$1,008.00
Current price CA$1,008.00
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  • Two dual-band filters for four narrowband channels with color cameras; also usable with mono cameras
  • Ha & OIII Filter: 3nm FWHM at 656.3nm and 500.7nm
  • SII & H-beta Filter: 3.5nm FWHM at 672.4nm and 486.1nm
  • Peak Transmission: Up to 90% (Ha/SII), 82% (OIII), and 85% (H-beta)
  • Light Pollution Suppression: ≥OD4.5 blocking from 300-1100nm
  • Best performance with optics slower than f/4
  • Substrate Quality: Lambda/4 transmitted wavefront or better
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  • Description
  • FAQ
  • Specifications
  • In the Box
  • Warranty
  • Antlia ALP-T Dual Band Ha&OIII 3nm + SII&Hb 3.5nm 2" Filter Set

    The Antlia ALP-T Dual Band Filter Set captures four key emission lines, combining a 3nm Ha/OIII filter with a 3.5nm SII/H-beta filter for four-channel narrowband imaging with color cameras. The first filter isolates Hydrogen-alpha at 656.3nm with 90% peak transmission and Oxygen-III at 500.7nm with 82% transmission. The second filter captures Sulfur-II at 672.4nm with 90% transmission and Hydrogen-beta at 486.1nm with 85% transmission. With light-blocking performance of OD4.5 or greater from 300nm to 1100nm, both filters are designed to suppress artificial lighting from Bortle 1 to Bortle 8.

    A 4-Channel Narrowband System for OSC and Mono Cameras

    This filter set is engineered to enable full, four-channel narrowband imaging using a one-shot-color (OSC) camera. By capturing data through each of the two filters sequentially, you can separate the Ha, OIII, SII, and H-beta signals during processing to create detailed false-color images using palettes like SHO or HOHb.

    With a monochrome camera, each filter can be used as a luminance filter to save imaging time. The two lines of one filter are recorded together and cannot be separated afterwards.

    The 3nm Ha/OIII Filter: 90% Peak Transmission at 656.3nm

    The first filter captures the two main emission wavebands, red and blue-green, at the same time. It has a 3nm bandpass (+0.6/-0.1nm) centred on H-alpha (656.3nm) and OIII (500.7nm), with 90% peak transmission for H-alpha and 82% for OIII. The Orion Nebula (M42) and the Veil Nebula are classic targets for these two lines.

    • Hydrogen-alpha (656.3nm): Captures the dominant red emission from ionized hydrogen gas, which forms the structural backbone of most emission nebulae.
    • Oxygen-III (500.7nm): Records the blue-green light from doubly ionized oxygen, often strong in planetary nebulae and supernova remnants.

    The 3.5nm SII/Hb Filter: Capturing Deep Red at 672.4nm

    The second filter provides the remaining two channels for a full narrowband palette, passing Sulfur-II at 672.4nm and Hydrogen-beta at 486.1nm with a 3.5nm bandpass (+/-0.5nm). Including H-beta is a deliberate design choice; while less common than Ha, it can reveal unique structures in certain nebulae that OIII does not. Peak transmission is 90% for SII and 85% for H-beta.

    This combination allows you to create classic S-H-O (Hubble palette) images by assigning the SII, Ha, and OIII channels to the red, green, and blue channels of your final image. H-beta adds palettes such as H-O-Hb and H-S-OHb.

    OD4.5 Blocking from 300nm to 1100nm

    Both filters provide an optical density of OD4.5 or greater across the entire 300nm to 1100nm spectrum outside of their narrow bandpasses. This blocks light pollution, moonlight and airglow and enhances nebula contrast.

    Antlia designed both filters to suppress artificial lighting from Bortle 1 to Bortle 8, for urban or rural use, and says the narrow bands allow longer exposures to capture detailed nebula signal.

    Lambda/4 Substrate and Halo Suppression

    Each filter is built on a single, non-glued optical substrate with a transmitted wavefront of Lambda/4 or better and parallelism of less than 30 arcseconds. Surface quality is 60/40 scratch/dig per MIL-O-13830.

    The filters feature advanced, multi-layer coatings applied using an Ion Gun Assisted Deposition process for durability and consistency. A halo suppression anti-reflective coating minimizes halos and internal reflections. These 2" filters are mounted; Antlia blackens the edges of its unmounted filters.

    Optics Slower than f/4

    Both filters are recommended for optics slower than f/4 for best performance. In faster systems, the steep light cone causes a spectral shift in the filter's bandpass, which can reduce transmission of the target emission line. This is a known trade-off with all narrow-band filters.

    For optics faster than f/4, a pre-shifted highspeed version is a better choice.

  • How do I use the Antlia ALP-T set with my color camera to get separate channels?

    You capture two sets of images, one with the Ha/OIII filter and another with the SII/Hb filter. In post-processing software, you can split the channels from each set. For example, the data from the Ha/OIII filter can be separated to isolate the red pixels (Ha) and the green/blue pixels (OIII). A similar process with the second filter separates SII and Hb, giving you four distinct monochrome images to combine into a false-color master.

    What is the advantage of the SII & H-beta filter in the Antlia ALP-T set?

    While Sulfur-II (SII) is crucial for the popular "Hubble Palette," the inclusion of Hydrogen-beta (H-beta) provides additional data that can reveal structures not visible in OIII. H-beta is the second most common hydrogen emission line after H-alpha and is prominent in certain objects. This gives you more flexibility in processing and can lead to richer, more detailed final images.

    Will the Antlia ALP-T filter set work well with my f/5 refractor?

    Yes. These filters are recommended for optics slower than f/4, and f/5 is within that range.

    Can I use these Antlia filters for visual observation of nebulae like the Orion Nebula (M42)?

    No. Night visual observation is not recommended; these filters are made for imaging with a camera.

    How do the 3nm and 3.5nm bandwidths on the ALP-T filters help in light-polluted skies?

    The narrow bands pass light only close to the emission lines, so most artificial light, moonlight and airglow is blocked (≥OD4.5 from 300nm to 1100nm). Antlia designed the filters for Bortle 1 to Bortle 8 skies.

    What kind of false-color palettes can I create with data from the Antlia ALP-T set?

    With four channels (Ha, OIII, SII, Hb), your options are extensive. Popular choices include:

    • S-H-O (Hubble Palette): Assign SII to Red, Ha to Green, and OIII to Blue.
    • H-O-S: A common variation where Ha is mapped to Red for a more natural look.
    • H-O-Hb: A creative palette that uses H-beta data, which can highlight different structures than SII.
    • H-S-OHb: Another custom combination that blends multiple channels.

    Antlia adds that you can use the narrowband data as a luminance layer to enhance a standard RGB color image of the same object.

    Why does the Antlia Ha&OIII filter have different peak transmission values (90% and 82%)?

    Antlia does not give a reason; 90% at 656.3nm and 82% at 500.7nm are its rated peak transmissions for each line. On a color camera with an RGGB Bayer pattern, OIII falls on twice as many green pixels as there are red pixels for H-alpha.

    Are these Antlia filters safe for solar imaging?

    No. Solar imaging is not recommended. Warning: do not look at the Sun with this filter directly; serious eye damage will result if you fail to observe the warning.

  • Filter Type Dual-band filter set (2 filters)
    Ha&OIII Filter CWL 656.3nm / 500.7nm, FWHM 3nm +0.6/-0.1nm, peak transmission 90% / 82%
    SII&H-beta Filter CWL 672.4nm / 486.1nm, FWHM 3.5nm +0.5/-0.5nm, peak transmission 90% / 85%
    Blocking ≥OD4.5 @ 300-1100nm
    Filter Thickness 2mm +/-0.05mm
    Substrate Optical, single / non-glued substrate
    Surface Quality (S/D) 60/40 (MIL-O-13830)
    Transmitted Wavefront Lambda/4 or better
    Parallelism less than 30 arcsec
    Recommended F-Ratio Slower than f/4 for best performance
    Filter Ring 2" mounted, M48x0.75 thread
    Not Recommended For Solar imaging, night visual observation
    Filter Size 2" mounted
    • Antlia ALP-T Dualband 3nm Ha&OIII filter, 2" mounted

      × 1

    • Antlia ALP-T Dualband 3.5nm SII&H-beta filter, 2" mounted

      × 1

    • Protective case

      × 2

  • Contact us for warranty details.