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IMPORTANT: Our store is located in Canada. All orders that include products manufactured outside of Canada or USA will be subject to tariffs and duties, regardless of the order value. US customers are responsible for all applicable duties and tariffs, and those will be billed by the carrier, except for the Lacerta upgrade kit, for which we collect them at checkout.

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Optolong Ha 7nm, OIII 6.5nm & SII 6.5nm Filter Set

par Optolong
UGC OPT-SHO-1.25
Prix d'origine $465.00 - Prix d'origine $669.00
Prix d'origine
$465.00
$465.00 - $669.00
Prix actuel $465.00
Égalisation de prix!
  • H-alpha Filter: 7nm Bandpass centered at 656nm
  • Oxygen-III Filter: 6.5nm Bandpass centered at 500nm
  • Sulphur-II Filter: 6.5nm Bandpass
  • Hubble Palette Ready: Complete SHO set for tri-band narrowband imaging
  • Format Options: Available in 1.25" Mounted, 2" Mounted, or 36mm Unmounted versions
En rupture temporaire
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  • Description
  • FAQ
  • Specifications
  • In the Box
  • Warranty
  • Optolong Ha 7nm, OIII 6.5nm & SII 6.5nm Filter Set

    The Optolong Ha 7nm, OIII 6.5nm & SII 6.5nm Filter Set provides the three essential filters for creating high-contrast Hubble Palette images from light-polluted skies. This trio isolates the key emission lines from nebulae—Hydrogen-alpha at 656nm, Oxygen-III at 500nm, and Sulphur-II—with tight 7nm and 6.5nm bandpasses that reject unwanted skyglow and artificial light sources.

    The Hubble Palette: 6.5nm/7nm Tri-Band Narrowband Imaging

    This filter set is engineered specifically for SHO imaging, where data from the Sulphur-II, Hydrogen-alpha, and Oxygen-III filters are mapped to the red, green, and blue channels of a final image. This technique, made famous by the Hubble Space Telescope, reveals incredible structural detail and color separation in emission nebulae like the Rosette Nebula (Caldwell 49) that are impossible to capture in broadband.

    Designed for use with monochrome astronomy cameras or modified DSLRs, each filter isolates a specific emission line, allowing you to capture deep, high-contrast data one channel at a time, even under a bright moon or from a city backyard.

    Precision Bandpasses: 7nm Ha, 6.5nm OIII, and 6.5nm SII

    The effectiveness of a narrowband filter is defined by its bandpass—the narrower, the better the contrast. The 7nm Ha filter captures the dominant 656nm wavelength present in nearly all emission nebulae. The even tighter 6.5nm bandpasses on the OIII and SII filters aggressively reject light pollution and background star signal, making faint nebular structures stand out dramatically.

    • H-Alpha (7nm): Reveals the foundational hydrogen structure of nebulae with maximum signal.
    • OIII (6.5nm): Isolates the 500nm blue-green light characteristic of planetary nebulae and supernova remnants, providing crucial detail and color contrast.
    • SII (6.5nm): Captures the deep red light from ionized sulfur, often tracing shock fronts and dense regions that differ from the Ha data.

    Advanced Coatings for 1.25", 2", and 36mm Formats

    Optolong utilizes an advanced ion-assisted deposition coating process across all filter sizes, ensuring durability and scratch resistance. This technology also provides a stable central wavelength (CWL) that does not drift with temperature changes during an imaging session, preventing signal loss.

    This meticulous manufacturing process results in excellent transmission at the target wavelengths and high optical density outside the passband. The coatings are engineered to significantly reduce halos around bright stars, a common issue in narrowband imaging, particularly noticeable in the improved OIII filter performance.

    Optolong 6.5nm/7nm SHO Set vs. Wider Narrowband Filters

    While wider filters, such as 12nm variants, can be a more forgiving starting point, the Optolong 6.5nm/7nm set offers a significant step up in imaging capability. The primary advantage of the tighter bandpass is superior contrast and the ability to resolve finer nebular details.

    The trade-off is that these filters require longer individual sub-exposure times to gather the same amount of signal as a wider filter. However, because they reject so much more background noise, the final integrated image achieves a much higher signal-to-noise ratio, producing cleaner, sharper, and more detailed results from any location.

  • What is the "Hubble Palette" and why do I need this Optolong SHO filter set for it?

    The "Hubble Palette" is an imaging technique where narrowband data is mapped to RGB channels to create false-color images with dramatic detail and contrast. This Optolong SHO set provides the three required filters: Sulphur-II (mapped to Red), Hydrogen-alpha (Green), and Oxygen-III (Blue), allowing you to produce these iconic images.

    Can I use the Optolong Ha 7nm, OIII 6.5nm & SII 6.5nm filters with my color camera?

    While technically possible, it is highly inefficient. These filters are designed for monochrome cameras. A color camera's Bayer matrix blocks roughly 2/3 of the incoming light for any given filter, requiring much longer exposures and producing lower-quality results. For color cameras, a multi-bandpass filter (like the L-eNhance or L-eXtreme) is a better choice.

    How will the Optolong 6.5nm OIII filter perform on the Orion Nebula (M42) from my city backyard?

    The Optolong 6.5nm OIII filter will excel on the Orion Nebula (M42) from a light-polluted location. Its tight 6.5nm bandpass will darken the sky background significantly, dramatically increasing the contrast of the delicate, wispy structures in the nebula's core and outer regions, which are rich in Oxygen-III emissions.

    What's the main benefit of using the Optolong 7nm Ha filter on the Rosette Nebula (Caldwell 49) with my monochrome camera?

    The primary benefit is immense contrast. The Rosette Nebula (Caldwell 49) is a massive cloud of hydrogen. The Optolong 7nm Ha filter isolates its dominant 656nm emission line, rejecting moonlight, skyglow, and broadband light from stars. This allows your monochrome camera to record deep, detailed structural information of the nebula itself, separate from the background.

    Why is the Ha filter in this Optolong set 7nm while the OIII and SII are 6.5nm?

    Hydrogen-alpha is typically the strongest signal in most emission nebulae. The slightly wider 7nm bandpass for the Ha filter ensures maximum signal capture for this critical channel. The OIII and SII signals are often weaker, so the tighter 6.5nm bandpass is used to maximize contrast by more aggressively rejecting background light pollution and skyglow, improving the signal-to-noise ratio for these fainter details.

    Do these Optolong narrowband filters require longer exposure times than LRGB filters?

    Yes, significantly longer. LRGB filters have very wide bandpasses to capture as much light as possible. The Optolong narrowband filters in this set have extremely narrow 6.5nm and 7nm bandpasses. While this is key to their high-contrast performance, it means individual sub-exposures must be much longer (typically 3-10 minutes or more) to achieve a strong signal.

  • Filter Set H-alpha, OIII, SII
    H-Alpha Bandpass 7nm
    H-Alpha Central Wavelength 656nm
    OIII Bandpass 6.5nm
    OIII Central Wavelength 500nm
    SII Bandpass 6.5nm
    Available Sizes 1.25" Mounted, 2" Mounted, 36mm Round Unmounted
    Coating Technology Ion-assisted deposition
    • H-Alpha 7nm Filter

      × 1

    • OIII 6.5nm Filter

      × 1

    • SII 6.5nm Filter

      × 1

  • Optolong 3-Year Warranty