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Askar Colour Magic SII/OIII C2 Filter - 2"

by Askar
SKU ASK-ASKAR2DBC2
Original price CA$167.00 - Original price CA$167.00
Original price
CA$167.00
CA$167.00 - CA$167.00
Current price CA$167.00
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  • Dual-band filter passing SⅡ (672nm) and OIII (500.7nm) emission lines
  • Designed for one-shot-color cameras to capture data often missed by Hα/OIII filters
  • 15nm±3nm bandpass for the Sulfur-II (SⅡ) line
  • 35nm±5nm bandpass for the Oxygen-III (OIII) line
  • 90% peak transmittance for high signal-to-noise ratio
  • OD3 blocking from 200-1000nm suppresses light pollution and unwanted signal
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  • Description
  • FAQ
  • Specifications
  • In the Box
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  • Askar Colour Magic SII/OIII C2 Filter - 2"

    The Askar Colour Magic C2 2" filter isolates the Sulfur-II and Oxygen-III emission lines, capturing the "missing" SⅡ channel for one-shot-color camera users. With a tight 15nm±3nm bandpass at 672nm for SⅡ and a wider 35nm±5nm bandpass at 500.7nm for OIII, it achieves over 90% peak transmittance on these critical wavelengths. This design allows you to gather data for full SHO (Hubble Palette) style images without switching to a monochrome camera and filter wheel.

    The "Missing Channel" Solution: Adding SⅡ Data to Color Images

    Most duo-band filters for color cameras focus on Hydrogen-alpha and Oxygen-III, leaving out the crucial Sulfur-II signal that reveals unique structures in many emission nebulae. The Askar Colour Magic C2 filter is engineered specifically to fill this gap. By capturing SⅡ and OIII simultaneously, it provides the data needed to complement your existing Hα/OIII images, unlocking the ability to create full tricolor narrowband composites with a single color camera.

    Asymmetrical Design: 15nm SⅡ and 35nm OIII Bandpasses

    The filter features two different bandpasses to optimize signal capture for each emission line. The tighter 15nm±3nm FWHM for the SⅡ line provides excellent contrast and aggressively rejects light pollution for this often-fainter signal. The broader 35nm±5nm FWHM for OIII allows for greater light collection on this typically stronger signal, which is beneficial for reducing exposure times while still offering a significant improvement over broadband filters.

    90% Peak Transmittance for Maximum Contrast

    Achieving over 90% peak transmittance at the 672nm and 500.7nm center wavelengths ensures that the maximum amount of valuable nebula light reaches your sensor. Combined with strong out-of-band blocking rated at OD3 from 200-1000nm, the C2 filter darkens the sky background significantly, even under moderately light-polluted skies. This high transmission and strong blocking work together to dramatically increase image contrast, making faint details in targets like the Trifid Nebula (M20) or the Eagle Nebula (M16) stand out clearly.

  • Why use the Askar C2 SⅡ/OIII filter instead of a standard Hα/OIII filter?

    The Askar C2 is not a replacement for an Hα/OIII filter; it's a complement. Standard duo-band filters capture Hα and OIII. The C2 filter captures SⅡ and OIII, providing the third channel of data necessary for creating Hubble Palette (SHO) images with a color camera. You use both filters to acquire all three datasets.

    How do I combine data from the Askar C2 filter with my other images?

    After capturing separate images with your Hα/OIII filter and the Askar C2 SⅡ/OIII filter, you would use image processing software like PixInsight or Photoshop. You can split the channels from each image to isolate the Hα, SⅡ, and OIII data, and then combine them into a single color image by assigning each signal to the Red, Green, and Blue channels as desired.

    Is the 35nm bandpass on the OIII channel of the Askar C2 filter wide enough for my light-polluted skies?

    A 35nm bandpass provides a good balance between light pollution suppression and signal strength. While not as restrictive as a 3nm or 7nm filter, it is significantly better than a broadband filter and is effective in most suburban environments. The key benefit is shorter exposure times compared to ultra-narrowband filters, which can be an advantage for many imagers.

    What types of celestial objects benefit most from the Askar C2 SⅡ/OIII filter?

    Emission nebulae with distinct regions of Sulfur-II emission are ideal targets. Objects like the Eagle Nebula (M16), the Trifid Nebula (M20), and the Rosette Nebula (NGC 2237) show dramatic structural differences when SⅡ data is included, allowing for the creation of vibrant and detailed Hubble Palette images.

    Can I use the Askar C2 SⅡ/OIII filter with a monochrome camera?

    While technically possible, it's not the intended use. With a monochrome camera, the sensor would capture both SⅡ and OIII light simultaneously, and you would not be able to separate them. For monochrome imaging, it is always better to use individual SⅡ and OIII single-bandpass filters to capture clean, isolated data for each channel.

    Why are the bandpasses different for SⅡ (15nm) and OIII (35nm) on the Askar C2 filter?

    This is a deliberate design choice to optimize performance. The SⅡ signal is often weaker, so a tighter 15nm bandpass is used to increase contrast and reject more background light. The OIII signal is typically stronger, so a wider 35nm bandpass allows more of this signal to be collected, reducing exposure times without sacrificing too much contrast.

  • Filter Type Dual-Band Narrowband
    Size 2" Mounted
    Center Wavelength (CWL) 500.7nm (OIII) & 672nm (SⅡ)
    Full Width Half-Max (FWHM) OIII: 35nm ±5nm / SⅡ: 15nm ±3nm
    Peak Transmittance >90%
    Blocking Range OD3 (0.1%) @ 200-1000nm
    Glass Thickness 2mm ± 0.05mm
    Surface Finish 60/40
    • Askar Colour Magic C2 SII/OIII Filter - 2"

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    • Protective Case

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  • Askar 1-Year Warranty