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Askar 3nm Colour Magic Ultra OIII/SII E2 Filter - 2"

by Askar
SKU ASK-ASKAR2DBE2
Original price CA$847.00 - Original price CA$847.00
Original price
CA$847.00
CA$847.00 - CA$847.00
Current price CA$847.00
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  • Dual-bandpass design captures OIII (500.7nm) and SII (672nm) simultaneously
  • Narrow 3.7nm (OIII) and 4.0nm (SII) FWHM for high-contrast imaging
  • Peak transmittance of 85% ensures high signal throughput
  • Deep ≥OD5 blocking from 200-1100nm eliminates unwanted light pollution
  • Standard 2" filter format with 1.85mm substrate thickness
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  • Description
  • FAQ
  • Specifications
  • In the Box
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  • Askar 3nm Colour Magic Ultra OIII/SII E2 Filter - 2"

    The Askar 3nm Colour Magic Ultra OIII/SII E2 Filter is engineered to solve a common problem for color camera imagers: capturing the full Hubble Palette. This dual-bandpass filter isolates nebula emissions at 500.7nm (OIII) and 672nm (SII) with narrow 3.7nm and 4.0nm bandpasses, respectively. With a peak transmittance of 85% and deep OD5 blocking across the 200-1100nm spectrum, this filter allows you to gather the missing Sulfur-II data needed for SHO compositions, even from light-polluted locations.

    The 672nm + 500.7nm Solution for Color Camera SHO Imaging

    While standard duo-narrowband filters for color cameras typically capture Hydrogen-alpha and Oxygen-III, they leave out the critical Sulfur-II signal. The Askar Ultra E2 filter is designed specifically to fill this gap. By passing light at 672nm (SII) and 500.7nm (OIII), it allows you to collect the remaining two channels for a full SHO dataset without a filter wheel or monochrome camera.

    Combine the data from this filter with Hydrogen-alpha data (captured separately or with an Hα/OIII filter) to unlock vibrant, detailed SHO images. This approach makes the celebrated Hubble Palette accessible and efficient for anyone using a one-shot-color astronomy camera.

    3.7nm & 4.0nm Bandpasses for Maximum Contrast

    This filter achieves its high contrast through extremely narrow full-width at half-maximum (FWHM) values: 3.7nm for OIII and 4.0nm for SII. These tight bandpasses aggressively reject streetlights, moonlight, and natural skyglow, causing faint nebula structures to stand out against a dark background. The ≥OD5 blocking from 200nm to 1100nm ensures no out-of-band wavelengths contaminate the image.

    • Peak Transmittance (85%): Despite the narrow bandpasses, the filter allows 85% of the crucial OIII and SII light to reach your sensor, preventing excessively long exposure times.
    • Halo Control: As part of Askar's "Ultra" series, this filter is optimized to minimize halos around bright stars, a common issue with narrowband filters.
    • Precision Substrate: The filter is built on a glass substrate with a parallelism of 30 arcseconds, maintaining the sharpness of your optical system.
  • What is the primary purpose of the Askar Ultra E2 OIII/SII filter?

    The Askar Ultra E2 is a specialized dual-narrowband filter designed for color camera users who want to capture images in the Hubble Palette (SHO). It isolates the Oxygen-III (OIII) and Sulfur-II (SII) emission lines, allowing you to collect the "S" and "O" channels to complement your Hydrogen-alpha ("H") data.

    How do I create an SHO image with the Askar Ultra E2 and a color camera?

    You will need to capture two sets of images. First, use a filter that passes Hydrogen-alpha (like an L-eXtreme, L-eNhance, or a dedicated Hα filter) to get your "H" data. Second, use this Askar Ultra E2 filter to capture your "S" and "O" data simultaneously. In post-processing, you will split the channels from both images and combine them using a tool like PixInsight's ChannelCombination to assign Hα to Red, SII to Green, and OIII to Blue (or any variation you prefer).

    Can I use the Askar Ultra E2 filter with a monochrome camera?

    While it is designed for color cameras, you can use it with a monochrome camera. However, because it passes both OIII and SII light at the same time, you cannot separate the two signals onto the mono sensor. For monochrome imaging, using individual OIII and SII filters is the standard and more flexible approach.

    Why does the Askar Ultra E2 filter have 3.7nm and 4.0nm bandpasses instead of just "3nm"?

    The "3nm" is a class or series designation. The actual measured FWHM is 3.7nm ± 0.3nm for OIII and 4.0nm ± 0.3nm for SII. These precise, ultra-narrow bandpasses are what provide the exceptional contrast and light pollution rejection by isolating the specific nebula emission lines from background skyglow.

    How would the Askar Ultra E2 filter perform on the Wizard Nebula (NGC 7380) from a city?

    The Wizard Nebula (NGC 7380) is rich in all three SHO gasses. From a city, the Askar Ultra E2 filter's narrow 3.7nm/4.0nm bandpasses would be highly effective at cutting through light pollution to reveal the intricate structures in the OIII and SII regions. It would darken the sky background significantly, increasing the contrast and making the faint nebulosity visible in your exposures.

    Will the Askar Ultra E2 filter work well with my fast f/4 telescope?

    Ultra-narrowband filters like this one can experience some band-shifting with very fast optical systems (typically f/4 and below). While it will still provide a significant contrast boost, you may see a slight reduction in transmission compared to its peak 85% rating. The filter's performance is optimal for systems at f/4.5 and slower, but it remains a powerful tool for light pollution suppression even on faster scopes.

  • FWHM (OIII) 3.7nm ± 0.3nm
    FWHM (SII) 4.0nm ± 0.3nm
    Center Wavelength (CWL) 500.7nm (OIII) & 672nm (SII)
    Peak Transmittance 85%
    Blocking Property ≥OD5 @ 200-1100nm
    Substrate Thickness 1.85 ± 0.05mm
    Surface Finish 60/40
    Parallelism 30″
    • Askar 3nm Colour Magic Ultra OIII/SII E2 Filter - 2"

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  • Askar 1-Year Warranty