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Baader Planetarium S-II Ultra-Narrowband-Filter (4nm) – CMOS-optimized

SKU BAA-2961475
Original price CA$389.00 - Original price CA$827.00
Original price
CA$389.00
CA$389.00 - CA$827.00
Current price CA$389.00
Price Match Policy!
  • 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 & 50.4mm Unmounted Round, and 50x50mm & 65x65mm Square Sizes
  • Isolates the Sulfur-II (S-II) Emission Line
  • Reflex-Blocker™ Hard-Coated and Polished
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  • Description
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  • Baader S-II Ultra-Narrowband-Filter (4nm) – CMOS-optimized

    The Baader S-II Ultra-Narrowband Filter isolates the critical 672.4nm Sulfur-II emission line with an extremely tight 4nm bandpass. Specifically engineered for modern CMOS sensors, it leverages its 4nm FWHM to deliver maximum contrast against light pollution and the moonlit sky, revealing faint, intricate details in emission nebulae that wider filters miss. It is available as a mounted 1.25" or 2" filter, as unmounted 31mm, 36mm and 50.4mm rounds for filter wheels, and as 50x50mm and 65x65mm squares for large-format sensors.

    The 4nm Advantage: Maximum Contrast on S-II Structures

    By restricting the incoming light to a mere 4nm sliver of the spectrum centered on the S-II line, this filter darkens the sky background to an almost pure black. This dramatic increase in contrast allows the faint, wispy structures of distant H-II regions and planetary nebulae to stand out with striking clarity, even from suburban locations.

    CMOS-Optimized Design: Eliminating Halos and Reflections

    Modern CMOS sensors are highly reflective, causing halos and internal reflections with traditional filters. Baader's CMOS-optimized design incorporates advanced Reflex-Blocker™ coatings and steep optical slopes to virtually eliminate these artifacts. The result is clean, high-fidelity data with tight, halo-free stars, even on the brightest targets in the field.

    S-II for the Hubble Palette: Capturing the Soul of H-II Regions

    The Sulfur-II signal is a crucial component of the "Hubble Palette" (SHO), a false-color imaging technique that assigns S-II, H-alpha, and O-III data to the red, green, and blue channels respectively. Every size of this 4nm filter provides the high-contrast S-II data needed to create vibrant, detailed images of iconic targets like the Pillars of Creation in the Eagle Nebula (M16) or the core of the Lagoon Nebula (M8).

    Baader 4nm vs. 7nm Filters: The Trade-Off Between Signal and Contrast

    Choosing between a 4nm and a wider 7nm filter involves a direct trade-off. While the 4nm filter provides superior contrast and background suppression, it requires longer exposure times to gather the same amount of signal as a 7nm filter.

    • Baader 4nm S-II: The ideal choice for heavily light-polluted skies or during bright moon phases, where maximizing contrast is the primary goal. It excels at separating fine details from the background glow.
    • Wider 7nm Filters: A better option for dark-sky sites or when using very fast optical systems, where collecting signal photons quickly is more important and the background is already dark. They are also more forgiving of band-shift effects in very fast optical systems.
  • What does "CMOS-optimized" mean for the Baader 4nm S-II filter?

    It means the filter is specifically designed to suppress reflections and halos that occur when using highly reflective modern CMOS sensors. Baader uses proprietary Reflex-Blocker™ coatings and carefully designed dielectric layers with steep edges to prevent internal reflections between the filter and the sensor, resulting in cleaner data and tighter stars.

    How does the 4nm bandpass on the Baader S-II filter improve my images?

    The ultra-narrow 4nm bandpass provides a significant increase in contrast compared to wider 6.5nm or 7nm filters. It more effectively blocks out light pollution, moonlight, and natural skyglow, making faint nebular details stand out more prominently against a darker background. This is especially beneficial when imaging from urban or suburban locations.

    What is the main benefit of the Baader 4nm S-II filter for Hubble Palette (SHO) imaging?

    In Hubble Palette imaging, the S-II signal is typically assigned to the red channel. The high-contrast data captured by the Baader 4nm S-II filter ensures that the structural details within emission nebulae, like the wispy filaments in the Veil Nebula (NGC 6960), are sharply defined. This clean S-II data is essential for producing vibrant and detailed false-color composites.

    Is the Baader 4nm S-II filter parfocal with other Baader filters?

    Baader engineers their CMOS-optimized filters to be parfocal, meaning you should not have to significantly refocus when switching between different filters in the same series (e.g., H-alpha, O-III, S-II). This saves valuable imaging time by minimizing the need for autofocus routines after each filter change.

    How will the Baader 4nm S-II filter perform on the Heart Nebula (IC 1805) from a light-polluted suburb?

    This is an ideal scenario for the Baader 4nm S-II filter. The Heart Nebula has extensive S-II regions, but they can be washed out by suburban skyglow. The filter's tight 4nm bandpass will reject the vast majority of this light pollution, allowing you to capture the delicate structures and gradients within the nebula with much longer sub-exposures than would otherwise be possible.

    Which size of the Baader 4nm S-II filter should I choose?

    Match the size to your filter wheel and sensor. The mounted 1.25" (M28.5 x 0.6 thread) and 2" filters suit standard 1.25" and 2" filter wheels and holders. The unmounted 31mm size fits wheels from makers like ZWO, QHY and Atik and is generally recommended for sensors up to APS-C; 36mm unmounted filters fit wheels made for that size. For full-frame sensors, choose the 50.4mm round or 50x50mm square format, while the 65x65mm square is designed for large, professional filter wheels and the largest sensors.

  • 1.25" Round Mounted

    Product Name Baader S-II 1.25" Ultra-Narrowband-Filter (4nm) – CMOS-optimized
    Filter Size 1.25"
    Filter Type Ultra-Narrowband
    Bandpass (FWHM) 4nm
    Target Wavelength Sulfur-II (S-II) at 672.4nm
    Sensor Compatibility CMOS Optimized
    Threads M28.5 x 0.6

    2" Round Mounted

    Filter Type Ultra-Narrowband S-II
    Bandwidth 4nm
    Size 2" Mounted
    Sensor Optimization CMOS

    31mm Round Unmounted Filter

    Filter Type Ultra-Narrowband
    Wavelength Sulfur-II (S-II)
    Bandpass (FWHM) 4nm
    Size 31mm
    Mounting Unmounted
    Sensor Compatibility CMOS-optimized

    36mm Round Unmounted Filter

    Filter Type Ultra-Narrowband
    Emission Line S-II (Sulfur-II) at 672.4nm
    Bandwidth (FWHM) 4nm
    Size 36 mm
    Format Unmounted
    Coatings CMOS-optimized, Anti-Reflection
    Substrate Optically Polished Glass

    50.4mm Round Unmounted Filter

    Filter Type Ultra-Narrowband S-II
    Bandpass 4nm
    Central Wavelength 672.4nm
    Size 50.4mm
    Format Unmounted, Round
    Optimization CMOS Sensors
    Coatings Reflex-Blocker™ Hard Coatings
    Polish Planeoptically Polished

    50x50mm Square Filter

    Filter Type Ultra-Narrowband Interference Filter
    Wavelength Sulfur-II (S-II)
    Bandpass (FWHM) 4nm
    Size 50mm x 50mm
    Mounting Unmounted
    Sensor Compatibility CMOS-optimized

    65x65mm Square Filter

    Filter Type Ultra-Narrowband
    Emission Line Sulfur-II (S-II)
    Bandpass (FWHM) 4nm
    Size 65 x 65mm
    Format Unmounted, Square
    Sensor Compatibility CMOS-optimized
    Coatings Reflex-Blocker™ Hard Coatings
    Polish Planeoptically Polished
  • Baader Planetarium Warranty