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Antlia H-alpha 2.5nm Ultra Narrowband Filter

par Antlia
UGC ANT-HA-2.5NM-RD36
Prix d'origine $465.00 - Prix d'origine $590.00
Prix d'origine
$465.00
$465.00 - $590.00
Prix actuel $465.00
Égalisation de prix!
  • Isolates the H-alpha emission line at 656.3nm
  • Ultra-narrow 2.5nm FWHM bandpass to maximize contrast
  • Peak transmission of 95% or greater
  • Deep >=OD5 (0.001%) blocking of off-band wavelengths
  • Recommended for optical systems f/3.5 or slower
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  • Description
  • FAQ
  • Specifications
  • In the Box
  • Warranty
  • Antlia H-alpha 2.5nm Ultra Narrowband Filter

    The Antlia H-alpha 2.5nm Ultra Narrowband Filter maximizes contrast by isolating the 656.3nm emission line with a narrow 2.5nm (+0.3/-0.1nm) full width at half maximum (FWHM). With a peak transmission of 95% or greater and out-of-band blocking rated at OD5 (0.001%), this filter gives an exceptionally high signal-to-noise ratio for deep sky imaging. Built on a 2mm thick, double-sided fine polished quartz glass substrate, it offers excellent thermal stability, and its thickness is identical to existing standards with care for parfocality.

    Ultra-Narrow 2.5nm Bandpass: 95% or Greater Transmission for Maximum Contrast

    By restricting the bandpass to just 2.5nm, this filter blocks light outside the H-alpha line, including much of the light from light pollution and the Moon. This darkens the sky background, allowing the faint, hydrogen-rich structures within nebulae to stand out. With a specified peak transmission of at least 95% at the 656.3nm H-alpha line, the signal from your target passes through efficiently while unwanted light is blocked.

    Recommended for f/3.5 or Slower: Flat-Top Spectrum and OD5 Blocking

    Antlia recommends the 2.5nm Ultra series for optics with a focal ratio of f/3.5 or slower for best optical performance. Its flat-top spectral profile minimizes the loss in transmission caused by the central wavelength shift that occurs in converging light cones. Out-of-band blocking of OD5 or greater (0.001%) blocks interference from other wavelengths and minimizes halos around bright stars.

    Quartz Substrate Construction: 2mm Thick for Thermal Stability and Parfocality

    The 2.5nm Ultra series is built on a quartz glass substrate. Quartz has an ultra-low coefficient of thermal expansion with outstanding thermal and mechanical properties. Each filter is double-sided fine polished to a 2mm thickness, identical to existing filter standards, with utmost care for parfocality.

    • Edge-Blackened: All filters are coated to the edge of the substrate, and unmounted filters are edge blackened to eliminate internal reflections from stray light.
    • Individual Scans: Every filter is 100% scanned and comes with its actual measured spectrum, transmission and blocking (OD) data.

    Antlia 2.5nm Ultra vs. 3nm Pro: Why a Quartz Substrate Matters

    Compared with Antlia's 3nm Pro series, the 2.5nm Ultra series filters coated on quartz glass have higher transmittance for the emission lines and a narrower FWHM. Antlia estimates these filters improve signal by 20-30% in your images.

    • Signal-to-Noise Ratio: The tighter 2.5nm bandpass of the Ultra series provides a higher signal-to-noise ratio, further suppressing background light for deeper exposures.
    • Thermal Stability: The quartz substrate has an ultra-low thermal expansion coefficient, while the 3nm Pro series uses an optical glass substrate.
    • Durability: Quartz offers better fracture and scratch resistance, and improved coating resilience to cleaning.
  • What makes the Antlia H-alpha 2.5nm Ultra filter different from the 3nm Pro series?

    The Antlia 2.5nm Ultra uses a quartz glass substrate with excellent thermal stability and has a narrower 2.5nm bandpass. Compared with the 3nm Pro series, which uses an optical glass substrate and a 3nm bandpass, Antlia states the Ultra has higher transmittance for the emission lines and estimates a 20-30% signal improvement, with an exceptionally high signal-to-noise ratio for deep sky imaging.

    What does OD5 blocking mean for my images with the Antlia 2.5nm filter?

    OD5 blocking means the filter attenuates out-of-band light by a factor of 100,000 (transmitting only 0.001%). Antlia designs this blocking to block interference from other wavelengths and minimize halos around bright stars, keeping the H-alpha signal of your target clean.

    How will the Antlia 2.5nm H-alpha filter perform on my f/4 refractor?

    An f/4 system is within Antlia's recommendation: the filter is recommended for optics of f/3.5 or slower for best optical performance. The filter's flat-top spectral profile minimizes the loss in transmission from the wavelength shift that occurs in faster light cones.

    Will this 2.5nm filter help me image the faint outer structures of the Pelican Nebula (IC 5070) from a Bortle 7 zone?

    The Pelican Nebula is a strong H-alpha emission target, so it suits this filter. The narrow 2.5nm bandpass around the 656.3nm line of ionized hydrogen blocks most light pollution, which darkens the sky background and helps faint, extended nebulosity stand out from a suburban location. Results from a Bortle 7 site still depend on your optics and total exposure time.

    Why is a "flat-top" spectrum important for this Antlia H-alpha filter?

    A flat-top spectrum means the filter maintains its high transmission across its entire 2.5nm bandpass, rather than having a sharp peak that quickly falls off. This makes the filter more tolerant to the slight shifts in wavelength (band-shift) caused by the converging light cones of fast telescopes (like f/4 or f/5 systems). Antlia states it minimizes the loss in transmission due to that shift.

    Can I use the Antlia 2.5nm filter for visual observing or solar imaging?

    No. Antlia does not recommend this filter for solar imaging or night visual observation. DO NOT LOOK AT THE SUN WITH THIS FILTER. Serious eye damage will result if you fail to observe the warning.

  • Filter Type H-alpha ultra narrowband
    Series SHO 2.5nm Ultra
    Central Wavelength (CWL) 656.3nm
    Peak Transmission >=95% at 656.3nm
    FWHM 2.5nm +0.3/-0.1nm
    Blocking >=OD5 (0.001%)
    Substrate Quartz glass
    Filter Thickness 2mm (+/-0.05mm on 2" mounted, +/-0.1mm on 36mm unmounted)
    Spectrum Profile Flat-top
    Recommended f-ratio f/3.5 or slower
    Edge Treatment Coated to the edge, unmounted are edge blackened
    Quality Control 100% of production individually scanned
    Not Recommended For Solar imaging, night visual observation
    Available Sizes 36mm Round Unmounted, 2" Mounted
    • Actual measured spectrum, transmission and blocking (OD) data for the filter

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  • 3-Year warranty against delamination.