ALTAIR F200QUADV2 filter, optimized...

ALTAIR F200QUADV2 filter, optimized 2" CMOS Quadband V2

ALTF200QUADV2
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Buy it now and receive it between on Monday, 25 November and Monday, 2 December with Home delivery - International

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Home delivery - International Home delivery - International

Monday, 25 November - Monday, 2 December

Home delivery - International

Home delivery - International

Estimated delivery:
Monday, 25 November - Monday, 2 December

 

Altair QuadBand is the new trend in light pollution filters for deep sky imaging of emission nebulae with CMOS, CCD and color DSLR cameras.

Altair V2 filter technology produces even better blocking of unwanted wavelengths, higher transmission and no halos. The result is a better signal-to-noise ratio for imaging emission nebulae with a DSLR or CMOS Astro camera.

The 35 nm passband not only makes the QuadBand V2 compatible with fast focal ratio telescopes and lenses, but also allows visual use with a relatively small telescope in urban locations. The brightest emission nebulae can be observed in urban conditions with a darker background.

This is the new QuadBand V2 coating technology that includes:

  • Anti-Halo coating on both surfaces to reduce reflection artifacts from reducers and camera lenses.
  • Increased blocking of unwanted ultraviolet, infrared and visual range wavelengths. Ultraviolet OD7 (T0.00001%), visual OD5 (T0.001%) and infrared OD4 (T0.01%) for the ultimate in blocking sky glow. An order of magnitude better than foreign filters.
  • Higher percentage transmission of desired wavelengths Ttop 95% (Average 5% higher transmission of desired wavelengths).
  • Ha and Oiii wavelengths at 35 nm FWHM with lower attenuation to reduce unwanted light pollution.

It is even compatible with fast telescopes, such as the Altair F6 refractors operating at F4.8 with reducers, and the Celestron RASA and Hyperstar F2.

It includes UVIR blocking for modified and unmodified DSLR cameras, plus an anti-reflection coating to reduce halos as much as possible.

Narrow-band bicolor imaging is a booming new trend in astrophotography, especially popular in areas with light pollution or for capturing images in rural areas by moonlight.

Now you can capture the two main emission bands of nebulae at the same time, while suppressing light pollution, moonlight and airglow. Capture more data in less time and open your time window to capture images, even in the summer months.

Altair's narrowband light pollution filters work by isolating the primary nebula emission zones in the red and blue/green wavelengths, and separating them into two main "zones" with a wide separation for easy capture with a color camera, all in a single exposure! Not only is capture very convenient, but processing is also easy, thanks to the wide separation of the green/blue and red "zones". Light pollution control is extremely effective and LED light is also significantly reduced, thanks to Rayleigh scattering effects.

Sensitive OSC or "One Shot Colour" CMOS cameras like the #Hypercam183C capture these wavelengths very efficiently and let them pass through the Bayer matrix. The filters also work with DSLRs (modified APS-C sensor cameras are the best, but regular ones work too). When you have the full stack of exposures, processing is relatively easy because of the large color separation. You can also use the quad band and tri-band filters as a "superluminance filter" for shooting nebulae with monochrome cameras.

A quick overview of the Altair filter family:

QuadBand filter: combines Sii and Ha in a red zone, and H-beta + Oiii in a green/blue zone. (Recommended for moderate light pollution and sky glow, used with color cameras).

TriBand filter: combines Ha in a red zone and H-beta + Oiii in a green/blue zone (recommended for higher light pollution, used with color cameras).

Dual band filter : separates the red Ha and blue Oiii channels even more clearly and with deeper blocking. (Recommended for severe light pollution, such as in built-up areas like cities. Used with color cameras).

Mono narrow band camera filter : isolate individual bands, so only one wavelength is captured per filter, such as Oiii, Ha or Sii, and are primarily used with mono B&W astronomical cameras. Separate sets of exposures are required with each filter.

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