Baader Planetarium

Baader Narrowband-/Highspeed Filter Selector

When selecting an (Ultra-)Narrowband/Highspeed filter, multiple factors must be considered

Detailed information about the newly introduced f/3 filter category and the influencing factors in filter selection, as well as detailed explanations why our high-speed filters must have a preshift to the respective center wavelength, can be found in this blog post and whitepaper .
  1. Desired Filter Wavelength (H-alpha / OIII / SII)
  2. Average Working Temperature
  3. Needed Halfbandwidth (6.5nm or 3.5/4nm)

After selecting the above criteria, a graphic will appear from which you can determine the required filter category based on this information:

  • Aperture ratio f/# (x-Axis)
  • Central Obstruction in % (y-Axis)

Filter-Selector-no-parameters-PWA

Step 1 – Select your optimal narrowband filter according to the criteria below:


Depending on Sky Quality. Ultra-Narrowband/Highspeed Filters with 3.5nm/4nm are only recommend for areas with high light pollution (Bortle 9/8/7/[6] Sky).

Please make a selection above to narrow down/select the graph you need


Step 2 – Determine filter category based on aperture ratio and central obstruction:


Now determine the appropriate filter category in the graph below using the focal ratio (x-axis) and the central obstruction (y-axis) of your telescope. In the near future, we will again enable you to conveniently enter your telescope data here. The legend with links to the respective categories can be found below the graph.

Step 3 – Select filter category based on your entries: