There are three options to refine the search:
Note that the filter scanner uses a rectangular beam of light to measure the throughput. In one dimension this beam has a f/9.0 focal ratio, while in the other dimension it is f/26.1. This will affect the measured central wavelength of interference filters; please consult Appendix D of the "Observers' Guide 1994" for more information regarding the central wavelength of interference filters in an uncollimated beam.
The scanner can only measure up to ~9000 Angstroms. Around this wavelength, noise is apparent in the throughput scans. As a result, some I and Z band scans show local throughputs greater than 100%.
Filter Database © 2006 Isaac Newton Group of Telescopes Developed by Robert Greimel and upgraded by Samantha Rix