True UV Bandpass Isolation
Our UV bandpass filters are tuned to pass only selected ultraviolet wavelengths such as:
- UVA (320–400 nm)
- UVB (280–320 nm)
- Narrowband UV lines for astronomy & spectroscopy
No visible. No infrared. Only pure ultraviolet.
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Precision UV-Bandpass Filters for Pure Ultraviolet Imaging
UVR Optics UV-Bandpass Filters are engineered for professionals who demand true ultraviolet transmission without visible or infrared leakage. Whether you are conducting astronomical UV observation, forensic imaging, materials analysis, or professional ultraviolet photography, your results depend on optical purity.
Unlike generic UV filters that allow infrared and visible light leakage, UVR Optics filters are designed with advanced multilayer dielectric coatings that isolate only the target UV wavelengths producing sharp, uncontaminated ultraviolet images every time.
The AndreaU MK II filter absorbs both the Visible (400nm - 700nm) and the Near Infrared (700nm--1100nm), passing only the central UVA wavelengths.
UVROptics' UVBplus captures the UVB range(290-320nm). "Pushing the limits of sensor technology".
UVROptics' Dichroic, peaking at 376nm, captures the greatest percentage of the solar UVA range.
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NIR-Block Filter
The NIR-Block provides those UV photographers who use stacks of ionic filters the opportunity to achieve a new maximum in NIR (Near-Infrared) blocking while still enjoying excellent UV transmission. In the NIR-Block we have exceeded the UV transmission of the Schott S8612 while also providing significantly greater out-of-band blocking.

CuRB NIR-Blocking Filter
UVROptics' CuRB is an acronym for our Copper (Cu) Red-Blocking filter. The CuRB is a water-tight cell, within a 52mm filter ring, containing a Copper sulphate (CuSO4) solution at a precise concentration. The CuSO4 blocks, through absorption, the high-red and Infrared wavelengths in the 670nm-1100nm range.The advantage of the CuSO4 over other Infrared blocking filters is the UV transmission of Copper sulphate as well as the red/NIR blocking beginning in the 690nm range. A UV photographer can use any of the common UV-transmitting, visible-light-absorbing filters, e.g., UG1, UG11, ZWB1, in conjunction with the CuRB to produce an IR free image.

UVR Optics eliminates these risks by using true bandpass engineering.
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Research published in Frontiers in Astronomy and Space Science highlights the importance of narrowband UV filtering to prevent spectral overlap.
Unlike standard UV filters, our optics reveal true ultraviolet reflectance and fluorescence without distortion.
Research in NCBI and ResearchGate optics journals shows that precise UV wavelength control increases detection reliability.
With no infrared or visible light contamination, UVR filters produce true ultraviolet contrast.
These technologies are documented in Wikipedia’s Optical Coating references and Frontiers in Applied Physics as the gold standard for spectral filtering.