CM-900 Cold Mirror & Longpass Filter

Block visible light and near-infrared; pass only short-wave infrared for selective thermal and spectroscopic analysis.

  • Reflection band (visible): 380 – 750 nm, ≥ 96.2 % R
  • Passband (IR): 908 – 1192 nm, 80.2 – 96.4 % T
  • Cut-on (T50): ≈ 899 nm
  • Edge steepness: ~32 nm (10 → 90 % transition)
  • Visible leakage: < 3.8 % T across 380 – 750 nm
  • AOI: 0° (normal incidence); custom angles available
  • Construction: Ion-assisted hard-oxide; 5 – 450 mm shapes, 0.21 – 3.8 mm thick
  • Custom options: Edge tuning, extended reflection band, custom AOI, rapid prototypes
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CM-900 Hybrid delivers Reflection band (visible) 380 – 750 nm, ≥ 96.2 % R, Passband (IR) 908 – 1192 nm, 80.2 – 96.4 % T, and Cut-on (T50) ≈ 899 nm.

The hard-oxide coating is built for repeated handling, heat, and cleaning.

Best suited for:

Block visible light and near-infrared; pass only short-wave infrared for selective thermal and spectroscopic analysis.

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Description

The CM-900 represents the longest cut-on point in the cold-mirror series at 899 nm, creating an aggressive blocking profile that isolates the deepest infrared signals. Peak transmission reaches 96.4 % at 1056 nm with a 50 % cut-on precisely at 899 nm. Visible extinction is near-total (UV 0.1 %, blue 0.5 %, green 0.9 %, yellow 1.0 %, red 1.2 %), while the entire near-infrared (700-850 nm) is virtually eliminated at 1.0 % transmission. The critical transition occurs in NIR (850-1000 nm) at 66.1 %, then climbs steeply to 92.9 % in SWIR (1000-1200 nm). This extreme-edge filter is engineered for applications demanding absolute separation of 900 nm+ deep-infrared from all ambient and thermal noise below.

Key Advantages

  • Ultra-Aggressive Visible-NIR Blocking - Transmits only 1.0 % of NIR (700-850 nm) and 66.1 % of NIR (850-1000 nm), creating the sharpest cutoff in the series for maximum stray-light rejection
  • SWIR-Optimized Performance - 92.9 % SWIR transmission above 900 nm isolates the deepest thermal signatures with minimal optical loss or background interference
  • Solar-Blind Operation - Blocks the vast majority of ambient solar radiation and visible-light scatter, enabling daylight-compatible deep-IR detection
  • Hard-Oxide Ion-Assisted Durability - Premium coating resists thermal gradients, environmental contamination, and mechanical stress in extreme field and laboratory conditions
  • Specialized Custom Formats - Manufactured in round, square, and free-form apertures from 5 mm to 450 mm with 0.21-3.8 mm thickness on Borofloat, soda-lime, Schott D263 T, or Corning Eagle XG

Typical Applications

  • Deep-SWIR Scientific Spectroscopy - Isolates 1000-1200 nm molecular and thermal signatures in atmospheric chemistry, materials analysis, and combustion diagnostics
  • Night-Vision Free-Space Optics - Enables secure, solar-blind communication and imaging by transmitting only deepest-IR channels unavailable to conventional visible-band systems
  • High-Altitude Thermal Reconnaissance - Rejects solar interference and visible-light background, enabling thermal imaging and temperature mapping from aircraft and satellites
  • Quantum-Cascade Laser Applications - Passes QCL mid-infrared output (1000-1300 nm range) while blocking visible alignment beams and thermal background
  • Emerging Hyperspectral SWIR Sensing - Feeds next-generation spectral imaging systems with pure deep-IR data for precision agriculture, mineral identification, and environmental monitoring

The CM-900 is built for cutting-edge deep-IR and SWIR applications at the frontier of thermal sensing. We specialize in rapid prototyping of complex specifications and scaling to production volumes without performance compromise.

FAQ

CM-900 FAQ

What is CM-900 and what is it used for?

CM-900 is a Ultra-Extended Cutoff Cold Mirror for SWIR-Exclusive Deep-Infrared Sensing and Thermal-Only Isolation. The CM-900 represents the longest cut-on point in the cold-mirror series at 899 nm, creating an aggressive blocking profile that isolates the deepest infrared signals. Peak transmission reaches 96.4 % at 1056 nm with a 50 % cut-on precisely at 899 nm. Common uses include Deep-SWIR Scientific Spectroscopy, Night-Vision Free-Space Optics, High-Altitude Thermal Reconnaissance, and Quantum-Cascade Laser Applications.

What are the key optical specs of CM-900?

Key published specs for CM-900 include Reflection band (visible): 380 – 750 nm, ≥ 96.2 % R; Passband (IR): 908 – 1192 nm, 80.2 – 96.4 % T; Cut-on (T50): ≈ 899 nm; Edge steepness: ~32 nm (10 → 90 % transition); Visible leakage: < 3.8 % T across 380 – 750 nm.

What applications is CM-900 best suited for?

CM-900 is commonly used for Deep-SWIR Scientific Spectroscopy, Night-Vision Free-Space Optics, High-Altitude Thermal Reconnaissance, and Quantum-Cascade Laser Applications. Deep-SWIR Scientific Spectroscopy - Isolates 1000-1200 nm molecular and thermal signatures in atmospheric chemistry, materials analysis, and combustion diagnostics.

Can CM-900 be customized for size, substrate, or coating requirements?

KUPO lists the construction for CM-900 as Ion-assisted hard-oxide; 5 – 450 mm shapes, 0.21 – 3.8 mm thick. Published custom options include Edge tuning, extended reflection band, custom AOI, rapid prototypes. SWIR-Optimized Performance - 92.9 % SWIR transmission above 900 nm isolates the deepest thermal signatures with minimal optical loss or background interference.

What should I know about angle of incidence and durability for CM-900?

The published angle of incidence for CM-900 is 0° (normal incidence); custom angles available. The hard-oxide coating is built for repeated handling, heat, and cleaning.

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