Thin-film interference filters · filter type (bandpass, longpass, shortpass, notch, dichroic), centre wavelength and FWHM, edge wavelengths, transmission and OD blocking, blocking range, angle of incidence and polarization splitting, cone angle, temperature shift, clear aperture and mounting
An optical filter transmits the wavelengths a sensor or imaging system needs and blocks the rest. In thin-film interference filters this is done by stacks of coating layers whose spectrum depends on angle and temperature. Settle three things before asking for quotes: the filter type and spectral features, the transmission and blocking levels and how they are specified, and the angle of incidence, temperature range, clear aperture and mounting in your system.
Thin-film interference optical filters — bandpass, longpass, shortpass, notch and dichroic — for optical sensors, spectroscopy, fluorescence imaging, lidar and machine vision, unmounted or in rings. Lenses, mirrors, prisms, absorptive glass windows sold as optics and complete filter wheels or spectrometers are outside this page; lenses, beam-steering mirrors and optical spectrometers have their own pages.
01
Alluxa defines cut-on wavelength as a rising edge, as in a longpass filter, and cut-off as a falling edge, as in a shortpass filter, each taken where transmission reaches 50% of peak. Centre wavelength (CWL) is the midpoint between adjacent cut-on and cut-off points of a passband or notch, and full-width at half-maximum (FWHM) is the distance between those 50% points; bandwidth can also be specified at other levels, such as 80% of peak. [1]
Chroma's handbook of optical filters uses the same 50% convention: the centre wavelength is the arithmetic mean of the wavelengths at 50% of peak transmission, and the FWHM is the bandwidth at that level. Longpass and shortpass filters are denoted by their 50% cut-on or cut-off wavelengths, and average transmission is calculated over the useful transmission region of the filter rather than over the entire spectrum. Slope, the sharpness of the transition from transmission to blocking, can be specified by stating the wavelength at which the filter must reach a given blocking level. [6]
Chroma's ET525/50m emission filter, for example, is specified with a 525 nm centre wavelength and 50 nm FWHM. Chroma designs its emission filters for 0° angle of incidence and its dichroics for 45°, and warns that changing the angle shifts spectral performance. [5]
Alluxa specifies 0° filters — edge, bandpass and notch — with transmission in percent and blocking in optical density, and dichroic filters and mirrors used at larger angles with reflection bands, since they direct the beam within the system. It asks buyers to state whether a band specification is an average or absolute value, because absolute specifications with tight transitions raise cost or reduce feasibility. [1]
The handbook explains how the coating works: a stack of layers, each around a quarter of a wavelength thick (about 1/10,000 of a millimetre), whose reflections at each interface combine through interference to reflect some wavelengths and transmit others. The number of layers and the thickness of each set the nominal wavelength, the bandwidth and the blocking level. [6]
Give the supplier the filter type, CWL and FWHM (or edge wavelengths) with tolerances, transmission level and band (average or absolute), blocking OD and range, ripple, angle of incidence and cone half-angle, operating temperature range, substrate, size, clear aperture, thickness, surface quality, mounting and quantity.
02
Alluxa defines optical density as OD = −log₁₀(T). Tilting an interference filter away from normal blue-shifts its spectrum towards shorter wavelengths, more strongly at larger angles, following λθ = λ₀√(1 − (n₀ sin θ / n_eff)²) for collimated light. Temperature also moves the spectrum — a red shift as temperature rises — and Alluxa states its hard-coated filters shift between 2 and 5 pm/°C over instrument operating temperatures, depending on substrate and design. [1] [2] [3]
Chroma's handbook defines blocking level and blocking range in optical density, OD = −log(T) or OD = −log(%T / 100), and gives the example OD 4.5 = 3 × 10⁻⁵ T (0.003 %T). It notes that thin-film interference filters block mainly by reflection, not absorption. Cross-talk is the minimum attenuation of two filters placed in series over a stated range, which matters when matching excitation and emission filters. [6]
Editorial calculation: OD 6 blocking means T = 10⁻⁶, one millionth of the light, while OD 4 passes 10⁻⁴. For a 525 nm filter and an assumed effective index of 2.0, a 10° tilt moves the centre to 525 × √(1 − (sin 10° ÷ 2.0)²) ≈ 523.0 nm, a 2 nm blue shift. A 60 °C swing at 5 pm/°C moves it 0.3 nm. [1] [2] [3]
Semrock's technical note on non-normal incidence describes two effects as the angle increases: spectral features shift to shorter wavelengths, and separate spectra emerge for s- and p-polarized light. On its RazorEdge longpass designs the p-polarized edge shifts more than the s-polarized edge (the reverse for shortpass), giving a shelf near 50% transmission in unpolarized light. On StopLine U- and S-grade notch filters, the notch moves to shorter wavelengths, loses depth and narrows. Semrock's FAQ adds that at larger angles the spectrum can become highly distorted and that the shift depends strongly on filter design. [7] [8]
Chroma's handbook states that a filter or beamsplitter used at any angle other than the usual 0° or 45° must be specified explicitly, and that in a converging or diverging beam the half-cone angle may also need to be specified; it can be given as the f-number or the numerical aperture, which equals the sine of the half-cone angle. [6]
Coatings and absorbing glass react to temperature on different scales. The handbook cites sharp-cut longpass filter glasses shifting their cut-on by about 0.1 to 0.15 nm/°C, against Alluxa's 2–5 pm/°C for its hard-coated filters. Editorial calculation: 0.1–0.15 nm/°C is 100–150 pm/°C, 20 to 75 times the 2–5 pm/°C range. [6] [3]
Alluxa defines clear aperture as the area over which specifications must be met and states that more than 90% can be achieved for unmounted filters, though it may be smaller for large parts with demanding spectra; parallelism and wedge are set by substrate polishing. [4]
03
Edmund Optics' 355 nm hard-coated OD 4.0 10 nm bandpass filter shows how a catalogue sheet states each field: centre wavelength 355.00 ±2.0 nm, FWHM 10.00 ±2.0 nm, minimum transmission ≥85%, average OD ≥4.0 over a blocking range of 200–1200 nm, angle of incidence 0°, diameter 25.00 +0.0/-0.1 mm, clear aperture 21.0 mm, surface quality 80-50, substrate thickness 3.5 ±0.5 mm and mount thickness 5.0 ±0.1 mm, mounted in a black anodized ring. [9]
Edmund states these filters are optimized for spectral performance rather than laser damage threshold, quoting 1 J/cm² at 532 nm, 10 ns for the series, and lists durability tests to MIL-PRF-13830B (adhesion, moderate abrasion) and MIL-STD-810H (humidity, temperature). The mount carries an arrow pointing to the filter-coated surface S1; the anti-reflection coating is on S2. [9]
Editorial calculation: a 21.0 mm clear aperture on a 25.00 mm mounted filter is (21.0 ÷ 25.0)² ≈ 71% of the face area, below the more than 90% Alluxa cites for unmounted filters. Editorial calculation: a ≥85% passband against OD 4.0 blocking (0.01%) gives a pass-to-block ratio of at least 8,500 to 1.
Blocking range has limits. Chroma's handbook states that interference coatings block over a finite wavelength range, and that adding interference or absorbing-glass blockers extends the range at the cost of transmission and thickness. On its product page Chroma says its excitation filters block 300–1000 nm or beyond outside the passband, and that its emission filters may not block that far out of band. [6] [5]
Ask each supplier for measured spectra at your angle of incidence, the blocking range in OD, thermal shift, clear aperture and the test method for each specification. [1] [2] [3]
04
This is a functional reference built from the sources cited; it is not a full specification.
| Part | What it controls | Fix in the order |
|---|---|---|
| Thin-film coating stack | Quarter-wave layers set CWL, FWHM, edges and OD. [1] [6] | Spectral spec. |
| Added blockers | Extra coatings or absorbing glass widen the blocking range; lower transmission, add thickness. [6] | Blocking range in OD. |
| Substrate | Thermal shift; beam deviation; wedge. [3] [2] [4] | Material; thickness. |
| Clear aperture and edge | Usable area. [4] | CA; size. |
| Mount or ring | Aperture; handling. [4] [5] | Mounted; unmounted. |
| Anti-reflection coating and orientation mark | AR on S2; mount arrow points to coated S1 (Edmund). [9] | Orientation in the beam. |
05
A filter quotation needs values for your optical system. The table explains each field, gives published values where a reviewed source states them, and says what to ask the supplier for.
| Field | What it means and published values | Ask the supplier for |
|---|---|---|
| Centre wavelength | Mean of the 50% points. Example: 355.00 ±2.0 nm (Edmund); 525 nm (Chroma ET525/50m). [6] [9] [5] | CWL and tolerance. |
| FWHM | Width at 50% of peak. Example: 10.00 ±2.0 nm (Edmund); 50 nm (Chroma). [1] [9] [5] | FWHM and tolerance. |
| Transmission | Average over the useful region or absolute. Example: ≥85% minimum (Edmund). [6] [1] [9] | Average or absolute; measured curve. |
| Blocking | OD = −log(T); example OD ≥4.0 average over 200–1200 nm (Edmund). [6] [9] | OD level and range. |
| Angle of incidence | 0° for filters, 45° for dichroics (Chroma); state any other angle. [5] [6] | Spectra at your AOI and polarization. |
| Cone half-angle | Half-cone angle, f-number or NA of the beam. [6] | Performance in your beam. |
| Thermal shift | 2–5 pm/°C hard-coated (Alluxa). [3] | Shift over your temperature range. |
| Clear aperture and size | More than 90% achievable unmounted (Alluxa); 21.0 mm CA on 25.00 mm (Edmund). [4] [9] | CA, diameter, thickness. |
| Laser damage | 1 J/cm² at 532 nm, 10 ns (Edmund series). [9] | LIDT at your wavelength and pulse. |
| Durability | MIL-PRF-13830B; MIL-STD-810H (Edmund). [9] | Test standards met. |
06
Paste it into your enquiry below or into an email to a maker, then replace every bracket.
Type: [bandpass; longpass; shortpass; notch; dichroic] Spectral: [CWL; FWHM; edges; tolerances] Transmission/blocking: [T% avg or abs; OD; range] Angle: [AOI; cone half-angle] Temperature: [°C; max shift] Mechanical: [size; CA; thickness; mount] Quantity: [units]
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Its website lists band-pass optical filters.
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Product scope checked 2026-10-12
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FWHM is the distance between the two 50%-of-peak edge points and CWL is their midpoint. [1]
Optical density, OD = −log₁₀(T). Chroma's example: OD 4.5 passes 3 × 10⁻⁵ of the light (0.003 %T). [1] [6]
Tilting an interference filter blue-shifts its spectrum to shorter wavelengths, more at larger angles. [2]
Alluxa states 2–5 pm/°C for its hard-coated filters, red-shifting as temperature rises. [3]
Semrock explains that as the angle increases, separate spectra emerge for s- and p-polarized light; on its longpass edge filters the p-polarized edge shifts more than the s-polarized edge. [7]
Sources checked 2026-10-12. Alluxa's optical filter specification pages, Chroma's handbook of optical filters and ET525/50m product page, Semrock's technical note and FAQ on angle of incidence, and an Edmund Optics catalogue page are used to show what an optical filter specification covers; values for your order must come from the supplier's datasheet and measured spectra.
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