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Architecture · Extended coverage

Dual and wide-range spectrometer architectures

Some measurements span a wider range than one detector can cover well. Dual spectrometer systems and wide-range architectures combine the appropriate optical benches, detectors, timing and calibration for extended UV-Vis-NIR and NIR workflows, with each detector in its own range and all of them on one trigger.

Architecture

One optical input, several detectors

180500800 14002500 WAVELENGTH (nm) INTENSITY
Broadband source
Si · UV-Vis InGaAs · NIR COMMON TRIGGER
Two benches, one trigger
BALANCED ACROSS THE BAND
Spectral balance

Dual spectrometer systems

Dual spectrometer systems: UV-Vis and NIR benches on one trigger

The DS series integrates a UV-Vis or visible spectrometer with an InGaAs NIR spectrometer in one compact system: coverage up to 180–1700 nm with configurable detector and grating options, a common trigger and SDK support for both benches. Each bench keeps its own integration time, so the visible channel can use a short exposure while the NIR channel integrates longer on the weak end of the source. The reasoning behind the pairing is explained in Spectral balance in broadband measurements.

  • Silicon detector for the UV-Vis and InGaAs for the NIR, each in its appropriate range
  • Common trigger and I/O so both spectra belong to the same event
  • Independent integration settings per channel
  • Y-splitter fiber or a single input optic feeding both benches
  • One SDK for both benches

Wide-range NIR

Wide-range NIR: two InGaAs channels toward 2500 nm

The 900–1700 nm and 1600–2500 nm regions have different signal levels, noise behavior and cooling needs. A single-input dual-detector NIR design gives each region its own InGaAs array behind one optical input, so both bands see the same sample spot while integration and gain are optimized independently.

Staged full range

Staged full-range coverage from the deep UV to 2500 nm

For film stacks and source monitoring that require coverage from 155 nm to 2500 nm, a multi-stage architecture combines a deep-UV bench, a UV-Vis bench and an NIR bench behind a single input architecture with coordinated acquisition. One detector cannot be optimal across that span. A staged system lets each detector operate in its useful range while preserving one optical input and one acquisition strategy. Contact Evolve Sensing for availability in a specific range.

When to use it

When a dual or wide-range architecture is appropriate

A dual or wide-range architecture is appropriate when the measurement requires extended coverage, heterogeneous samples, high dynamic range across the band, synchronized acquisition or detector-specific optimization. When a single bench covers the wavelengths the model uses, a single bench is the better instrument: lower in cost, smaller and simpler to integrate.

FAQ

Frequently asked questions

Is a wider wavelength range always better?
No. The appropriate design depends on resolution, detector response, signal level, integration time and the model that consumes the spectrum. The range in use is the range to specify.
Can Evolve customize the optical configuration?
Yes. Wavelength range, slit, grating, detector, fiber interface, software and OEM requirements are all configurable, and an evaluation unit is available before purchase.
How do the two channels stay synchronized?
A common hardware trigger starts both benches, so each pair of spectra corresponds to the same event.

Next step

Discuss a wide-range configuration with an engineer

Send the wavelength range, the source, the sample and the integration constraints. An engineer will recommend one bench, two benches or a staged system for the measurement.