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Fibre-Optic Spectrometer · TE-cooled, back-illuminated CCD

Metal

Metal TE-Cooled Fibre-Optic Spectrometer

A thermoelectrically cooled spectrometer with a Hamamatsu back-illuminated area-array CCD. Cooling 20 °C below ambient lowers the dark current enough for 60 s integrations, so weak Raman and fluorescence signals build up without the noise floor rising with them.

−20 °C

Below ambient, TE-cooled

60 s

Maximum integration

16-bit

A/D conversion

200–1100 nm

Detector range

Metal TE-Cooled Fibre-Optic Spectrometer
Best for: Weak Raman and fluorescence signals, long integrations, and UV work where a back-illuminated sensor pays off.

Features

  • High signal-to-noise ratio
  • Single-stage thermoelectric cooling
  • Back-illuminated area-array CCD detector
  • High precision and low temperature drift
  • High UV response
  • Spectral Analysis 5.0 software included

Applications

  • Raman and fluorescence spectroscopy
  • Life science
  • Scientific research
  • Material analysis
  • Industrial environments
  • Instrumentation

Technical Specifications

Metal Specifications

Detector

DetectorHamamatsu cooled area-array CCD, back-illuminated
Wavelength range200–1100 nm
Pixels2048
Pixel size14 µm × 14 µm
Cooling3 A at 5 V DC; 20 °C below room temperature (typical)

Spectrometer

Optical designf/4, symmetrically crossed Czerny-Turner
Optical resolutionDepends on grating groove density and slit size; many options
Integration time17 ms – 60 s
Dimensions192 × 109 × 61.2 mm
Weight1790 g

Electronics

A/D conversion16-bit
InterfaceUSB 2.0
Power consumption450 mA at 5 V DC (plus cooling)
Supported systemsWindows XP / 7 / 10

Final specifications depend on the configured wavelength range, entrance aperture and grating. We confirm the configuration before quotation.

Figures

Drawings, Photos and Measured Data

Metal spectrometer dimension drawing, 192 × 109 × 61.2 mm
Dimensions: 192 (L) × 109 (W) × 61.2 (H) mm

Datasheets

Full specification sheets for the Metal.

Configure the Metal for your measurement

Tell us the wavelength range, the resolution you need and what you are measuring; we will propose the grating, slit and accessories to match.