Detector Selection Chart

The table below can be used to identify which type of linear array detector best suits your spectroscopy application based on:

  • Wavelength range
  • High sensitivity versus high signal-to-noise ratio
  • Integration time

For wavelengths below 1100 nm (UV, VIS, NIR), you should use silicon detectors (CCD or CMOS/NMOS), and for wavelengths above 1100 nm, you should choose InGaAs detectors.

For silicon detectors, choose CCD’s when you have low light levels and therefore need high sensitivity, and choose CMOS/NMOS, when you have higher light levels and want the best signal-to-noise ratio

Choose cooled detectors, when your application requires long integration times.

UV-VIS-NIR 190-1100 nm wavelength rangeNIR 900-2500 nm wavelength range
High SensitivityHigh SNR
Integration timeDetector typeExamplesDetector typeExamplesDetector typeExamples
Deep cooled CCDAndor iDus
10 sec-
1-2 stage TE cooled BT-CCDHamamatsu S7031 seriesCooled CMOS/NMOSHamamatsu s5931 series2-stage TE cooled InGaAsHamamatsu G9206
1 sec-
Non-cooled BT-CCDHamamatsu s10420 seriesNon-cooled NMOS/CMOSHamamatsu S390x series
Hamamatsu S838x series
1-stage TE cooled InGaAsHamamatsu G9203/G9204
100 msec-
10 msec-
Non-cooled CCDSONY ILX511B
Hamamatsu S11639
CMOS with global shutterPanavision ELIS1024Non-cooled InGaAsHamamatsu G9204 series
1 msec-
Non-cooled BT-CCD w. Global shutterHamamatsu S11156
100 microsec-
10 microsec-
1 microsec-