PyLoN LN - Cooled Spectroscopy Detector - eXcelon-Enabled
No other spectroscopy CCD camera is this cool, this quiet and this fast!

Features and Benefits

  • Supported by LightField™ - PI's powerful 64-bit data acquisition software
  • Optional patent-pending IntelliCal™ wavelength and intensity calibration packages and hardware timestamping.
  • No external controller - all electronics inside the camera head while maintaining the ultra-low noise performance.
  • More ADC speeds - 4X as fast as its predecessor’s 1 MHz top speed.
  • Indium metal seals - for improved vacuum longevity.
  • Ideal for low-light, long acquisition applications - including Raman, TERS, single molecule spectroscopy and photoluminescence
  • Gig-E communication - permits remote operation up to 50 m.
  • Digital correlated double sampling - even lower noise
  • PI’s exclusive eXcelon technology - available on selected models
  • Reduced binning noise - optimizing it for spectroscopy applications
  • AR coatings from Acton Optics - available on windows
PyLoN LN Cooled Spectroscopy Detector

Superior Cooling Technology
PyLoN models reduce dark current and inherent noise contribution to negligible levels via cryogenically cooling the CCD down to -120°C with liquid nitrogen. To optimise the temperature dependent quantum efficiency in the near IR, the CCD temperature may be set by software between -90°C and –120°C.

PyLoN™, a new line of controllerless, cryogenically cooled CCD cameras designed for quantitative spectroscopy applications that demand the highest possible sensitivity. In creating the new PyLoN platform, Princeton Instruments redesigned its industry-leading Spec-10 family of cameras to remove the external controller, increasing experimental flexibility while further improving the ultra-low-noise electronics. Liquid nitrogen cooling virtually eliminates dark current, and indium metal seals enhance vacuum longevity. Binning noise has been further reduced from the already low levels in the Spec-10 platform.

Dual capacity mode and Variable System Gain
One on CCD output amplifier is optimised to high dynamic range of typical 1 Me and a read-noise of 10-e rms and the other for lower full well capacity ( 250.000 e) but offering read-noise of typically 2-4 e. The PyLoN: 2K gives spectroscopists this feature that provides the ability to select either high-capacity mode for applications like absorbance spectroscopy, or high-sensitivity mode for applications such as low-light Raman and fluorescence expect system gain is set so that the full well of the CCD matches the full range of the 16-bit digitizer. The gain can be selected under software control to meet the needs of a given application.

Spec-10 Datasheets
Model Imaging Array Pixel Size Sensor Type
100F/LN 1340x100, F/I 20 x 20 µm F/I
100B/LN_eXcelon 1340x100, B/I 20 x 20 µm B/I
100B/LN 1340x100, B/I 20 x 20 µm B/I
100BR/LN_eXcelon 1340x100, B/I DD 20 x 20 µm B/ IDD
100BR/LN 1340x100, B/I DD 20 x 20 µm B/ IDD
400F/LN 1340x400, F/I 20 x 20 µm F/I
400B/LN_eXcelon 1340x400, B/I DD 20 x 20 µm B/I
400B/LN 1340x400, B/I 20 x 20 µm B/I
400BR/LN_eXcelon 1340x400, B/I DD 20 x 20 µm B/ IDD
400BR/LN 1340x400, B/I DD 20 x 20 µm B/ IDD
 F/I - Front Illuminated | B/I - Back Illuminated | DD - Deep Depletion

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