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Photon etc IMA Hyperspectral microscope

Global hyperspectral microscope

IMA is a hyperspectral microscope delivering spectral and spatial information in the VIS, NIR, and SWIR range (400 nm – 1620 nm). This system rapidly maps photoluminescence, electroluminescence, fluorescence, reflectance, and transmittance. Based on high throughput global-imaging filters, IMA is faster and more efficient than standard point-by-point or line-scan based systems.

IMA Applications Overview

  • Perform complex material analyses such as solar cell characterization and semiconductor quality control
  • Study of sample formation, degradation and identification of deficient areas
  • Imaging of multiplexed emitters
  • Access to the second biological window (900 – 1620 nm)
  • Mapping of spectral heterogeneities
  • Study IR markers in complex environments including live cells and tissue.
  • Fast imaging – 1.4 million spectra in minutes
  • Retrieve darkfield images and obtain a contrast of transparent and unstained samples such as polymers, crystals or live cells.

 

Technical Specifications
VIS SWIR
Spectral range 400-1000 nm 900-1620 nm
Spectral resolution (FWHM) < 2 nm < 4 nm
Spectral channels Continuously tunable Continuously tunable
Spatial resolution Sub-micron – limited by the microscope objective NA Sub-micron – limited by the microscope objective NA
Camera CCD, EMCCD, sCMOS Photon etc. InGaAs camera (ZephIR™ 1.7 or Alizé™ 1.7)
Excitation wavelengths (up to 3 lasers) 405, 447, 532, 561, 660, 730, 785, 808 nm (other wavelenghts available upon request) 405, 447, 532, 561, 660, 730, 785, 808 nm (other wavelenghts available upon request)
Microscope Upright or inverted, scientific grade Upright or inverted, scientific grade
White light illumination Diascopic, episcopic, Hg, halogen Diascopic, episcopic, Hg, halogen
Illumination options Epifluorescence module, darkfield module (oil or dry) Epifluorescence module, darkfield module (oil or dry)