We collected the backscattered light by the microscope objective and passed it through a notch filter (NF785-33, Thorlabs) to reduce the Rayleigh scattered laser line. Further, to increase the signal-to-noise ratio, we mounted a 150 m diameter pinhole in the focal point of the telescope. The filtered light was coupled into our spectrometer (Model 207, McPherson) through a 150 m wide entrance slit where a 600 grooves/mm holographic grating disperses the light [63 (link)]. The Raman spectrum was then captured using a Peltier cooled CCD detector (Newton 920N-BR-DDXW-RECR, Andor) operated at -95 C. Our system has a Raman wavenumber spectral resolution of < 3 cm and accuracy of 3 cm .
Raman Spectroscopy of Spores using LTRS
We collected the backscattered light by the microscope objective and passed it through a notch filter (NF785-33, Thorlabs) to reduce the Rayleigh scattered laser line. Further, to increase the signal-to-noise ratio, we mounted a 150 m diameter pinhole in the focal point of the telescope. The filtered light was coupled into our spectrometer (Model 207, McPherson) through a 150 m wide entrance slit where a 600 grooves/mm holographic grating disperses the light [63 (link)]. The Raman spectrum was then captured using a Peltier cooled CCD detector (Newton 920N-BR-DDXW-RECR, Andor) operated at -95 C. Our system has a Raman wavenumber spectral resolution of < 3 cm and accuracy of 3 cm .
Corresponding Organization : Umeå University
Other organizations : University of Plymouth
Variable analysis
- Laser wavelength (785 nm)
- Laser power (100 mW, 60 mW in the sample)
- Raman spectra of spores
- Inverted microscope (IX71, Olympus)
- Dichroic shortpass mirror with a cut-off wavelength of 650 nm (DMSP650, Thorlabs)
- 60× water immersion objective (UPlanSApo60xWIR, Olympus) with a numerical aperture of 1.2 and a working distance of 0.28 mm
- Notch filter (NF785-33, Thorlabs) to reduce the Rayleigh scattered laser line
- 150 μm diameter pinhole in the focal point of the telescope to increase the signal-to-noise ratio
- Spectrometer (Model 207, McPherson) with a 600 grooves/mm holographic grating
- Peltier cooled CCD detector (Newton 920N-BR-DDXW-RECR, Andor) operated at -95 °C
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