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Option
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Basic
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Full
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Editable data collection parameters per channel, such as detector integration time, auto-dark correction, signal averaging, spline interpolation and spectral smoothing
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X
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X
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Display data in scope-, transmittance-, absorbance-, or relative irradiance mode. Multiple spectrometer channels are displayed in the same graph, optional grid display. 3D display for multiple spectra in time series (USB2 only)
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X
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X
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Zoom-, (Auto)scale- and panning functions to expand quickly an interesting part of the spectrum (both X- and Y-axis) to the full graph, save graph to RTF file.
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X
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X
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Mouse drag controls movement of a data cursor for instantaneous readout of wavelength- and y-axis magnitude. Peak finder for moving cursor fast to nearest peak
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X
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X
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Save spectra, and display online measurements against (multiple) saved spectra background. Print (multiple) spectra in color. Convert saved spectra to ASCII format in equidistance (nm) with start wavelength in nm
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X
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X
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Help menu option to find quickly a description about any AvaSoft topic
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X
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X
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History Channel Application, in which the output of (up to 8) user defined functions, integrals, peaks (intensity, wavelength) can be followed simultaneously against time. Functions can be entered in Visual-Basic script. Time series measurements can be saved/loaded and printed. Zoom- and panning functions can be applied to expand quickly an interesting part of the time series measurement to the full graph.
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X
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Auto Wavelength Calibration. In combination with a Mercury-Argon Light Source, a number of peaks can be detected automatically. These peaks are then compared with the wavelengths where they should have been detected, and a regression fit is performed to calculate the best wavelength calibration coefficients.
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X
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Correct for drift. Master and slave channels with similar range can be used to correct the other channel data for changes in the light source. This option also works for the FOS-2-inline to correct for one channel spectrometer temperature fluctuations.
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X
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Automatic save spectra periodically (save a spectrum every x seconds)
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X
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| Store to RAM for ultrafast Data saving for a limited amount of scans (USB2 only) |
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X |
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External Trigger control to acquire spectral data only if a TTL signal is presented with optional integration time delay settings.
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X
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Convert spectra to J-CAMP format for further data processing e.g. in GRAMS32
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X
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| Convert spectra to Excel, multiple spectra in one file, multiple channels in worksheets |
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X |
| Merging spectra of multiple channels to one spectrum (USB2 only) |
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X |
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Full Width Half Max calculations, online or on saved spectra. Graphically displayed
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X
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Integral calculations, online or on saved spectra, graphically displayed
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X
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Auto-configure integration time: AvaSoft searches for an optimal integration time
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X
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Automatic Save Dark by TTL shutter.
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X
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Auto-detect saturated pixels in a spectrum, optionally autocorrect inverted saturated pixels, optionally visualize saturated pixels and log saturated wavelength regions in time series.
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X
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LIBS application (USB2 platform)
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X
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