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General| Software | OMNIC |
|---|---|
| Type | FT-IR Spectrometer |
| Detector Type | DTGS |
| Beamsplitter | KBr |
| Source | EverGlo mid-IR source |
| Wavenumber Accuracy | 0.01 cm-1 |
| Operating System | Windows |
Describes available software guides and wizards for learning.
Introduces basic software operation and features.
Provides instructions for hardware, maintenance, and troubleshooting.
Instructions for turning on the spectrometer and its components.
Steps to launch the OMNIC software.
Steps to collect a background and sample spectrum.
Instructions on how to save collected spectra.
Describes the main OMNIC software interface.
Describes the indicator for spectrometer status.
Details on choosing experiment files.
How to change spectrum Y-axis units.
Steps for labeling peaks in spectra.
How to perform spectral searches against libraries.
Identifies front-view components of the spectrometer.
Details the internal optical layout of the spectrometer.
Shows connectors and ports on the spectrometer's rear.
Discusses spectrometer configuration options.
Tips for enhancing spectral data precision and accuracy.
Methods to enhance signal-to-noise ratio.
Overview of smart accessories and their features.
Lists additional sampling accessories like external mirrors.
Lists accessories requiring specialized installation.
Setup and procedures for collecting spectra.
Monitoring spectra quality and baseline correction.
Using, creating, and searching spectral libraries.
Using screens/filters for detector optimization.
Removing cover, when to align spectrometer.
Detector cooling needs and desiccant maintenance.
Procedures for computer upgrades and software reinstallation.
How to perform basic and advanced spectrometer diagnostics.
Procedures for ensuring optimal system performance.
Solving issues with spectrum resolution.
Reasons and solutions for a dimmed Quantify command.
Troubleshooting library addition issues.
Resolving issues preventing data collection.
Troubleshooting display issues.
Causes and solutions for unstable baselines.
Identifying and fixing spectrum fringes.
Removing CO2 interference.
Reducing noise in spectra.
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