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Select an article below to learn how to use Thermo Scientific OMNIC Paradigm Software to set up and measure a sample spectrum.
Measurement settings allow you to specify how your sample is measured and how the data is processed after the spectrum is collected. Your settings control both how the instrument and sampling accessory measure the sample and how OMNIC Paradigm Software processes the data.
After adjusting your measurement settings, you can use them immediately or save them for later use.
This guide describes how to set, save, and use common measurement options. For a discussion of advanced settings, see “Advanced Measurement Settings.”
Set and save your measurement settings or use previously saved settings before starting a measurement.
In OMNIC Paradigm Software for touchscreen, edit individual settings or import a settings file (.expx) before you measure your sample. To edit or review measurement settings, select an analysis type from the home screen.
Figure 1. Review measurement settings in the Summary, Details, and Background tabs
Set and save your measurement settings from the dashboard, or update a few options while previewing a sample spectrum.
Figure 1. Edit measurement settings in the New Measurement pane.
In OMNIC Paradigm Software for touchscreen, edit individual settings or import a settings file (.expx) before you measure your sample. To edit or review measurement settings, select an analysis type from the home screen.
Figure 1. Review measurement settings in the Summary, Details, and Background tabs
Set and save your measurement settings from the dashboard, or update a few options while previewing a sample spectrum.
Figure 1. Edit measurement settings in the New Measurement pane.
The following table describes the settings you will use most frequently.
Option | Description | Default Setting |
---|---|---|
Measurement name | The name of your sample data. This name will appear when you save or open this data and in any reports you generate. The default name is the date and time of collection. | Date and Time |
Number of sample scans | How many times the sample is scanned during 10 the measurement. The resulting data reflects the average of all the scans. More scans will result in more accurate data but will take longer to measure. | 10 |
Resolution (cm-1) | Like the resolution of a photo or video, a better resolution will mean finer detail in your spectral data. For example, a better resolution will distinguish between two very close peaks while a poor resolution might combine them. A smaller value results in a higher (better) resolution, but also takes longer to measure. Typically, resolutions of 4 are used for solid and liquid samples. For gas samples, use a resolution of 1 or 0.5. | 4 |
Analysis type | With OMNIC Paradigm for touchscreen, you select your analysis type from the home screen rather than selecting from a list. Allows you to automatically process your data after it’s collected. Use None to measure a sample without additional analysis. Search performs a correlation search. Use search to identify an unknown sample. Edit search settings in the Search Setup view. QCheck results indicate a match value between your sample and a reference. Use QCheck to verify the composition of a known sample. Edit QCheck settings in the QCheck Setup view. Quantify is used to quantify the components of a sample using a pre-selected quantification method. Select Identify > Quantify Setup to specify a quantification method. | None |
Tag | Allows you to add a tag to the spectrum. Tags can later be used when searching for a spectrum. | |
Final format | Determines the units used for the collected data. You can convert your data to another Y-axis unit after collection in the View/Display menu. | Absorbance |
Sampling accessory | The sampling accessory used to measure the sample. Smart accessories are detected automatically. |
Name and save your measurement settings so that you can easily select them from the dashboard for later use. Settings for Search, QCheck, and Quantify analyses are not saved in these settings.
Saved settings are added to the Settings list for later use.
Once you have saved your measurement settings, you can edit or delete the settings.
Your new settings are now saved under the old setting name and are available in the Settings menu.
Name and save your measurement settings so that you can easily select them from the dashboard for later use. Settings for Search, QCheck, and Quantify analyses are not saved in these settings.
Saved settings are added to the Settings list for later use.
Once you have saved your measurement settings, you can edit or delete the settings.
Your new settings are now saved under the old setting name and are available in the Settings menu.
Import a settings file to automatically update your current measurement settings to those you saved previously. When importing settings, you can import an OMNIC Experiment file (.exp) or an OMNIC Paradigm settings file (.expx).
OMNIC Paradigm software is compatible with .exp files that were created with OMNIC software. However, with OMNIC Paradigm, you can export only .expx files, which are not compatible with earlier versions of OMNIC software.
Importing an OMNIC Experiment file updates your measurement settings, but does not alter your analysis settings, such as Search Setup or QCheck Setup.
The settings file is now saved and ready for future use.
The settings file is now saved and ready for future use.
Accurate sample spectra require an accurate and current measurement of the background.
When you collect a background spectrum, you are collecting a measurement of the environment in the spectrometer without a sample in place, including characteristics of the detector and atmosphere inside the spectrometer. This background spectrum is then used to eliminate any signals in your sample spectrum that are due to the spectrometer or to the background environment. Without a measurement of the background, there would be no way to know whether you were seeing data from the sample you measured or from the background environment.
Because the background environment in the spectrometer can change over time, you should update your background spectrum frequently.
In addition to collecting a new background spectrum periodically as the environment changes, collect a new background after any of the following circumstances:
There are several options for when and how to measure the background. These options determine when and if you are prompted to collect a new measurement of the background.
To select a different background option, select an analysis option and open the Background tab.
Figure 1. Select a background setting in the Background tab.
To select a different background option, click More in the New Measurement pane of the dashboard and scroll to the Background group.
Figure 1. Select a background setting in the Background pane.
To select a different background option, select an analysis option and open the Background tab.
Figure 1. Select a background setting in the Background tab.
To select a different background option, click More in the New Measurement pane of the dashboard and scroll to the Background group.
Figure 1. Select a background setting in the Background pane.
The following table describes the background settings.
Option | Description |
---|---|
Background scans | How many times the background will be measured. The resulting spectrum represents the average of all scans. More scans will produce a more accurate spectrum but will require a longer collection time. The default is 10. |
Measure before every sample | If this option is selected, you will be prompted to collect a new background spectrum before every sample measurement. This is a good option when you are measuring only a few samples, as it ensures a current measurement, but it can slow down the measurement process. Allows you to measure many samples using the same background spectrum. You can enter any integer value between 1 and 1024, but note that the background environment may change over time and your sample spectra may become less accurate as time passes. |
Smart background | Smart background measures the background automatically, so that you always have a current measurement without having to manually measure the background. |
Use previous background | Allows you to select a previous background spectrum. This option should be used only rarely and under unusual circumstances (for example, if it would be impossible to load or remove the sample without changing the system environment). In this case, you would collect and save a background spectrum earlier, using conditions as close as possible to the conditions under which you will measure the sample. |
Measuring the background requires only a few simple steps. If you attempt to measure a sample without a current background spectrum, you will be prompted to measure the background before proceeding.
Measuring a sample requires you to prepare your sample, to set and save your measurement settings, to measure a background spectrum, and finally to measure the sample.
Once your sample is measured, you can process or analyze it in the spectral view, or you can measure another sample. To measure another sample from the Spectral view, touch Measure New Sample.
See “Measurement Settings” for a description of each setting.
For details on setting up your analysis, see “Identify an Unknown with ATR.”
Once your sample is measured, you can process or analyze it in the Spectral view, or you can measure another sample. To measure another sample from the Spectral view, click More to review common measurement settings, and then click Measure New Sample to begin.
Once your sample is measured, you can process or analyze it in the spectral view, or you can measure another sample. To measure another sample from the Spectral view, touch Measure New Sample.
See “Measurement Settings” for a description of each setting.
For details on setting up your analysis, see “Identify an Unknown with ATR.”
Once your sample is measured, you can process or analyze it in the Spectral view, or you can measure another sample. To measure another sample from the Spectral view, click More to review common measurement settings, and then click Measure New Sample to begin.
Measuring a sample with OMNIC Paradigm Software requires only a few simple steps. Before measuring the sample, review your measurement settings and ensure that you have a recent background spectrum in use.
With your spectrum measured, you’re ready to identify, verify, or quantity the spectra. See “Identify an Unknown with ATR” for a guide to using a library search to identify your sample.
Use advanced measurement settings to control apodization, zero fill, range limits, instrument-specific settings, and more.
These advanced settings should typically be left in their default state. Only in rare or specific circumstances should you edit these settings.
To review or edit advanced settings, open the Details tab.
Figure 1. The Details tab displays advanced measurement settings.
To review or edit advanced settings, click More in the New Measurement pane.
Figure 1. Advanced measurement settings are available from the dashboard
To review or edit advanced settings, open the Details tab.
Figure 1. The Details tab displays advanced measurement settings.
To review or edit advanced settings, click More in the New Measurement pane.
Figure 1. Advanced measurement settings are available from the dashboard
The following table describes each of the advanced settings.
Option | Description | Default setting |
---|---|---|
Detector | The detector is a device inside the spectrometer that produces an electrical signal in response to the infrared beam striking it.
| |
Optical velocity | Determines the optical velocity in the interferometer. The default value is determined by the type of detector you are using, and can only be changed on certain spectrometers. On the Nicolet Summit spectrometer, the default value is 0.4747 and cannot be changed. | |
Zero fill | Interpolates data points between the collected data points. This doesn’t increase the actual resolution of the data, but can smooth out sharp features and improve the line shape of a spectrum. Options
| 2 |
Source | The component inside the spectrometer that emits the infrared radiation that travels to the detector. The source type is determined by your spectrometer setup. See your spectrometer user guide for details on the source. | |
Apodization | Apodization refers to a mathematical function that is applied to the single beam data to reduce or remove peak side-lobes that can occur because the interferogram is not an infinite set of data. Strong apodization reduces more noise but can also reduce the resolution of the data and broaden peaks. You may want to consider weaker apodization, such as Boxcar, if you are measuring spectra with very narrow peaks, such as high-resolution gas spectra. See Apodization Functions for a description of each type of apodization. | Norton-Beer Strong |
Automatic Atmospheric Suppression | Suppresses the effects of water vapor and carbon dioxide on the spectra you have collected. In general, it is better to control for atmospheric conditions using a current background spectrum. If you measure the background frequently or if atmospheric conditions change slowly, there is no need to use this feature. Use this feature only if you measure the background infrequently or when atmospheric conditions change rapidly. | Deselected |
Range Limits | Sets the limits for the range of frequencies, in wavenumber, included in the collected spectrum. | Max: 4,000 Min: 400 |
Aperture | Controls the intensity of the infrared radiation that reaches the sample. Aperture can only be changed when using spectrometers with adjustable apertures. In general, larger apertures will result in a better signal-to-noise ratio while smaller apertures result in better stability and accuracy. Small apertures are better for high-resolution measurements. You may need to use small apertures to acquire true high-resolution spectra. |
Apodization refers to a mathematical function that is applied to the single beam data to reduce or remove peak side-lobes that can occur because the interferogram is not an infinite set of data.
Strong apodization reduces more noise but can also reduce the resolution of the data and broaden peaks.
See FTIR Spectroscopy Academy for a general introduction to apodization.
The following table describes the available apodization types:
Option | Description |
---|---|
Boxcar | The interferogram is unweighted; that is, the data are simply truncated at the beginning and end. Use this type when you are measuring a gas sample, want maximum resolution and are not concerned about ringing effects (side lobes). The greatest amount of ringing will be present with this type. |
Cosine | This setting suppresses side lobes and only moderately degrades the resolution of the spectrum. This setting is similar to the Happ-Genzel and Norton-Beer medium apodization. Cosine is normally used only to reproduce the results of other experiments that used it. |
Happ-Genzel | Suppresses side lobes more effectively than the Triangular type and with less reduction in resolution than that type. (It results in more reduction in resolution than the boxcar type.) |
Norton-Beer Weak | This setting has a less pronounced smoothing effect on data than do the Norton-Beer Medium and Norton-Beer Strong types and degrades the resolution less than those types. Side lobes appear on both sides of peaks and are more pronounced for sharper peaks. Use this setting only when the best possible resolution is required. This setting is generally not recommended and is normally used only to reproduce the results of other experiments that used it. |
Norton-Beer Medium | This type has a smoothing effect on data which is between that of the Norton-Beer Weak and Norton-Beer Strong types. It suppresses side lobes as much as possible given that it only moderately degrades the resolution of the spectrum. The side lobe suppression is more significant than for Norton-Beer Weak apodization. This setting is suitable for most normal samples; it gives results virtually identical to those obtained with Happ-Genzel. |
Norton-Beer Strong | Norton-Beer Strong is the recommended apodization for the Nicolet Summit and Summit Pro spectrometers. This setting has a greater smoothing effect on data than do the Norton-Beer Weak and Norton-Beer Medium types and degrades the resolution of the spectrum more. The side-lobe suppression is more significant than for Norton-Beer Medium apodization. |
Triangular | Mathematically weights interferogram data to reduce ringing effects (side lobes), resulting in lower resolution than that obtained with the boxcar and Happ-Genzel types. Some ringing will usually be present with this type. This setting is normally used only to reproduce the results of other experiments that used it. |
Blackman-Harris | The 4-term Blackman-Harris function is a strong apodization function that is better than any of the others at suppressing side lobes. However, it results in greater line broadening than any of the others. In practice this has the effect of reducing random noise in a spectrum while causing band broadening. |