14 Reasons to Choose a Prodigy0 pages
14 Reasons to Choose the
Prodigy High Dispersion ICP
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• Prodigy’s superior
optical resolution of
0.0075 nm results in
fewer spectral interferences,
better accuracy and fewer QC failures.
Designed for Superior Performance,
Productivity and Reliability
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High Resolution Spectrometer
• For the high performance applications,
Prodigy also offers an optional user selectable
input slit allowing optical resolutions as high as 0.005 nm
to be selected. This feature further improves performance
in spectrally complex sample types.
Simultaneous ICP with State-of-the-art Array Detection
• Improves laboratory productivity because simultaneous
design permits measurement of multiple wavelengths at
the same time without extending the sample analysis time.
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Superior Wavelength Coverage
• Prodigy’s optical design allows the user to access all wavelengths
from 160 to 900 nm. This opens up previously inaccessible
wavelengths for many elements giving the analyst the ability
to achieve superior detection limits for some elements.
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• Advanced array detector permits operator to add or
change the elements of interest directly from the
instrument software.
Lower stray light
The following benefits are provided by Prodigy’s
Technically Advanced Optical Spectrometer Design
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Compact High Resolution Benchtop Instrument
• Prodigy provides superior analytical performance without
taking up more of your valuable laboratory space.
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Axial, Radial or Dual View Configurations to suit all of
today’s applications
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Image Stabilized ICP Source for fast warm-up and superior
long-term stability
• Prodigy’s long focal length optical spectrometer (800 mm)
results in lower stray light and superior performance
in complex sample matrices. Stray light is inversely
proportional to the square of the focal length. Because
Prodigy’s focal length is 2 times greater than most
competing systems it has 4 times lower the stray light.
Why choose a Prodigy ICP? For its:
State of the Art Array Detection
Compact Benchtop Design
Axial, Radial or Dual View Capability
Long-term Stability
High Resolution
Superior Wavelength Coverage
Wide Dynamic Range
Superior Productiviy