Mantis 5000 Especificaciones Pagina 80

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UV/VIS 0%T Correction
This calibrates the photomultipliers for 0%T (electronic zero) effects. This is executed
every time the instrument is switched on except if a DRA is installed (where the DRA
correction factors stored in the DRA EEPROM are used).
Instrument check: If high precision is needed at high absorbance, measure the 0%T error
at 500 nm in the UV-VIS (blocked sample beam). The error should be less than 0.01 %T.
Calibrate with the instrument fully warmed up. It may be desirable to calibrate Calibrate
PGA prior to this. Click here
for the instrument parameters.
NIR 0%T Correction
This is the NIR equivalent for 0%T error.
Instrument check: After instrument has fully warmed up, go to wavelength 1200 nm with
grating change at 800 nm and block the sample beam with a black metal mask. If the
error exceeds 0.1 %T calibration may be required.
Calibration using Cary Win UV Software
The recommended method for performing calibration is by using the Auto Calibrate
function in the Validate application.
Caution
Both instrument and DRA are calibrated at the factory and should be recalibrated only
when tests indicate the need for it. Failure to complete or the use of incorrect filters may
render the instrument unusable.
Signal processing
This causes the Cary system to calibrate the programmable gain amplifiers on the
photomultiplier tube. This test is performed during initialization of the Cary
4000/5000/6000i instruments.
UV/Vis 0 %T correction
This causes the Cary system to close the shutter and calibrate the UV/Vis detector for 0
%T errors. If a DRA is connected a mask must be placed in front of the transmission port
(rear instrument beam) during the calibration process. The software will prompt you for
this.
Note
This calibration is part of the normal initialization procedure, however calibration
is advised when working at high absorbance where a repeat calibration after the
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