
PIXIE-4 User’s Manual
V2.69
©
XIA
2015. All rights reserved.
ix
Figure 2.3:
O
SCILLOSCOPE
panel with typical pulses from a pulser.
3.
In the
Energy
tab of the P
ARAMETER
S
ETUP
panel, input an estimated preamplifier
exponential RC decay time for
Tau
, and then click on
Auto Find Tau
to determine the
actual Tau value for all channels of the current module. You can also enter a known
good Tau value directly in the
Tau
control field, or use the controls in the
O
SCILLOSCOPE
to manually fit Tau for a pulse.
4.
Save the modified parameter settings to file. To do so, click on the
Save
button at the
bottom of the P
ARAMETER
S
ETUP
panel to open a save file dialog. Create a new file
name to avoid overwriting the default settings file.
5.
Save the Igor experiment using
File -> Save Experiment As
from the top menu. This
saves the current state of the interface with all open panels and the settings for file paths
and slot numbers (the settings independent of module parameters).
6.
Click on the
Run Control
tab, set
Run Type
to “0x301 MCA Mode”,
Poll time
to 1
second, and
Run time
to 30 seconds or so, then click on the
Start Run
button. A spinning
wheel will appear occasionally in the lower left corner of the screen as long as the
system is waiting for the run to finish. If you click the
Update
button in the M
AIN
panel,
the count rates displayed in the Results group are updated.
7.
After the run is complete, select
MCA Spectrum
from the
Open Panels
popup menu in
the Results group of the M
AIN
panel. The MCA
SPECTRUM
graph
shows the MCA
histograms for all four channels. You can deselect other channels while working on
only one channel. After defining a range in the spectrum with the cursors and setting
the fit option to
fit peaks between cursors
, you can apply a Gauss fit to the spectrum by
selecting the channels to be fit in the
Fit
popup menu. You can alternatively enter the
fit limits using the
Min
and
Max
fields in the table or by specifying a
Range
around the
tallest peak or the peak with the highest energy. To scale the spectrum in keV, enter the
appropriate ratio in the field
keV/bin
.