Difference between revisions of "GEM Cosmic V792 Measurements"
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[[Image:ADC_measurement_GEMDetector_HV3800V_ADC1_11-07-08.gif|300px]][[Image:ADC_measurement_GEMDetector_HV3800V_ADC1_11-07-08_Landau_fit.gif|300px]]<br> | [[Image:ADC_measurement_GEMDetector_HV3800V_ADC1_11-07-08.gif|300px]][[Image:ADC_measurement_GEMDetector_HV3800V_ADC1_11-07-08_Landau_fit.gif|300px]]<br> | ||
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| + | =11-10-08= | ||
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| + | The pulse coming from the strips is delayed and amplified using the Timing Filter Amplifier Model_474(X6). The amplified pulse is connected to the V792 QDC.<br> | ||
| + | Run 55?<br> | ||
[http://www.iac.isu.edu/mediawiki/index.php/GEMS Go Back] | [http://www.iac.isu.edu/mediawiki/index.php/GEMS Go Back] | ||
Revision as of 00:39, 8 November 2008
11-07-08
The pulse coming from the strips is delayed and amplified using the Timing Filter Amplifier Model_474(X6). The amplified pulse is connected to the V792 QDC.
Run 550
Start Time: Nov 6 19:58:03; End Time: Nov 7 09:45:57
11-10-08
The pulse coming from the strips is delayed and amplified using the Timing Filter Amplifier Model_474(X6). The amplified pulse is connected to the V792 QDC.
Run 55?