Difference between revisions of "GEM Cosmic V792 Measurements"
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[[Image:ADC_measurement_GEMDetector_HV3800V_ADC1_11-04-08.gif|300px]][[Image:ADC_measurement_GEMDetector_HV3800V_ADC1_11-04-08_log_scale.gif|300px]]<br> | [[Image:ADC_measurement_GEMDetector_HV3800V_ADC1_11-04-08.gif|300px]][[Image:ADC_measurement_GEMDetector_HV3800V_ADC1_11-04-08_log_scale.gif|300px]]<br> | ||
[[Image:ADC_measurement_GEMDetector_HV3800V_ADC1_11-04-08_zoomed_in.gif|400px]]<br> | [[Image:ADC_measurement_GEMDetector_HV3800V_ADC1_11-04-08_zoomed_in.gif|400px]]<br> | ||
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| + | =11-05-08= | ||
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| + | The pulse coming from the strips is delayed and amplified using the Timing Filter Amplifier Model_474(Fine gain ~6). The amplified pulse is connected to the V792 QDC. | ||
Revision as of 01:02, 5 November 2008
11-04-08
11-05-08
The pulse coming from the strips is delayed and amplified using the Timing Filter Amplifier Model_474(Fine gain ~6). The amplified pulse is connected to the V792 QDC.