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| | These show data taken using the old preamp, GPC-01. | | These show data taken using the old preamp, GPC-01. |
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| − | 2000V - cosmics - amplitude, old preamp, tracked (left) and untracked (right)
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| − | |width="415pt"|[[Image:tracked_cosmic_amplitude_2000V_old_preamp.jpg|thumb|none|400px|old preamp, tracked cosmics, 50/50 Ar/CO2, 2000V]]
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| − | |width="415pt"|[[Image:cosmic_amplitude_2000V_old_preamp.jpg|thumb|none|400px|old preamp, cosmics, 50/50 Ar/CO2, 2000V]]
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| − | 2000V - cosmics - energy, old preamp, tracked (left) and untracked (right)
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| − | |width="415pt"|[[Image:tracked_cosmic_energy_2000V_old_preamp.jpg|thumb|none|400px|old preamp, tracked cosmics, energy, 50/50 Ar/CO2, 2000V]]
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| − | |width="415pt"|[[Image:cosmic_energy_2000V_old_preamp.jpg|thumb|none|400px|old preamp, cosmics, energy, 50/50 Ar/CO2, 2000V]]
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Revision as of 16:52, 14 June 2010
The pictures below show ADC amplitude histograms for tracked cosmic ray data with 50/50 Ar/CO2 gas mixture (the maximum ADC amplitude for each event contributes one entry for that amplitude in the histogram) and energy spectra obtained by integrating the amplitude histograms.
These show data taken using the old preamp, GPC-01.
2050V - cosmics - amplitude, old preamp, tracked (left) and untracked (right)
 old preamp, tracked cosmics, 50/50 Ar/CO2, 2050V |
 old preamp, cosmics, 50/50 Ar/CO2, 2050V |
2050V - cosmics - energy, old (left) and new (right) preamps
 old preamp, tracked cosmics, energy, 50/50 Ar/CO2, 2050V |
 old preamp, cosmics, energy, 50/50 Ar/CO2, 2050V |
