AIDA
GELINA
BRIKEN
nToF
CRIB
ISOLDE
CIRCE
nTOFCapture
DESPEC
DTAS
EDI_PSA
179Ta
CARME
StellarModelling
DCF
K40
DTAS
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<p>Start: 16:25</p> <p>Stop: 17:25</p> <p>Background in the same conditions as before (right after the Co measurement)</p> <p>Listmode: Background_201905201614_035.dlt .... Background_201905201614_036.dlt</p> <p>Root file: 201905201725_background.root</p> <p>Rates:</p> <p>Dynodes: 8.5 kHz</p> <p>Anodes: 1.8 kHz</p> <p>Anod1: 120 Hz</p> <p>Anod15: 173 Hz</p> <p>Dynod1: 80 Hz</p> <p>Dynod 15: 166 Hz</p> <p>Pulser set to 10 Hz</p> <p>Rate of Dynode 5, 15, 17 seem a little higher than the others. The same for Anode 11, 15, 17</p> <p>Not clear why the Dynodes rate is so high compared with the anodes. There is not such a big</p> <p>difference in rate of the individual detectors. </p> <p>(Dynodes and Anodes rates are taken from the Python script written by Jorge, that correspond to the full card)</p> <p>Later it become evident that probably we need to increase the threshold of detector 8 again (Dy08).</p> <p>Before it was not like that, but now seems to be triggering in the noise.</p> <p> </p> <p> </p>
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