The XENON 100 Detector for Dark Matter Searches
The XENON 100 Detector for Dark Matter Searches
The XENON 100 Detector for Dark Matter Searches
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S1 signal<br />
Calibration with 137 Cs source<br />
Drift time correction<br />
2000<br />
1800<br />
14<br />
S1 [phe]<br />
1600<br />
1400<br />
1200<br />
<strong>100</strong>0<br />
800<br />
600<br />
400<br />
200<br />
12<br />
10<br />
8<br />
6<br />
4<br />
2<br />
S2 [phe]<br />
0<br />
0 20 40 60 80 <strong>100</strong> 120 140 160<br />
drift time [µs]<br />
S2 signal<br />
xe<strong>100</strong>_090629_1227<br />
xe<strong>100</strong>_090601_1622<br />
3<br />
"10<br />
200<br />
S2<br />
180<br />
160<br />
140<br />
!"#$%&'( ()*+,+<br />
-&."(/( ((0*123<br />
(51,53&6+,<br />
-&."(4(,105,&6+,<br />
!"#$%&'( (*+5)<br />
-&."(( ((001+5<br />
-&."(4(<br />
! 3 (7("89(<br />
()):1;(7(,2<br />
?=@&(((( (!+1++,*53( #(+1++++;0<br />
120<br />
<strong>100</strong><br />
80<br />
60<br />
40<br />
20<br />
0<br />
0 20 40 60 80 <strong>100</strong> 120 140 160<br />
drift time [!s]<br />
0<br />
4.5<br />
4<br />
3.5<br />
3<br />
2.5<br />
2<br />
1.5<br />
1<br />
0.5<br />
0<br />
Alexander Kish | <strong>XENON</strong>-<strong>100</strong> | 5th Patras Workshop on Axions, WIMPs and WISPs | University of Durham | July 13, 2009 | Slide 21
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