implementation of silicon photomultipliers in scintillation detector systems of the gamma-400 space...
TRANSCRIPT
Implementation of silicon photomultipliers in scintillation detector systems of the
GAMMA-400 space gamma-ray telescope
М.F. RUNTSO, A.I. ARKHANGELSKYI, I.V. ARKHANGELSKAYA, А.М. GALPER, М.D. KHEIMITZ, V.А. KAPLIN, А.А. LEONOV, V.А. LOGINOV, P. YU. NAUMOV, YU.T. YURKIN ON BEHALF OF GАММА-400 COLLABORATION, S.N. FEDOTOV, V.V. KUSHIN, S.D. LAZAREV, Е.F. MAKLYAEV, YU. A. MELIKYAN, P.P. NAUMOV, М.P. SHARAPOV, A.А. SOLODOVNIKOV
National Research Nuclear University “Moscow Engineering Physics Institute”
1The International Conference on New Photo-Detectors (PD15), Moscow, Russia, July 6 - 9, 2015
“GAMMA-400 “ Gamma-ray telescope [1]
2The International Conference on New Photo-Detectors (PD15), Moscow, Russia, July 6 - 9, 2015
Test setup for the detector’s time and amplitude characteristics study (SiPM with standart output: SensL (MICRO FB-6035-SMT)
and KITEK (PM6660-B66T99S-Q3) [2].
The International Conference on New Photo-Detectors (PD15), Moscow, Russia, July 6 - 9, 2015 3
Bicron-408
The International Conference on New Photo-Detectors (PD15), Moscow, Russia, July 6 - 9, 2015 4
Overlapping of particle and noice signals of one SiPM [6x6 mm] by Ketek and SensL
Cou
nts
per
chan
nel
QDC channel
The International Conference on New Photo-Detectors (PD15), Moscow, Russia, July 6 - 9, 2015 5
Overlapping of particle and noice signals of 6 SiPM [6x6 mm] by Ketek and SensL [2]
Noise events Particle events
SensL SiPM MICRO FB-6035-SMT biasing
The International Conference on New Photo-Detectors (PD15), Moscow, Russia, July 6 - 9, 2015 6
Snandard Output
-Vbias
0V
Test setup for the detector’s time and amplitude characteristics study (SiPM with fast output)
The International Conference on New Photo-Detectors (PD15), Moscow, Russia, July 6 - 9, 2015 7
Bicron-408
SensL SiPM MICRO FB-6035-SMT
The International Conference on New Photo-Detectors (PD15), Moscow, Russia, July 6 - 9, 2015 8
Time resolution for the tested scintillation detector as a function of the distance between the
beta-source and the appropriate set of SiPM
The International Conference on New Photo-Detectors (PD15), Moscow, Russia, July 6 - 9, 2015 9
0 20 40 60 80 1000,0
0,2
0,4
0,6
0,8
1,0
1,2 SensL KETEK SensL fast output
Tim
e r
eso
lurio
n (
FW
HM
), n
s
Distance between the beta-source and the appropriate set of SiPM, cm
The signal amplitude as a function of the distance between the beta-source and the detecting set of SiPM
The International Conference on New Photo-Detectors (PD15), Moscow, Russia, July 6 - 9, 2015 10
The dependence of the scintillation detection efficiency for the tested scintillation detectors on the distance between the
beta-source and the detecting set of SiPM [2]
The International Conference on New Photo-Detectors (PD15), Moscow, Russia, July 6 - 9, 2015 11
References
[1] O. Adriani, R.L. Aptekar, I.V. Arkhangelskaja. Status of the GAMMA-400 project.
Advances in Space Research 51 (2) , pp. 297-300
[2] Kaplin V.A., Makliaev E.F., Melikyan Yu.A. et al, Ground testing of fast scintillation
detector system of the GAMMA-400 gamma-ray telescope. Conference of
Fundamental Research and Particle Physics 18-20 February 2015 Scientific Session
MEPhI-2015 of National Research Nuclear University (MEPhI), Elsevier (in press).
The International Conference on New Photo-Detectors (PD15), Moscow, Russia, July 6 - 9, 2015 12
Thank You for Your Attention
The International Conference on New Photo-Detectors (PD15), Moscow, Russia, July 6 - 9, 2015 13