Polaris Cd Zn Te GammaRay Imaging Spectrometer Systems

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Polaris Cd. Zn. Te Gamma-Ray Imaging Spectrometer Systems Zhong He On behalf of the

Polaris Cd. Zn. Te Gamma-Ray Imaging Spectrometer Systems Zhong He On behalf of the Orion group ISOE International ALARA Symposium Tokyo, Japan, 27 -29 August, 2013

Polaris Systems Eighteen 2 2 1. 5 cm 3 Cd. Zn. Te detectors (108

Polaris Systems Eighteen 2 2 1. 5 cm 3 Cd. Zn. Te detectors (108 cm 3, 648 grams = 1. 43 lb) Performance Goals E/E 1% FWHM (at 662 ke. V) Real-time Imaging + isotope I. D. E 1 E 2 Number of photons: 97 18 2033 4 3 2 1

Polaris 1. 1 (GMI ASIC) – August 2010

Polaris 1. 1 (GMI ASIC) – August 2010

137 Cs Energy Spectra of the 1 st Polaris system #1. 1 (From all

137 Cs Energy Spectra of the 1 st Polaris system #1. 1 (From all 18 detectors of Polaris, 24 o. C, uncollimated 137 Cs) - 1 -pixel events - 2 -pixel events - 3 -pixel events - 4 -pixel events Counts 662 ke. V 1. 44% All FWHM events Energy (ke. V)

2 nd-Generation Polaris System #2. 1 (BNL ASIC) (From all 18 detectors, room-temperature, uncollimated

2 nd-Generation Polaris System #2. 1 (BNL ASIC) (From all 18 detectors, room-temperature, uncollimated 137 Cs) 662 ke. V Single-pixel events 0. 61% (4. 0 ke. V) FWHM

2 nd-Generation Polaris System #2. 1 (BNL ASIC) (From all 18 detectors, room-temperature, uncollimated

2 nd-Generation Polaris System #2. 1 (BNL ASIC) (From all 18 detectors, room-temperature, uncollimated 137 Cs) 662 ke. V All events – no selection July 2012 0. 86% (5. 7 ke. V) FWHM Peak-to-Compton ratio 20. 5

Next-Generation digital 3 -D Cd. Zn. Te detectors (VAD_UM digital ASIC, Room-temperature, uncollimated 137

Next-Generation digital 3 -D Cd. Zn. Te detectors (VAD_UM digital ASIC, Room-temperature, uncollimated 137 Cs) Counts Energy resolutions (FWHM) of all events measured on best detectors Detector # 4 E-1 4 R-169 Entire volume 0. 56% 0. 61% From better ~50% volume 0. 46% 0. 51% E/E is still limited by ASIC noise ! Peak-to-Compton ratio 22. 5 ( 25. 1 if no event selection) Energy (ke. V) 662 ke. V 0. 46% FWHM

Counts 228 Th Energy Spectra Polaris-2 D. E. Energy (ke. V) S. E. 2614

Counts 228 Th Energy Spectra Polaris-2 D. E. Energy (ke. V) S. E. 2614 ke. V

Weiyi Wang Yuefeng Zu Willy Kaye He 60 Co 22 Na Chris Wahl 137

Weiyi Wang Yuefeng Zu Willy Kaye He 60 Co 22 Na Chris Wahl 137 Cs Polar Angle Target specific -Spec. 23 min. data EIID Azimuthal Angle

Real-Time Combined Coded Aperture and Compton Imaging for Locating Sources From all 18 detectors

Real-Time Combined Coded Aperture and Compton Imaging for Locating Sources From all 18 detectors Isotope selected: 57 Co, 22 Na, 137 Cs 122 ke. V 662 ke. V 511 ke. V 1275 ke. V

Detection Sensitivity of Polaris Image of 650 E 674 ke. V SBP with 2

Detection Sensitivity of Polaris Image of 650 E 674 ke. V SBP with 2 – 4 pixel events 208 Tl 583. 2 Source Present 214 Bi 609. 3 -Background - 137 Cs present 40 K 1461 All events A 30 Ci Cs-137 source behind a wall at ~4 m A 12 -hour “background” Measurement

Today and Tomorrow

Today and Tomorrow