14 MHz rate photon counting with room temperature InGaAs/InP avalanche photodiodes

2004 ◽  
Vol 51 (9-10) ◽  
pp. 1369-1379
Author(s):  
Paul L. Voss ◽  
Kahraman G. Köprülü ◽  
Sang-Kyung Choi ◽  
Sarah Dugan ◽  
Prem Kumar
2004 ◽  
Vol 51 (9-10) ◽  
pp. 1369-1379 ◽  
Author(s):  
Paul L. Voss ◽  
Kahraman G. Köprülü ◽  
Sang-Kyung Choi ◽  
Sarah Dugan ◽  
Prem Kumar

2000 ◽  
Vol 76 (26) ◽  
pp. 3938-3940 ◽  
Author(s):  
K. A. McIntosh ◽  
R. J. Molnar ◽  
L. J. Mahoney ◽  
K. M. Molvar ◽  
N. Efremow ◽  
...  

2020 ◽  
Vol 27 (2) ◽  
pp. 319-328 ◽  
Author(s):  
Leonardo Abbene ◽  
Fabio Principato ◽  
Gaetano Gerardi ◽  
Antonino Buttacavoli ◽  
Donato Cascio ◽  
...  

In this work, the spectroscopic performances of new cadmium–zinc–telluride (CZT) pixel detectors recently developed at IMEM-CNR of Parma (Italy) are presented. Sub-millimetre arrays with pixel pitch less than 500 µm, based on boron oxide encapsulated vertical Bridgman grown CZT crystals, were fabricated. Excellent room-temperature performance characterizes the detectors even at high-bias-voltage operation (9000 V cm−1), with energy resolutions (FWHM) of 4% (0.9 keV), 1.7% (1 keV) and 1.3% (1.6 keV) at 22.1, 59.5 and 122.1 keV, respectively. Charge-sharing investigations were performed with both uncollimated and collimated synchrotron X-ray beams with particular attention to the mitigation of the charge losses at the inter-pixel gap region. High-rate measurements demonstrated the absence of high-flux radiation-induced polarization phenomena up to 2 × 106 photons mm−2 s−1. These activities are in the framework of an international collaboration on the development of energy-resolved photon-counting systems for high-flux energy-resolved X-ray imaging.


1995 ◽  
Vol 151 ◽  
pp. 129-130
Author(s):  
D. Dravins ◽  
L. Lindegren ◽  
E. Mezey

AbstractInstrumentation and observing methods are developed for optical high-speed astrophysics, aiming at exploring milli-, micro-, and nanosecond variability. Such rapid fluctuations can be expected from instabilities in accretion flows, and in the fine structure of photon emission. For the optical, we have constructed a dedicated instrument, whose first version was tested on La Palma to study atmospheric scintillation on very short timescales. A second version is now under development, using photon-counting avalanche photodiodes as detectors.


2017 ◽  
Author(s):  
S. Masoodian ◽  
J. Ma ◽  
D. Starkey ◽  
T. J. Wang ◽  
Y. Yamashita ◽  
...  

1993 ◽  
Vol 32 (21) ◽  
pp. 3894 ◽  
Author(s):  
Henri Dautet ◽  
Pierre Deschamps ◽  
Bruno Dion ◽  
Andrew D. MacGregor ◽  
Darleene MacSween ◽  
...  

2002 ◽  
Vol 27 (4) ◽  
pp. 219 ◽  
Author(s):  
Alison Y. Loudon ◽  
Philip A. Hiskett ◽  
Gerald S. Buller ◽  
Roger T. Carline ◽  
Dave C. Herbert ◽  
...  

2006 ◽  
Vol 89 (11) ◽  
pp. 111102 ◽  
Author(s):  
E. A. Dauler ◽  
P. I. Hopman ◽  
K. A. McIntosh ◽  
J. P. Donnelly ◽  
E. K. Duerr ◽  
...  

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