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Titel: Development of a 3D CZT detector prototype for Laue Lens telescope
Type: Conference articleConference article
Person(er):
Forfatter:  Caroli, Ezio
IASF-Bologna, INAF

Forfatter:  Auricchio, Natalia
IASF-Bologna, INAF

Forfatter:  Del Sordo, Stefano
IASF-Palermo, INAF

Forfatter:  Abbene, Leonardo
IASF-Palermo, INAF

Forfatter:  Budtz-Jørgensen, Carl (Cwisno: 38278)
Technical University of Denmark
Email:

Forfatter:  Casini, Fabio
IASF-Milano, INAF

Forfatter:  Curado da Silva, Rui M.
Universidade de Coimbra, Departamento de Física

Forfatter:  Kuvvetli, Irfan (Cwisno: 7703)
Technical University of Denmark
Email:

Forfatter:  Milano, Luciano
Università di Ferrara, Dipartimento di Fisica

Forfatter:  Natalucci, Lorenzo
IASF-Roma, INAF

Forfatter:  Quadrini, Egidio M.
IASF-Milano, INAF

Forfatter:  Stephen, John B.
IASF-Bologna, INAF

Forfatter:  Ubertini, Pietro
IASF-Roma, INAF

Forfatter:  Zanichelli, Massimiliano
IMEM, CNR

Forfatter:  Zappettini, Andrea
IMEM, CNR

Uddrag: We report on the development of a 3D position sensitive prototype suitable as focal plane detector for Laue lens telescope. The basic sensitive unit is a drift strip detector based on a CZT crystal, (~19×8 mm2 area, 2.4 mm thick), irradiated transversally to the electric field direction. The anode side is segmented in 64 strips, that divide the crystal in 8 independent sensor (pixel), each composed by one collecting strip and 7 (one in common) adjacent drift strips. The drift strips are biased by a voltage divider, whereas the anode strips are held at ground. Furthermore, the cathode is divided in 4 horizontal strips for the reconstruction of the third interaction position coordinate. The 3D prototype will be made by packing 8 linear modules, each composed by one basic sensitive unit, bonded on a ceramic layer. The linear modules readout is provided by a custom front end electronics implementing a set of three RENA-3 for a total of 128 channels. The front-end electronics and the operating logics (in particular coincidence logics for polarisation measurements) are handled by a versatile and modular multi-parametric back end electronics developed using FPGA technology.
Publiceret: in journal: Proceedings of SPIE, the International Society for Optical Engineering (ISSN: 0277-786X) (DOI: http://dx.doi.org/10.1117/12.858120), vol: 7742, pages: 77420V, 2010
DOI:
Fil(er):
Præsenteret ved: High Energy, Optical, and Infrared Detectors for Astronomy, San Diego, California United States
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