Gas Pixel Detectors for X-ray Polarimetry applications

• Main Authors: Bellazzini, R, Angelini, F, Baldini, L, Bitti, F, Brez, A, Cavalca, F, Del Prete, M, Kuss, M, Latronico, L, Omodei, N, Pinchera, M, Massai, M. M, Minuti, M, Razzano, M, Sgro, C, Spandre, G, Tenze, A, Costa, E, Soffitta, P
• Format: Journal Article
• Language: English
• Published: 09-12-2005
• Subjects: Physics - Astrophysics of Galaxies; Physics - Cosmology and Nongalactic Astrophysics; Physics - Earth and Planetary Astrophysics; Physics - High Energy Astrophysical Phenomena; Physics - High Energy Physics - Phenomenology; Physics - Instrumentation and Detectors; Physics - Instrumentation and Methods for Astrophysics; Physics - Solar and Stellar Astrophysics
• DOI: 10.48550/arxiv.astro-ph/0512242

Nucl.Instrum.Meth.A560:425-434,2006 We discuss a new class of Micro Pattern Gas Detectors, the Gas Pixel Detector
(GPD), in which a complete integration between the gas amplification structure
and the read-out electronics has been reached. An Application-Specific
Integrated Circuit (ASIC) built in deep sub-micron technology has been
developed to realize a monolithic device that is, at the same time, the
pixelized charge collecting electrode and the amplifying, shaping and charge
measuring front-end electronics. The CMOS chip has the top metal layer
patterned in a matrix of 80 micron pitch hexagonal pixels, each of them
directly connected to the underneath electronics chain which has been realized
in the remaining five layers of the 0.35 micron VLSI technology. Results from
tests of a first prototype of such detector with 2k pixels and a full scale
version with 22k pixels are presented. The application of this device for
Astronomical X-Ray Polarimetry is discussed. The experimental detector response
to polarized and unpolarized X-ray radiation is shown. Results from a full
MonteCarlo simulation for two astronomical sources, the Crab Nebula and the
Hercules X1, are also reported.