Title: | Design, construction, and test of the Gas Pixel Detectors for the IXPE mission |
Authors: | Baldini, L. Barbanera, M. Bellazzini, R. Bonino, R. Borotto, F. Brez, A. Caporale, C. Cardelli, C. Castellano, S. Ceccanti, M. Citraro, S. Di Lalla, N. Latronico, L. Lucchesi, L. Magazzù, C. Magazzù, G. Maldera, S. Manfreda, A. Marengo, M. Marrocchesi, A. Mereu, P. Minuti, M. Mosti, F. Nasimi, H. Nuti, A. Oppedisano, C. Orsini, L. Pesce-Rollins, M. Pinchera, M. Profeti, A. Sgrò, C. Spandre, G. Tardiola, M. Zanetti, D. AMICI, FABRIZIO Andersson, H. ATTINA', Primo BACHETTI, Matteo Baumgartner, W. BRIENZA, Daniele Carpentiero, R. Castronuovo, M. Cavalli, L. Cavazzuti, E. CENTRONE, Mauro COSTA, Elia D'Alba, E. D'Amico, F. DEL MONTE, Ettore Di Cosimo, S. DI MARCO, Alessandro DI PERSIO, GIUSEPPE Donnarumma, I. EVANGELISTA, YURI FABIANI, Sergio Ferrazzoli, R. Kitaguchi, T. LA MONACA, Fabio LEFEVRE, CARLO LOFFREDO, Pasqualino Lorenzi, P. Mangraviti, E. Matt, G. Meilahti, T. MORBIDINI, Alfredo MULERI, FABIO Nakano, T. Negri, B. Nenonen, S. O'Dell, S. L. PERRI, Matteo PIAZZOLLA, RAFFAELE Pieraccini, S. PILIA, Maura Puccetti, S. Ramsey, B. D. Rankin, J. Ratheesh, A. Rubini, A. SANTOLI, Francesco Sarra, P. Scalise, E. Sciortino, A. SOFFITTA, PAOLO Tamagawa, T. Tennant, A. F. TOBIA, ANTONINO TROIS, Alessio Uchiyama, K. Vimercati, M. Weisskopf, M. C. XIE, FEI Zanetti, F. Zhou, Y. |
Issue Date: | 2021 |
Journal: | ASTROPARTICLE PHYSICS |
Number: | 133 |
First Page: | 102628 |
Abstract: | Due to be launched in late 2021, the Imaging X-ray Polarimetry Explorer (IXPE) is a NASA Small Explorer mission designed to perform polarization measurements in the 2-8 keV band, complemented with imaging, spectroscopy and timing capabilities. At the heart of the focal plane is a set of three polarization-sensitive Gas Pixel Detectors (GPD), each based on a custom ASIC acting as a charge-collecting anode. <P />In this paper we shall review the design, manufacturing, and test of the IXPE focal-plane detectors, with particular emphasis on the connection between the science drivers, the performance metrics and the operational aspects. We shall present a thorough characterization of the GPDs in terms of effective noise, trigger efficiency, dead time, uniformity of response, and spectral and polarimetric performance. In addition, we shall discuss in detail a number of instrumental effects that are relevant for high-level science analysis-particularly as far as the response to unpolarized radiation and the stability in time are concerned. |
URI: | http://hdl.handle.net/20.500.12386/35882 |
URL: | https://www.sciencedirect.com/science/article/pii/S0927650521000670?via%3Dihub https://www.sciencedirect.com/science/article/pii/S0927650521000670?via%3Dihub |
ISSN: | 0927-6505 |
DOI: | 10.1016/j.astropartphys.2021.102628 |
Bibcode ADS: | 2021APh...13302628B |
Fulltext: | open |
Appears in Collections: | 1.01 Articoli in rivista
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