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A&A Supplement series, Vol. 122, April II 1997, 357-369

Received May 15; accepted June 3, 1996

The high energy instrument PDS on-board the BeppoSAX X-ray astronomy satellite

F. Fronteratex2html_wrap1264 - E. Costatex2html_wrap1266 - D. Dal Fiumetex2html_wrap1268 - M. Ferocitex2html_wrap1270 - L. Nicastrotex2html_wrap1272 - M. Orlandinitex2html_wrap1274 - E. Palazzitex2html_wrap1276 - G. Zavattinitex2html_wrap1278

Send offprint request: frontera@tesre.bo.cnr.it

tex2html_wrap1280  Istituto Tecnologie e Studio Radiazioni Extraterrestri, CNR, Via Gobetti, 101, 40129 Bologna, Italy
tex2html_wrap1282  Dipartimento di Fisica, Università di Ferrara, Via Paradiso, 11, 44100 Ferrara, Italy
tex2html_wrap1284  Istituto di Astrofisica Spaziale, CNR, Via E. Fermi, 21, 00044 Frascati, Italy

Abstract:

BeppoSAX/PDS experiment is one of four narrow field instruments of the BeppoSAX payload, that also includes two wide field cameras. The goal of PDS is to extend the energy range of BeppoSAX to hard X-rays. The operative energy range of PDS is 15 to 300 keV, where the experiment can perform sensitive spectral and temporal studies of celestial sources. The PDS detector is composed of 4 actively shielded NaI(Tl)/CsI(Na) phoswich scintillators with a total geometric area of tex2html_wrap_inline1252 and a field of view of 13 (FWHM). In this paper we describe the experiment design and discuss its functional performance and calibration data analysis system.

keywords: instrumentation: detectors -- space vehicles -- X-ray: general





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