Development of a hard X-ray polarimeter for astrophysics

Citation
Ml. Mcconnell et al., Development of a hard X-ray polarimeter for astrophysics, IEEE NUCL S, 46(4), 1999, pp. 890-896
Citations number
11
Categorie Soggetti
Apllied Physucs/Condensed Matter/Materiales Science","Nuclear Emgineering
Journal title
IEEE TRANSACTIONS ON NUCLEAR SCIENCE
ISSN journal
00189499 → ACNP
Volume
46
Issue
4
Year of publication
1999
Part
1
Pages
890 - 896
Database
ISI
SICI code
0018-9499(199908)46:4<890:DOAHXP>2.0.ZU;2-I
Abstract
We have been developing a Compton scatter polarimeter for measuring the lin ear polarization of hard X-rays (100-300 keV) from astrophysical sources. A laboratory prototype polarimeter has been used to successfully demonstrate the reliability of our Monte Carlo simulation code and to demonstrate our ability to generate a polarized photon source in the lab. Our design concep t places a self-contained polarimeter module on the front-end of a a 5-inch position-sensitive PMT (PSPMT), We are currently working on the fabricatio n of a science model based on this PSPMT concept. Although the emphasis of our development effort is towards measuring hard X-rays from solar flares, our design has the advantage that it is sensitive over a rather large field -of-view (> 1 steradian), a feature that makes it especially attractive for gamma-ray burst studies.