Characterization of X-ray Detectors in the MIT X-ray Polarimetry Beamline

被引:1
作者
Heine, Sarah N. T. [1 ]
Marshall, Herman L. [1 ]
Schneider, Benjamin [1 ]
LaMarr, Beverly [1 ]
Kothnur, Nithya [1 ]
Garner, Alan [1 ]
机构
[1] MIT, Kavli Inst, Cambridge, MA 02139 USA
来源
X-RAY, OPTICAL, AND INFRARED DETECTORS FOR ASTRONOMY XI | 2024年 / 13103卷
关键词
X-ray; astronomy; sCMOS; detectors; polarimetry;
D O I
10.1117/12.3020451
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The MIT X-ray Polarimetry Beamline is a facility that we developed for testing components for possible use in X-ray polarimetry. Over the past few years, we have demonstrated that the X-ray source can generate nearly 100% polarized X-rays at various energies from 183 eV (Boron K alpha) to 705 eV (Fe L alpha) using a laterally graded multilayer coated mirror (LGML) oriented at 45 degrees to the source. The position angle of the polarization can be rotated through a range of roughly 150 degrees. In a downstream chamber, we can orient a Princeton Instruments MTE1300B CCD camera to observe the polarized light either directly or after reflection at 45 degrees by a second LGML. In support of the REDSoX Polarimeter project, we have tested four other detectors by directly comparing them to the PI camera. Two were CCD cameras: a Raptor Eagle XV and a CCID94 produced by MIT Lincoln Laboratories, and two had sCMOS sensors: the Sydor Wraith with a GSENSE 400BSI sensor and a custom Sony IMX290 sensor. We will show results comparing quantum efficiencies and event images in the soft X-ray band.
引用
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页数:12
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