A pixel-by-pixel equalization method for the X-ray imaging polarimeter on board the IXPE mission

被引:1
|
作者
Rankin, John [1 ]
Muleri, Fabio [1 ]
Costa, Enrico [1 ]
Di Marco, Alessandro [1 ]
Fabiani, Sergio [1 ]
La Monaca, Fabio [1 ]
Soffitta, Paolo [1 ]
Baldini, Luca [2 ]
Manfreda, Alberto [3 ]
O'Dell, Stephen L. [4 ]
Perri, Matteo [5 ]
Puccetti, Simonetta [6 ]
Ramsey, Brian D. [4 ]
Sgro, Carmelo [3 ]
Tennant, Allyn F. [4 ]
Weisskopf, Martin C. [4 ]
机构
[1] INAF Ist Astrofis & Planetol Spaziali, Rome, Italy
[2] Univ Pisa, Pisa, Italy
[3] Ist Nazl Fis Nucl, Pisa, Italy
[4] NASA Marshall Space Flight Ctr, Huntsville, AL 35808 USA
[5] INAF Osservatorio Astron Roma, Rome, Italy
[6] Agenzia Spaziale Italiana, Rome, Italy
来源
SPACE TELESCOPES AND INSTRUMENTATION 2022: ULTRAVIOLET TO GAMMA RAY | 2022年 / 12181卷
基金
美国国家航空航天局;
关键词
X-ray polarimetry; gas pixel detectors; X-ray Astronomy; Pixel Calibration;
D O I
10.1117/12.2630042
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
On December 9, 2021, the Imaging X-ray Polarimetry Explorer (IXPE) observatory was launched, carrying three X-ray polarimeters based upon the Gas Pixel Detector (GPD). These devices measure the photoelectron's ionization track following absorption of an X-ray, from which the photoelectron's initial direction (correlated to the polarization position angle) is determined. Here we describe a method for event-by-event correction of pixel-by-pixel gain variations, which are found to be +/-20%, by comparing the charge in each pixel with the average at the same relative position inside tracks of the same shape. Using the large dataset acquired during on-ground calibration of the IXPE detectors, we have individually calibrated each of the 300x352 pixels of each detector's ASIC. We discuss the performance improvements obtained using this method, which may be relevant to other instruments that detect individual events through images.
引用
收藏
页数:10
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