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2017 Fiscal Year Final Research Report

Improvement of the time resolution for X-ray CCD camera by new clocking mode

Research Project

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Project/Area Number 26800144
Research Category

Grant-in-Aid for Young Scientists (B)

Allocation TypeMulti-year Fund
Research Field Particle/Nuclear/Cosmic ray/Astro physics
Research InstitutionTohoku Gakuin University

Principal Investigator

Murakami Hiroshi  東北学院大学, 教養学部, 准教授 (00415902)

Research Collaborator UMEZU Rika  
Project Period (FY) 2014-04-01 – 2018-03-31
KeywordsCCD / X線天文学 / 人工衛星 / 電子デバイス・機器
Outline of Final Research Achievements

CCD camera is the standard detector in X-ray astronomy. The problem of the CCD camera is long exposure time of the frame. We cannot observe rapid variation of the X-ray objects with CCD cameras. The long exposure time also invoke another problem. If two or more X-ray photons irradiate narrow region, the X-ray events are mixed, and cannot be distinguished. To avoid these problem, we try new clocking method. During the exposure, several lines are transferred, and X-ray photons irradiate elongated region. We estimate the effectivity of new clocking mode. We also drive CCD camera with new clock, and confirm the availability of the mode.

Free Research Field

X線天文学

URL: 

Published: 2019-03-29  

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