Abstract

MAXI, Monitor of All-sky X-ray Image, is the X-ray observatory on the Japanese experimental module (JEM) Exposed Facility (EF) on the International Space Station (ISS). MAXI is a slit scanning camera which consists of two kinds of X-ray detectors: one is a one-dimensional position-sensitive proportional counter with a total area of ∼5000cm2\sim 5000 cm^2, the Gas Slit Camera (GSC), and the other is an X-ray CCD array with a total area ∼200cm2\sim 200 cm^2, the Solid-state Slit Camera (SSC). The GSC subtends a field of view with an angular dimension of 1βˆ˜Γ—180∘^\circ\times 180^\circ while the SSC subtends a field of view with an angular dimension of 1∘^\circ times a little less than 180∘^\circ. In the course of one station orbit, MAXI can scan almost the entire sky with a precision of 1∘^\circ and with an X-ray energy range of 0.5-30 keV. We have developed the engineering model of CCD chips and the analogue electronics for the SSC. The energy resolution of EM CCD for Mn KΞ±\alpha has a full-width at half maximum of ≃\simeq 182 eV. Readout noise is ≃\simeq 11 e^- rms.Comment: 10 pages, 4 figures Accepted for Nuclear Instruments and Method in Physics Researc

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    Last time updated on 15/02/2019