Ionization by photoelectrons and their secondaries. X-ray sensors, incident X-ray photons are converted into a number ofД®lectron-hole pairs via photoelectric absorption and subsequent The XIS is composed of four units of Si-based X-rayД¬harge coupled device (CCD) cameras (Fig. Weight of 48.7kg and consumes 67W at a bus voltage of 50V during The instrument has been operated successfully since The X-ray Imaging Spectrometer (XIS, Koyama et al., 2007) celebrated itsДЇirst light on 2006, August 11, about a month after the launch of 7.4.1 Pulse Height Determination & Hot Pixel Rejection.7.3.4.2.3 NXB contamination due to the day Earth.7.3.4.2.2 NXB change due to the XIS1 SCI increase.7.3.4.2.1 NXB change due to the XIS0 anomaly.7.3.4.2 NXB Notes for Users & Proposers.7.3.4.1.2 NXB cut-off rigidity dependence.7.3.3.2 Contamination Notes for Users & Proposers.7.3.3.1.3 Spatial dependence of the thickness of the contaminant.7.3.3.1.2 Time dependence of the thickness of the contaminant.7.3.3.1.1 Time dependence of the chemical composition of the contaminant.

7.3.3.1 Contamination Calibration Results.7.3.3 Contamination & Low Energy Quantum Efficiency Degradation.7.3.2.4 Energy Calibration Notes for Users & Proposers.7.3.2.3 Energy Calibration Results (3) - Other Editing Modes.7.3.2.2 Energy Calibration Results (2) - Other Clocking Modes.7.3.2.1 Energy Calibration Results (1) - Normal Mode (No Options).7.3.1.3 SCI Notes for Users & Proposers.7.3.1 Spaced-Row Charge Injection (SCI).7.2.2 Systematic Observational Effects and their Mitigation.7.2.1.2.3 Editing modes for diagnastics.7.2.1.2.1 Editing modes for observations.7.2.1.0.3 Declaration of the use of non-default setting.7.2.1.0.2 Observations requiring non-default settings.7.1.2.1.3 Optical blocking filter (OBF).Next: Bibliography Up: Suzaku Technical Description Previous: 6.

Ae pixel sorter 1.0.2