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Multi-Wavelength Astronomy
X-ray Detectors
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    • Preamble
    • Introduction
    • History of Multiwavelength Astronomy
    • Why Multi-Wavelength Astronomy?
    • Radiative Processes
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    • Optical Astronomy
    • X-ray Detectors
    • $\gamma $-ray Telescopes and Introduction to Multiwavelength Blazar Observations
    • Multiwavelength Observing Campaigns of Blazars and Other AGN
Introduction
Introduction
Proportional counters
Ionization chamber, Proportional Counters, Pulse Amplification, Detector Gas, Cascade, PSPC, Energy Resolution, Quenching, Ageing, Example: RXTE-PCA
Wolter Telescopes
Imaging, Wolter Telescopes, Mirror manufacture, Practical Example: XMM-Newton, Practical Example: Chandra
Charge Coupled Devices
X-ray CCDs, XMM-Newton: EPIC-pn CCD, XMM-Newton: EPIC-MOS CCD, Chandra: ACIS
Imaging above 10keV
Collimators, Coded Mask Telescopes, INTEGRAL: IBIS, INTEGRAL: SPI
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Introduction: IntroductionProportional counters: Ionization chamberProportional counters: Proportional CountersProportional counters: Pulse Amplification
Proportional counters: Detector GasProportional counters: Detector GasProportional counters: CascadeProportional counters: Cascade
Proportional counters: PSPCProportional counters: Energy ResolutionProportional counters: QuenchingProportional counters: Ageing
Proportional counters: Example: RXTE-PCAProportional counters: Example: RXTE-PCAProportional counters: Example: RXTE-PCAProportional counters: Example: RXTE-PCA
Proportional counters: Example: RXTE-PCAProportional counters: Example: RXTE-PCAProportional counters: Example: RXTE-PCAWolter Telescopes: Imaging
Wolter Telescopes: ImagingWolter Telescopes: ImagingWolter Telescopes: ImagingWolter Telescopes: Imaging
Wolter Telescopes: ImagingWolter Telescopes: Wolter TelescopesWolter Telescopes: Wolter TelescopesWolter Telescopes: Mirror manufacture
Wolter Telescopes: Mirror manufactureWolter Telescopes: Mirror manufactureWolter Telescopes: Mirror manufactureWolter Telescopes: Practical Example: XMM-Newton
Wolter Telescopes: Practical Example: XMM-NewtonWolter Telescopes: Practical Example: XMM-NewtonWolter Telescopes: Practical Example: XMM-NewtonWolter Telescopes: Practical Example: XMM-Newton
Wolter Telescopes: Practical Example: XMM-NewtonWolter Telescopes: Practical Example: XMM-NewtonWolter Telescopes: Practical Example: ChandraWolter Telescopes: Practical Example: Chandra
Charge Coupled Devices: X-ray CCDsCharge Coupled Devices: X-ray CCDsCharge Coupled Devices: XMM-Newton: EPIC-pn CCDCharge Coupled Devices: XMM-Newton: EPIC-pn CCD
Charge Coupled Devices: XMM-Newton: EPIC-pn CCDCharge Coupled Devices: XMM-Newton: EPIC-pn CCDCharge Coupled Devices: XMM-Newton: EPIC-MOS CCDCharge Coupled Devices: XMM-Newton: EPIC-MOS CCD
Charge Coupled Devices: Chandra: ACISCharge Coupled Devices: Chandra: ACISCharge Coupled Devices: Chandra: ACISImaging above 10keV: Collimators
Imaging above 10keV: Coded Mask TelescopesImaging above 10keV: Coded Mask TelescopesImaging above 10keV: Coded Mask TelescopesImaging above 10keV: INTEGRAL: IBIS
Imaging above 10keV: INTEGRAL: IBISImaging above 10keV: INTEGRAL: IBISImaging above 10keV: INTEGRAL: IBISImaging above 10keV: INTEGRAL: IBIS
Imaging above 10keV: INTEGRAL: IBISImaging above 10keV: INTEGRAL: SPIImaging above 10keV: INTEGRAL: SPI
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Jörn Wilms / joern.wilms@sternwarte.uni-erlangen.de