Search results for "International X-ray Observatory"

showing 4 items of 4 documents

The IXO Wide-Field Imager

2010

The Wide Field Imager (WFI) of the International X-ray Observatory (IXO) is an X-ray imaging spectrometer based on a large monolithic DePFET (Depleted P-channel Field Effect Transistor) Active Pixel Sensor. Filling an area of 10 × 10 cm² with a format of 1024 × 1024 pixels it will cover a field of view of 18 arcmin. The pixel size of 100 × 100 μm² corresponds to a fivefold oversampling of the telescope's expected 5 arcsec point spread function. The WFI's basic DePFET structure combines the functionalities of sensor and integrated amplifier with nearly Fano-limited energy resolution and high efficiency from 100 eV to 15 keV. The development of dedicated control and amplifier ASICs allows for…

X-ray AstronomyImaging spectrometerWide Field ImagerField of viewSettore ING-INF/01 - ElettronicaIntegrated amplifierlaw.inventionTelescopeOpticslawWFIDePFETX-ray SpectroscopyInternational X-ray Observatory; IXO; Wide Field Imager; WFI; X-ray Astronomy; X-ray Spectroscopy; X-ray Imaging; DePFET; Active Pixel SensorPhysicsCMOS sensorActive Pixel SensorPixelSpectrometersezelebusiness.industryAmplifierIXObusinessInternational X-ray ObservatoryX-ray Imaging
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The Wide Field Imager of the International X-ray Observatory

2010

The International X-ray Observatory (IXO) will be a joint X-ray observatory mission by ESA, NASA and JAXA. It will have a large effective area (3 m 2 at 1.25 keV) grazing incidence mirror system with good angular resolution (5 arcsec at 0.1–10 keV) and will feature a comprehensive suite of scientific instruments: an X-ray Microcalorimeter Spectrometer, a High Time Resolution Spectrometer, an X-ray Polarimeter, an X-ray Grating Spectrometer, a Hard X-ray Imager and a Wide-Field Imager. The Wide Field Imager (WFI) has a field-of-view of 18 ft � 18 ft. It will be sensitive between 0.1 and 15 keV, offer the full angular resolution of the mirrors and good energy resolution. The WFI will be imple…

X ray astronomyNuclear and High Energy PhysicsInternational X-ray ObservatorySettore ING-INF/01 - Elettronicalaw.inventionImagingOpticsObservatorylawAngular resolutionInstrumentationSpectroscopyPhysicsActive Pixel SensorsezeleSpectrometerbusiness.industryAmplifierTransistorDetectorPolarimeterIXOOptoelectronicsbusinessDEPFETIXO; X ray astronomy; DEPFET; Active Pixel Sensor; Imaging; Spectroscopy
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The wide field imager for the International X-ray Observatory

2009

The large collecting area of the X-ray optics on the International X-ray Observatory (IXO), their good angular resolution, the wide bandwidth of X-ray energies and the high radiation tolerance required for the X-ray detectors in the focal plane have stimulated a new development of devices which unify all those science driven specifications in one single detector. The concept of a monolithic, back-illuminated silicon active pixel sensor (APS) based on the DEPFET structure is proposed for the IXO mission, being a fully depleted, back-illuminated 450 μm thick detector with a physical size of about 10 × 10 cm 2 corresponding to the 18 arcmin field of view. The backside will be covered with an i…

PhysicsCMOS sensorbusiness.industryDetectorInternational X-ray ObservatoryX-ray detectorX-ray opticsField of viewSettore ING-INF/01 - ElettronicaOpticsObservatoryOptoelectronicsbusinessImage resolutionSPIE Proceedings
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The wide-field imager for IXO: status and future activities

2010

The Wide Field Imager (WFI) of the International X-ray Observatory (IXO) is an X-ray imaging spectrometer based on a large monolithic DePFET (Depleted P-channel Field Effect Transistor) Active Pixel Sensor. Filling an area of 10 x 10 cm2 with a format of 1024 x 1024 pixels it will cover a field of view of 18 arcmin. The pixel size of 100 x 100 μm2 corresponds to a fivefold oversampling of the telescope's expected 5 arcsec point spread function. The WFI's basic DePFET structure combines the functionalities of sensor and integrated amplifier with nearly Fano-limited energy resolution and high efficiency from 100 eV to 15 keV. The development of dedicated control and amplifier ASICs allows for…

X-ray AstronomyImaging spectrometerWide Field ImagerField of viewSettore ING-INF/01 - ElettronicaIntegrated amplifierlaw.inventionTelescopeOpticslawWFIDePFETX-ray SpectroscopyInternational X-ray Observatory; IXO; Wide Field Imager; WFI; X-ray Astronomy; X-ray Spectroscopy; X-ray Imaging; DePFET; Active Pixel SensorPhysicsCMOS sensorActive Pixel SensorsezelePixelSpectrometerbusiness.industryAmplifierIXOInternational X-ray ObservatorybusinessX-ray ImagingSpace Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray
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