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[PDF] Top 20 The ATHENA X-ray Integral Field Unit (X-IFU)

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The ATHENA X-ray Integral Field Unit (X-IFU)

The ATHENA X-ray Integral Field Unit (X-IFU)

... The X-IFU is the cryogenic micro-calorimeter of the Athena space X-ray observatory, the second large mission of the Cosmic Vision Program of ... Voir le document complet

15

The X-ray Integral Field Unit (X-IFU) for Athena

The X-ray Integral Field Unit (X-IFU) for Athena

... implement the Hot and Energetic Universe science theme selected by the European Space Agency for the second large mission of its Cosmic Vision ...program. The Athena science payload ... Voir le document complet

13

The Athena X-ray Integral Field Unit (X-IFU)

The Athena X-ray Integral Field Unit (X-IFU)

... 3.2.10 The reference X-IFU cyrogenic chain The X-IFU cyrogenic chain, and its potential evolution is presented in ...from the Athena Concurrent Design Facility ... Voir le document complet

41

De l'astrophysique des amas de galaxies à la physique des microcalorimètres en rayons X : performances scientifiques et calibration du X-ray integral field unit de la mission Athena

De l'astrophysique des amas de galaxies à la physique des microcalorimètres en rayons X : performances scientifiques et calibration du X-ray integral field unit de la mission Athena

... from the operating temperature of the outer vessel (OV) around ∼ 300 K, the X-IFU detectors will be surrounded by a closed cryostat made of six different temperature ...shields. ... Voir le document complet

260

The Athena X-ray observatory and the Liège contribution to the X-IFU instrument

The Athena X-ray observatory and the Liège contribution to the X-IFU instrument

... • X-ray Integral Field Unit: cryogenic imaging spectrometer, based on Transition Edge Sensors, operated at 50 mK • Energy resolution ... Voir le document complet

13

Développement d'un simulateur pour le X-ray integral field unit : du signal astrophysique à la performance instrumentale

Développement d'un simulateur pour le X-ray integral field unit : du signal astrophysique à la performance instrumentale

... My work has been mostly organized into two steps: the first part concerned the study of the dynamics of accretion disks around neutron stars which allowed me to familiarize myself with X-[r] ... Voir le document complet

186

ATHENA X-IFU thermal filters development status toward the end of the instrument phase-A

ATHENA X-IFU thermal filters development status toward the end of the instrument phase-A

... The X-IFU, based on an array of 3840 transition edge sensors (TES) microcalorimeters, will provide integral field spectroscopy in the energy range ...a field of view of 5 ... Voir le document complet

15

A CHANGE IN THE QUIESCENT X-RAY SPECTRUM OF THE NEUTRON STAR LOW-MASS X-RAY BINARY MXB 1659–29

A CHANGE IN THE QUIESCENT X-RAY SPECTRUM OF THE NEUTRON STAR LOW-MASS X-RAY BINARY MXB 1659–29

... consider the other possibility, that the spectrum is now dominated by a power-law ...that the neutron star surface cooled dramatically between 2008 and ...Unfortunately, the data quality does ... Voir le document complet

7

X-CIGALE: Fitting AGN/galaxy SEDs from X-ray to infrared

X-CIGALE: Fitting AGN/galaxy SEDs from X-ray to infrared

... by the afore- mentioned dust ...to the SED. Since the UV/optical SEDs of galaxies are generally redder than those of unobscured AGNs ...investigate the cause of SED reddening, we can compare ... Voir le document complet

19

X-ray microtomography of macadamia nuts

X-ray microtomography of macadamia nuts

... using X-ray microtomography, in order to determine a link between structural properties and storage ...of the predominantly grown hybrid varieties (A38, 816, 842, Daddow and 246) are scanned, ... Voir le document complet

6

X-Ray Sobolev Variational Auto-Encoders

X-Ray Sobolev Variational Auto-Encoders

... hand the ”kernel trick” that en- ables to compute functional quantities on Euclidian spaces; on the other hand the ”sliced distances” that average, in a sense to be made precise, the distances ... Voir le document complet

26

The ASTRO-H (Hitomi) x-ray astronomy satellite

The ASTRO-H (Hitomi) x-ray astronomy satellite

... . The half power diameter of the HXTs is ...After the launch, the first light data were obtained from an observation of the supernova remnant ...0.9. The HPD of the two ... Voir le document complet

19

Tolerance of arteries to microplanar X-ray beams.: Microplanar X-ray beam irradiation of arteries

Tolerance of arteries to microplanar X-ray beams.: Microplanar X-ray beam irradiation of arteries

... irradiation, the TM in the MPB paths was thinner in the high-dose group (mean thickness 5 ± 1 µ m) than in the 312 Gy group (20 ± 3 µ ...of the TM were wider in the 2000 Gy group ... Voir le document complet

16

Fast X-ray reflectivity measurements using an X-ray pixel area detector at the DiffAbs beamline, Synchrotron SOLEIL

Fast X-ray reflectivity measurements using an X-ray pixel area detector at the DiffAbs beamline, Synchrotron SOLEIL

... after the description of the samples investigated in this study, the use of the area detector combined with the continuous acquisition mode is ...sample. The supporting ... Voir le document complet

12

1-kHz table-top ultrashort hard x-ray source for time-resolved x-ray protein

1-kHz table-top ultrashort hard x-ray source for time-resolved x-ray protein

... ␣ x-ray yield. 17 X-rays are collected through a 17 mm diameter beryllium window placed 16 mm from the ...target. The deposition of debris on the beryllium window is prevented by ... Voir le document complet

4

Broad-band soft X-ray polarimetry

Broad-band soft X-ray polarimetry

... on the X-ray spectra and polarization that can be tested with soft X-ray ...Measuring the polarization of the radiation from magnetars in the X-ray ... Voir le document complet

11

Obscured sources and Supergiant Fast X-ray Transients: new classes of high mass X-ray binaries

Obscured sources and Supergiant Fast X-ray Transients: new classes of high mass X-ray binaries

... than the absorption in ...that the material absorbing in the X-rays was concentrated around the compact object, while the material absorbing in the optical/NIR was ... Voir le document complet

8

Multi-wavelength observations of Galactic hard X-ray sources discovered by INTEGRAL. I. The nature of the companion star

Multi-wavelength observations of Galactic hard X-ray sources discovered by INTEGRAL. I. The nature of the companion star

... 4.4. The nature of INTEGRAL HMXBs Let us now consider our results, summarized and put together with other characteristics of these sources in Table ...13 INTEGRAL sources, concentrated both towards ... Voir le document complet

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Multi-wavelength observations of Galactic hard X-ray sources discovered by INTEGRAL. II. The environment of the companion star

Multi-wavelength observations of Galactic hard X-ray sources discovered by INTEGRAL. II. The environment of the companion star

... all the INTEGRAL sources are refer- enced ( ...at the European Southern Observatory, Chile (through programmes ...of the SIMBAD and VizieR databases operated at the CDS, Strasbourg, ... Voir le document complet

17

Image-guided treatment using an X-ray therapy unit and gold nanoparticles: Test of concept

Image-guided treatment using an X-ray therapy unit and gold nanoparticles: Test of concept

... have the potential to enhance the radiation dose locally in external radio- therapy with kV ...In the kilovoltage region, gold has an attenuation coefficient two orders of mag- nitude greater than ... Voir le document complet

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