0000000000084819

AUTHOR

Graziella Branduardi-raymont

showing 5 related works from this author

Thermal Filters for the ATHENA X-IFU: Ongoing Activities Toward the Conceptual Design

2016

ATHENA is the L2 mission selected by ESA to pursue the science theme “Hot and Energetic Universe.” One of the two focal plane instruments is the X-ray Integral Field Unit, an array of TES microcalorimeters operated at T $$<$$ 100 mK. To allow the X-ray photons focused by the telescope to reach the detector, windows have to be opened on the cryostat thermal shields. X-ray transparent filters need to be mounted on these open windows to attenuate the IR radiation from warm surfaces, to attenuate RF electromagnetic interferences on TES sensors and SQUID electronics, and to protect the detector from contamination. This paper reviews the ongoing activities driving the design of the X-IFU thermal …

CryostatX-ray AstronomyAtomic and Molecular Physics and OpticATHENA; Thermal Filters; X-IFU; X-ray Astronomy; Condensed Matter Physics; Atomic and Molecular Physics and Optics; Materials Science (all)ShieldsCondensed Matter Physic01 natural sciencesThermal Filterlaw.invention010309 opticsTelescopeATHENA; Thermal Filters; X-IFU; X-ray Astronomy; Atomic and Molecular Physics and Optics; Materials Science (all); Condensed Matter PhysicsOpticsSettore FIS/05 - Astronomia E AstrofisicaConceptual designlawAtomic and Molecular Physics0103 physical sciencesGeneral Materials ScienceElectronics010303 astronomy & astrophysicsThermal FiltersPhysicsX-ray astronomyX-IFUbusiness.industryDetectorCondensed Matter PhysicsAtomic and Molecular Physics and OpticsATHENACardinal pointMaterials Science (all)and Opticsbusiness
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The Voyage of Metals in the Universe from Cosmological to Planetary Scales: the need for a Very High-Resolution, High Throughput Soft X-ray Spectrome…

2019

Metals form an essential part of the Universe at all scales. Without metals we would not exist, and the Cosmos would look completely different. Metals are primarily born through nuclear processes in stars. They leave their cradles through winds or explosions, and then start their journey through space. This can lead them in and out of astronomical objects on all scales, ranging from comets, planets, stars, entire galaxies, groups and clusters of galaxies to the largest structures of the Universe. Their wanderings are fundamental in determining how these objects, and the entire universe, evolve. In addition, their bare presence can be used to trace what these structures look like. The scope …

Very high resolutionAstronomical ObjectsCosmology and Nongalactic Astrophysics (astro-ph.CO)010504 meteorology & atmospheric sciencesGalaxy-ISM-CGM-IGM feedbackFOS: Physical sciencesSpace (mathematics)Cycle of baryons and metals7. Clean energy01 natural sciencesCycle of baryons and metals; Galaxy-ISM-CGM-IGM feedback; High-resolution X-ray spectrometer; X-ray gratingsSettore FIS/05 - Astronomia E Astrofisica0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]X-ray gratingsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsThroughput (business)0105 earth and related environmental sciencesCycle of baryons and metalHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSoft x rayCOSMIC cancer databaseSpectrometerSettore FIS/05AstronomyAstronomy and AstrophysicsHigh-resolution X-ray spectrometerAstrophysics - Astrophysics of GalaxiesStars13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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The filter wheel and filters development for the X-IFU instruments onboard Athena

2016

Athena is the large mission selected by ESA in 2013 to investigate the science theme “Hot and Energetic Universe” and presently scheduled for launch in 2028. One of the two instruments located at the focus of the 12 m-long Athena telescope is the X-ray Integral Field Unit (X-IFU). This is an array of TES microcalorimeters that will be operated at temperatures of 50 mK in order to perform high resolution spectroscopy with an energy resolution down to 2.5 eV at energies &lt; 7 keV. In order to cope with the large dynamical range of X-ray fluxes spanned by the celestial objects Athena will be observing, the X-IFU will be equipped with a filter wheel. This will allow the user to fine tune the i…

Physicsbusiness.industrymedia_common.quotation_subject01 natural sciencesUniverselaw.invention010309 opticsTelescopeOpticsSettore FIS/05 - Astronomia E AstrofisicalawRange (aeronautics)0103 physical sciencesCalibrationAthena X-rays Filter Wheel Filters radioactive calibration sourcesDevelopment (differential geometry)Focus (optics)business010303 astronomy & astrophysicsHost (network)Energy (signal processing)media_common
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Astrophysics with the Laser Interferometer Space Antenna

2023

Full list of authors: Amaro-Seoane, Pau; Andrews, Jeff; Sedda, Manuel Arca; Askar, Abbas.; Baghi, Quentin; Balasov, Razvan; Bartos, Imre; Bavera, Simone S.; Bellovary, Jillian; Berry, Christopher P. L.; Berti, Emanuele; Bianchi, Stefano; Blecha, Laura; Blondin, Stephane; Bogdanovic, Tamara; Boissier, Samuel; Bonetti, Matteo; Bonoli, Silvia; Bortolas, Elisa; Breivik, Katelyn; Capelo, Pedro R.; Caramete, Laurentiu; Cattorini, Federico; Charisi, Maria; Chaty, Sylvain; Chen, Xian; Chruslinska, Martyna; Chua, Alvin J. K.; Church, Ross; Colpi, Monica; D'Orazio, Daniel; Danielski, Camilla; Davies, Melvyn B.; Dayal, Pratika; De Rosa, Alessandra; Derdzinski, Andrea; Destounis, Kyriakos; Dotti, Massi…

AstrofísicaACTIVE GALACTIC NUCLEICosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Black holeAstronomyStellar remnantFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)TIDAL DISRUPTION EVENTSGeneral Relativity and Quantum CosmologyGravitational wavesMOCCA-SURVEY DATABASESettore FIS/05 - Astronomia e AstrofisicaStellar remnantsSoftware ScienceMulti-messengerGRAVITATIONAL-WAVE SOURCESInstrumentation and Methods for Astrophysics (astro-ph.IM)Extreme mass ratio in-spiralsSolar and Stellar Astrophysics (astro-ph.SR)High Energy Astrophysical Phenomena (astro-ph.HE)Black holes; Extreme mass ratio in-spirals; Gravitational waves; Multi-messenger; Stellar remnantsBlack holesData ScienceAstrophysics::Instrumentation and Methods for AstrophysicsExtreme mass ratio in-spiralAM-CVN STARSAstrophysics - Astrophysics of GalaxiesWHITE-DWARF BINARIESDOUBLE NEUTRON-STARSAstrophysics - Solar and Stellar Astrophysics[SDU]Sciences of the Universe [physics]Astrophysics of Galaxies (astro-ph.GA)AstronomiaMASSIVE BLACK-HOLEAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsX-RAY BINARIESCOMMON-ENVELOPE EVOLUTIONGravitational waveAstrophysics - Cosmology and Nongalactic Astrophysics
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The optical blocking filter for the ATHENA wide field imager: Ongoing activities towards the conceptual design

2015

ATHENA is the L2 mission selected by ESA to pursue the science theme "Hot and Energetic Universe" (launch scheduled in 2028). One of the key instruments of ATHENA is the Wide Field Imager (WFI) which will provide imaging in the 0.1-15 keV band over a 40'x40' large field of view, together with spectrally and time-resolved photon counting. The WFI camera, based on arrays of DEPFET active pixel sensors, is also sensitive to UV/Vis photons. Optically generated electron-hole pairs may degrade the spectral resolution as well as change the energy scale by introducing a signal offset. For this reason, the use of an X-ray transparent optical blocking filter is needed to allow the observation of all …

PhysicsfilterOffset (computer science)PhotonPixelbusiness.industryElectronic Optical and Magnetic MaterialApplied MathematicsAstrophysics::Instrumentation and Methods for AstrophysicsComputer Science Applications1707 Computer Vision and Pattern RecognitionCondensed Matter PhysicPhoton countingATHENAVibrationInstrumentation for AstrophysicX-rayOpticsConceptual designWFIField-effect transistorSpectral resolutionElectrical and Electronic Engineeringbusiness
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