Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/30486
Titolo: | ATHENA X-IFU thermal filters development status toward the end of the instrument phase-A | Autori: | Barbera, Marco LO CICERO, UGO SCIORTINO, LUISA D'ANCA, FABIO Lo Cicero, Giuseppe Parodi, Giancarlo SCIORTINO, Salvatore Rauw, Gregor Branduardi-Raymont, Graziella VARISCO, Salvatore FERRUGGIA BONURA, Salvatore COLLURA, Alfonso CANDIA, Roberto DI CICCA, Gaspare GIGLIO, Paolo BUTTACAVOLI, ANTONINO CUTTAIA, FRANCESCO VILLA, FABRIZIO CAPPI, MASSIMO Lam Trong, Thien Mesnager, Jean-Michel Peille, Philippe den Hartog, Roland den Herder, Jan Willem Jackson, Brian Barret, Didier PIRO, LUIGI |
Data pubblicazione: | 2018 | Titolo del volume in cui è pubblicato il poster: | Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray | Curatore/i del volume in cui è pubblicato il contributo: | den Herder, Jan-Willem A.; Nikzad, Shouleh; Nakazawa, Kazuhiro | Serie: | PROCEEDINGS OF SPIE | Numero: | 10699 | Da pagina:: | 106991R | Abstract: | The X-ray Integral Field Unit (X-IFU) is one of the two instruments of the Athena astrophysics space mission approved by ESA in the Cosmic Vision 2015-2025 Science Programme. The X-IFU consists of a large array of transition edge sensor micro-calorimeters that will operate at 100 mK inside a sophisticated cryostat. A set of thin filters, highly transparent to X-rays, will be mounted on the opening windows of the cryostat thermal shields in order to attenuate the IR radiative load, to attenuate radio frequency electromagnetic interferences, and to protect the detector from contamination. Thermal filters are critical items in the proper operation of the X-IFU detector in space. They need to be strong enough to survive the launch stresses but very thin to be highly transparent to X-rays. They essentially define the detector quantum efficiency at low energies and are fundamental to make the photon shot noise a negligible contribution to the energy resolution budget. In this paper, we review the main results of modeling and characterization tests of the thermal filters performed during the phase A study to identify the suitable materials, optimize the design, and demonstrate that the chosen technology can reach the proper readiness before mission adoption. | Note: | Copyright 2018 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited. | Titolo del convegno: | Space Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray | Luogo del convegno: | Austin, Texas, United States | Periodo del convegno: | 10-15 June, 2018 | URI: | http://hdl.handle.net/20.500.12386/30486 | URL: | https://www.spiedigitallibrary.org/conference-proceedings-of-spie/10699/2314450/ATHENA-X-IFU-thermal-filters-development-status-toward-the-end/10.1117/12.2314450.full | ISSN: | 0277-786X | ISBN: | 9781510619517 9781510619524 |
DOI: | 10.1117/12.2314450 | Bibcode ADS: | 2018SPIE10699E..1RB | Fulltext: | open |
È visualizzato nelle collezioni: | 3.01 Contributi in Atti di convegno |
File in questo documento:
File | Descrizione | Dimensioni | Formato | |
---|---|---|---|---|
2018 Barbera - ATHENA X-IFU thermal filters development status toward the end of the instrument phase-A.pdf | Pdf editoriale | 1.35 MB | Adobe PDF | Visualizza/apri |
Page view(s)
87
controllato il 18-apr-2024
Download(s)
50
controllato il 18-apr-2024
Google ScholarTM
Check
Altmetric
Altmetric
Tutti i documenti in DSpace sono pubblicati ad Accesso Aperto, salvo diversa indicazione per alcuni documenti specifici.