Barret D, Lam Trong T, Den Herder JW, Piro L, Barcons X, Huovelin J, Kelley R, Mas-Hesse JM, Mitsuda K, Paltani S, Rauw G, Rozanska A, Wilms J, Barbera M, Bozzo E, Ceballos MT, Charles I, Decourchelle A, Den Hartog R, Duval JM, Fiore F, Gatti F, Goldwurm A, Jackson B, Jonker P, Kilbourne C, Macculi C, Méndez M, Molendi S, Orleanski P, Pajot F, Pointecouteau E, Porter F, Pratt GW, Prêle D, Ravera L, Renotte E, Schaye J, Shinozaki K, Valenziano L, Vink J, Webb N, Yamasaki N, Delcelier-Douchin F, Le Du M, Mesnager JM, Pradines A, Branduardi-Raymont G, Dadina M, Finoguenov A, Fukazawa Y, Janiuk A, Miller J, Nazé Y, Nicastro F, Sciortino S, Torrejon JM, Geoffray H, Hernandez I, Luno L, Peille P, André J, Daniel C, Etcheverry C, Gloaguen E, Hassin J, Hervet G, Maussang I, Moueza J, Paillet A, Vella B, Campos Garrido G, Damery JC, Panem C, Panh J, Bandler S, Biffi JM, Boyce K, Clénet A, DiPirro M, Jamotton P, Lotti S, Schwander D, Smith S, Van Leeuwen BJ, Van Weers H, Brand T, Cobo B, Dauser T, De Plaa J, Cucchetti E (2016)
Publication Status: Published
Publication Type: Conference contribution, Conference Contribution
Publication year: 2016
Publisher: SPIE
Book Volume: 9905
Article Number: 99052F
ISBN: 9781510601895
DOI: 10.1117/12.2232432
The X-ray Integral Field Unit (X-IFU) on board the Advanced Telescope for High-ENergy Astrophysics (Athena) will provide spatially resolved high-resolution X-ray spectroscopy from 0.2 to 12 keV, with ∼ 5" pixels over a field of view of 5 arc minute equivalent diameter and a spectral resolution of 2.5 eV up to 7 keV. In this paper, we first review the core scientific objectives of Athena, driving the main performance parameters of the X-IFU, namely the spectral resolution, the field of view, the effective area, the count rate capabilities, the instrumental background. We also illustrate the breakthrough potential of the X-IFU for some observatory science goals. Then we brie y describe the X-IFU design as defined at the time of the mission consolidation review concluded in May 2016, and report on its predicted performance. Finally, we discuss some options to improve the instrument performance while not increasing its complexity and resource demands (e.g. count rate capability, spectral resolution).
APA:
Barret, D., Lam Trong, T., Den Herder, J.W., Piro, L., Barcons, X., Huovelin, J.,... Cucchetti, E. (2016). The Athena X-ray Integral Field Unit (X-IFU). In Proceedings of the Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray. SPIE.
MLA:
Barret, Didier, et al. "The Athena X-ray Integral Field Unit (X-IFU)." Proceedings of the Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray SPIE, 2016.
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