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

Beitrag bei einer Tagung
(Konferenzbeitrag)


Details zur Publikation

Autorinnen und Autoren: 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, Mendez 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
Verlag: SPIE
Jahr der Veröffentlichung: 2016
Band: 9905
ISBN: 9781510601895


Abstract

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).


FAU-Autorinnen und Autoren / FAU-Herausgeberinnen und Herausgeber

Brand, Thorsten
Professur für Astronomie und Astrophysik
Dauser, Thomas Dr.
Dr.Karl-Remeis-Sternwarte Bamberg, Astronomisches Institut
Wilms, Jörn Prof. Dr.
Professur für Astronomie und Astrophysik


Einrichtungen weiterer Autorinnen und Autoren

Center for Theoretical Physics of the Polish Academy of Sciences
Helsingin yliopisto / University of Helsinki
Hiroshima University
Instituto de Física de Cantabria (IFCA)
Instituto Nacional Técnica Aeroespacial (INTA)
Japan Aerospace eXploration Agency (JAXA)
Leiden University
National Aeronautics and Space Administration (NASA)
National Center for Scientific Research / Centre national de la recherche scientifique (CNRS)
National Centre for Space Studies / Centre national d'études spatiales (CNES)
National Institute for Astrophysics / Istituto Nazionale Astrofisica (INAF)
Netherlands Institute for Space Research / Stichting Ruimteonderzoek Nederland (SRON)
Nicolaus Copernicus Astronomical Centre of the Polish Academy of Sciences
Space Research Centre / Centrum Badań Kosmicznych
Università degli Studi di Palermo
Universitat d'Alacant (UA) / University of Alicante
University College London (UCL)
University of Amsterdam
University of Geneva / Université de Genève (UNIGE)
University of Genova / Università degli Studi di Genova
University of Grenoble Alpes (UGA) / Université de Grenoble
University of Groningen / Rijksuniversiteit Groningen
University of Liège (ULg) / Université de Liège
University of Michigan
University of Paris 7 - Denis Diderot / Université Paris VII Denis Diderot


Zitierweisen

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.

BibTeX: 

Zuletzt aktualisiert 2019-25-05 um 01:08