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

被引：51

作者：

Pajot, F. ^{[1
]}

Barret, D. ^{[1
]}

Lam-Trong, T. ^{[2
]}

den Herder, J. -W. ^{[3
]}

Piro, L. ^{[4
]}

Cappi, M. ^{[5
]}

Huovelin, J. ^{[6
]}

Kelley, R. ^{[7
]}

Mas-Hesse, J. M. ^{[8
]}

Mitsuda, K. ^{[9
]}

Paltani, S. ^{[10
]}

Rauw, G. ^{[11
]}

Rozanska, A. ^{[12
]}

Wilms, J. ^{[13
]}

Barbera, M. ^{[14
,15
]}

Douchin, F. ^{[2
]}

Geoffray, H. ^{[2
]}

den Hartog, R. ^{[3
]}

Kilbourne, C. ^{[7
]}

Le Du, M. ^{[2
]}

Macculi, C. ^{[4
]}

Mesnager, J. -M. ^{[2
]}

Peille, P. ^{[2
]}

机构：

[1] Univ Paul Sabatier, IRAP CNRS, 9 Ave Colonel Roche, F-31028 Toulouse 4, France

[2] CNES, 18 Ave Edouard Belin, F-31401 Toulouse 9, France

[3] SRON, Sorbonnelaan 2, NL-3584 CA Utrecht, Netherlands

[4] IAPS, INAF, Via Fosso del Cavaliere 100, I-00133 Rome, Italy

[5] IASF, INAF, Via Gobetti 101, I-40129 Bologna, Italy

[6] Univ Helsinki, Dept Phys, Div Geophys & Astron, POB 48, Helsinki 00014, Finland

[7] NASA, Goddard Space Flight Ctr, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA

[8] CSIC, INTA, Ctr Astrobiol, Ctra Torrejon Ajalvir,4 Km, Madrid 28850, Spain

[9] Japan Aerosp Explorat Agcy JAXA, ISAS, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan

[10] Univ Geneva, Dept Astron, Chemin Ecogia 16, CH-1290 Versoix, Switzerland

[11] Univ Liege, Inst Astrophys & Geophys, Allee 6 Aout 19c, B-4000 Liege, Belgium

[12] Polish Acad Sci, Nicolaus Copernicus Astron Ctr, Ul Bartycka 18, PL-00716 Warsaw, Poland

[13] Univ Erlangen Nurnberg, ECAP, Sternwartstr 7, D-96049 Bamberg, Germany

[14] Univ Palermo, Dipartimento Fis & Chim, Via Archira 36, I-90123 Palermo, Italy

[15] Osservatorio Astron Palermo GS Vaiana, INAF, Piazza Parlamento 1, I-90134 Palermo, Italy

来源：

JOURNAL OF LOW TEMPERATURE PHYSICS | 2018年 / 193卷 / 5-6期

基金：

欧盟地平线“2020”;

关键词：

X-ray astronomy; Imaging spectroscopy; Microcalorimeter;

D O I：

10.1007/s10909-018-1904-5

中图分类号：

O59 [应用物理学];

学科分类号：

摘要：

The X-ray Integral Field Unit (X-IFU) of the Advanced Telescope for High-ENergy Astrophysics (Athena) large-scale mission of ESA 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 (FWHM) up to 7 keV. The core scientific objectives of Athena drive the main performance parameters of the X-IFU. We present the current reference configuration of the X-IFU, and the key issues driving the design of the instrument.

引用

页码：901 / 907

页数：7

共 31 条

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