The space infrared telescope for cosmology and astrophysics: SPICA A joint mission between JAXA and ESA

被引：114

作者：

Swinyard, Bruce ^{[1
]}

Nakagawa, Takao ^{[2
]}

Merken, Patrick ^{[16
]}

Royer, Pierre ^{[19
]}

Souverijns, Tim ^{[16
]}

Vandenbussche, Bart ^{[19
]}

Waelkens, Christoffel ^{[19
]}

Davis, Peter ^{[3
]}

Di Francesco, James ^{[13
]}

Halpern, Mark ^{[49
]}

Houde, Martin ^{[57
]}

Johnstone, Doug ^{[13
]}

Joncas, Gilles ^{[53
]}

Naylor, David ^{[54
]}

Plume, Rene ^{[50
]}

Scott, Douglas ^{[49
]}

Abergel, A. ^{[18
]}

Bensammar, S. ^{[11
]}

Braine, J. ^{[28
]}

Buat, V.

Burgarella, D.

Cais, Ph. ^{[28
]}

Dole, H. ^{[18
]}

Duband, L. ^{[6
]}

Elbaz, D. ^{[7
]}

Gerin, M. ^{[30
]}

Giard, M. ^{[8
]}

Goicoechea, J. ^{[30
]}

Joblin, C. ^{[8
]}

Jones, A. ^{[18
]}

Kneib, J. P.

Lagache, G. ^{[18
]}

Madden, S. ^{[7
]}

Pons, R. ^{[8
]}

Pajot, F. ^{[18
]}

Rambaud, D. ^{[8
]}

Ravera, L. ^{[8
]}

Ristorcelli, I. ^{[8
]}

Rodriguez, L. ^{[7
]}

Vives, S.

Zavagno, A.

Geis, Norbert ^{[32
]}

Krause, Oliver ^{[31
]}

Lutz, Dieter ^{[32
]}

Poglitsch, Albrecht ^{[32
]}

Raab, Walfried ^{[32
]}

Stegmaier, Jutta ^{[31
]}

Sturm, Eckhard ^{[32
]}

Tuffs, Richard ^{[33
]}

Lee, Hyung Mok ^{[43
]}

机构：

[1] Rutherford Appleton Lab, Sci & Technol Facil Council, Didcot OX11 0QX, Oxon, England

[2] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2298510, Japan

[3] BlueSky Spect Inc, Lethbridge, AB, Canada

[4] CALTECH, Pasadena, CA 91125 USA

[5] Cardiff Univ, Cardiff CF10 3AX, S Glam, Wales

[6] CEA Grenoble, CENG, Serv Basses Temp, F-38054 Grenoble, France

[7] CEA Saclay, DAPNIA, Serv Astrophys, Saclay, France

[8] Univ Toulouse 3, CNRS, Ctr Etud Spatiale Rayonnements, F-31062 Toulouse, France

[9] Cornell Univ, Ithaca, NY 14853 USA

[10] CSIC, IEM, Dept Astrofas Mol & InfraRoja, Madrid, Spain

[11] CNRS, Observ Paris, GEPI, F-75700 Paris, France

[12] Univ Groningen, NL-9700 AB Groningen, Netherlands

[13] Herzberg Inst Astrophys, Victoria, BC, Canada

[14] Hiroshima Univ, Hiroshima 730, Japan

[15] Ibaraki Univ, Mito, Ibaraki, Japan

[16] IMEC RMA, Leuven, Belgium

[17] Univ London Imperial Coll Sci Technol & Med, London, England

[18] CNRS Paris XI, Inst Astrophys Spatiale, Orsay, France

[19] Katholieke Univ Leuven, Inst Sterrenkunde, Leuven, Belgium

[20] Ist Fis Spazio Interplanetario, Rome, Italy

[21] Japan Aerosp Explorat Agcy, Chofu, Tokyo, Japan

[22] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA

[23] Korea Astron & Space Sci Inst, Daejon, South Korea

[24] Kobe Univ, Kobe, Hyogo 657, Japan

[25] Kyoto Sangyo Univ, Kyoto 603, Japan

[26] Kyoto Univ, Kyoto, Japan

[27] Kyung Hee Univ, Seoul, South Korea

[28] CNRS, OASU, Lab Astrophys Bordeaux, Bordeaux, France

[29] Leiden Univ, Leiden Observ, NL-2300 RA Leiden, Netherlands

[30] CNRS, Observ Paris, LERMA, F-75700 Paris, France

[31] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany

[32] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany

[33] Max Planck Inst Kernphys, D-69117 Heidelberg, Germany

[34] Univ Coll London, Mullard Space Sci Lab, Holmbury St Mary, Dorking RH5 6NT, Surrey, England

[35] Nagoya Univ, Nagoya, Aichi 4648601, Japan

[36] Nagoya City Univ, Nagoya, Aichi, Japan

[37] Natl Inst Nat Sci, Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo, Japan

[38] SRON Netherlands Inst Space Res, Utrecht, Netherlands

[39] Niigata Univ, Niigata 95021, Japan

[40] Rikkyo Univ, Tokyo 171, Japan

[41] Rutherford Appleton Lab, Didcot OX11 0QX, Oxon, England

[42] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[43] Seoul Natl Univ, Seoul, South Korea

[44] Strathclyde Univ, Glasgow, Lanark, Scotland

[45] Univ Sussex, Brighton BN1 9RH, E Sussex, England

[46] Open Univ, Milton Keynes MK7 6AA, Bucks, England

[47] Tokyo Inst Technol, Tokyo 152, Japan

[48] UK Astron Technol Ctr, Edinburgh, Midlothian, Scotland

[49] Univ British Columbia, Vancouver, BC V5Z 1M9, Canada

[50] Univ Calgary, Calgary, AB T2N 1N4, Canada

来源：

EXPERIMENTAL ASTRONOMY | 2009年 / 23卷 / 01期

基金：

英国工程与自然科学研究理事会;

关键词：

Space missions; Infrared; POLYCYCLIC AROMATIC-HYDROCARBON; SUBMILLIMETER GALAXIES; STAR-FORMATION; SPITZER; MODEL; EMISSION; SPECTRUM; UNIVERSE; PAHS; IR;

D O I：

10.1007/s10686-008-9090-0

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Space Infrared telescope for Cosmology and Astrophysics (SPICA) is planned to be the next space astronomy mission observing in the infrared. The mission is planned to be launched in 2017 and will feature a 3.5 m telescope cooled to < 5 K through the use of mechanical coolers. These coolers will also cool the focal plane instruments thus avoiding the use of consumables and giving the mission a long lifetime. SPICA's large, cold aperture will provide a two order of magnitude sensitivity advantage over current far infrared facilities (> 30 microns wavelength). We describe the scientific advances that will be made possible by this large increase in sensitivity and give details of the mission, spacecraft and focal plane conceptual design.

引用

页码：193 / 219

页数：27

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