Space Project for Astrophysical and Cosmological Exploration (SPACE), an ESA stand-alone mission and a possible contribution to the Origins Space Telescope

被引:0
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作者
Denis Burgarella
Andrew Bunker
Rychard Bouwens
Laurent Pagani
Jose Afonso
Hakim Atek
Marc Audard
Sylvie Cabrit
Karina Caputi
Laure Ciesla
Christopher Conselice
Asantha Cooray
Giovanni Cresci
Mirko Curti
José Miguel Rodríguez Espinosa
Marc Ferrari
Chiaki Kobayashi
Nadège Lagarde
Jesus Gallego Maestro
Roberto Maiolino
Katarzyna Malek
Filippo Mannucci
Julien Montillaud
Pascal Oesch
Chris Pearson
Agnieszka Pollo
Céline Reylé
David Rosario
Itsuki Sakon
Daniel Schaerer
Ray Sharples
David Sobral
Frédéric Zamkotsian
机构
[1] Aix Marseille Univ,Department of Physics
[2] CNRS,Leiden Observatory
[3] CNES,Observatoire de Geneve
[4] LAM,Kapteyn Astronomical Institute
[5] University of Oxford,Centre for Astronomy and Particle Theory
[6] Leiden University,School of Physics, Astronomy and Mathematics, Centre for Astrophysics Research
[7] LERMA & UMR8112 du CNRS,Departamento de Física de la Tierra y Astrofísica, Facultad CC Físicas, Instituto de Física de Partículas y del Cosmos, IPARCOS
[8] Observatoire de Paris,Centre for Extragalactic Astronomy, Department of Physics
[9] PSL University,Department of Astronomy, Graduate School of Science
[10] Sorbonne Universités,Center for Advanced Instrumentation, Department of Physics
[11] CNRS,Department of Physics
[12] Instituto de Astrofísica e Ciências do Espaço,undefined
[13] Faculdade de Ciências,undefined
[14] Universidade de Lisboa,undefined
[15] OAL,undefined
[16] Sorbonne Université,undefined
[17] CNRS UMR 7095,undefined
[18] Institut d’Astrophysique de Paris,undefined
[19] Université de Geneve,undefined
[20] University of Groningen,undefined
[21] University of Nottingham,undefined
[22] University of California,undefined
[23] Irvine,undefined
[24] INAF - Osservatorio Astrofisico di Arcetri,undefined
[25] Kavli Institute for Cosmology – University of Cambridge,undefined
[26] Instituto de Astrofısica de Canarias (IAC),undefined
[27] University of Hertfordshire,undefined
[28] Institut UTINAM,undefined
[29] CNRS UMR6213,undefined
[30] Univ. Bourgogne Franche-niversidaComté,undefined
[31] OSU THETA Franche-Comté-Bourgogne,undefined
[32] Observatoire de Besançon,undefined
[33] Universidad Complutense de Madrid,undefined
[34] National Centre for Nuclear Research,undefined
[35] RAL Space,undefined
[36] STFC Rutherford Appleton Laboratory,undefined
[37] Durham University,undefined
[38] The University of Tokyo,undefined
[39] Durham University,undefined
[40] Lancaster University,undefined
来源
Experimental Astronomy | 2021年 / 51卷
关键词
Extragalactic astrophysics; Cosmology; First stars; First dust grains; First galaxies; Reionization;
D O I
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学科分类号
摘要
We propose a new mission called Space Project for Astrophysical and Cosmological Exploration (SPACE) as part of the ESA long term planning Voyage 2050 programme. SPACE will study galaxy evolution at the earliest times, with the key goals of charting the formation of the heavy elements, measuring the evolution of the galaxy luminosity function, tracing the build-up of stellar mass in galaxies over cosmic time, and finding the first super-massive black holes (SMBHs) to form. The mission will exploit a unique region of the parameter space, between the narrow ultra-deep surveys with HST and JWST, and shallow wide-field surveys such as the Roman Space Telescope and EUCLID, and should yield by far the largest sample of any current or planned mission of very high redshift galaxies at z > 10 which are sufficiently bright for detailed follow-up spectroscopy. Crucially, we propose a wide-field spectroscopic near-IR + mid-IR capability which will greatly enhance our understanding of the first galaxies by detecting and identifying a statistical sample of the first galaxies and the first supermassive black holes, and to chart the metal enrichment history of galaxies in the early Universe – potentially finding signatures of the very first stars to form from metal-free primordial gas. The wide-field and wavelength range of SPACE will also provide us a unique opportunity to study star formation by performing a wide survey of the Milky Way in the near-IR + mid-IR. This science project can be enabled either by a stand-alone ESA-led M mission or by an instrument for an L mission (with ESA and/or NASA, JAXA and other international space agencies) with a wide-field (sub-)millimetre capability at λ > 500 μm.
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页码:625 / 660
页数:35
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