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

Authors :
Sylvie Cabrit
Katarzyna Małek
Jose Afonso
Jose Miguel Rodriguez Espinosa
Filippo Mannucci
Roberto Maiolino
Laure Ciesla
David J. Rosario
Hakim Atek
Itsuki Sakon
Pascal Oesch
David Sobral
Chris P. Pearson
Rychard Bouwens
Frederic Zamkotsian
Marc Ferrari
Andrew Bunker
Nadège Lagarde
Jesús Gallego Maestro
Laurent Pagani
Giovanni Cresci
Ray M. Sharples
Marc Audard
Mirko Curti
Christopher J. Conselice
J. Montillaud
Agnieszka Pollo
Denis Burgarella
Daniel Schaerer
Asantha Cooray
Karina Caputi
Chiaki Kobayashi
Céline Reylé
Laboratoire d'Astrophysique de Marseille (LAM)
Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES)
Burgarella, D [0000-0002-4193-2539]
Apollo - University of Cambridge Repository
Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA (UMR_8112))
Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-CY Cergy Paris Université (CY)
Institut d'Astrophysique de Paris (IAP)
Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Univers, Transport, Interfaces, Nanostructures, Atmosphère et environnement, Molécules (UMR 6213) (UTINAM)
Université de Franche-Comté (UFC)
Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)
Astronomy
Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique et Atmosphères = Laboratory for Studies of Radiation and Matter in Astrophysics and Atmospheres (LERMA)
École normale supérieure - Paris (ENS-PSL)
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-CY Cergy Paris Université (CY)
Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université de Franche-Comté (UFC)
Université Bourgogne Franche-Comté [COMUE] (UBFC)-Université Bourgogne Franche-Comté [COMUE] (UBFC)
Source :
Experimental Astronomy, 51(3), 625-660, Experimental Astronomy, Experimental Astronomy, Springer Link, 2021, 51 (3), pp.625-660. ⟨10.1007/s10686-021-09703-1⟩, Experimental Astronomy, springer Link, 2021, 51 (3), pp.625-660. ⟨10.1007/s10686-021-09703-1⟩, Experimental Astronomy, 51, 625-660. SPRINGER, Experimental Astronomy, 2021, 51 (3), pp.625-660. ⟨10.1007/s10686-021-09703-1⟩
Publication Year :
2020

Abstract

We propose a new mission called Space Project for Astrophysical and Cosmological Exploration (SPACE) as part on 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 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 SMBH, 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 wavelength > 500 microns.<br />Submitted to Experimental Astronomy as one of the proposals for the European Space Agency Voyage 2050 Programme

Details

Language :
English
ISSN :
09226435 and 15729508
Database :
OpenAIRE
Journal :
Experimental Astronomy, 51(3), 625-660, Experimental Astronomy, Experimental Astronomy, Springer Link, 2021, 51 (3), pp.625-660. ⟨10.1007/s10686-021-09703-1⟩, Experimental Astronomy, springer Link, 2021, 51 (3), pp.625-660. ⟨10.1007/s10686-021-09703-1⟩, Experimental Astronomy, 51, 625-660. SPRINGER, Experimental Astronomy, 2021, 51 (3), pp.625-660. ⟨10.1007/s10686-021-09703-1⟩
Accession number :
edsair.doi.dedup.....1c16bd3ef3b896c35aad552a60fb3168
Full Text :
https://doi.org/10.1007/s10686-021-09703-1⟩