Cosmology with Phase 1 of the Square Kilometre Array: Red Book 2018: Technical specifications and performance forecasts

Autor: Bacon, DJ, Battye, RA, Bull, P, Camera, S, Ferreira, PG, Harrison, I, Parkinson, D, Pourtsidou, A, Santos, MG, Wolz, L, Abdalla, F, Akrami, Y, Alonso, D, Andrianomena, S, Ballardini, M, Bernal, JL, Bertacca, D, Bengaly, CAP, Bonaldi, A, Bonvin, C, Brown, ML, Chapman, E, Chen, S, Chen, X, Cunnington, S, Davis, TM, Dickinson, C, Fonseca, J, Grainge, K, Harper, S, Jarvis, MJ, Maartens, R, Maddox, N, Padmanabhan, H, Pritchard, JR, Raccanelli, A, Rivi, M, Roychowdhury, S, Sahlen, M, Schwarz, DJ, Siewert, TM, Viel, M, Villaescusa-Navarro, F, Xu, Y, Yamauchi, D, Zuntz, J, Group, Square Kilometre Array Cosmology Science Working
Přispěvatelé: Laboratoire de physique de l'ENS - ENS Paris (LPENS (UMR_8023)), Fédération de recherche du Département de physique de l'Ecole Normale Supérieure - ENS Paris (FRDPENS), Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris)-Centre National de la Recherche Scientifique (CNRS)-École normale supérieure - Paris (ENS Paris)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), SKA, Astrophysique, Laboratoire de physique de l'ENS - ENS Paris (LPENS), Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)-Sorbonne Université (SU)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)-Sorbonne Université (SU)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)-École normale supérieure - Paris (ENS Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), European Commission, European Research Council
Jazyk: angličtina
Rok vydání: 2018
Předmět:
cosmological model
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
cosmology
galaxy redshift surveys
intensity mapping
radio telescopes
weak lensing
General relativity
FOS: Physical sciences
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
baryon: oscillation: acoustic
01 natural sciences
Cosmology
Metric expansion of space
NO
General Relativity and Quantum Cosmology
statistical analysis
gravitation: lens
0103 physical sciences
general relativity
Cluster analysis
010303 astronomy & astrophysics
Weak gravitational lensing
STFC
Physics
010308 nuclear & particles physics
PE9_14
Astrophysics::Instrumentation and Methods for Astrophysics
Intensity mapping
RCUK
Astronomy and Astrophysics
ST/P000649/1
Galaxy
observatory
Computer Science::Graphics
Space and Planetary Science
Physics::Space Physics
non-Gaussianity
Dark energy
astro-ph.CO
radio telescopes
cosmology
galaxy redshift surveys
weak lensing
intensity mapping
galaxy
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Astrophysics - Cosmology and Nongalactic Astrophysics
dark energy: equation of state
Zdroj: Square Kilometre Array Cosmology Science Working Group, Bacon, D J & Maartens, R 2020, ' Cosmology with Phase 1 of the Square Kilometre Array Red Book 2018: technical specifications and performance forecasts ', Publications of the Astronomical Society of Australia, vol. 37, e007 . https://doi.org/10.1017/pasa.2019.51
Publ.Astron.Soc.Austral.
Publ.Astron.Soc.Austral., 2020, 37, pp.e007. ⟨10.1017/pasa.2019.51⟩
Square Kilometre Array Cosmology Science Working Group 2020, ' Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018 : Technical specifications and performance forecasts ', Publications of the Astronomical Society of Australia . https://doi.org/10.1017/pasa.2019.51
Digital.CSIC. Repositorio Institucional del CSIC
instname
DOI: 10.1017/pasa.2019.51
Popis: Square Kilometre Array Cosmology Science Working Group: et al.
arXiv:1811.02743v1
We present a detailed overview of the cosmological surveys that we aim to carry out with Phase 1 of the Square Kilometre Array (SKA1) and the science that they will enable. We highlight three main surveys: a medium-deep continuum weak lensing and low-redshift spectroscopic HI galaxy survey over 5 000 deg2; a wide and deep continuum galaxy and HI intensity mapping (IM) survey over 20 000 deg2 from to 3; and a deep, high-redshift HI IM survey over 100 deg2 from to 6. Taken together, these surveys will achieve an array of important scientific goals: measuring the equation of state of dark energy out to with percent-level precision measurements of the cosmic expansion rate; constraining possible deviations from General Relativity on cosmological scales by measuring the growth rate of structure through multiple independent methods; mapping the structure of the Universe on the largest accessible scales, thus constraining fundamental properties such as isotropy, homogeneity, and non-Gaussianity; and measuring the HI density and bias out to z = 6. These surveys will also provide highly complementary clustering and weak lensing measurements that have independent systematic uncertainties to those of optical and near-infrared (NIR) surveys like Euclid, LSST, and WFIRST leading to a multitude of synergies that can improve constraints significantly beyond what optical or radio surveys can achieve on their own. This document, the 2018 Red Book, provides reference technical specifications, cosmological parameter forecasts, and an overview of relevant systematic effects for the three key surveys and will be regularly updated by the Cosmology Science Working Group in the run up to start of operations and the Key Science Programme of SKA1.
RB, CD, and SH acknowledge support from an STFC Consolidated Grant (ST/P000649/1). SC is supported by the Italian Ministry of Education, University and Research (MIUR) through Rita Levi Montalcini project ‘PROMETHEUS—Probing and Relating Observables with Multi-wavelength Experiments To Help Enlightening the Universe’s Structure’, and by the ‘Departments of Excellence 2018-2022’ Grant awarded by MIUR (L. 232/2016). PGF acknowledges support from ERC Grant No: 693024, the Beecroft Trust and STFC. RM and MGS acknowledge support from the South African Square Kilometre Array Project and National Research Foundation (Grant Nos. 75415 and 84156). LW is supported by an ARC Discovery Early Career Researcher Award (DE170100356). YA acknowledges support from the Netherlands Organization for Scientific Research (NWO) and the Dutch Ministry of Education, Culture and Science (OCW), and also from the D-ITP consortium, a programme of the NWO that is funded by the OCW. YA is also supported by LabEx ENS-ICFP: ANR-10-LABX-0010/ANR-10-IDEX0001-02 PSL∗. HP’s research is supported by the Tomalla Foundation. AR has received funding from the People Programme (Marie Curie Actions) of the European Union H2020 Programme under REA grant agreement number 706896 (COSMOFLAGS). TS and DJS gratefully acknowledge support from the Deutsche Forschungsgemeinschaft (DFG) within the Research Training Group 1620 ‘Models of Gravity’.
Databáze: OpenAIRE
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