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Cosmic backgrounds from the radio to the far-infrared: recent results and perspectives from cosmological and astrophysical surveys

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    SYSNO ASEP0567309
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleCosmic backgrounds from the radio to the far-infrared: recent results and perspectives from cosmological and astrophysical surveys
    Author(s) Burigana, C. (IT)
    Battistelli, E.S. (IT)
    Bonavera, L. (ES)
    Choudhury, T.R. (IN)
    Lopez-Caniego, M. (ES)
    Skordis, Constantinos (FZU-D) ORCID
    Sullivan, R.M. (CA)
    Tanimura, H. (FR)
    Tizchang, S. (IR)
    Tristram, M. (FR)
    Weltman, A. (ZA)
    Number of authors11
    Article number2230012
    Source TitleInternational Journal of Modern Physics D. - : World Scientific Publishing - ISSN 0218-2718
    Roč. 31, č. 07 (2022)
    Number of pages31 s.
    Languageeng - English
    CountrySG - Singapore
    Keywordscosmology ; background radiations ; observational cosmology
    Subject RIVBE - Theoretical Physics
    OECD categoryParticles and field physics
    R&D ProjectsEF15_003/0000437 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    Method of publishingLimited access
    Institutional supportFZU-D - RVO:68378271
    UT WOS000807421800011
    EID SCOPUS85126045407
    DOI10.1142/S0218271822300129
    AnnotationCosmological and astrophysical surveys in various wavebands, in particular from the radio to the far-infrared, offer a unique view of the universe’s properties and the formation and evolution of its structures. After a preamble on the so-called tension problem, which occurs when different types of data are used to determine cosmological parameters, we discuss the role of fast radio bursts in cosmology, in particular for the missing baryon problem, and the perspectives from the analysis of the 21 cm redshifted line from neutral hydrogen. We then describe the Planck Legacy Archive, its wealth of scientific information and next developments, and the promising perspectives expected from higher resolution observations, in particular for the analysis of the thermal Sunyaev–Zel’dovich effect.
    WorkplaceInstitute of Physics
    ContactKristina Potocká, potocka@fzu.cz, Tel.: 220 318 579
    Year of Publishing2023
    Electronic addresshttps://doi.org/10.1142/S0218271822300129
Number of the records: 1  

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