Submm/FIR astronomy in Antarctica : potential for a large telescope facility

V. Minier, L. Olmi, P.-O. Lagage, L. Spinoglio, G. A. Durand, E. Daddi, D. Galilei, H. Gallée, C. Kramer, D. Marrone, E. Pantin, L. Sabbatini, N. Schneider, N. F. H. Tothill, L. Valenziano, C. Veyssière

    Research output: Chapter in Book / Conference PaperConference Paperpeer-review

    10 Citations (Scopus)

    Abstract

    ![CDATA[Preliminary site testing datasets suggest that Dome C in Antarctica is one of the best sites on Earth for astronomical observations in the 200 to 500-μm regime, i.e. for far-infrared (FIR) and submillimetre (submm) astronomy. We present an overview of potential science cases that could be addressed with a large telescope facility at Dome C. This paper also includes a presentation of the current knowledge about the site characterics in terms of atmospheric transmission, stability, sky noise and polar constraints on telescopes. Current and future site testing campaigns are finally described.]]
    Original languageEnglish
    Title of host publicationProceedings of 2nd ARENA Conference: The Astrophysical Science Cases at Dome C, 17-21 September 2007, Potsdam, Germany
    PublisherEDP Sciences
    Pages21-40
    Number of pages20
    ISBN (Print)9782759803804
    DOIs
    Publication statusPublished - 2008
    EventARENA Conference -
    Duration: 11 May 2009 → …

    Publication series

    Name
    ISSN (Print)1633-4760

    Conference

    ConferenceARENA Conference
    Period11/05/09 → …

    Fingerprint

    Dive into the research topics of 'Submm/FIR astronomy in Antarctica : potential for a large telescope facility'. Together they form a unique fingerprint.

    Cite this