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Science from an Ultra-Deep, High-Resolution Millimeter-Wave Survey

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arxiv 1903.03263 v1 pith:TBKXVXQY submitted 2019-03-08 astro-ph.CO astro-ph.GAhep-ph

classification astro-ph.COastro-ph.GAhep-ph
keywords surveydarkmattermillimeter-waveparticleyieldadvancesallow
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Opening up a new window of millimeter-wave observations that span frequency bands in the range of 30 to 500 GHz, survey half the sky, and are both an order of magnitude deeper (about 0.5 uK-arcmin) and of higher-resolution (about 10 arcseconds) than currently funded surveys would yield an enormous gain in understanding of both fundamental physics and astrophysics. In particular, such a survey would allow for major advances in measuring the distribution of dark matter and gas on small-scales, and yield needed insight on 1.) dark matter particle properties, 2.) the evolution of gas and galaxies, 3.) new light particle species, 4.) the epoch of inflation, and 5.) the census of bodies orbiting in the outer Solar System.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. The Atacama Large Aperture Submillimeter Telescope (AtLAST)

    astro-ph.IM 2019-07 unverdicted novelty 4.0 of 10

    Proposes the AtLAST 50m submm telescope concept with 1-degree field of view and advanced instruments to achieve transformative wide-field mapping of the sub-mm sky.

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