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Cosmoglobe SIGNED

Cosmoglobe -- mapping the universe from the Milky Way to the Big Bang

Total Cost €

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EC-Contrib. €

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Partnership

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 Cosmoglobe project word cloud

Explore the words cloud of the Cosmoglobe project. It provides you a very rough idea of what is the project "Cosmoglobe" about.

sky    generation    theoretical    holds    aftermath    cosmological    baseline    frequency    jointly    magnitude    free    date    experiments    orders    co    planck    critical    spider    window    mapping    resolution    source    mhz    gravity    pasiphae    cib    sub    toward    cmb    dust    bicep2    ultimate    waves    opening    published    detect    led    cosmoglobe    structure    forecast    observations    effort    precision    comap    polarization    utmost    world    emission    2014    litebird    came    data    reionization    cosmology    algorithmic    sz    sensitivity    radio    optimally    detector    thz    direct    synchrotron    undergone    wmap    astrophysical    cosmic    angular    strongest    breakthroughs    analyze    separation    optimize    myself    piece    first    thermal    true    3d    observational    microwave    bass    breakthrough    limits    noise    obscuring    break    hunt    foregrounds    s4    maps    transition    2015    mm    gravitational    veil    model    leverage    spinning    dawn    intensity    inflationary    milky    form    models    derive    potentially   

Project "Cosmoglobe" data sheet

The following table provides information about the project.

Coordinator
UNIVERSITETET I OSLO 

Organization address
address: PROBLEMVEIEN 5-7
city: OSLO
postcode: 313
website: www.uio.no

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 Coordinator Country Norway [NO]
 Total cost 1˙999˙382 €
 EC max contribution 1˙999˙382 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2018-COG
 Funding Scheme ERC-COG
 Starting year 2019
 Duration (year-month-day) from 2019-06-01   to  2024-05-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    UNIVERSITETET I OSLO NO (OSLO) coordinator 1˙999˙382.00

Map

 Project objective

In the aftermath of the high-precision Planck and BICEP2 experiments, cosmology has undergone a critical transition. Before 2014, most breakthroughs came as direct results of improved detector technology and increased noise sensitivity. After 2014, the main source of uncertainty will be due to astrophysical foregrounds, typically in the form of dust or synchrotron emission from the Milky Way. Indeed, this holds as true for the study of reionization and the cosmic dawn as it does for the hunt for inflationary gravitational waves. To break through this obscuring veil, it is of utmost importance to optimally exploit every piece of available information, merging the world's best observational data with the world's most advanced theoretical models. A first step toward this ultimate goal was recently published as the Planck 2015 Astrophysical Baseline Model, an effort led and conducted by myself.

Here I propose to build Cosmoglobe, a comprehensive model of the radio, microwave and sub-mm sky, covering 100 MHz to 10 THz in both intensity and polarization, extending existing models by three orders of magnitude in frequency and a factor of five in angular resolution. I will leverage a recent algorithmic breakthrough in multi-resolution component separation to jointly analyze some of the world's best data sets, including C-BASS, COMAP, PASIPHAE, Planck, SPIDER, WMAP and many more. This will result in the best cosmological (CMB, SZ, CIB etc.) and astrophysical (thermal and spinning dust, synchrotron and free-free emission etc.) component maps published to date. I will then use this model to derive the world's strongest limits on, and potentially detect, inflationary gravity waves using SPIDER observations; forecast, optimize and analyze observations from the leading next-generation CMB experiments, including LiteBIRD and S4; and derive the first 3D large-scale structure maps from CO intensity mapping from COMAP, potentially opening up a new window on the cosmic dawn.

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The information about "COSMOGLOBE" are provided by the European Opendata Portal: CORDIS opendata.

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