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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.

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

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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