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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.

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

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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