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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.

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

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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