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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.

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

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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