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BeyondPlanck SIGNED

Beyond Planck -- delivering state-of-the-art observations of the microwave sky from 30 to 70 GHz for the next decade

Total Cost €

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EC-Contrib. €

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Partnership

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 BeyondPlanck project word cloud

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

primordial    detection    nothing    modern    decades    alone    lfi    breaking    systematics    foregrounds    successfully    engine    processed    cosmological    foreground    time    milky    world    wmap    clear    legacy    solution    joint    last    greatest    waves    central    critical    interactions    breath    itself    signal    bass    specifications    break    created    sampling    synchrotron    bicep2    volume    extremely    representing    maps    fold    complicated    sensitive    optimizing    data    planck    play    polarized    basic    opposed    ranks    ground    100    94    thermal    sufficient    mehods    designing    instrumental    achievements    critically    orders    ultra    combine    sensitivity    frequency    latest    intellectual    observations    emission    linear    wave    gravity    gravitational    input    ghz    astrophysical    progress    radiation    experiments    magnitude    contamination    big    floor    bang    gibbs    estimation    instrument    inflationary    few    form    unavoidable    cmb    obscures    ordered    components    raw    23    characterization    science    respect    dust    instance    frequencies    separation   

Project "BeyondPlanck" 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˙659˙795 €
 EC max contribution 1˙499˙397 € (90%)
 Programme 1. H2020-EU.2.1.6.3. (Enabling exploitation of space data)
 Code Call H2020-COMPET-2017
 Funding Scheme RIA
 Starting year 2018
 Duration (year-month-day) from 2018-03-01   to  2020-08-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    UNIVERSITETET I OSLO NO (OSLO) coordinator 617˙812.00
2    PLANETEK HELLAS ETAIREIA PERIORISMENIS EFTHYNIS YPIRESIES CHARTOGRAFISIS MESO DORYFOROU EL (MAROUSSI) participant 300˙000.00
3    UNIVERSITA DEGLI STUDI DI MILANO IT (MILANO) participant 261˙750.00
4    ISTITUTO NAZIONALE DI ASTROFISICA IT (ROMA) participant 234˙610.00
5    HELSINGIN YLIOPISTO FI (HELSINGIN YLIOPISTO) participant 85˙225.00

Map

 Project objective

The detection of primordial gravity waves created during the Big Bang ranks among the greatest potential intellectual achievements in modern science. During the last few decades, the instrumental progress necessary to achieve this has been nothing short of breath taking. However, from the latest ultra-sensitive experiments such as BICEP2 and Planck, it is clear that instrumental sensitivity alone will not be sufficient to make a robust detection of gravitational waves. Contamination in the form of astrophysical radiation from the Milky Way, for instance thermal dust and synchrotron radiation, obscures the cosmological signal by orders of magnitude. Even more critically are second-order interactions between this radiation and the instrument characterization itself that lead to a highly non-linear and complicated problem.

We propose a ground-breaking solution to this problem that allows for joint estimation of cosmological parameters, astrophysical components, and instrument specifications. The engine of this method is called Gibbs sampling, which we have already applied extremely successfully to basic CMB component separation. The new and critical step is to apply this method to raw time-ordered observations observed directly by the instrument, as opposed to pre-processed frequency maps. While representing a ~100-fold increase in input data volume, this step is unavoidable in order to break through the current foreground-induced systematics floor. We will apply this method to the Planck LFI observations, and deliver a new set of legacy Planck LFI maps that are robust with respect to instrumental systematics and astrophysical foregrounds. We will also combine these data with similar observations from WMAP (23-94 GHz) and C-BASS (5 GHz), to produce the world’s best measurements of polarized synchrotron emission at CMB frequencies. These data products and mehods will play a central role in designing and optimizing future inflationary gravitational wave experiments.

 Deliverables

List of deliverables.
Final gain estimation module Other 2020-02-12 18:04:13
Tuned MADAM module Other 2020-02-12 18:04:08
Prototype flagging module Demonstrators, pilots, prototypes 2020-02-12 11:55:24
Reproducible research methodology report Documents, reports 2020-02-12 18:04:14
Proto Gibbs sampler Demonstrators, pilots, prototypes 2020-02-12 11:55:27
Protoype gain estimation module Demonstrators, pilots, prototypes 2020-02-12 18:04:03
Operational Gibbs sampler Other 2020-02-12 18:04:03
GitHub repository Other 2020-02-12 18:04:09
WP methodology report Documents, reports 2020-02-12 18:04:05
First astrophysical sky model products Demonstrators, pilots, prototypes 2020-02-12 11:55:23
Cosmological interpretation module Other 2020-02-12 11:55:24

Take a look to the deliverables list in detail:  detailed list of BeyondPlanck deliverables.

Are you the coordinator (or a participant) of this project? Plaese send me more information about the "BEYONDPLANCK" project.

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

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