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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.

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

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

Leaflet | Map data © OpenStreetMap contributors, CC-BY-SA, Imagery © Mapbox

 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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