The page lists 29 deliverables related to the research project "RADIOFOREGROUNDS".
title and desprition | type | last update |
---|---|---|
Dissemination planDissemination plan organising the activities to be carried out in order to better spreading the results of the project [M4] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Documents, reports | 2019-09-06 |
Improved 3D parametric magnetic field and matter distribution models, and associated softwareImproved 3D parametric magnetic field and matter distribution models, and associated software to implement them by varying their parameters. [M20] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Data Management Plan (DMP)Data Management Plan (DMP) [M6]. Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Documents, reports | 2019-09-06 |
RHPC Infrastructure (RADIOFOREGROUND High Performance Computing)RHPC Infrastructure (RADIOFOREGROUND High Performance Computing) (R, Other) [M18] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Documents, reports | 2019-09-06 |
Data model methodology and RADIOFOREGROUNDS DatabasesData model methodology and RADIOFOREGROUNDS Databases (R, SW). [M12] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Documents, reports | 2019-09-06 |
Software packages for the single and multi-frequency detection/estimation of polarized radio sourcesDevelopment of software packages for the single and multi-frequency detection/estimation of polarized radio sources. [M16]. Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Project websiteWebsite with detailed information about the project and a description of each work-package and all public deliverables: The first version of the site will be made public in month 3. Information will be added after this date as the results of the project and deliverables are completed. The final website is to be completed in month 6. [M3] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Websites, patent fillings, videos etc. | 2019-09-06 |
Visualization software for 3D galactic magnetic field and matter distribution modelsVisualization software for 3D galactic magnetic field and matter distribution models. [M20] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Component separated maps for radio foregrounds: AME and synchrotron (intensity and polarization) and freefree in intensityComponent maps for the main radio foregrounds in the northern sky: AME and synchrotron in both intensity and polarization and free-free in intensity. Month of delivery: M20 (preliminary results with second set of data from WP2), M32 (results with final set of data). Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Production of multifrequency catalogues of polarized radio sourcesProduction of multi-frequency catalogues of polarized radio sources. [M20, M32]. Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Constrainst on inflationary and reionization parameters from an optimal likelihoodConstraints on inflationary and reionization parameters from an optimal likelihood [M26, M36]. Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Open Research Data Pilot | 2019-09-06 |
Code to generate AME maps based on best-fit parameters for any frequency, sky position or resolutionA code to generate AME maps based on best-fit parameters for any frequency, sky position or resolution. [M22, M34] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Updated multifrequency evolutionary models of radio sources in total intensity and in polarizationUpdated multifrequency evolutionary models of radio sources in total intensity and in polarization. [M32]. Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Documents, reports | 2019-09-06 |
Additional ancillary data from follow-up observationsAdditional ancillary data from follow-up observations. [M34]. Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Northern-sky maps and model of the AME (intensity and polarization)Refined northern-sky map and model of the AME emission, both in intensity and polarization. [M22, M34] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Forecasted Galactic and extragalactic residual foregroundsGalactic and extragalactic residual foregrounds, as a function of the instrumental and observational properties of a given polarization experiment. [M30, M36] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Documents, reports | 2019-09-06 |
Filtered QUIJOTE and Planck maps to common scalesSet of four QUIJOTE maps (11, 13, 17, 19GHz) and nine Planck maps (30, 44, 70, 100, 143, 217, 353, 545, 857 GHz) at a common resolution and common angular scales [M3, M12, M24] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Error budget in those mapsEstimated error budget of the remaining systematic uncertainties in those 13 maps. [M3, M12, M24] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Algorithm to filter maps to same scalesAlgorithm to filter any ancillary map (WMAP, Haslam, etc.) to the same common resolutions and angular scales. [M3, M12, M24] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Northern-sky maps and model of the synchrotron emission (intensity and polarization)Refined northern sky map and model of the synchrotron emission in temperature and polarization from the integration of the magnetic field and matter distribution models [M22, M34] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Online documents and publicationsOnline documents and publications: These will be made available through the website or journals as these are completed or published. The delivery of the first document will be in month 12, while the remaining will be delivered between month 12 and month 36. [M12, M24, M36] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Documents, reports | 2019-09-06 |
RADIOFOREGROUNDS ToolsRADIOFOREGROUNDS Tools (SW). [M36] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Combined 3D Galactic magnetic field modelProduce a combined 3D Galactic magnetic field model that best fits the data [M22, M34]. Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
SED for a set of compact sources dominated by AMESpectral Energy Distribution (SED) for a list of compact sources dominated by AME. [M24, M36]. Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Realistic simulated observations of Planck, QUIJOTE and other data setsRealistic simulated observations of Planck, QUIJOTE and other data sets in temperature and polarization. These simulations will be available 3 months after each release of the maps from WP2, to allow time to generate the simulations. [M6, M15, M27]. Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Updated tools for simulating the spatial distribution of polarized sourcesUpdated tools for simulating the spatial distribution of polarized sources as a function of polarized flux density and of frequency. [M24, M32] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Forecasted cross-correlation between the radiosources catalogue and future surveysForecasted cross-correlation between the radiosources catalogue and future surveys [M36]. Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Documents, reports | 2019-09-06 |
Production of single frequency catalogues of polarized radio sourcesProduction of single frequency catalogues of polarized radio sources. [M20, M32]. Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Other | 2019-09-06 |
Study of the relationships of radio source magnetic fields with cosmic time and with source propertiesStudy of the relationships of radio source magnetic fields with cosmic time on one side and with source properties (radio luminosity, radio morphology, spectral index, ...) on the other. [M32] Programme: H2020-EU.2.1.6. - Topic(s): COMPET-05-2015 |
Documents, reports | 2019-09-06 |