Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/24112| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | VACCA, VALENTINA | en_US |
| dc.contributor.author | Oppermann, Niels | en_US |
| dc.contributor.author | Ensslin, Torsten A. | en_US |
| dc.contributor.author | Selig, Marco | en_US |
| dc.contributor.author | Junklewitz, Henrik | en_US |
| dc.contributor.author | Greiner, Maksim | en_US |
| dc.contributor.author | Jasche, Jens | en_US |
| dc.contributor.author | Hales, Chris A. | en_US |
| dc.contributor.author | Reneicke, Martin | en_US |
| dc.contributor.author | CARRETTI, ETTORE | en_US |
| dc.contributor.author | Feretti, Luigina | en_US |
| dc.contributor.author | Ferrari, Chiara | en_US |
| dc.contributor.author | Giovannini, Gabriele | en_US |
| dc.contributor.author | GOVONI, FEDERICA | en_US |
| dc.contributor.author | Horellou, Cathy | en_US |
| dc.contributor.author | Ideguchi, Shinsuke | en_US |
| dc.contributor.author | Johnston-Hollitt, Melanie | en_US |
| dc.contributor.author | MURGIA, MATTEO | en_US |
| dc.contributor.author | Paladino, Rosita | en_US |
| dc.contributor.author | Pizzo, Roberto | en_US |
| dc.contributor.author | Scaife, Anna | en_US |
| dc.date.accessioned | 2020-04-20T13:22:35Z | - |
| dc.date.available | 2020-04-20T13:22:35Z | - |
| dc.date.issued | 2015 | en_US |
| dc.identifier.issn | 1824-8039 | en_US |
| dc.identifier.uri | http://hdl.handle.net/20.500.12386/24112 | - |
| dc.description.abstract | To better understand the origin and properties of cosmological magnetic fields, a detailed knowledge of magnetic fields in the large-scale structure of the Universe (galaxy clusters, filaments) is crucial. We propose a new statistical approach to study magnetic fields on large scales with the rotation measure grid data that will be obtained with the new generation of radio interferometers. | en_US |
| dc.language.iso | eng | en_US |
| dc.title | Statistical methods for the analysis of rotation measure grids in large scale structures in the SKA era | en_US |
| dc.type | Conference paper | - |
| dc.identifier.doi | 10.22323/1.215.0114 | en_US |
| dc.identifier.url | https://pos.sissa.it/215/114/ | en_US |
| dc.relation.medium | ELETTRONICO | en_US |
| dc.relation.volume | 215 | en_US |
| dc.relation.firstpage | 114 | en_US |
| dc.type.referee | REF_1 | en_US |
| dc.relation.ispartofbook | Advancing Astrophysics with the Square Kilometre Array (AASKA14) | en_US |
| dc.relation.conferencename | Advancing Astrophysics with the Square Kilometre Array (AASKA14) | en_US |
| dc.relation.conferenceplace | Giardini Naxos, Italy | en_US |
| dc.relation.conferencedate | 9-13 June, 2014 | en_US |
| dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
| dc.relation.journal | POS PROCEEDINGS OF SCIENCE | en_US |
| dc.type.miur | 273 Contributo in Atti di convegno | - |
| dc.identifier.adsbibcode | 2015aska.confE.114V | en_US |
| dc.description.apc | no | en_US |
| dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
| item.grantfulltext | open | - |
| item.fulltext | With Fulltext | - |
| item.languageiso639-1 | en | - |
| crisitem.author.dept | O.A. Cagliari | - |
| crisitem.author.dept | IRA Bologna | - |
| crisitem.author.dept | IRA Bologna | - |
| crisitem.author.dept | O.A. Cagliari | - |
| crisitem.author.dept | O.A. Cagliari | - |
| crisitem.author.dept | IRA Bologna | - |
| crisitem.author.orcid | 0000-0003-1997-0771 | - |
| crisitem.author.orcid | 0000-0002-3973-8403 | - |
| crisitem.author.orcid | 0000-0003-4916-6362 | - |
| crisitem.author.orcid | 0000-0003-3644-3084 | - |
| crisitem.author.orcid | 0000-0002-4800-0806 | - |
| crisitem.author.orcid | 0000-0001-9143-6026 | - |
| Appears in Collections: | 3.01 Contributi in Atti di convegno | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Vacca_etal2015.pdf | 187.65 kB | Adobe PDF | View/Open |
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