Galactic magnetic field deflection of high energy astroparticles

Informazioni relative al progetto

GADGET

ID dell’accordo di sovvenzione: 101107047

DOI

10.3030/101107047

Progetto chiuso

Data della firma CE 3 Aprile 2023

Data di avvio 1 Agosto 2023

Data di completamento 31 Luglio 2025

Finanziato da

• Marie Skłodowska-Curie Actions (MSCA)

Costo totale

Nessun dato

Contributo UE

€ 191 760,00

Coordinato da

UNIVERSITE LIBRE DE BRUXELLES
Belgium

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I link ai risultati e alle pubblicazioni dei progetti del 7° PQ, così come i link ad alcuni tipi di risultati specifici come dataset e software, sono recuperati dinamicamente da .OpenAIRE .

Risultati finali

Data Management Plan (1)

Data Management Plan

The Data Management Plan describes the data management life cycle for all data sets that will be collected, processed or generated by the action. It is a document describing what data will be collected, processed or generated and following what methodology and standards, whether and how this data will be shared and/or made open, and how it will be curated and preserved.

Documents, reports (1)

Communication, Dissemination & Exploitation Plan

The plan describes the planned measures to maximize the impact of the project, including the dissemination and exploitation measures that are planned, and the target group(s) addressed. Regarding communication measures and public engagement strategy, the aim is to inform and reach out to society and show the activities performed, and the use and the benefits the project will have for citizens.

Pubblicazioni

Peer reviewed articles (2)

An analytical model for the magnetic field in the thick shell of Galactic bubbles with uniform initial conditions

Autori: V. Pelgrims, M. Unger, I. C. Mariş
Pubblicato in: Astronomy & Astrophysics, Numero 695, 2025, ISSN 0004-6361
Editore: EDP Sciences
DOI: 10.48550/ARXIV.2411.06277

An analytical model for the magnetic field in the thick shell of Galactic bubbles with uniform initial conditions <i>(Corrigendum)</i>

Autori: V. Pelgrims, M. Unger, I. C. Mariş
Pubblicato in: Astronomy &amp; Astrophysics, Numero 701, 2025, ISSN 0004-6361
Editore: EDP Sciences
DOI: 10.1051/0004-6361/202556797E

Conference proceedings (2)

Does the Local Bubble bias Galactic magnetic field models used to backtrack UHECRs?

Autori: Vincent Pelgrims, Michael Unger, Ioana Codrina Maris
Pubblicato in: Proceedings of 7th International Symposium on Ultra High Energy Cosmic Rays — PoS(UHECR2024), 2025, ISSN 1824-8039
Editore: PoS Proceedings of sciences
DOI: 10.22323/1.484.0108

The Effect of Our Cosmic Neighborhood’s Magnetic Field on UHECR Propagation

Autori: Vincent Pelgrims, Michael Unger, Ioana Codrina Maris
Pubblicato in: Proceedings of 39th International Cosmic Ray Conference — PoS(ICRC2025), 2025, ISSN 1824-8039
Editore: PoS proceedings of sciences
DOI: 10.22323/1.501.0357