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  Flaremodel: An open-source Python package for one-zone numerical modelling of synchrotron sources

Dallilar, Y., Fellenberg, S. v., Bauboeck, M., de Zeeuw, P. T., Drescher, A., Eisenhauer, F., et al. (2022). Flaremodel: An open-source Python package for one-zone numerical modelling of synchrotron sources. Astronomy and Astrophysics, 658: A111. doi:10.1051/0004-6361/202142458.

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Flaremodel An open-source Python package for one-zone numerical modelling of synchrotron sources.pdf (beliebiger Volltext), 353KB
 
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Flaremodel An open-source Python package for one-zone numerical modelling of synchrotron sources.pdf
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Synchrotron processes, the radiative processes associated with the interaction of energetic charged particles with magnetic field, are of interest in many areas in astronomy, from the interstellar medium to extreme environments near compact objects. Consequently, observations of synchrotron sources carry information on the physical properties of the sources themselves and those of their close vicinity. In recent years, novel observations of such sources with multi-wavelength collaborations reveal complex features and peculiarities, especially near black holes. Exploring the nature of these sources in more detail necessitates numerical tools complementary to analytical one-zone modelling efforts. In this paper, we introduce an open-source Python package tailored to this purpose, FLAREMODEL. The core of the code consists of low-level utility functions to describe physical processes relevant to synchrotron sources, which are written in C for performance and parallelised with OpenMP for scalability. The Python interface provides access to these functions and built-in source models are provided as a guidance. At the same time, the modular design of the code and the generic nature of these functions enable users to build a variety of source models applicable to many astrophysical synchrotron sources. We describe our methodology and the structure of our code along with selected examples demonstrating capabilities and options for future modelling efforts.
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Dallilar, Y.1, Autor           
Fellenberg, S. von1, Autor           
Bauboeck, M.1, Autor           
de Zeeuw, P. T.1, Autor           
Drescher, A.1, Autor           
Eisenhauer, F.1, Autor           
Genzel, R.1, Autor           
Gillessen, S.1, Autor           
Habibi, M.1, Autor           
Ott, T.1, Autor           
Ponti, G.2, Autor           
Stadler, J.1, Autor           
Straub, O.1, Autor           
Widmann, F.1, Autor           
Witzel, G., Autor
Young, A.1, Autor           
Affiliations:
1Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society, ou_159889              
2High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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 Zusammenfassung: Synchrotron processes, the radiative processes associated with the interaction of energetic charged particles with magnetic field, are of interest in many areas in astronomy, from the interstellar medium to extreme environments near compact objects. Consequently, observations of synchrotron sources carry information on the physical properties of the sources themselves and those of their close vicinity. In recent years, novel observations of such sources with multi-wavelength collaborations reveal complex features and peculiarities, especially near black holes. Exploring the nature of these sources in more detail necessitates numerical tools complementary to analytical one-zone modelling efforts. In this paper, we introduce an open-source Python package tailored to this purpose, FLAREMODEL. The core of the code consists of low-level utility functions to describe physical processes relevant to synchrotron sources, which are written in C for performance and parallelised with OpenMP for scalability. The Python interface provides access to these functions and built-in source models are provided as a guidance. At the same time, the modular design of the code and the generic nature of these functions enable users to build a variety of source models applicable to many astrophysical synchrotron sources. We describe our methodology and the structure of our code along with selected examples demonstrating capabilities and options for future modelling efforts.

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Sprache(n): eng - English
 Datum: 2022-02-07
 Publikationsstatus: Online veröffentlicht
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 Art der Begutachtung: -
 Identifikatoren: DOI: 10.1051/0004-6361/202142458
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Titel: Astronomy and Astrophysics
  Andere : Astron. Astrophys.
Genre der Quelle: Zeitschrift
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Ort, Verlag, Ausgabe: France : EDP Sciences S A
Seiten: - Band / Heft: 658 Artikelnummer: A111 Start- / Endseite: - Identifikator: ISSN: 1432-0746
CoNE: https://pure.mpg.de/cone/journals/resource/954922828219_1