دورية أكاديمية
Towards open and reproducible multi-instrument analysis in gamma-ray astronomy
العنوان: | Towards open and reproducible multi-instrument analysis in gamma-ray astronomy |
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المؤلفون: | Nigro, C., Deil, C., Zanin, R., Hassan, T., King, J., Ruíz, José Enrique, Saha, L., Terrier, R., Brügge, K., Nöthe, M., Bird, R., Lin, T.T.Y., Aleksic, J., Boisson, C., Contreras, J.L., Donath, A., Jouvin, L., Kelley-Hoskins, N., Khelifi, B., Kosack, K., Rico, J., Sinha, A. |
المساهمون: | Helmholtz Association, German Research Foundation, European Commission |
بيانات النشر: | EDP Sciences |
سنة النشر: | 2019 |
المجموعة: | Digital.CSIC (Consejo Superior de Investigaciones Científicas / Spanish National Research Council) |
مصطلحات موضوعية: | Methods: data analysis, Gamma rays: general |
الوصف: | The analysis and combination of data from different gamma-ray instruments involves the use of collaboration proprietary software and case-by-case methods. The effort of defining a common data format for high-level data, namely event lists and instrument response functions (IRFs), has recently started for very-high-energy gamma-ray instruments, driven by the upcoming Cherenkov Telescope Array (CTA). In this work we implemented this prototypical data format for a small set of MAGIC, VERITAS, FACT, and H.E.S.S. Crab nebula observations, and we analyzed them with the open-source gammapy software package. By combining data from Fermi-LAT, and from four of the currently operating imaging atmospheric Cherenkov telescopes, we produced a joint maximum likelihood fit of the Crab nebula spectrum. Aspects of the statistical errors and the evaluation of systematic uncertainty are also commented upon, along with the release format of spectral measurements. The results presented in this work are obtained using open-access on-line assets that allow for a long-term reproducibility of the results.© ESO 2019. ; This work was supported by the Young Investigators Program of the Helmholtz Association, by the Deutsche Forschungsgemeinschaft (DFG) within the Collaborative Research Center SFB 876 >Providing Information by Resource-Constrained Analysis>, project C3 and by the European Commision through the ASTERICS Horizon2020 project (id 653477). ; Peer Reviewed |
نوع الوثيقة: | article in journal/newspaper |
اللغة: | unknown |
تدمد: | 1432-0746 |
العلاقة: | #PLACEHOLDER_PARENT_METADATA_VALUE#; info:eu-repo/grantAgreement/EC/H2020/653477; Publisher's version; http://doi.org/10.1051/0004-6361/201834938Test; Sí; Astronomy and Astrophysics 625: A10 (2019); http://hdl.handle.net/10261/189000Test; http://dx.doi.org/10.13039/501100001656Test; http://dx.doi.org/10.13039/501100000780Test; http://dx.doi.org/10.13039/501100001659Test |
DOI: | 10.1051/0004-6361/201834938 |
DOI: | 10.13039/501100001656 |
DOI: | 10.13039/501100000780 |
DOI: | 10.13039/501100001659 |
الإتاحة: | https://doi.org/10.1051/0004-6361/201834938Test https://doi.org/10.13039/501100001656Test https://doi.org/10.13039/501100000780Test https://doi.org/10.13039/501100001659Test http://hdl.handle.net/10261/189000Test |
حقوق: | open |
رقم الانضمام: | edsbas.555C6B30 |
قاعدة البيانات: | BASE |
تدمد: | 14320746 |
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DOI: | 10.1051/0004-6361/201834938 |