X-ray spectra of the Fe-L complex
| Main Author: | |
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| Publication Date: | 2022 |
| Other Authors: | , , , , , , , , , , , , , , , |
| Format: | Article |
| Language: | eng |
| Source: | Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) |
| Download full: | http://hdl.handle.net/10362/145734 |
Summary: | Acknowledgements. SRON is supported financially by NWO, the Netherlands Organization for Scientific Research. C.S. acknowledges the support by an appointment to the NASA Postdoctoral Program at the NASA Goddard Space Flight Center, administered by Oak Ridge Associated Universities under contract with NASA and by Max-Planck-Gesellschaft (MPG). J.M. acknowledges the support from STFC (UK) through the University of Strathclyde UK APAP network grant ST/R000743/1. P.A. acknowledges the support from Fundação para a Ciência e a Tecnologia (FCT), Portugal, under Grant No. UID/FIS/04559/2020(LIBPhys). N.W. is supported by the GACR grant 21-13491X. The research leading to these results has received funding from the European Union’s Horizon 2020 Programme under the AHEAD2020 project (grant agreement n. 871158). |
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X-ray spectra of the Fe-L complexIII. Systematic uncertainties in atomic dataAtomsGalaxiesIron compoundsUncertainty analysisAcknowledgements. SRON is supported financially by NWO, the Netherlands Organization for Scientific Research. C.S. acknowledges the support by an appointment to the NASA Postdoctoral Program at the NASA Goddard Space Flight Center, administered by Oak Ridge Associated Universities under contract with NASA and by Max-Planck-Gesellschaft (MPG). J.M. acknowledges the support from STFC (UK) through the University of Strathclyde UK APAP network grant ST/R000743/1. P.A. acknowledges the support from Fundação para a Ciência e a Tecnologia (FCT), Portugal, under Grant No. UID/FIS/04559/2020(LIBPhys). N.W. is supported by the GACR grant 21-13491X. The research leading to these results has received funding from the European Union’s Horizon 2020 Programme under the AHEAD2020 project (grant agreement n. 871158).There has been a growing request from the X-ray astronomy community for a quantitative estimate of systematic uncertainties originating from the atomic data used in plasma codes. Though there have been several studies looking into atomic data uncertainties using theoretical calculations, in general, there is no commonly accepted solution for this task. We present a new approach for estimating uncertainties in the line emissivities for the current models of collisional plasma, mainly based upon a dedicated analysis of observed high resolution spectra of stellar coronae and galaxy clusters. We find that the systematic uncertainties of the observed lines consistently show an anticorrelation with the model line fluxes, after properly accounting for the additional uncertainties from the ion concentration calculation. The strong lines in the spectra are in general better reproduced, indicating that the atomic data and modeling of the main transitions are more accurate than those for the minor ones. This underlying anticorrelation is found to be roughly independent of source properties, line positions, ion species, and the line formation processes. We further applied our method to the simulated XRISM and Athena observations of collisional plasma sources and discuss the impact of uncertainties on the interpretation of these spectra. The typical uncertainties are 1-2% on temperature and 3-20% on abundances of O, Ne, Fe, Mg, and Ni.DF – Departamento de FísicaLIBPhys-UNLRUNGu, L.Shah, C.Mao, J.Raassen, A. J. J.Plaa, J. dePinto, CiroAkamatsu, H.Werner, N.Simionescu, A.Mernier, F.Sawada, M.Mohanty, P.Amaro, P.Gu, M. FengPorter, F. ScottLópez-Urrutia, J. R. C.Kaastra, J. S.2022-11-23T22:25:09Z2022-082022-08-01T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article17application/pdfhttp://hdl.handle.net/10362/145734eng0004-6361PURE: 46050322https://doi.org/10.1051/0004-6361/202039943info:eu-repo/semantics/openAccessreponame:Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)instname:FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiainstacron:RCAAP2024-05-22T18:06:52Zoai:run.unl.pt:10362/145734Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireinfo@rcaap.ptopendoar:https://opendoar.ac.uk/repository/71602025-05-28T17:37:19.403052Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) - FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiafalse |
| dc.title.none.fl_str_mv |
X-ray spectra of the Fe-L complex III. Systematic uncertainties in atomic data |
| title |
X-ray spectra of the Fe-L complex |
| spellingShingle |
X-ray spectra of the Fe-L complex Gu, L. Atoms Galaxies Iron compounds Uncertainty analysis |
| title_short |
X-ray spectra of the Fe-L complex |
| title_full |
X-ray spectra of the Fe-L complex |
| title_fullStr |
X-ray spectra of the Fe-L complex |
| title_full_unstemmed |
X-ray spectra of the Fe-L complex |
| title_sort |
X-ray spectra of the Fe-L complex |
| author |
Gu, L. |
| author_facet |
Gu, L. Shah, C. Mao, J. Raassen, A. J. J. Plaa, J. de Pinto, Ciro Akamatsu, H. Werner, N. Simionescu, A. Mernier, F. Sawada, M. Mohanty, P. Amaro, P. Gu, M. Feng Porter, F. Scott López-Urrutia, J. R. C. Kaastra, J. S. |
| author_role |
author |
| author2 |
Shah, C. Mao, J. Raassen, A. J. J. Plaa, J. de Pinto, Ciro Akamatsu, H. Werner, N. Simionescu, A. Mernier, F. Sawada, M. Mohanty, P. Amaro, P. Gu, M. Feng Porter, F. Scott López-Urrutia, J. R. C. Kaastra, J. S. |
| author2_role |
author author author author author author author author author author author author author author author author |
| dc.contributor.none.fl_str_mv |
DF – Departamento de Física LIBPhys-UNL RUN |
| dc.contributor.author.fl_str_mv |
Gu, L. Shah, C. Mao, J. Raassen, A. J. J. Plaa, J. de Pinto, Ciro Akamatsu, H. Werner, N. Simionescu, A. Mernier, F. Sawada, M. Mohanty, P. Amaro, P. Gu, M. Feng Porter, F. Scott López-Urrutia, J. R. C. Kaastra, J. S. |
| dc.subject.por.fl_str_mv |
Atoms Galaxies Iron compounds Uncertainty analysis |
| topic |
Atoms Galaxies Iron compounds Uncertainty analysis |
| description |
Acknowledgements. SRON is supported financially by NWO, the Netherlands Organization for Scientific Research. C.S. acknowledges the support by an appointment to the NASA Postdoctoral Program at the NASA Goddard Space Flight Center, administered by Oak Ridge Associated Universities under contract with NASA and by Max-Planck-Gesellschaft (MPG). J.M. acknowledges the support from STFC (UK) through the University of Strathclyde UK APAP network grant ST/R000743/1. P.A. acknowledges the support from Fundação para a Ciência e a Tecnologia (FCT), Portugal, under Grant No. UID/FIS/04559/2020(LIBPhys). N.W. is supported by the GACR grant 21-13491X. The research leading to these results has received funding from the European Union’s Horizon 2020 Programme under the AHEAD2020 project (grant agreement n. 871158). |
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2022 |
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2022-11-23T22:25:09Z 2022-08 2022-08-01T00:00:00Z |
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info:eu-repo/semantics/publishedVersion |
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info:eu-repo/semantics/article |
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eng |
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0004-6361 PURE: 46050322 https://doi.org/10.1051/0004-6361/202039943 |
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