X-ray spectra of the Fe-L complex

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 wit...

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Bibliographic Details
Main Author: Gu, L. (author)
Other Authors: Shah, C. (author), Mao, J. (author), Raassen, A. J. J. (author), Plaa, J. de (author), Pinto, Ciro (author), Akamatsu, H. (author), Werner, N. (author), Simionescu, A. (author), Mernier, F. (author), Sawada, M. (author), Mohanty, P. (author), Amaro, P. (author), Gu, M. Feng (author), Porter, F. Scott (author), López-Urrutia, J. R. C. (author), Kaastra, J. S. (author)
Format: article
Language:eng
Published: 2022
Subjects:
Atoms
Galaxies
Iron compounds
Uncertainty analysis
Online Access:http://hdl.handle.net/10362/145734
Country:Portugal
Oai:oai:run.unl.pt:10362/145734
Description
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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