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The coronal parameters of local Seyfert galaxies

Marinucci, A. and Tortosa, A. (2016) The coronal parameters of local Seyfert galaxies. Astronomische Nachrichten, 337 (4-5). pp. 490-494. ISSN 00046337. http://resolver.caltech.edu/CaltechAUTHORS:20160527-102828359

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Abstract

One of the open problems for AGN is the nature of the primary X-ray emission: It is likely due to Comptonization of soft UV photons, but the optical depth and temperature of the emitting corona were largely unknown before the launch of the Nuclear Spectroscopic Telescope Array (NuSTAR). It is the first focusing hard X-ray telescope on orbit, ∼ 100 times more sensitive in the 10-79 keV band compared to previous observatories, enabling the study of AGN at high energies with high precision. We present and discuss the results on the hot corona parameters of active galactic nuclei that have been recently measured with NuSTAR (often in coordination with XMM-Newton, Suzaku, or wift) with unprecedented accuracy, in a number of local Seyfert galaxies.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1002/asna.201612335DOIArticle
http://arxiv.org/abs/1511.01332arXivDiscussion Paper
http://onlinelibrary.wiley.com/doi/10.1002/asna.201612335/abstractPublisherArticle
Additional Information:© 2016 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim. AM and AT acknowledge financial support from Italian Space Agency under grant ASI/INAF I/037/12/0-011/13 and from the European Union Seventh Framework Programme (FP7/2007-2013) under grant agreement n.312789. This work was supported under NASA Contract No. NNG08FD60C, and made use of data from the NuSTAR mission, a project led by the California Institute of Technology, managed by the Jet Propulsion Laboratory, and funded by the National Aeronautics and Space Administration. We thank the NuSTAR Operations, Software and Calibration teams for support with the execution and analysis of these observations. This research has made use of the NuSTAR Data Analysis Software (NuSTARDAS) jointly developed by the ASI Science Data Center (ASDC, Italy) and the California Institute of Technology (USA).
Group:NuSTAR
Funders:
Funding AgencyGrant Number
Agenzia Spaziale Italiana (ASI)I/037/12/0-011/13
Istituto Nazionale di Astrofisica (INAF)UNSPECIFIED
European Union Seventh Framework Programme (FP7/2007-2013)312789
NASANNG08FD60C
NASA/JPL/CaltechUNSPECIFIED
Record Number:CaltechAUTHORS:20160527-102828359
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20160527-102828359
Official Citation:Marinucci, A. and Tortosa, A. (2016), The coronal parameters of local Seyfert galaxies. Astron. Nachr., 337: 490–494. doi: 10.1002/asna.201612335
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:67440
Collection:CaltechAUTHORS
Deposited By: Joy Painter
Deposited On:27 May 2016 17:51
Last Modified:27 May 2016 17:51

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