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High-energy monitoring of Seyfert galaxies: The case of NGC 4593

Ursini, F. and Petrucci, P.-O. and Matt, G. and Bianchi, S. and Cappi, M. and De Marco, B. and De Rosa, A. and Malzac, J. and Ponti, G. (2016) High-energy monitoring of Seyfert galaxies: The case of NGC 4593. Astronomische Nachrichten, 337 (4-5). pp. 552-556. ISSN 0004-6337. doi:10.1002/asna.201612346. https://resolver.caltech.edu/CaltechAUTHORS:20160527-092521863

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Abstract

We discuss preliminary results from a joint XMM-Newton and NuSTAR monitoring program on the active galactic nucleus NGC 4593, consisting of 5×20 ks observations, spaced by two days, performed in January 2015. The source is found to be variable, both in flux and spectral shape, on time scales as short as a few ks. The spectrum clearly softens when the source brightens. A simple timing analysis suggests the presence of a variable soft excess that correlates with the primary continuum.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1002/asna.201612346DOIArticle
http://onlinelibrary.wiley.com/doi/10.1002/asna.201612346/abstractPublisherArticle
http://arxiv.org/pdf/1510.01966arXivDiscussion Paper
ORCID:
AuthorORCID
Matt, G.0000-0002-2152-0916
Bianchi, S.0000-0002-4622-4240
De Rosa, A.0000-0001-5668-6863
Ponti, G.0000-0003-0293-3608
Additional Information:© 2016 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.
Group:NuSTAR
Issue or Number:4-5
DOI:10.1002/asna.201612346
Record Number:CaltechAUTHORS:20160527-092521863
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20160527-092521863
Official Citation:Ursini, F., Petrucci, P.-O., Matt, G., Bianchi, S., Cappi, M., De Marco, B., De Rosa, A., Malzac, J. and Ponti, G. (2016), High-energy monitoring of Seyfert galaxies: The case of NGC 4593. Astron. Nachr., 337: 552–556. doi: 10.1002/asna.201612346
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:67432
Collection:CaltechAUTHORS
Deposited By: Joy Painter
Deposited On:27 May 2016 16:35
Last Modified:04 Oct 2022 17:09

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