Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/30520
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Ursini, Francesco | en_US |
dc.contributor.author | Petrucci, P. -O. | en_US |
dc.contributor.author | Matt, G. | en_US |
dc.contributor.author | BIANCHI, STEFANO | en_US |
dc.contributor.author | CAPPI, MASSIMO | en_US |
dc.contributor.author | De Marco, B. | en_US |
dc.contributor.author | DE ROSA, ALESSANDRA | en_US |
dc.contributor.author | Malzac, J. | en_US |
dc.contributor.author | PONTI, GABRIELE | en_US |
dc.date.accessioned | 2021-02-22T15:11:55Z | - |
dc.date.available | 2021-02-22T15:11:55Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0004-6337 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30520 | - |
dc.description.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. | en_US |
dc.language.iso | eng | en_US |
dc.title | High-energy monitoring of Seyfert galaxies: The case of NGC 4593 | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1002/asna.201612346 | en_US |
dc.identifier.scopus | 2-s2.0-84964776904 | en_US |
dc.identifier.isi | 000375725600036 | en_US |
dc.identifier.url | http://arxiv.org/abs/1510.01966v1 | en_US |
dc.identifier.url | https://onlinelibrary.wiley.com/doi/abs/10.1002/asna.201612346 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 337 | en_US |
dc.relation.firstpage | 552 | en_US |
dc.relation.lastpage | 556 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | ASTRONOMISCHE NACHRICHTEN | en_US |
dc.type.miur | 262 Articolo in rivista | en_US |
dc.identifier.adsbibcode | 2016AN....337..552U | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | IAPS Roma | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.orcid | 0000-0001-9442-7897 | - |
crisitem.author.orcid | 0000-0001-6966-8920 | - |
crisitem.author.orcid | 0000-0001-5668-6863 | - |
crisitem.author.orcid | 0000-0003-0293-3608 | - |
crisitem.journal.journalissn | 0004-6337 | - |
crisitem.journal.ance | E016235 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
1510.01966.pdf | postprint | 675.74 kB | Adobe PDF | View/Open |
asna.201612346.pdf | [Administrators only] | 204.28 kB | Adobe PDF |
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