Testing the X-ray reverberation model KYNREFREV in a sample of Seyfert 1 Active Galactic Nuclei

Caballero-García, María Dolores; Papadakis, I.E.; Dovčiak, Michal; Bursa, Michal; Epitropakis, A.; Karas, Vladimír; Svoboda, Jiří

doi:https://dx.doi.org/10.1093/mnras/sty1990

Number of the records: 1

Testing the X-ray reverberation model KYNREFREV in a sample of Seyfert 1 Active Galactic Nuclei

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SYSNO ASEP	0496036
Document Type	J - Journal Article
R&D Document Type	Journal Article
Subsidiary J	Článek ve WOS
Title	Testing the X-ray reverberation model KYNREFREV in a sample of Seyfert 1 Active Galactic Nuclei
Author(s)	Caballero-García, María Dolores (ASU-R)_ORCID Papadakis, I.E. (GR) Dovčiak, Michal (ASU-R)_{RID, ORCID} Bursa, Michal (ASU-R)_{RID, ORCID} Epitropakis, A. (GR) Karas, Vladimír (ASU-R)_{RID, ORCID} Svoboda, Jiří (ASU-R)_{RID, ORCID}
Source Title	Monthly Notices of the Royal Astronomical Society. - : Oxford University Press - ISSN 0035-8711 Roč. 480, č. 2 (2018), s. 2650-2659
Number of pages	10 s.
Publication form	Online - E
Language	eng - English
Country	GB - United Kingdom
Keywords	black hole physics ; active galaxies ; X-rays
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
OECD category	Astronomy (including astrophysics,space science)
R&D Projects	GA18-00533S GA ČR - Czech Science Foundation (CSF)
Institutional support	ASU-R - RVO:67985815
UT WOS	000449614800094
DOI	10.1093/mnras/sty1990
Annotation	We present the first results obtained by the application of the KYNREFREV-reverberation model, which is ready for its use in XSPEC. This model computes the time-dependent reflection spectra of the disc as a response to a flash of primary power-law radiation from a point source corona located on the axis of the black hole accretion disc (lamp-post geometry). Full relativistic effects are taken into account. The ionization of the disc is set for each radius according to the amount of the incident primary flux and the density of the accretion disc. We tested the model by fitting model predictions to the observed time-lag spectra of three Narrow-Line Seyfert 1 galaxies (ARK 564, MCG-6-30-15, and 1H 0707-495), assuming either a rapidly or zero-spinning black hole (BH).
Workplace	Astronomical Institute
Contact	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2019

Number of the records: 1