Počet záznamů: 1
Testing the X-ray reverberation model KYNREFREV in a sample of Seyfert 1 Active Galactic Nuclei
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SYSNO ASEP 0496036 Druh ASEP J - Článek v odborném periodiku Zařazení RIV J - Článek v odborném periodiku Poddruh J Článek ve WOS Název Testing the X-ray reverberation model KYNREFREV in a sample of Seyfert 1 Active Galactic Nuclei Tvůrce(i) 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, ORCIDZdroj.dok. Monthly Notices of the Royal Astronomical Society. - : Oxford University Press - ISSN 0035-8711
Roč. 480, č. 2 (2018), s. 2650-2659Poč.str. 10 s. Forma vydání Online - E Jazyk dok. eng - angličtina Země vyd. GB - Velká Británie Klíč. slova black hole physics ; active galaxies ; X-rays Vědní obor RIV BN - Astronomie a nebeská mechanika, astrofyzika Obor OECD Astronomy (including astrophysics,space science) CEP GA18-00533S GA ČR - Grantová agentura ČR Institucionální podpora ASU-R - RVO:67985815 UT WOS 000449614800094 DOI 10.1093/mnras/sty1990 Anotace 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). Pracoviště Astronomický ústav Kontakt Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Rok sběru 2019
Počet záznamů: 1