An XMM-Newton Observation of the Seyfert 1 Galaxy 1h 0419-577 in an Extreme Low State. K A Pounds
- Author: K A Pounds
- Date: 06 Aug 2013
- Publisher: Bibliogov
- Language: English
- Book Format: Paperback::28 pages, ePub, Audiobook
- ISBN10: 1287283284
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2016 XMM-Newton Observation of IRAS 13224-3809 Large-amplitude X-ray variability and the accretion disc/corona connection in the Seyfert 1 galaxy PG 1404+226 First Author: Mallick, L. The X-ray Universe 2017, Proceedings of the Abstract Previous observations of the luminous Seyfert 1 galaxy 1H 0419-577 have found its X-ray spectrum to range from that of a typical Seyfert 1 with 2 1 The DRGs are identified their very red infrared colours with (J K)AB > 1.3, selected over galaxies: evolution, galaxies: high-redshift, cosmology: observations It is centred on the Subaru/XMM Newton Deep Survey field (SXDS Sekiguchi et al. Figure 1. Lower panel: (J K)AB against KAB for sources in the UDS. An XMM-Newton Observation of the Seyfert 1 Galaxy 1h 0419-577 in an Extreme Low State K A Pounds, 9781287283287, available at Book 998 J.M. Miller: Fe K Lines in Black Holes Fig.1 The data/model ratio above shows the relativistic Fe K emission line profile revealed after fitting a phenomenological model to a recent XMM-Newton observation of Cygnus X-1 in a high flux state (Miller et al. 2006, in We report results obtained from six XMM-Newton observations of the Seyfert galaxy 1H 0419 577. The source was observed in a wide range of different f. In a particularly low-flux state in which the X-ray spectrum is rather peculiar and exhibits a very flat hard spectrum (with spectral index close to 1 in the 2 10 keV band), An XMM-Newton observation of the Seyfert 1 galaxy 1H 0419-577 in an extreme low state ( ) 3 2013 ( ) PPT 5 Abstract We present the results of a 500 ks long XMM Newton observation and a 120 ks long quasi-simultaneous Chandra observation of the Narrow-Line Seyfert 1 galaxy 1H 0707 495 performed in 2010 September. Consistent with earlier results Fabian et Request PDF on ResearchGate | An XMM-Newton Observation of the Seyfert 1 Galaxy 1H 0419 577 in an Extreme Low State | Previous AN XMM-NEWTON OBSERVATION OF THE SEYFERT 1 GALAXY 1H 0419-577 IN AN EXTREME LOW STATE Autores: J. N. Reeves, K. A. Pounds Localización: Astrophysical journal, ISSN 0004-637X, Vol. 605, Nº. 2, 2004, págs. 670-676 Idioma: inglés The highly variable X-ray spectrum of the luminous Seyfert 1 galaxy 1H 0419-577_ An XMM-Newton observation of the luminous Seyfert 1 galaxy 1H 0419-577 is presented. We find that the spectrum is well fitted a power law of canonical slope An XMM-Newton Observation of the Seyfert 1 Galaxy 1h 0419-577 in an Extreme Low State [K. A. Pounds, Nasa Technical Reports Server (Ntrs), Et Al] on *FREE* shipping on qualifying offers. Previous observations of the luminous Seyfert 1 galaxy An XMM-Newton Observation of the Seyfert 1 Galaxy 1H 0419 577 in an Extreme Low State. K. A. Pounds1, J. N. Reeves2,3, K. L. Page1, and P. T. O'Brien1. Contributed posters: Chandra HETG Observation of the Ultrasoft Narrow-line Seyfert 1 Galaxy 1H0707-495,and FUSE Observation of the Narrow-line Seyfert 1 Galaxy RE 1034+39 Workshop on X-ray Spectroscopy of Active Galactic Nuclei with Chandra and XMM-Newton,Max-Planck Institute für extraterrestriche Physik, Garching, Germany, December 3-6, 2001. XMM-Newton and Suzaku analysis of the Fe K complex in the type 1 Seyfert galaxy Mrk 509 Ponti,G. Et al. 25 701093010 701093020 701093030 701093040 225 2009 MNRAS, 395, 657G X-ray observations of the galaxy cluster PKS0745-191: to the virial radius The near (z=0.104) luminous QSO, 1H 0419-577, shows a strong hard X-ray excess and our NuSTAR AO-1 observation surprisingly revealed one of the most extreme high energy cut-offs observed to date from any AGN. If its origin is due to thermal XMM-Newton observation of a spectral state transition in the peculiar radio/X-ray/gamma-ray source LS I +61 303 The highly variable X-ray spectrum of the luminous Seyfert 1 galaxy 1H 0419-577 Monthly Notices of the Royal Astronomical Society An XMM-Newton observation of the luminous Seyfert 1 galaxy 1H 0419-577 in September 2002, when the source was in an extreme low-flux state, found a very hard X-ray spectrum at 1-10 keV with a strong soft excess below ~1 keV. Pounds KA, Reeves JN, Page KL, O Brien PT (2004a) An XMM-Newton observation of the Seyfert 1 galaxy 1H 0419-577 in an extreme low state. Astrophys J 605: 670 676. Doi: 10.1086/382678 arXiv:astro-ph/0401026 ADS Google Scholar 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A Photoionised gas in Seyfert 1 Galaxies revealed through emission lines in high resolution X-ray spectra I will present the observation of the Seyfert 1 Galaxy Mrk 335 performed XMM-Newton during an unusually low flux state that unveiled an emission line-rich An XMM-Newton Observation of the Seyfert 1 Galaxy 1h 0419-577 in an Extreme Low State K A Pounds 06 Aug 2013 Paperback US$16.25
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