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相关论文: Long-term spectral changes in the partial-covering…

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We apply a reflection-dominated model to the second XMM-Newton observation of the Narrow Line Seyfert 1 galaxy 1H 0707-495. As in the first XMM-Newton observation a sharp spectral drop is detected with energy that has shifted from 7 keV to…

天体物理学 · 物理学 2009-09-17 A. C. Fabian , G. Miniutti , L. Gallo , Th. Boller , Y. Tanaka , S. Vaughan , R. R. Ross

We report the first detection of a sharp spectral feature in a Narrow-Line Seyfert 1 galaxy. Using XMM-Newton we have observed 1H0707-495 and find a drop in flux by a factor of more than 2 at a rest-frame energy of ~7 keV without any…

天体物理学 · 物理学 2009-09-17 Th. Boller , A. C. Fabian , R. Sunyaev , J. Truemper , S. Vaughan , D. R. Ballantyne , W. N. Brandt , R. Keil , K. Iwasawa

The X-ray spectrum of 1H 0707-495 obtained with XMM-Newton showing a deep flux drop at ~7 keV (Boller et al. 2002) is studied based on the partial covering concept. The previously inferred extreme iron overabundance can be reduced down to…

天体物理学 · 物理学 2015-06-24 Yasuo Tanaka , Thomas Boller , Luigi Gallo , Ralph Keil , Yoshihiro Ueda

We present the results of a 500 ksec long XMM-Newton observation and a 120 ksec long quasi-simultaneous Chandra observation of the Narrow Line Seyfert 1 galaxy 1H0707-495 performed in 2010 September. Consistent with earlier results by…

高能天体物理现象 · 物理学 2015-06-03 T. Dauser , J. Svoboda , N. Schartel , J. Wilms , M. Dovciak , M. Ehle , V. Karas , M. Santos-Lleo , H. Marshall

We present preliminary results from a long Chandra HETG observation of the luminous Narrow-line Seyfert 1 galaxy 1H 0707-495. We find a complex X-ray spectrum comprised of a two-component continuum with superimposed emission and absorption…

天体物理学 · 物理学 2007-05-23 Karen M. Leighly , Andrzej A. Zdziarski , Toshihiro Kawaguchi , Chiho Matsumoto

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. Comparison with…

天体物理学 · 物理学 2009-11-10 K. A. Pounds , J. N. Reeves , K. L. Page , P. T. O'Brien

We present the second XMM-Newton observation (85 ks) of the narrow-line Seyfert 1 galaxy (NLS1) I Zw 1 and describe its mean spectral and timing characteristics. On average, I Zw 1 is ~35 per cent dimmer in 2005 than in the shorter (20 ks)…

天体物理学 · 物理学 2008-11-26 L. C. Gallo , W. N. Brandt , E. Costantini , A. C. Fabian , K. Iwasawa , I. E. Papadakis

The Narrow-line Seyfert 1 galaxy 1H0707-495 is known to exhibit significant X-ray spectral variations. Its X-ray energy spectrum is characterized by a strong soft excess emission, an extremely deep iron K-edge structure at ~7 keV, and a…

高能天体物理现象 · 物理学 2015-06-22 Misaki Mizumoto , Ken Ebisawa , Hiroaki Sameshima

We examine archival XMM-Newton data on the extremely variable narrow-line Seyfert 1 (NLS1) active galactic nucleus (AGN) 1H 0707-495. We construct fractional excess variance (Fvar) spectra for each epoch, including the recent 2019…

The X-ray spectra of the narrow line Seyfert 1 galaxy, 1H 0707-495, obtained with XMM-Newton, from time periods of varying X-ray luminosity are analysed in the context of understanding the changes to the X-ray emitting corona that lead to…

高能天体物理现象 · 物理学 2015-06-22 D. R. Wilkins , E. Kara , A. C. Fabian , L. C. Gallo

We present results from two XMM-Newton observations of the bright classical Seyfert 2 galaxy NGC 7582 taken four years apart (2001 May and 2005 April). We present the analysis of the high-resolution (0.3-1 keV) RGS and low-resolution…

天体物理学 · 物理学 2009-11-13 E. Piconcelli , S. Bianchi , M. Guainazzi , F. Fiore , M. Chiaberge

The soft X-ray band of many active galactic nuclei (AGNs) is affected by obscuration due to partially ionised matter crossing our line of sight. In this context, two past XMM-Newton observations (6 months apart) and a simultaneous…

We present results from the spectral analysis of a long XMM-Newton observation of the radio-loud NLS1 galaxy PKS0558-504. The source is highly variable, on all sampled time scales. We did not observe any absorption features in either the…

宇宙学与河外天体物理 · 物理学 2015-05-14 I. E. Papadakis , W. Brinkmann , M. Gliozzi , C. Raeth , F. Nicastro , M. L. Conciatore

We present the temporal analysis of X-ray observations of the radio-loud Narrow-Line Seyfert 1 galaxy (NLS1) PKS 0558-504 obtained during the XMM-Newton Calibration and Performance Verification (Cal/PV) phase. The long term light curve is…

天体物理学 · 物理学 2009-10-31 M. Gliozzi , W. Brinkmann , P. T. O'Brien , J. N. Reeves , K. A. Pounds , M. Trifoglio , F. Gianotti

The Narrow Line Seyfert 1 galaxy NGC4051 shows unusual low flux states, lasting several months, when the 2-10 keV X-ray spectrum becomes unusually hard (photon index<1) while the spectrum at lower X-ray energies is dominated by a large soft…

天体物理学 · 物理学 2009-11-10 P. Uttley , R. D. Taylor , I. M. McHardy , M. J. Page , K. O. Mason , G. Lamer , A. Fruscione

We report on the first XMM-Newton observation of the highly X-ray variable, radio-quiet, Narrow-Line Seyfert 1 galaxy IRAS 13224-3809 obtained during the guaranteed time programme with a 64 ks exposure. The most remarkable spectral feature…

天体物理学 · 物理学 2009-11-07 Th. Boller , Y. Tanaka , A. Fabian , W. N. Brandt , L. Gallo , N. Anabuki , Y. Haba , S. Vaughan

We present results from several XMM-Newton observations of the radio loud Narrow-line Seyfert 1 galaxy (NLS1) PKS 0558-504. We find evidence for strong and persistent X-ray variability, both on short and long time-scales. On short time…

天体物理学 · 物理学 2009-11-10 W. Brinkmann , P. Arevalo , M. Gliozzi , E. Ferrero

We report the results of two Chandra ACIS-S observations from February and August 2003 of the highly X-ray variable Narrow-Line Seyfert 1 galaxy RX J2217.9--5941. Observations spanning the time from the ROSAT All Sky Survey (RASS) through…

天体物理学 · 物理学 2009-11-10 D. Grupe , K. M. Leighly , V. Burwitz , P. Predehl , S. Mathur

An XMM-Newton observation of the luminous Seyfert 1 galaxy 1H 0419-577 is presented. We find that the spectrum is well fitted by a power law of canonical slope (gamma ~ 1.9) and 3 blackbody components (to model the strong soft excess). The…

天体物理学 · 物理学 2009-11-07 K. L. Page , K. A. Pounds , J. N. Reeves , P. T. O'Brien

We report on two XMM-Newton observations of the bright narrow-line Seyfert 1 galaxy Ark 564 taken one year apart (2000 June and 2001 June). The 0.6-10 keV continuum is well described by a soft blackbody component (kT~140-150 eV) plus a…

天体物理学 · 物理学 2009-11-10 C. Vignali , W. N. Brandt , Th. Boller , A. C. Fabian , S. Vaughan
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