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相关论文: XMM-Newton observation of Mrk 110

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Six XMM-Newton observations of the bright narrow line Seyfert 1, Mrk 110, from 2004-2020, are presented. The analysis of the grating spectra from the Reflection Grating Spectrometer (RGS) reveals a broad component of the He-like Oxygen…

高能天体物理现象 · 物理学 2021-05-03 J. N. Reeves , D. Porquet , V. Braito , N. Grosso , A. Lobban

In the recent literature on AGNs it has been often reported that spectra of Seyfert 1 Galaxies show resonant absorption lines of Fe K which are redshifted from the rest frame position. Such lines are often found with marginal significance…

天体物理学 · 物理学 2007-05-23 A. L. Longinotti , S. Sim , K. Nandra , P. O'Neill , M. Cappi

We present the results of a ~160 ks-long XMM-Newton observation of the Seyfert 1 galaxy Mrk 279. The spectrum shows evidence of both broad and narrow emission features. The Fe K alpha line may be equally well explained by a single broad…

宇宙学与河外天体物理 · 物理学 2015-05-18 E. Costantini , J. S. Kaastra , K. Korista , J. Ebrero , N. Arav , G. Kriss , K. C. Steenbrugge

A 100ks XMM-Newton observation of the nearby Seyfert 2 galaxy Mrk 3 offers a unique opportunity to explore the complexity of its X-ray spectrum. We find the \~3-8 keV continuum to be dominated by reflection from cold matter, with…

天体物理学 · 物理学 2007-05-23 K. A. Pounds , K. L. Page

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

Results are presented from a 500ks long XMM-Newton observation of the Narrow-Line Seyfert 1 galaxy IRAS13224-3809. The source is rapidly variable on timescales down to a few 100s. The spectrum shows strong broad Fe-K and L emission features…

We report the discovery of strong soft X-ray emission lines and a hard continuum above 2 keV in the Narrow-Line Seyfert 1 galaxy Mrk 335 during an extremely low X-ray flux state. Mrk 335 was observed for 22 ks by XMM-Newton in July 2007 as…

We present XMM-Newton observations of Mrk 359, the first Narrow Line Seyfert 1 galaxy discovered. Even among NLS1s, Mrk 359 is an extreme case with extraordinarily narrow optical emission lines. The XMM-Newton data show that Mrk 359 has a…

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

XMM-Newton observations of the bright Seyfert 1.9 galaxy MCG-5-23-16 have revealed a broad FeKalpha emission line which is nearly symmetric in contrast to the broad and red-shifted asymmetric FeKalpha line sometimes observed from Seyfert 1…

天体物理学 · 物理学 2009-11-07 G. C. Dewangan , R. E. Griffiths , N. J. Schurch

We present a new analysis of a 9-day long XMM-Newton monitoring of the Narrow Line Seyfert 1 galaxy Mrk 766. We show that the strong changes in spectral shape which occurred during this observation can be interpreted as due to Broad Line…

宇宙学与河外天体物理 · 物理学 2015-05-19 G. Risaliti , E. Nardini , M. Salvati , M. Elvis , G. Fabbiano , R. Maiolino , P. Pietrini , G. Torricelli-Ciamponi

We present results based on an XMM-Newton observation of the high luminosity narrow-line QSO PHL 1092 performed in 2003 January. The 0.3 - 10 keV spectrum is well described by a model which includes a power-law (Gamma ~ 2.1) and two…

天体物理学 · 物理学 2009-11-10 Surajit Dasgupta , A. R. Rao , G. C. Dewangan

We present a spectral analysis of the Seyfert 1.8 ESO 113-G010 observed with XMM-Newton for 4 ks. The spectrum shows a soft excess below 0.7 keV and more interestingly a narrow emission Gaussian line at 5.4 keV (in its rest-frame), most…

天体物理学 · 物理学 2009-11-10 D. Porquet , J. N. Reeves , P. Uttley , T. J. Turner

This paper reports on a partially simultaneous observation of the bright Seyfert 1 Galaxy Mrk590, performed by XMM-Newton and Chandra. The long exposure (~100 ks) allows to investigate with great detail the Fe K complex at 6-7 keV and the…

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

Since the discovery of the first broad iron-K line in 1995 from the Seyfert Galaxy MCG--6-30-15, broad iron-K lines have been found in several other Seyfert galaxies, from accreting stellar mass black holes and even from accreting neutron…

The rapid and seemingly random fluctuations in X-ray luminosity of Seyfert galaxies provided early support for the standard model in which Seyferts are powered by a supermassive black hole fed from an accretion disc. However, since EXOSAT…

天体物理学 · 物理学 2009-09-17 S. Vaughan , A. C. Fabian , K. Iwasawa

We report on the XMM-Newton observation of the bright Seyfert 1 galaxy, MCG+8-11-11. Data from the EPIC/p-n camera, the Reflection Gratings Spectrometers (RGS) and the Optical Monitor (OM) have been analyzed. The p-n spectrum is well fitted…

天体物理学 · 物理学 2009-11-11 G. Matt , S. Bianchi , A. De Rosa , P. Grandi , G. C. Perola

(Abridged) We present here a long (100ks) XMM-Newton follow-up of the Seyfert 1.8 galaxy ESO113-G010 performed in November 2005, in order to study over a longer time-scale its main X-ray properties. The source was found in a higher/softer…

The narrow-line Seyfert 1 galaxy Markarian 766 was observed for 60 ks with the XMM-Newton observatory. The source shows a complex X-ray spectrum. The 2-10 keV spectrum can be adequately represented by a power law and broad Fe Ka emission.…

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
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