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相关论文: New changing look case in NGC 1566

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We present results from a joint Xmm-Newton/NuSTAR monitoring of the Seyfert 1 NGC 4593, consisting of 5x20 ks simultaneous observations spaced by two days, performed in January 2015. The source is variable, both in flux and spectral shape,…

高能天体物理现象 · 物理学 2016-08-17 F. Ursini , P. -O. Petrucci , G. Matt , S. Bianchi , M. Cappi , B. De Marco , A. De Rosa , J. Malzac , A. Marinucci , G. Ponti , A. Tortosa

We present a new analysis of the soft and medium energy X-ray spectrum of the Seyfert 1 galaxy NGC 3516 taken with the Reflection Grating Spectrometer (RGS) and European Photon Imaging Camera (EPIC) on board the XMM-Newton observatory. We…

宇宙学与河外天体物理 · 物理学 2015-05-18 M. Mehdipour , G. Branduardi-Raymont , M. J. Page

We report the first broad band X-ray spectra of the low luminosity active galactic nuclei (LLAGN) NGC 1566 (type 1.5) and NGC 4941 (type 2) observed with Suzaku and Swift/BAT covering the 0.5-195 keV band. Both targets have hard X-ray…

星系天体物理 · 物理学 2015-06-15 Taiki Kawamuro , Yoshihiro Ueda , Fumie Tazaki , Yuichi Terashima

An XMM-Newton observation of the luminous Seyfert galaxy PG1211+143 in 2001 revealed the first clear evidence for a highly ionised high speed wind (in a non-BAL AGN), with a velocity of v~0.09c based on the identification of blue-shifted…

高能天体物理现象 · 物理学 2015-06-17 K. A. Pounds

This paper reports on two XMM-Newton observations of the Seyfert 1 Galaxy H0557-385 obtained in 2006, which show the source at an historical low flux state, more than a factor of 10 lower than a previous XMM-Newton look in 2002. The low…

天体物理学 · 物理学 2009-11-13 A. L. Longinotti , S. Bianchi , L. Ballo , I. de la Calle , M. Guainazzi

We study the X-ray spectra of a sample of 19 obscured, optically-selected Seyfert galaxies (Sy 1.8, 1.9 and 2) in the local universe ($d \leq 175$~Mpc), drawn from the CfA Seyfert sample. Our analysis is driven by the high sensitivity of…

We report on a study of long-term flux variations in a sample of more than 1000 AGN observed with ROSAT and in the XMM-Newton slew survey. Over a period of 3-19 years, NLS1 galaxies as a class are found to be only slightly more variable…

宇宙学与河外天体物理 · 物理学 2011-06-20 Richard Saxton , Andrew Read , Pilar Esquej , Giovanni Miniutti , Emilio Alvarez

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 have analyzed the two longest (elapsed time > 3 days) BeppoSAX observations of the X-ray brightest Seyfert galaxy, NGC 4151, to search for spectral variability on time-scales from a few tens of ksec to years. We found in both cases…

天体物理学 · 物理学 2008-11-26 S. Puccetti , F. Fiore , G. Risaliti , M. Capalbi , M. Elvis , F. Nicastro , .

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

Thirty years ago the optical counterpart of the x-ray source 1H0707-495 was discovered to be a 15th magnitude broad-line Seyfert galaxy with a rich Fe II emission line spectrum typical of the AGN subclass sometimes referred to as the I Zw 1…

星系天体物理 · 物理学 2017-08-08 Hartmut Winkler , Bynish Paul

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

We present the results from a 500 ks Chandra observation of the Seyfert 1 galaxy NGC 5548. We detect broadened emission lines of O VII and C VI in the spectra, similar to those observed in the optical and UV bands. The source was…

(Abridged) We present a detailed broadband X-ray spectrum of NGC 4258, with the goal of precisely measuring the coronal luminosity and accretion flow properties of the AGN, and track any possible variation across two decades of…

高能天体物理现象 · 物理学 2022-07-20 Alberto Masini , J. V. Wijesekera , Annalisa Celotti , Peter G. Boorman

Results from an analysis of low resolution (R~250) near-IR long-slit spectra covering simultaneously the I, J, H, and K bands, for a sample of 15 Seyfert galaxies and the N5253 starburst nucleus, are presented. The Seyfert galaxies were…

天体物理学 · 物理学 2009-10-31 Claudia Winge , Thaisa Storchi-Bergmann , Martin J. Ward , Andrew S. Wilson

We present serendipitous simultaneous radio and X-ray light curves of the dwarf Seyfert galaxy UGC 6728 spanning 5 years. The X-ray light curve exhibits a flaring period, followed by a gradual rise and decline. Throughout these events, the…

星系天体物理 · 物理学 2026-01-23 Krista Lynne Smith , Macon Magno , Michael Koss

In this paper we present the analysis of two broad band (0.1-150 keV) BeppoSAX observations of the Seyfert 1 galaxy NGC 3516. The two observations were taken 4 months apart, on 1996 November 8 and 1997 March 12 respectively. We report a…

The local Seyfert 1.5 active galactic nucleus (AGN), NGC 6814, is known to exhibit complex variability, eclipses, and even changing-look behaviour. In this work, we utilize optical-to-X-ray data obtained over 10-years with the Neil Gehrels…

高能天体物理现象 · 物理学 2025-06-10 L. K. Pothier-Bogoslowski , L. C. Gallo , A. G. Gonzalez , M. Z. Buhariwalla , J. M. Miller

We present the first photo- and spectropolarimetric observations of the changing-look active galactic nucleus NGC~1346 taken with the Perkins telescope (November 2022, March 2025) and VLT/FORS2 (August and September 2024), which have…

星系天体物理 · 物理学 2025-07-14 F. Marin , D. Hutsemékers , S. Jorstad

We report on a powerful and variable off-nuclear X-ray source in the nearby spiral galaxy NGC 4945. Two ROSAT PSPC observations show the source to brighten in 0.5--2.0 keV flux by a factor of about 9 on a time-scale of 11 months or less. It…

天体物理学 · 物理学 2016-06-08 W. N. Brandt , K. Iwasawa , C. S. Reynolds
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