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We present a detailed analysis of the intrinsic X-ray absorption in the Seyfert 1 galaxy NGC 4151 using Chandra/HETGS data obtained 2002 May, as part of a program which included simultaneous UV spectra using HST/STIS and FUSE. NGC 4151 was…

A fraction of active galactic nuclei (AGN) exhibit dramatic variability, which is observed on timescales down to minutes in the X-ray band. We introduce the case study of 1H 1934-063 (z = 0.0102), a Narrow-line Seyfert 1 (NLS1) among the…

High Energy Astrophysical Phenomena · Physics 2018-11-07 Sara E. Frederick , Erin Kara , Christopher S. Reynolds , Ciro Pinto , Andrew C. Fabian

We report the discovery of large-amplitude X-ray variability from the direction of the previously unknown, optically inactive galaxy pair RXJ1242.6-1119. The X-ray source shows variability by a factor > 20 between the ROSAT all-sky survey…

Astrophysics · Physics 2008-11-26 Stefanie Komossa , Jochen Greiner

Comparison of 8.4-GHz radio images of a sample of 11 early-type Seyfert galaxies with previous observations reveals possible variation in the nuclear radio flux density in 5 of them over a 7-yr period. We find no correlation between radio…

Cosmology and Nongalactic Astrophysics · Physics 2009-09-28 C. G. Mundell , P. Ferruit , N. Nagar , A. S. Wilson

An-energy dependent variation of the X-ray emission from the archetypical "Compton-thick'' Seyfert 2 galaxy NGC1068 has been observed between two BeppoSAX observations, performed one year apart. This variation (at the 2.6 sigma level) is…

Astrophysics · Physics 2009-10-31 M. Guainazzi , S. Molendi , P. Vignati , G. Matt , K. Iwasawa

NGC 1275 is a gamma-ray-emitting radio galaxy at the center of the Perseus cluster. Its multi-wavelength spectrum is similar to that of blazers, and thus a jet-origin of gamma-ray emissions is believed. In the optical and X-ray region, NGC…

High Energy Astrophysical Phenomena · Physics 2015-03-11 Ikumi Edahiro , Yasushi Fukazawa , Kenji Kawaguchi , Yasuyuki Tanaka , Ryosuke Itoh , Yuka Kanda , Kensei Shiki

We report on the results of a three-year program of coordinated X-ray and optical monitoring of the narrow-line Seyfert 1 galaxy NGC 4051. The rapid continuum variations observed in the X-ray spectra are not detected in the optical,…

We report on some results from a three-year program of RXTE observations of 4 Seyfert galaxies: NGC 4051, NGC 5548, MCG-6-30-15 and NGC 5506. We focus here on color-color and color-flux diagrams obtained using the count-rates of the PCA…

Astrophysics · Physics 2007-05-23 P. O. Petrucci , I. Papadakis , F. Haardt , L. Maraschi , I. McHardy , P. Uttley

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 present a detailed X-ray variability study of the low mass Active Galactic Nuclei (AGN) NGC 7314 using the two newly obtained XMM-Newton observations ($140$ and $130$ ks), together with two archival data sets of shorter duration ($45$…

High Energy Astrophysical Phenomena · Physics 2016-07-27 D. Emmanoulopoulos , I. M. McHardy , S. Vaughan , I. E. Papadakis

We present the results of timing analysis of the XMM-Newton observation of the Seyfert 2 galaxy NGC 6300. The hard X-ray spectrum above 2 keV consists of a Compton-thin-absorbed power law, as is often seen in Seyfert 2 galaxies. We clearly…

Astrophysics · Physics 2009-11-13 H. Awaki , H. Murakami , K. M. Leighly , C. Matsumoto , K. Hayashida , D. Grupe

The Seyfert Galaxy Mrk 335 is known for its frequent changes of flux and spectral shape in the X-ray band occurred during recent years. These variations may be explained by the onset of a wind that previous, non-contemporaneous…

X-ray point sources in galaxies are dominated by X-ray binaries (XRBs) that are variables or transients and whether their variability would alter the X-ray luminosity functions (XLF) is still in debate. Here we report on NGC 7331 as an…

High Energy Astrophysical Phenomena · Physics 2019-07-17 Ruolan Jin , Albert K. H. Kong

We report on observations of the narrow line Seyfert galaxy NGC 5506 with the Rossi X-ray TIming Explorer. The observations cover a time interval of ~1000 days during which the source showed strong flux and spectral variability. The…

Astrophysics · Physics 2011-05-10 G. Lamer , P. Uttley , I. M. McHardy

We examine a 200 ks XMM-Newton observation of the narrow-line Seyfert 1 galaxy Mrk 493. The active galaxy was half as bright as in a previous 2003 snapshot observation and the current lower flux enables a study of the putative reflection…

High Energy Astrophysical Phenomena · Physics 2018-04-18 K. Bonson , L. C. Gallo , D. R. Wilkins , A. C. Fabian

The recent detection of gamma-ray emission from four radio-loud narrow-line Seyfert 1 galaxies suggests that the engine driving the AGN activity of these objects share some similarities with that of blazars, namely the presence of a…

High Energy Astrophysical Phenomena · Physics 2015-05-20 G. Calderone , L. Foschini , G. Ghisellini , M. Colpi , L. Maraschi , F. Tavecchio , R. Decarli , G. Tagliaferri

We present the results of a search for X-ray variability in the galactic open cluster NGC 2516. This cluster has been observed on 8 occasions using XMM-Newton making it an excellent target for such a study. We find 4 sources which show…

Astrophysics · Physics 2008-11-26 Gavin Ramsay , Louise Harra , Hilary Kay

We discuss preliminary results from a joint XMM-Newton and NuSTAR monitoring program on the active galactic nucleus NGC 4593, consisting of 5x20 ks observations, spaced by two days, performed in January 2015. The source is found to be…

High Energy Astrophysical Phenomena · Physics 2016-05-25 F. Ursini , P. -O. Petrucci , G. Matt , S. Bianchi , M. Cappi , B. De Marco , A. De Rosa , J. Malzac , G. Ponti

We report on the multi-year evolution of the population of X-ray sources in the nuclear region of NGC 3621 based on Chandra, XMM-Newton and Swift observations. Among these, two sources, X1 and X5, after their first detection in 2008, seem…

We present an analysis of the rms variability spectra of a sample of 18 observations of 14 Seyfert galaxies observed by XMM-Newton, which exhibit sufficient variability and signal-to-noise ratio to examine the variations in the iron K-band.…

Cosmology and Nongalactic Astrophysics · Physics 2016-03-02 Shyam Bhayani , Kirpal Nandra
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