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We present the first high-resolution X-ray spectrum of the Seyfert 1.5 galaxy NGC 4151. Observations with the Chandra High Energy Transmission Grating Spectrometer reveal a spectrum dominated by narrow emission lines from a spatially…

Astrophysics · Physics 2009-10-31 P. M. Ogle , H. L. Marshall , J. C. Lee , C. R. Canizares

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…

Astrophysics · Physics 2009-11-11 G. Matt , S. Bianchi , A. De Rosa , P. Grandi , G. C. Perola

We present the first results from a detailed analysis of a new, long ($\sim100$ ks) XMM-Newton observation of the narrow-line Seyfert 1 galaxy PG 1404$+$226 which showed a large-amplitude, rapid X-ray variability by a factor of $\sim7$ in…

High Energy Astrophysical Phenomena · Physics 2018-08-29 Labani Mallick , Gulab C. Dewangan

BeppoSAX observed the Seyfert 1 galaxy NGC 3783 for ~ 5 days from 1998 June 6 to 1998 June 10. The average flux during the observation was F(2-10 keV) ~ 6 X 10^{-11} erg cm^-2 s^-1. The long exposure provided a very high quality spectrum…

Astrophysics · Physics 2009-11-07 A. De Rosa , L. Piro , F. Fiore , P. Grandi , L. Maraschi , G. Matt , F. Nicastro , P. O. Petrucci

We discuss the origin of a very unusual spectral structure observed in the Fe-K band of the Seyfert galaxy Mrk 1513, a local ($z$=0.063) active galactic nucleus (AGN) that is efficiently accreting matter onto its central supermassive black…

High Energy Astrophysical Phenomena · Physics 2023-12-20 R. Middei , E. Nardini , G. A. Matzeu , S. Bianchi , V. Braito , M. Perri , S. Puccetti

We present an X-ray analysis of three different XMM-Newton observations together with simultaneous NICER and NuSTAR observations of the ultraluminous X-ray source NGC 4190 ULX-1. Our goal is to constrain the structure of the accretion disk…

Any cold, optically-thick matter in the vicinity of an accreting black hole, such as the accretion disk, can intercept and reprocess some fraction of the hard X-ray continuum emission, thereby imprinting atomic features into the observed…

Astrophysics · Physics 2007-05-23 C. S. Reynolds

The XMM-Newton data presented here are the first X-ray observation of the Seyfert 2 galaxy NGC4138. Although the galaxy has been pointed by ROSAT-HRI, it was not detected, with a flux upper limit of about 1.1x10^-13 erg cm^-2 s^-1 in the…

We report on the X-ray spectral variability of the Seyfert 1 galaxy NGC 4051 observed with the Rossi X-ray Timing Explorer (RXTE) during a 1000 day period between May 1996 and March 1999. The spectra were obtained as part of monitoring…

Astrophysics · Physics 2009-11-07 G. Lamer , I. M. McHardy , P. Uttley , K. Jahoda

We use the full broad-band XMM-Newton EPIC data to examine the X-ray spectrum of the nearby Seyfert 2 galaxy NGC 1068, previously shown to be complex with the X-ray continuum being a sum of components reflected/scattered from cold (neutral)…

Astrophysics · Physics 2009-11-11 K. Pounds , S. Vaughan

Using a Monte Carlo method, we derive spectra arising from Comptonization taking place close to a Kerr black hole. We consider a model consisting of a hot thermal corona Comptonizing seed photons emitted by a cold accretion disc. We find…

Astrophysics · Physics 2009-11-10 Andrzej Niedzwiecki

We report the results from a Chandra TOO observation of the low-luminosity Narrow Line Seyfert 1 galaxy NGC 4051, obtained during a 6-week duration low-flux state in 2001 February. During the Chandra observation, the 2-10 keV source flux…

Astrophysics · Physics 2009-11-07 P. Uttley , A. Fruscione , I. McHardy , G. Lamer

We performed a detailed broadband spectral and timing analysis of a small flaring event of ~120 ks in a narrow-line Seyfert 1 galaxy NGC 4051 using simultaneous XMM-Newton and NuSTAR observations. The ~300 ks long NuSTAR observation and the…

High Energy Astrophysical Phenomena · Physics 2023-03-29 Neeraj Kumari , Arghajit Jana , Sachindra Naik , Prantik Nandi

We report the detection with the Rossi X-ray Timing Explorer of a Compton reflection signature in the Seyfert galaxy MCG-5-23-16. RXTE also resolves the Fe K-alpha fluorescence line with FWHM ~48,000 km s^{-1}. This measurement provides the…

Astrophysics · Physics 2009-10-30 K. A. Weaver , J. H. Krolik , E. A. Pier

We have monitored the Seyfert galaxy NGC 3227 with the Rossi X-ray Timing Explorer (RXTE) since January 1999. During late 2000 and early 2001 we observed an unusual hardening of the 2-10 keV X-ray spectrum which lasted several months. The…

Astrophysics · Physics 2009-11-07 G. Lamer , P. Uttley , I. M. McHardy

Spectra of Seyfert Is are commonly modelled as emission from an X-ray illuminated flat accretion disc orbiting a central black hole. This provides both a reprocessed and direct component of the X-ray emission as required by observations of…

Astrophysics · Physics 2009-10-31 Eric G. Blackman

We have analyzed spectra for all active galactic nuclei in the Rossi X-ray Timing Explorer (RXTE) archive. We present long-term average values of absorption, Fe line equivalent width, Compton reflection and photon index, as well as…

High Energy Astrophysical Phenomena · Physics 2015-06-16 Elizabeth Rivers , Alex Markowitz , Richard Rothschild

We present new results from BeppoSAX observations of reflection-dominated Seyfert galaxies, and namely: 1) the Compton-thick Seyfert 2s NGC1068 and Circinus Galaxy; 2) the Seyfert 1 NGC4051, whose nucleus was observed on May 1998 to have…

Astrophysics · Physics 2009-10-31 M. Guainazzi , G. Matt , F. Fiore

We consider implications of a possible presence of a Thomson-thick, low-temperature, plasma cloud surrounding the compact object in the binary system Cyg X-3. The presence of such a cloud was earlier inferred from the energy-independent…

High Energy Astrophysical Phenomena · Physics 2011-04-07 A. A. Zdziarski , R. Misra , M. Gierlinski

We report the XMM-Newton discovery of the first Compton-thick obscured AGN in a Broad Line Radio Galaxy, the Gigahertz Peaked-Spectrum source Mkn668 (OQ+208). The remarkably flat 2-10 keV X-ray spectrum (observed photon index, \Gamma ~…

Astrophysics · Physics 2009-11-10 M. Guainazzi , A. Siemiginowska , P. Rodriguez-Pascual , C. Stanghellini