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相关论文: X-ray spectral variability in NGC 3783

200 篇论文

Accreting supermassive black holes at the centres of galaxies are the engine of active galactic nuclei (AGN). X-ray light curves of unabsorbed AGN show dramatic random variability on timescales ranging from seconds to years. The power…

高能天体物理现象 · 物理学 2025-10-29 Mehdy Lefkir , Simon Vaughan , Mike Goad , Daniela Huppenkothen , Phil Uttley

The analysis of a series of seven observations of the nearby ($z=0.0809$) QSO, PG 1211+143, taken with the Reflection Grating Spectrometer (RGS) on-board XMM-Newton in 2014, are presented. The high resolution soft X-ray spectrum, with a…

高能天体物理现象 · 物理学 2018-02-21 James Reeves , Andrew Lobban , Ken Pounds

We present the analysis of X-ray spectral varability made on a sample of 7 Seyfert 1 bright galaxies, using XMM-Newton data. From the "XMM-Newton Science Archive" we selected those bright Seyfert 1 showing one or more prominent flares in…

天体物理学 · 物理学 2008-11-26 B. De Marco , M. Cappi , M. Dadina , G. G. C. Palumbo

We present RXTE monitoring observations of the Seyfert 2 galaxy Mrk 348 spanning a 6 month period. The time-averaged spectrum in the 3-20 keV band shows many features characteristic of a Compton-thin Seyfert 2 galaxy, namely a hard…

天体物理学 · 物理学 2009-10-31 David A. Smith , Ioannis Georgantopoulos , Robert S. Warwick

We present a flux-resolved X-ray analysis of the dwarf Seyfert 1.8 galaxy NGC 4395, based on three archival $XMM-Newton$ and one archival $NuSTAR$ observations. The source is known to harbor a low mass black hole ($\sim 10^4- {\rm a~…

We present a spectroscopic analysis of XMM-Newton and NuSTAR observations of the 'complex' NLS1 PG 1535+547 at redshift $z=0.038$. These observations span three epochs: 2002 and 2006 with XMM-Newton alone, covering the $0.3-10$ keV energy…

We report the detection of an absorbed central X-ray source and its strong, rapid variability in NGC4395, the least luminous Seyfert nucleus known. The X-ray source exhibits a number of flares with factors of 3-4 flux changes during a half…

天体物理学 · 物理学 2009-09-17 K. Iwasawa , A. C. Fabian , O. Almaini , P. Lira , A. Lawrence , K. Hayashida , H. Inoue

In this paper, we make a multi-epoch analysis of NGC 1052, one of the prototypical LLAGN, using XMM-Newton, Suzaku and NuSTAR observations, taken from 2001 to 2017. This is the first time that results from NuSTAR observations are reported…

We present results from analysis of the X-ray archive data of MCG-2-58-22, acquired with ROSAT from 1991 to 1993 and with ASCA from 1993 to 1997. By analyzing light curves, we find that MCG-2-58-22 shows a clear time variability in X-ray…

天体物理学 · 物理学 2007-05-23 Chul-Sung Choi , Tadayasu Dotani , Insu Yi , ChulHee Kim

We present the analysis of the X-ray variability and spectral timing properties of the ultraluminous X-ray source (ULX) NGC 5408 X-1, one of the most variable ULXs known so far. The variability properties are used as a diagnostic of the…

高能天体物理现象 · 物理学 2015-06-17 B. De Marco , G. Ponti , G. Miniutti , T. Belloni , M. Cappi , M. Dadina , T. Muñoz-Darias

We analyse the spectra of the archival XMM-Newton data of the Seyfert 1 AGN Zw 229.015 in the energy range $0.3 - 10.0$ keV. When fitted with a simple power-law, the spectrum shows signatures of weak soft excess below 1.0 keV. We find that…

星系天体物理 · 物理学 2016-12-21 Oluwashina Adegoke , Suvendu Rakshit , Banibrata Mukhopadhyay

We report X-ray spectral variability in an ultraluminous X-ray source NGC 1042 ULX1, using archival XMM-Newton and recent NuSTAR observations. In long-term evolution, the source has shown a trend of variation in spectral hardness. The…

高能天体物理现象 · 物理学 2022-11-09 Tanuman Ghosh , Vikram Rana

We analyse the spectral variability of MCG--06-30-15 with 600 ks of XMM-Newton data, including 300 ks of new data from the joint XMM-Newton and NuSTAR 2013 observational campaign. We use principal component analysis to find high resolution,…

高能天体物理现象 · 物理学 2015-06-17 M. L. Parker , A. Marinucci , L. Brenneman , A. C. Fabian , E. Kara , G. Matt , D. J. Walton

The bright type I Seyfert galaxy NGC 3516 was observed by {\it Suzaku} twice, in 2005 October 12--15 and 2009 October 28--November 2, for a gross time coverage of 242 and 544 ksec and a net exposure of 134 and 255 ksec, respectively. The…

高能天体物理现象 · 物理学 2014-06-20 Hirofumi Noda , Kazuo Makishima , Kazuhiro Nakazawa , Shin'ya Yamada

We present a spectral variability study of the ultraluminous X-ray source NGC 4490 ULX-8 based on 14 Chandra, 6 XMM-Newton and 19 Swift-XRT observations obtained between 2000 and 2024. The X-ray spectra are modelled using absorbed power-law…

高能天体物理现象 · 物理学 2026-05-25 Tarang Vashisht , Aru Beri , Tanuman Ghosh , Aman Upadhyay , Vikram Rana

Variability studies offer a compelling glimpse into black hole dynamics, and NICER's (Neutron Star Interior Composition Explorer) remarkable temporal resolution propels us even further. NICER observations of an Active Galactic Nucleus…

高能天体物理现象 · 物理学 2025-01-23 B. Rani , Jungeun Kim , I. Papadakis , K. C. Gendreau , M. Masterson , K. Hamaguchi , E. Kara , S. -S. Lee , R. Mushotzky

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 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…

天体物理学 · 物理学 2009-11-07 G. Lamer , I. M. McHardy , P. Uttley , K. Jahoda

We report an intrinsic absorber with decreasing outflow velocity in the Seyfert 1 galaxy NGC 3783. This is the first detection of a change in radial velocity in an outflow associated with a Seyfert galaxy. These results are based on…

We study the Frequency Resolved Spectra of the Seyfert galaxy MCG -6-30-15 obtained during two recent XMM-Newton observations. Splitting the Fourier spectra in soft (<2 keV) and hard (>2 keV) bands, we find that the soft band has a…

天体物理学 · 物理学 2009-11-11 I. E. Papadakis , D. Kazanas , A. Akylas