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Related papers: Rapid N_H changes in NGC 4151

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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

We present a new X-ray analysis of the dwarf Seyfert galaxy NGC 4395, based on two archival XMM-Newton and Suzaku observations. This source is well known for a series of remarkable properties: one of the smallest estimated black hole masses…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Emanuele Nardini , Guido Risaliti

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 narrow-line quasar PHL 1092 was observed by XMM-Newton at two epochs separated by nearly thirty months. Timing analyses confirm the extreme variability observed during previous X-ray missions. A measurement of the radiative efficiency…

Astrophysics · Physics 2009-09-17 L. C. Gallo , Th. Boller , W. N. Brandt , A. C. Fabian , D. Grupe

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…

Astrophysics · Physics 2009-11-10 D. Grupe , K. M. Leighly , V. Burwitz , P. Predehl , S. Mathur

Aims: We used data from the 58 month long, continuous Swift/Burst Alert Telescope (BAT) observations of the five brightest Seyfert galaxies at hard X-rays, to study their flux and spectral variability in the 20-100 keV energy band. The…

High Energy Astrophysical Phenomena · Physics 2015-05-30 M. D. Caballero-Garcia , I. E. Papadakis , F. Nicastro , M. Ajello

We present evidence of flux variability, on both short (hours) and long (months) time scales of the Seyfert 2 galaxy NGC 7172. These results are based on the ASCA observation of NGC 7172 performed on May 1996. The source was detected at a…

Astrophysics · Physics 2009-10-30 M. Guainazzi , G. Matt , L. A. Antonelli , F. Fiore , L. Piro , S. Ueno

We report results from a Suzaku observation of the narrow-line Seyfert 1 NGC 4051. During our observation, large amplitude rapid variability is seen and the averaged 2--10 keV flux is 8.1x10^-12 erg s^-1 cm^-2, which is several times lower…

Observations of the C IV and Mg II absorption lines in the Seyfert 1 galaxy NGC 4151 obtained with the GHRS in October 1994 are presented. The data from the STScI archive show multiple broad and narrow components in both species. In…

Astrophysics · Physics 2007-05-23 Gerard A. Kriss

We present the variability analysis of a 100 ks XMM-Newton observation of the Seyfert 1.5 active galaxy NGC 3227. The observation found NGC 3227 in a period where its hard power-law component displayed remarkably little long-term…

Astrophysics of Galaxies · Physics 2015-06-18 P. Arévalo , A. Markowitz

Direct time-resolved spectral fitting has been performed on continuous RXTE monitoring of seven Seyfert 1 galaxies in order to study their broadband spectral variability and Fe K alpha variability characteristics on time scales of days to…

Astrophysics · Physics 2009-11-10 A. Markowitz , R. Edelson , S. Vaughan

We present the results of recent Chandra High-Energy Transmission Grating Spectrometer and Hubble Space Telescope Cosmic Origins Spectrograph observations of the nearby Seyfert 1 galaxy NGC 3783 which shows a strong, non-varying X-ray warm…

High Energy Astrophysical Phenomena · Physics 2015-06-23 A. E. Scott , W. N. Brandt , E. Behar , D. M. Crenshaw , J. R. Gabel , R. R. Gibson , S. Kaspi , S. B. Kraemer , T. J. Turner

We obtained observations of NGC 4639 with ASCA in order to investigate its mildly active Seyfert 1 nucleus at hard X-ray energies. Koratkar et al. (1995) have previously shown that the nucleus is a pointlike source in the ROSAT soft X-ray…

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 present the results of ultraviolet spectral monitoring of the Seyfert galaxy NGC 4151 performed by the Hopkins Ultraviolet Telescope during the Astro-2 mission. We show how the response of the Lyman continuum optical depth to variations…

Astrophysics · Physics 2007-05-23 J. H. Krolik , G. A. Kriss

We present a multi-wavelength spectral study of NGC 4151 based on five epochs of simultaneous AstroSat observations in the near ultra-violet (NUV) to hard X-ray band ($\sim 0.005-80$ keV) during $2017 - 2018$. We derived the intrinsic…

We present the results of the Suzaku observation of the Seyfert 2 galaxy NGC 4507. This source is one of the X-ray brightest Compton-thin Seyfert 2s and a candidate for a variable absorber. Suzaku caught NGC 4507 in a highly absorbed state…

High Energy Astrophysical Phenomena · Physics 2015-06-11 V. Braito , L. Ballo , J. N. Reeves , A. Ptak , G. Risaliti , T. J. Turner

Results of a long-term spectral monitoring of the active galactic nucleus of NGC 4151 are presented (11 years, from 1996 to 2006). High quality spectra (S/N>50 in the continuum near Halpha and Hbeta) were obtained in the spectral range…

Results of the long-term (11 years, from 1996 to 2006) H$\alpha$ and H$\beta$ line variations of the active galactic nucleus of NGC 4151 are presented. High quality spectra (S/N>50 and R~8A) of H$\alpha$ and H$\beta$ were investigated. We…

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…

Astrophysics · Physics 2016-06-08 W. N. Brandt , K. Iwasawa , C. S. Reynolds