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相关论文: EUVE-RXTE simultaneous observations of NGC 4051: v…

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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 present a flux variability study of simultaneous RXTE and EUVE observations of the highly variable Seyfert galaxy NGC4051. We find a strong correlation between variability in the EUV and medium energy X-ray bands,indicating that both are…

天体物理学 · 物理学 2009-10-31 P. Uttley , I. M. McHardy , I. E. Papadakis , I. Cagnoni , A. Fruscione

We present spectral and timing analysis of all the data collected by the Extreme Ultraviolet Explorer for the BL Lac object Mrk 421 from 1994 to 1997. During these years Mrk 421 has been observed by EUVE 4 times with the DS/Spectrograph and…

天体物理学 · 物理学 2007-05-23 Ilaria Cagnoni , Antonella Fruscione , Iossif E. Papadakis

We present simultaneous observations by EUVE, ASCA, and RXTE of the type~1 Seyfert galaxy NGC 5548. These data indicate that variations in the EUV emission (at $\sim 0.2 $keV) appear to lead similar modulations in higher energy ($\ga 1…

天体物理学 · 物理学 2009-10-31 J. Chiang , C. S. Reynolds , O. M. Blaes , M. A. Nowak , N. Murray , G. Madejski , H. L. Marshall , P. Magdziarz

We analyse 15 XMM-Newton observations of the Seyfert galaxy NGC 4051 obtained over 45 days to determine the ultraviolet (UV) light curve variability characteristics and search for correlated UV/X-ray emission. The UV light curve shows…

高能天体物理现象 · 物理学 2015-06-11 W. N. Alston , S. Vaughan , P. Uttley

We present intensive quasi-simultaneous X-ray and radio monitoring of the narrow line Seyfert 1 galaxy NGC 4051, over a 16 month period in 2000-2001. Observations were made with the Rossi Timing X-ray Explorer (RXTE) and the Very Large…

高能天体物理现象 · 物理学 2015-05-20 Sadie Jones , Ian McHardy , Derek Moss , Nick Seymour , Elme Breedt , Phil Uttley , Elmar Kording , Valeriu Tudose

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…

天体物理学 · 物理学 2007-05-23 P. O. Petrucci , I. Papadakis , F. Haardt , L. Maraschi , I. McHardy , P. Uttley

We present the results of an intensive ultraviolet monitoring campaign on the Seyfert 1 galaxy NGC 4151, as part of an effort to study its short time-scale variability over a broad range in wavelength. The nucleus of NGC 4151 was observed…

天体物理学 · 物理学 2010-12-16 D. M. Crenshaw et al

We analyzed the ~950 ks of spectroscopic data accumulated by the Extreme Ultraviolet Explorer (EUVE) satellite between 1994 and 1997 for the BL Lacertae object Markarian 421. The EUV spectrum is well detected in the 70-110 A (112-177 eV)…

天体物理学 · 物理学 2009-10-31 Ilaria Cagnoni , Antonella Fruscione

The Extreme Ultraviolet Explorer (EUVE) satellite accumulated ~one million seconds of public data between 1994 and 1997 for the BL Lacertae object Markarian 421. This is the second of two papers in which we present the results of spectral…

天体物理学 · 物理学 2009-10-31 Ilaria Cagnoni , Antonella Fruscione , Iossif E. Papadakis

We present the results of an extensive analysis of the ``ASCA'' AO2 observation of the Seyfert 1 galaxy NGC4051. The target exhibits broadband [0.5--10 keV] variability by a factor $\sim 8$ on time scales $\sim 10^4 s$, with a typical…

天体物理学 · 物理学 2015-06-24 Matteo Guainazzi , Tatehiro Mihara , Chiko Otani , Masaru Matsuoka

On 9-11 May 1998, the highly-variable, low luminosity Seyfert 1 galaxy NGC4051 was observed in an unusual low flux state by BeppoSAX (Guainazzi et al. 1998) RXTE and EUVE. We present fits of the 4-15 keV RXTE spectrum and BeppoSAX MECS…

天体物理学 · 物理学 2009-10-31 P. Uttley , I. M. McHardy , I. E. Papadakis , M. Guainazzi , A. Fruscione

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,…

The Deep Survey instrument on the Extreme Ultraviolet Explorer satellite (EUVE) obtained long, nearly continuous soft X-ray light curves of 5-33 days duration for 14 Seyfert galaxies and QSOs. We present a uniform reduction of these data,…

天体物理学 · 物理学 2009-11-07 J. P. Halpern , K. M. Leighly , H. L. Marshall

The Narrow Line Seyfert 1 galaxy NGC 4051 was observed in one of its prolonged low-lux states by XMM-Newton in November 2002. Here we present the results of an analysis of EPIC-pn data obtained during the observation. Within the low state,…

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

We present a comprehensive examination of the X-ray variability of the narrow line Seyfert 1 (NLS1) galaxy NGC4051. We combine over 6.5 years of frequent monitoring observations by RXTE with a >100ks continuous observation by XMM-Newton and…

天体物理学 · 物理学 2009-11-10 I. M. McHardy , I. E. Papadakis , P. Uttley , K. O. Mason , M. J. Page

We report on two Chandra observations, and a simultaneous Hubble Space Telescope ultraviolet observation, of the dwarf Seyfert 1 galaxy NGC 4395. Each Chandra observation had a duration of ~30 ks, with a separation of ~50 ks. The spectrum…

We present the first X-ray monitoring observations of the X-ray bright FRI radio galaxy NGC6251 observed with RXTE for 1 year. The primary goal of this study is to shed light on the origin of the X-rays, by investigating the spectral…

天体物理学 · 物理学 2009-11-13 M. Gliozzi , I. E. Papadakis , R. M. Sambruna

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…

We present a series of RXTE observations of the nearby obscured Seyfert galaxies ESO103-G35, IC5063, NGC4507 and NGC7172. The period of monitoring ranges from seven days for NGC7172 up to about seven months for ESO103-G035. The spectra of…

天体物理学 · 物理学 2009-10-31 I. Georgantopoulos , I. Papadakis
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