English
Related papers

Related papers: Studying X-ray reprocessing and continuum variabil…

200 papers

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…

In March 2009 the well-studied quasar, PG 0844+349, was discovered with Swift to be in an X-ray weak state. A follow-up XMM-Newton observation several weeks later generated a good quality spectrum of the source, showing substantial…

High Energy Astrophysical Phenomena · Physics 2015-05-20 L. C. Gallo , D. Grupe , N. Schartel , S. Komossa , G. Miniutti , A. C. Fabian , M. Santos-Lleo

We examine simultaneous X-ray and UV light curves from multi-epoch 8 day XMM Newton observations of the narrow line Seyfert 1 galaxy 1H 0707-495. The simultaneous observations reveal that both X-ray and UV emission are variable and that the…

High Energy Astrophysical Phenomena · Physics 2015-07-21 Damien Robertson , Luigi C. Gallo , Abderahmen Zoghbi , Andrew C. Fabian

We present results from intensive (x3 daily), three-month-long X-ray, UV and optical monitoring of the bright Seyfert active galactic nucleus (AGN) MCG+08-11-11 with Swift, supported by optical-infrared ground-based monitoring. The 12…

We present the results from a study of the timing properties and the energy spectrum of the radio-quiet quasar PG0804+761, based on monitoring RXTE PCA observations that lasted for a year. This is a systematic study of the X-ray variations…

Astrophysics · Physics 2009-11-07 I. E. Papadakis , P. Reig , K. Nandra

The narrow-line Seyfert 1 galaxy (NLS1) Mrk 335 has been continuously monitored with Swift since May 2007 when it fell into a long-lasting, X-ray low-flux interval. Results from the nearly 11 years of monitoring are presented here.…

High Energy Astrophysical Phenomena · Physics 2018-05-16 L. C. Gallo , D. M. Blue , D. Grupe , S. Komossa , D. R. Wilkins

We report on the results of a multiwavelength monitoring campaign of the bright, nearby Seyfert galaxy, Ark 120 using a ~50-day observing programme with Swift and a ~4-month co-ordinated ground-based observing campaign, predominantly using…

The X-ray emission from active galactic nuclei (AGN) is believed to come from a combination of inverse Compton scattering of photons from the accretion disk and reprocessing of the direct X-ray emission by reflection. We present hard (10-80…

High Energy Astrophysical Phenomena · Physics 2023-12-01 Cora A. DeFrancesco , Xinyu Dai , Mark Mitchell , Abderahmen Zoghbi , Christopher W. Morgan

We present the results from the multi-wavelength monitoring observations of the Narrow-Line Seyfert 1 galaxy Mrk 335 with AstroSat. We analysed both the X-ray (SXT & LAXPC) and UV (UVIT) data of the source at two epochs, separated by ~18…

High Energy Astrophysical Phenomena · Physics 2021-06-30 Savithri H. Ezhikode , Gulab C. Dewangan , Ranjeev Misra

We propose a theoretical model to explain the spectrum of the quasar PG1211+143 emitted in the Optical/X-ray bands. In particular, we suggest that the inner accretion disk may develop a warm, optically thick skin, which produces a profound…

Astrophysics · Physics 2007-05-23 Agnieszka Janiuk , Bozena Czerny , Grzegorz M. Madejski

We present optical observations of the low-luminosity Seyfert 1 nucleus of NGC 4395, as part of a multiwavelength reverberation-mapping program. Observations were carried out over two nights in 2004 April at Lick, Wise, and Kitt Peak…

We analyse the X-ray time-lags in the Narrow Line Seyfert 1 (NLS1) galaxy PG 1244+026 ($M_{\rm BH}\sim 10^7 M_{\rm sun}$, $L/L_{\rm Edd}\sim 1$). The time delay between the soft (0.3--0.7~keV) and harder (1.2--4.0~keV) variations shows…

High Energy Astrophysical Phenomena · Physics 2015-06-18 William Alston , Chris Done , Simon Vaughan

Active galactic nuclei are known to exhibit flux variations across the entire electromagnetic spectrum. Among these, correlations between UV/optical and X-ray flux variations serve as a key diagnostics for understanding the physical…

Astrophysics of Galaxies · Physics 2026-01-09 M. Reshma , C. S. Stalin , Amit Kumar Mandal , Abhijit Kayal , S. B. Gudennavar , Prajwel Joseph

This paper combines data from the three preceding papers in order to analyze the multi-waveband variability and spectral energy distribution of the Seyfert~1 galaxy NGC~4151 during the December 1993 monitoring campaign. The source, which…

Astrophysics · Physics 2009-10-28 R. A. Edelson et al

We present the first results of a high-cadence Swift monitoring campaign ($3-4$ visits per day for $75$ days) of the Seyfert 1.5 galaxy NGC 6814 characterizing its variability throughout the X-ray and UV/optical wavebands. Structure…

High Energy Astrophysical Phenomena · Physics 2023-08-31 Adam G. Gonzalez , Luigi C. Gallo , Jon M. Miller , Elias S. Kammoun , Akshay Ghosh , Ben A. Pottie

We present the results of an intensive six-month optical continuum reverberation mapping campaign of the Seyfert 1 galaxy PG 2130+099 at redshift z=0.063. The ground-based photometric monitoring was conducted on a daily basis with the…

Astrophysics of Galaxies · Physics 2022-03-14 C. Fian , D. Chelouche , S. Kaspi , C. Sobrino Figaredo , S. Catalan , T. Lewis

The Narrow-line Seyfert 1 galaxy (NLS1) Mkn 335 is remarkable because it has repeatedly shown deep, long X-ray low-states which show pronounced spectral structure. It has become one of the prototype AGN in deep minimum X-ray states. Here we…

High Energy Astrophysical Phenomena · Physics 2015-06-04 D. Grupe , S. Komossa , L. C. Gallo , A. L. Longinotti , A. C. Fabian , A. K. Pradhan , M. Gruberbauer , D. Xu

We present a revised analysis of the photometric reverberation mapping campaign of the narrow-line Seyfert 1 galaxy PKS 0558-504 carried out with the Swift Observatory during 2008--2010. Previously, Gliozzi et al.\ found using the Discrete…

We present a detailed multi-frequency analysis of an intense monitoring programme of Seyfert 1 galaxy NGC 4593 over a duration of nearly for a month with Swift observatory. We used 185 pointings to study the variability in six…

High Energy Astrophysical Phenomena · Physics 2019-08-17 Main Pal , Sachindra Naik

PHL 1092 is a z~0.4 high-luminosity counterpart of the class of Narrow-Line Seyfert 1 galaxies. In 2008, PHL 1092 was found to be in a remarkably low X-ray flux state during an XMM-Newton observation. Its 2 keV flux density had dropped by a…

High Energy Astrophysical Phenomena · Physics 2015-06-05 G. Miniutti , W. N. Brandt , D. P. Schneider , A. C. Fabian , L. C. Gallo , Th. Boller