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Using the latest 70 month Swift-BAT catalog we examined hard X-ray selected Seyfert I galaxies which are relatively little known and little studied, and yet potentially promising to test the ionized relativistic reflection model. From this…

Astrophysics of Galaxies · Physics 2014-12-03 Andrew C. Liebmann , Andrew C. Fabian , Sachiko Tsuruta

Utilizing a range of techniques including multi-band light curves, softness ratio analysis, structure functions, rms spectra, cross-correlation functions, and ratios of spectra from different intervals, we present a comprehensive study of…

High Energy Astrophysical Phenomena · Physics 2024-10-31 Lu-Xin Ren , Jun-Xian Wang , Jia-Lai Kang

We present results of a high-resolution soft X-ray (0.2-2 keV) spectroscopic study of a sample of 69 nearby obscured Active Galactic Nuclei (AGN) observed with the Reflection Grating Spectrometer (RGS) on board XMM-Newton. This is the…

Astrophysics · Physics 2008-11-26 Matteo Guainazzi , Stefano Bianchi

MCG-5-23-16 is one of the first AGN where relativistic reverberation in the iron K line originating in the vicinity of the supermassive black hole was found, based on a short XMM-Newton observation. In this work, we present the results from…

We develop a physically motivated, spherical corona model to investigate the frequency-dependent time lags in AGN. The model includes the effects of Compton up-scattering between the disc UV photons and coronal electrons, and the subsequent…

High Energy Astrophysical Phenomena · Physics 2022-08-31 P. Chainakun , A. Watcharangkool , A. J. Young , S. Hancock

We present the Granger causality (GC) test for the X-ray reverberation analysis of Active Galactic Nuclei (AGN). If the light curves in the continuum-dominated band help predict (Granger cause) those dominated by reflection, the Granger…

High Energy Astrophysical Phenomena · Physics 2024-04-09 N. Nakhonthong , P. Chainakun , W. Luangtip , A. J. Young

Large-scale outflows are generally considered as a possible evidence that active galactic nuclei (AGNs) can severely affect their host galaxies. Recently an ultraluminous IR galaxy (ULIRG) at $z=0.49$, AKARI J0916248+073034, was found to…

We present the first systematic study of the molecular gas and star formation efficiency in a sample of ten narrow-line Seyfert 1 galaxies selected to have X-ray Ultra Fast Outflows and, therefore, to potentially show AGN feedback effects.…

We present a spectral analysis of the NuSTAR and XMM-Newton observations of the Seyfert 1h galaxy/ULIRG IRAS 05189-2524 taken in 2013. We find evidence for relativistic disk reflection in the broadband X-ray spectrum: a highly asymmetric…

High Energy Astrophysical Phenomena · Physics 2017-03-08 Yanjun Xu , Mislav Balokovic , Dominic J. Walton , Fiona A. Harrison , Javier A. Garcia , Michael J. Koss

We present the results from an X-ray variability study of IRAS 13224-3809. This is probably the best source for X-ray reverberation studies since it is X-ray bright, extremely variable, and it has been extensively observed with XMM-Newton.…

High Energy Astrophysical Phenomena · Physics 2020-09-02 M. D. Caballero-Garcia , I. E. Papadakis , M. Dovciak , M. Bursa , J. Svoboda , V. Karas

We report the discovery and analysis of the follow-up ROSAT pointed observation, an ASCA observation and optical and radio observations of the enigmatic soft X-ray AGN RX J0134.2-4258. In the optical, RX J0134.2-4258 appears as an extreme…

Astrophysics · Physics 2007-05-23 D. Grupe , K. M. Leighly , H. -C. Thomas , S. A. Laurent-Muehleisen

A bright, soft X-ray source was detected on 2010 July 14 during an XMM--Newton slew at a position consistent with the galaxy GSN 069 (z=0.018). Previous ROSAT observations failed to detect the source and imply that GSN 069 is now >240 times…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 G. Miniutti , R. D. Saxton , P. M. Rodriguez-Pascual , A. M. Read , P. Esquej , M. Colless , P. Dobbie , M. Spolaor

Recent active galactic nucleus (AGN) and quasar surveys have revealed a population showing rapid AGN luminosity variability by a factor of $\sim10$. Here we present the most drastic AGN luminosity decline by a factor of $\gtrsim 10^{3}$…

High Energy Astrophysical Phenomena · Physics 2019-10-02 Kohei Ichikawa , Taiki Kawamuro , Megumi Shidatsu , Claudio Ricci , Hyun-Jin Bae , Kenta Matsuoka , Jaejin Shin , Yoshiki Toba , Junko Ueda , Yoshihiro Ueda

MCG-5-23-16 is a Seyfert 1.9 galaxy at redshift z=0.00849. We analyse here the X-ray spectra obtained with XMM-Newton and NuSTAR data, which are the first contemporaneous observations with these two X-ray telescopes. Two reflection…

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…

Astrophysics of Galaxies · Physics 2016-12-21 Oluwashina Adegoke , Suvendu Rakshit , Banibrata Mukhopadhyay

The primary X-ray emission in active galactic nuclei (AGN) originates in a compact region called the corona located very close to the super-massive black hole and the accretion disk. The knowledge of the cut-off energy ($E_{cut}$) of the…

High Energy Astrophysical Phenomena · Physics 2019-01-30 Priyanka Rani , C. S. Stalin , K. D. Goswami

We analyse high-quality NuSTAR observations of the local (z = 0.011) Seyfert 2 active galactic nucleus (AGN) IC 3639, in conjunction with archival Suzaku and Chandra data. This provides the first broadband X-ray spectral analysis of the…

We report on a study of the narrow Fe K$\alpha$ line and reflection spectrum in the well-known Seyfert-2 AGN, NGC 4388. X-ray spectra summed from two extensive NICER monitoring campaigns, separated by years, show strong evidence of…

High Energy Astrophysical Phenomena · Physics 2024-03-05 B. Gediman , J. M. Miller , A. Zoghbi , P. Draghis , Z. Arzoumanian , W. N . Brandt , K. Gendreau

We present a series of X-ray variability results from a long XMM-Newton + NuSTAR campaign on the bright, variable AGN NGC 3227. We present an analysis of the lightcurves, showing that the source displays typically softer-when-brighter…

High Energy Astrophysical Phenomena · Physics 2020-04-30 A. P. Lobban , T. J. Turner , J. N. Reeves , V. Braito , L. Miller

We investigate the nature of the soft excess below 1 keV observed in AGN. We use the XMM-Newton data of the low redshift, optically bright quasar, PG 1211+143, and we compare it with the Narrow Line Seyfert 1 galaxy, 1H 0707-495, which has…

Astrophysics · Physics 2016-08-30 Malgorzata Sobolewska , Chris Done