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Related papers: X-ray absorption variability in NGC 4507

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We present a detailed study of the highly obscured active galaxy NGC 4507, performed using four Nuclear Spectroscopic Telescope Array (NuSTAR) observations carried out between May and August in 2015 (~ 130 ks in total). Using various…

We present new evidence of X-ray absorption variability on time scales from a few hours to a few days for several nearby bright AGNs. The observed N_H variations imply that the X-ray absorber is made of clouds eclipsing the X-ray source…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Guido Risaliti

We present an analysis of the extreme obscuration variability observed during an XMM-Newton 5-days continuous monitoring of the AGN in NGC 1365. The source was in a reflection-dominated state in the first ~1.5 days, then a strong increase…

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

During an extensive multiwavelength campaign that we performed in 2013-14 the prototypical Seyfert 1 galaxy NGC 5548 has been found in an unusual condition of heavy and persistent obscuration. The newly discovered "obscurer" absorbs most of…

We present a time, spectral and imaging analysis of the X-ray reflector in NGC 4945, which reveals its geometrical and physical structure with unprecedented detail. NGC 4945 hosts one of the brightest AGN in the sky above 10 keV, but it is…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 A. Marinucci , G. Risaliti , Junfeng Wang , E. Nardini , M. Elvis , G. Fabbiano , S. Bianchi , G. Matt

Variable X-ray absorption has been observed in active galactic nuclei (AGN) on several time scales. Observations allow us to identify the absorber with clouds associated either with the clumpy torus (parsec scales, long timescales) or with…

High Energy Astrophysical Phenomena · Physics 2018-10-18 Mario Sanfrutos , Giovanni Miniutti , Michal Dovčiak , Beatriz Agís-González

We present a Chandra monitoring campaign of the highly variable Seyfert galaxy UGC 4203 (the "Phoenix Galaxy") which revealed variations in the X-ray absorbing column density on time scales of two weeks. This is the third, clear case, after…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 G. Risaliti , M. Elvis , S. Bianchi , G. Matt

We present a study of the variations in the absorbing column density of 25 X-ray defined Seyfert 2 galaxies, as inferred from hard X-ray observations, on timescales from months to several years. We show that a significant variation of N$_H$…

Astrophysics · Physics 2009-11-06 G. Risaliti , M. Elvis , F. Nicastro

NGC 7582 (z = 0.005264; D = 22.5 Mpc) is a highly variable, changing-look AGN. In this work, we explore the X-ray properties of this source using XMM-Newton and NuSTAR archival observations in the 3-40 keV range, from 2001 to 2016. NGC 7582…

High Energy Astrophysical Phenomena · Physics 2023-04-12 Mehdy Lefkir , Elias Kammoun , Didier Barret , Peter Boorman , Gabriele Matzeu , Jon M. Miller , Emanuele Nardini , Abderahmen Zoghbi

In 2016 we carried out a Swift monitoring program to track the X-ray hardness variability of eight type-I AGN over a year. The purpose of this monitoring was to find intense obscuration events in AGN, and thereby study them by triggering…

We present an analysis of multi-timescale variability in line-of-sight X-ray absorbing gas as a function of optical classification in a large sample of Seyfert AGN to derive the first X-ray statistical constraints for clumpy-torus models.…

Astrophysics of Galaxies · Physics 2014-02-21 Alex Markowitz , Mirko Krumpe , Robert Nikutta

We present an extraordinary variation of the X-ray spectrum of the obscured AGN in NGC 1365, which was observed by Chandra to change from Compton-thin to Compton-thick and back to Compton-thin in four days. This fast variation imply a a…

Astrophysics · Physics 2007-05-23 G. Risaliti

Photoionized absorbers of outflowing gas are commonly found in the X-ray spectra of active galactic nuclei (AGN). While most of these absorbers are seldom significantly variable, some ionized obscurers have been increasingly found to…

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

We report monitoring of the 0.3-10 keV spectrum of NGC4258 with XMM over 1.5 years.We als o report reprocessing of an overlapping series of archival Chandra observations. By including earlier ASCA and SAX observations, we present a new,…

We present a complete analysis of the hard X-ray (2-10 keV) properties of the Seyfert galaxy NGC 1365, based on a 60 ks XMM-Newton observation performed in January 2004. The two main results are: 1) We detect an obscuring cloud with…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-11 G. Risaliti , G. Miniutti , G. Fabbiano , M. Salvati , A. Baldi , V. Braito , S. Bianchi , G. Matt , J. Reeves , R. Soria , A. Zezas

We present a detailed analysis of the X-ray spectrum of the Seyfert 2 galaxy NGC454E, belonging to the interacting system NGC454. Observations performed with Suzaku, XMM-Newton and Swift allowed us to detect a dramatic change in the…

Cosmology and Nongalactic Astrophysics · Physics 2016-10-26 Elena Marchese , Valentina Braito , Roberto Della Ceca , Alessandro Caccianiga , Paola Severgnini

We present the first results from the ongoing, intensive, multi-wavelength monitoring program of the luminous Seyfert 1 galaxy Mrk 817. While this AGN was, in part, selected for its historically unobscured nature, we discovered that the…

Between July 2012 and February 2013, NuSTAR and XMM-Newton performed four long-look joint obser- vations of the type 1.8 Seyfert, NGC 1365. We have analyzed the variable absorption seen in these observations in order to characterize the…

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