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Related papers: The Phoenix galaxy as seen by NuSTAR

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We present NuSTAR observations of the bright Seyfert 2 galaxy NGC 2110 obtained in 2012, when the source was at the highest flux level ever observed, and in 2013, when the source was at a more typical flux level. We include archival…

In recent years, several Seyfert 2 galaxies have been discovered that change state when observed in X-rays a few years apart, switching from Compton-thin to reflection-dominated or viceversa. We observed a member of this class of…

High Energy Astrophysical Phenomena · Physics 2009-11-13 G. Matt , S. Bianchi , H. Awaki , A. Comastri , M. Guainazzi , K. Iwasawa , E. Jimenez-Bailon , F. Nicastro

We report on a dramatic transition between a Compton-thick, reflection-dominated state and a Compton-thin state in the Seyfert 2 galaxy UGC4203, discovered by comparing a recent (May 2001) XMM-Newton observation with ASCA observations…

Astrophysics · Physics 2009-11-07 M. Guainazzi , G. Matt , F. Fiore , G. C. Perola

We analyse the properties of the X-ray emission from Seyfert 2 NGC 7172 which are based on the 32 ks observational data from NuSTAR in 2014. This source showed a constant Compton-thin obscuration $N_{H}\approx 8\cdot 10^{22} cm^{-2}$, which…

High Energy Astrophysical Phenomena · Physics 2021-05-19 Anatoliy Vasylenko

We present analysis of NuSTAR X-ray observations in the 3-79 keV energy band of the Seyfert 2 galaxy NGC 4388, taken in 2013. The broadband sensitivity of NuSTAR, covering the Fe K$\alpha$ line and Compton reflection hump, enables tight…

High Energy Astrophysical Phenomena · Physics 2017-07-19 N. Kamraj , E. Rivers , F. A. Harrison , M. Brightman , M. Balokovic

We present a NuSTAR and XMM-Newton monitoring campaign in 2014/2015 of the Compton-thick Seyfert 2 galaxy, NGC 1068. During the August 2014 observation, we detect with NuSTAR a flux excess above 20 keV ($32\pm6 \%$) with respect to the…

We present two NuSTAR observations of the local Seyfert 2 active galactic nucleus (AGN) and an ultraluminous X-ray source (ULX) candidate in NGC 5643. Together with archival data from Chandra, XMM-Newton and Swift-BAT, we perform a…

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

Results from BeppoSAX observations of Compton--thick Seyfert 2 galaxies are summarized and reviewed, and their general properties derived and discussed. In five out of the seven observed sources, the nucleus is directly visible at high…

Astrophysics · Physics 2016-08-30 G. Matt , A. C. Fabian , M. Guainazzi , K. Iwasawa , L. Bassani , G. Malaguti

We report on the short and long term X-ray properties of the bright nearby Seyfert 2 galaxy NGC 2992, which was extensively observed with Swift, XMM-Newton and NuSTAR. Swift targeted the source more than 100 times between 2019 and 2021 in…

High Energy Astrophysical Phenomena · Physics 2022-05-25 R. Middei , A. Marinucci , V. Braito , S. Bianchi , B. De Marco , A. Luminari , G. Matt , E. Nardini , M. Perri , J. N. Reeves , F. Vagnetti

We present X-ray spectral analyses for three Seyfert 2 active galactic nuclei, NGC 424, NGC 1320, and IC 2560, observed by NuSTAR in the 3-79 keV band. The high quality hard X-ray spectra allow detailed modeling of the Compton reflection…

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 present the results of the latest NuSTAR monitoring campaign of the Compton-thick Seyfert 2 galaxy NGC 1068, composed of four $\sim$50 ks observations performed between July 2017 and February 2018 to search for flux and spectral…

Astrophysics of Galaxies · Physics 2020-01-17 A. Zaino , S. Bianchi , A. Marinucci , G. Matt , F. E. Bauer , W. N. Brandt , P. Gandhi , M. Guainazzi , K. Iwasawa , S. Puccetti , C. Ricci , D. J. Walton

We present a broad-band (~0.3-70 keV) spectral and temporal analysis of NuSTAR observations of the luminous infrared galaxy NGC 6240, combined with archival Chandra, XMM-Newton and BeppoSAX data. NGC 6240 is a galaxy in a relatively early…

We study the X-ray spectra of a sample of 19 obscured, optically-selected Seyfert galaxies (Sy 1.8, 1.9 and 2) in the local universe ($d \leq 175$~Mpc), drawn from the CfA Seyfert sample. Our analysis is driven by the high sensitivity of…

High Energy Astrophysical Phenomena · Physics 2020-10-14 E. S. Kammoun , J. M. Miller , M. Koss , K. Oh , A. Zoghbi , R. F. Mushotzky , D. Barret , E. Behar , W. N. Brandt , L. W. Brenneman , J. S. Kaastra , A. M. Lohfink , D. Proga , D. Stern

A 100ks XMM-Newton observation of the nearby Seyfert 2 galaxy Mrk 3 offers a unique opportunity to explore the complexity of its X-ray spectrum. We find the \~3-8 keV continuum to be dominated by reflection from cold matter, with…

Astrophysics · Physics 2007-05-23 K. A. Pounds , K. L. Page

We present the results from a long term X-ray analysis of Mrk 279 during the period 2018-2020. We use data from multiple missions - AstroSat, NuSTAR and XMM-Newton, for the purpose. The X-ray spectrum can be modelled as a double…

High Energy Astrophysical Phenomena · Physics 2024-05-15 K. Akhila , Ranjeev Misra , Savithri H. Ezhikode , K. Jeena

We present results from a ~55 ks long XMM-Newton observation of the obscured AGN, NGC 5643, performed in July 2009. A previous, shorter (about 10 ks) XMM-Newton observation in February 2003 had left two major issues open, the nature of the…

High Energy Astrophysical Phenomena · Physics 2015-06-16 G. Matt , S. Bianchi , A. Marinucci , M. Guainazzi , K. Iwawasa , E. Jimenez Bailon

We present the results of a joint {\it XMM-Newton} and {\it NuSTAR} campaign on the active galactic nucleus (AGN) IC 4329A, consisting of 9 $\times$ 20 ks {\it XMM-Newton} observations, and 5 $\times$ 20 ks {\it NuSTAR} observations within…

We test the two-corona accretion scenario for active galactic nuclei in the case of the `bare' Seyfert 1 galaxy HE 1143-1810. We perform a detailed study of the broad-band UV--X-ray spectral properties and of the short-term variability. We…

High Energy Astrophysical Phenomena · Physics 2020-02-12 F. Ursini , P. -O. Petrucci , S. Bianchi , G. Matt , R. Middei , G. Marcel , J. Ferreira , M. Cappi , B. De Marco , A. De Rosa , J. Malzac , A. Marinucci , G. Ponti , A. Tortosa
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