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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

High resolution X-ray spectroscopy of the warm absorber in the nearby X-ray bright Seyfert 1 galaxy, Mrk 1040 is presented. The observations were carried out in the 2013-2014 timeframe using the Chandra High Energy Transmission Grating with…

High Energy Astrophysical Phenomena · Physics 2017-03-08 James Reeves , Valentina Braito , Ehud Behar , Travis Fischer , Steve Kraemer , Andrew Lobban , Emanuele Nardini , Delphine Porquet , Jane Turner

We have studied the correlation among X-ray absorption, optical reddening and nuclear dust morphology in Seyfert 2 galaxies. Two main conclusions emerge: a) the Balmer decrement and the amount of X-ray absorption are anticorrelated on a…

Astrophysics · Physics 2009-11-06 M. Guainazzi , F. Fiore , G. Matt , G. C. Perola

We present a comprehensive analysis of the timing and spectral properties of NGC 7314, a Seyfert 1.9 galaxy, using X-ray observations from {\it XMM-Newton}, {\it NuSTAR}, and {\it RXTE}/PCA. The timing analysis reveals significant…

High Energy Astrophysical Phenomena · Physics 2024-10-03 Debjit Chatterjee , Arghajit Jana , A. Mangalam , Hsiang-Kuang Chang

We have made BeppoSAX observations of the Seyfert 2/1.9 galaxy ESO103-G35, which contains a nuclear maser source and is known to be heavily absorbed in the X-rays. Analysis of the X-ray spectra observed by SAX in October 1996 and 1997…

We analyze the \textit{Chandra} High Energy Transmission Grating Spectrometer (HETGS) observation of the Seyfert $2$ AGN IRAS\,18325-5926. We detect a $v=-360^{+41}_{-66}$~km~s$^{-1}$ blueshifted ionized absorber in the X-ray spectrum, with…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Philip Mocz , Julia C. Lee , Kazushi Iwasawa , Claude R. Canizares

A Suzaku observation of the nucleus of the radio-loud AGN Centaurus A in 2005 has yielded a broadband spectrum spanning 0.3 to 250 keV. The net exposure times after screening were: 70 ks per X-ray Imaging Spectrometer (XIS) camera, 60.8 ks…

Mkn 3 is a Seyfert 2 galaxy that is widely regarded as an exemplary Compton-thick AGN. We study the Suzaku X-ray spectrum using models of the X-ray reprocessor that self-consistently account for the Fe K$\alpha$ fluorescent emission line…

High Energy Astrophysical Phenomena · Physics 2015-10-07 T. Yaqoob , M. M. Tatum , A. Scholtes , A. Gottlieb , T. J. Turner

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

We analyze the high-resolution X-ray spectrum of the Seyfert 1 galaxy NGC 5548, for the full 0.1-10 keV band, using improved calibration results of the Chandra-LETGS instrument. The warm absorber consists of at least three ionization…

We present Chandra ACIS-S observations of the enigmatic Seyfert-2 galaxy NGC4698. This object together with several other bona-fide Seyfert-2 galaxies show no absorption in the low spatial resolution ASCA data, in contrast to the standard…

Astrophysics · Physics 2016-08-30 I. Georgantopoulos , A. Zezas

Active galaxies are thought to be both fueled and obscured by neutral gas removed from the host galaxy and funneled into a central accretion disk. We performed a VLA imaging survey of 21 cm absorption in Seyfert and starburst nuclei to…

Astrophysics · Physics 2009-10-31 J. F. Gallimore , S. A. Baum , C. P. O'Dea , A. Pedlar , E. Brinks

We present an XMM-Newton observation of NGC 7469, including studies of the X-ray and UV variability, 0.2-10 keV spectral continuum, Fe K-alpha emission line and the first-ever high-resolution X-ray spectrum of the soft X-ray warm absorber.…

The absorption lines in the soft X-ray spectrum of MCG--6-30-15 are studied using the Reflection Grating Spectrometer data from the 2001 XMM-Newton 320 ks observation. A line search of the full time-averaged spectrum reveals 51 absorption…

Astrophysics · Physics 2009-09-17 A. K. Turner , A. C. Fabian , J. C. Lee , S. Vaughan

We report conclusive verification of the detection of associated HI 21 cm absorption in the early-type host galaxy of the compact radio source PMNJ2054-4242. We estimate an effective spectral line velocity width of 418 +/- 20 km s^{-1} and…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-12 J. R. Allison , S. J. Curran , E. M. Sadler , S. N. Reeves

We report results from the XMM-Newton observation of IRAS 13197-1627, a luminous IR galaxy with a Seyfert 1.8 nucleus. The hard X-ray spectrum is steep and is absorbed by Compton-thin neutral gas. We detect an Fe emission line at 6.4 keV,…

Astrophysics · Physics 2008-11-26 G. Miniutti , G. Ponti , M. Dadina , M. Cappi , G. Malaguti

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…

We present the analysis of three XMM observations of the Seyfert 2 galaxy NGC 7590. The source was found to have no X-ray absorption in the low spatial resolution ASCA data. The XMM observations provide a factor of 10 better spatial…

High Energy Astrophysical Phenomena · Physics 2010-09-21 X. W. Shu , T. Liu , J. X. Wang

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 a detailed analysis of a long, 100 ksec, observation of NGC 4151 by ASCA, contemporaneous with an observation by the CGRO/OSSE. We fit the data with physical models including an Fe K line and Compton reflection both…