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Related papers: The elusive radio loud Seyfert 2 galaxy NGC 2110

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We present spectral analysis of two Suzaku observations of the Seyfert 2 galaxy, NGC 2110. This source has been known to show complex, variable absorption which we study in depth by analyzing these two observations set seven years apart and…

We present the results from an XMM-Newton observation (January 24, 2001) of the bright Seyfert 1 galaxy ESO 198-G24 (z=0.045). We found that this Seyfert has an intrinsic 2-10 keV luminosity of about 10^44 erg s-1. This source shows no…

Astrophysics · Physics 2009-11-07 D. Porquet , J. S. Kaastra , K. L. Page , P. T. O'Brien , M. J. Ward , J. Dubau

We report on our analysis of XMM-Newton observations of the Seyfert 2 galaxy ESO 138-G1 (z = 0.0091). These data reveal a complex spectrum in both its soft and hard portions. The 0.5-2 keV band is characterized by a strong 'soft-excess'…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 E. Piconcelli , S. Bianchi , C. Vignali , E. Jimenez-Bailon , F. Fiore

I present ASCA observations of IRAS00317-2142, the most luminous (Lx~10^43 erg s-1 0.1-2 keV) of the 'composite' class of galaxies. This enigmatic class of objects presents narrow-emission line optical spectra classifying these galaxies as…

Astrophysics · Physics 2009-10-31 I. Georgantopoulos

The Seyfert 2 galaxy NGC 7674 has been observed within the BeppoSAX Core Programme with the onboard narrow field instruments between 0.1 and 100 keV. The broad-band spectrum shows four most relevant spectral components: a) a soft excess…

We present a combined, non-simultaneous, ASCA GIS and CGRO OSSE spectrum of the Seyfert 2 galaxy, NGC 7172, and make broad band spectral fits. The only Seyfert 2 galaxy previously studied over such a broad band is NGC 4945. We find that the…

Astrophysics · Physics 2016-08-30 Felix Ryde , Juri Poutanen , Roland Svensson , Stefan Larsson , Shiro Ueno

We present results on the Seyfert 2 galaxy NGC4388 in the Virgo cluster observed with ASCA during its PV phase. The 0.5-10 keV X-ray spectrum consists of multiple components; (1) a continuum component heavily absorbed by a column density NH…

Astrophysics · Physics 2015-06-24 K. Iwasawa , A. C. Fabian , S. Ueno , H. Awaki , Y. Fukazawa , K. Matsushita , K. Makishima

We present the results of an ASCA observation of the radio-loud NLS1 galaxy RGB J0044+193. The X-ray data are complemented by radio observations and a new optical spectrum for this source. We find evidence for variable radio emission and an…

We report the results of 20, 6, and 2 cm VLA and 1.5 cm OVRO observations of the optically-selected CfA Seyfert galaxies and the bolometric-flux-limited 12-Micron active galaxy sample. Every object observed was detected at 6 cm. Only 6-8%…

Astrophysics · Physics 2009-10-28 Brian Rush , Matthew A. Malkan , Richard A. Edelson

We present long-term (months-years) X-ray spectral variability of the Seyfert 1.8 galaxy NGC 1365 as observed by Swift, which provides well sampled observations over a much longer timescale (6 years) and a much larger flux range than is…

High Energy Astrophysical Phenomena · Physics 2014-04-21 S. D. Connolly , I. M. McHardy , T. Dwelly

The Seyfert 2 galaxies NGC 2992 and NGC 3081 have been observed by INTEGRAL and Swift. We report about the results and the comparison of the spectrum above 10 keV based on INTEGRAL IBIS/ISGRI, Swift/BAT, and BeppoSAX/PDS. A spectrum can be…

Astrophysics · Physics 2009-06-23 Volker Beckmann , Neil Gehrels , Jack Tueller

We present results of the ASCA observation of the Seyfert 2 galaxy NGC 4507. The 0.5-10 keV spectrum is rather complex and consists of several components: (1) a hard X-ray power law heavily absorbed by a column density of about 3 10^23…

Astrophysics · Physics 2009-10-30 A. Comastri , C. Vignali , M. Cappi , G. Matt , R. Audano , H. Awaki , S. Ueno

We present results from new Chandra and archival HST and VLA imaging observations of the circumnuclear extended emission in the nearby Type 2 Seyfert galaxy NGC 2110. We find resolved soft-band X-ray emission 4'' (~160 pc) north of the…

We present an XMM-Newton observation of the Seyfert-LINER galaxy NGC 7213. The RGS soft X-ray spectrum is well fitted with a power law plus soft X-ray collisionally ionised thermal plasma (kT = 0.18 +0.03/-0.01 keV). We confirm the presence…

Astrophysics · Physics 2009-11-10 R. L. C. Starling , M. J. Page , G. Branduardi-Raymont , A. A. Breeveld , R. Soria , K. Wu

We present an analysis of the time-averaged spectrum of the Seyfert-2 active galaxy NGC 4388, obtained by NICER. The intrinsic strength of the reflection spectrum in NGC 4388, the large collecting area and favorable pass band of NICER, and…

High Energy Astrophysical Phenomena · Physics 2019-11-06 J. M. Miller , E. Kammoun , R. M. Ludlam , K. Gendreau , Z. Arzoumanian , E. Cackett , F. Tombesi

The latest observations of line and continuum spectra emitted from the extended narrow line region (ENLR) of the Seyfert 2 galaxy NGC 7212 are analysed using models accounting for photoionization from the active nucleus and shocks. The…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 M. Contini , V. Cracco , S. Ciroi , G. La Mura

A fraction of Narrow Line Seyfert 1 galaxies (NLS1) are hosted by galaxies that present a disturbed morphology, in some cases hinting for merger processes, that are putative sources of gas replenishment. We have been investigating the…

Astrophysics of Galaxies · Physics 2018-09-06 Sonia Anton , Alessandro Caccianiga , Luca Bizzocchi , Jose Afonso

We present the first INTEGRAL observations of the type 1.5 Seyfert galaxy NGC 4151. Combining several INTEGRAL observations performed during 2003, totaling about 400 ks of exposure time, allows us to study the spectrum in the 2 - 300 keV…

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…

The 0.5-150 keV broad-band spectra of a sample of nine bright type 1 Seyfert galaxies are analyzed here. These sources have been discovered/detected by INTEGRAL and subsequently observed with XMM--Newton for the first time with high…