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The Unified Model of AGN predicts the sole difference between Seyfert 1 and Seyfert 2 nuclei is the viewing angle with respect to an obscuring structure around the nucleus. High energy photons above 20 keV are not affected by this…

Astrophysics · Physics 2015-05-13 Matthew Middleton , Chris Done , Nick Schurch

Steep soft X-ray (0.1-2 keV) quasars share several unusual properties: narrow Balmer lines, strong FeII emission, large and fast X-ray variability, rather steep 2-10 keV spectrum. These intriguing objects have been suggested to be the…

Astrophysics · Physics 2009-10-30 F. Fiore , G. Matt , M. Cappi , M. Elvis , K. M. Leighly , F. Nicastro , L. Piro , A. Siemiginowska , B. J. Wilkes

We report the discovery and analysis of the follow-up ROSAT pointed observation, an ASCA observation and optical and radio observations of the enigmatic Narrow-Line Seyfert 1 galaxy RX J0134.2-4258. While its spectrum was one of the softest…

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

Active galactic nuclei (AGN) showing dramatic spectral and flux variations, either due to changes in the accretion rate (changing-state, CS-AGN) of the supermassive black hole or in the line-of-sight column density (changing-obscuration,…

High Energy Astrophysical Phenomena · Physics 2026-05-08 A. Vietri , A. Tortosa , D. Ilić , S. Ciroi , M. Berton , E. Järvelä , C. Ricci , E. Sani , L. Crepaldi , B. Dalla Barba , S. Chen , E. Congiu , P. Condò , I. Varglund , G. Rodighiero

We present XMM observations of the AGN SDSS 1430-0011. The low S/N spectrum of this source obtained in a snap shot Chandra observation showed an unusually flat continuum. With the follow up XMM observations we find that the source spectrum…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 S. Mathur , E. C. Golowacz , R. Williams , R. Pogge , D. Fields , D. Grupe

In the present work we report the BeppoSAX serendipitous discovery of the type 2 AGN 1SAXJ2234.8-2541 in the MECS field of view when pointing at the Seyfert 2 galaxy NGC7314. The source is optical identified with the bright (m_B=14.40)…

Astrophysics · Physics 2007-05-23 A. Malizia , L. Bassani , I. Negueruela

SAX J1819.3-2525 is a nearby X-ray transient which exhibited a fast and large X-ray outburst on Sep. 15, 1999 (Smith et al. 1999). The Wide Field Cameras and the Narrow Field Instruments (NFI) on board BeppoSAX observed SAX J1819.3-2525 at…

As part of the TANAMI multiwavelength progam, we discuss new X-ray observations of the $\gamma$-ray and radio-loud Narrow Line Seyfert galaxy ($\gamma$-NLS1) PKS 2004-447. The active galaxy is a member of a small sample of radio-loud NLS1s…

The radio galaxy Centaurus A was observed by the BeppoSAX satellite five times from 1997 to 2000. From July 6 1999 to August 17 1999, the source was also simultaneously pointed by COMPTEL on-board of the satellite CGRO. Centaurus A has a…

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

The Seyfert 1.9 galaxy MCG-05-23-016 has been shown to exhibit a complex X-ray spectrum. This source has moderate X-ray luminosity, hosts a comparably low-mass black hole, but accretes at a high Eddington rate, and allows us to study a…

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 present results from a BeppoSAX (July 2001) observation of the FRI radio galaxy NGC6251, together with a re-analysis of archival ASCA (October 1994) and Chandra (September 2000) data. The weak detection above 10 keV and the lack of iron…

Astrophysics · Physics 2009-11-10 M. Guainazzi , P. Grandi , A. Comastri , G. Matt

We present the emission line properties of a sample of 76 bright soft X-ray selected ROSAT Active Galactic Nuclei. All optical counterparts are Seyfert 1 galaxies with rather narrow permitted lines, strong optical FeII line blends, and weak…

Astrophysics · Physics 2007-05-23 D. Grupe , K. Beuermann , K. Mannheim , H. -C. Thomas

This paper presents a comprehensive study of the X-ray properties of low-ionization nuclear emission-line regions (LINERs) and low-luminosity Seyfert galaxies based on observations obtained with ASCA. We analyzed data of 53 observations of…

Astrophysics · Physics 2009-11-07 Yuichi Terashima , Naoko Iyomoto , Luis C. Ho , Andrew F. Ptak

The broad band 0.1-200 keV spectra of a sample of 5 Seyfert 2 galaxies (NGC 7172, Mkn 3, NGC 2110, NGC 4507 and NGC 7674) have been measured within the first year of the $BeppoSAX$ Core program. All sources have been detected up to \~ 100…

This paper presents new Chandra and BeppoSAX observations aimed at investigating the optical/X-ray mismatch in the enigmatic class of the Composite galaxies, discovered by a cross-correlation of IRAS and ROSAT all sky survey catalogues.…

We investigate the narrow-line region (NLR) of two radio-quiet QSOs, PG1012+008 and PG1307+085, using high signal-to-noise spatially resolved long-slit spectra obtained with FORS1 at the Very Large Telescope. Although the emission is…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 Semyeong Oh , Jong-Hak Woo , Vardha N. Bennert , Bruno Jungwiert , Martin Haas , Christian Leipski , Marcus Albrecht

We present a deep study of the average hard X-ray spectra of Seyfert galaxies. We analyzed all public INTEGRAL IBIS/ISGRI data available on all the 165 Seyfert galaxies detected at z<0.2. Our final sample consists of 44 Seyfert 1's, 29…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-27 Claudio Ricci , Roland Walter , Thierry J. -L. Courvoisier , Stephane Paltani

We present optical and X-ray spectra of a radio-quiet X-ray selected AGN, RX J1042+1212 ($z$=0.271). The Halpha and Hbeta emission lines are very broad (with full widths at half maximum of ~10000 km s-1) and have double-peaked profiles.…

Astrophysics · Physics 2015-06-24 E. M. Puchnarewicz , K. O. Mason , F. J. Carrera
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