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Related papers: Indecent Exposure in Seyfert 2 Galaxies: A Close L…

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We report on simultaneous optical and X-ray observations of the Seyfert galaxy, NGC3147. The XMM-Newton spectrum shows that the source is unabsorbed in the X-rays ($N_H<5\times10^{20}$ cm$^{-2}$). On the other hand, no broad lines are…

Astrophysics · Physics 2009-11-13 S. Bianchi , A. Corral , F. Panessa , X. Barcons , G. Matt , L. Bassani , F. J. Carrera , E. Jimenez-Bailon

The Swift Burst Alert Telescope (BAT) survey of Active Galactic Nuclei (AGN) is providing an unprecedented view of local AGNs (<z> = 0.03) and their host galaxy properties. In this paper, we present an analysis of the optical spectra of a…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Lisa M. Winter , Karen T. Lewis , Michael Koss , Sylvain Veilleux , Brian Keeney , Richard F. Mushotzky

We investigate the properties of the two-dimensional distribution and kinematics of ionised gas and stars in the central kiloparsecs of a matched sample of nearby active (Seyfert) and inactive galaxies, using the SAURON Integral Field Unit…

Astrophysics · Physics 2009-09-29 Gaelle Dumas , Carole Mundell , Eric Emsellem , Neil Nagar

We present the results of our identification of eight objects from a preliminary catalogue of X-ray sources detected in the 4-12 keV energy band by the Mikhail Pavlinsky ART-XC telescope aboard the SRG observatory during its first all-sky…

A complete flat-spectrum radio-loud sample of AGN includes a significant fraction of Seyfert-like AGN including a NLS1. Analysis of their optical spectra suggests that the reddest continuum colours are either associated with AGN in nearby…

Motivated by theoretical expectations that Nuclear Star Clusters (NSCs) in galactic centers may provide a favorable environment for super-massive black holes to form and/or efficiently grow, we set out to measure the fraction of nearby…

High Energy Astrophysical Phenomena · Physics 2017-05-31 Adi Foord , Elena Gallo , Edmund Hodges-Kluck , Brendan P. Miller , Vivienne F. Baldassare , Kayhan Gultekin , Oleg Y. Gnedin

We observed 37 AGN candidates and classified them on the basis of their spectroscopic properties; three are confirmed QSOs, one is a BL Lac object, nine are Seyfert 1 galaxies, four Seyfert 2s, while twenty are HII regions.

Astrophysics · Physics 2009-10-30 A. C. Goncalves , P. Veron , M. -P. Veron-Cetty

We present spectropolarimetric and spectrophotometric observations of the peculiar active galactic nucleus (AGN) SDSS J120300.19+162443.7 (hereafter J1203+1624) at $z=0.1656$. Its optical total flux spectra clearly show broad emission lines…

The discovery in 2008 of high-energy gamma-rays from Narrow-Line Seyfert 1 Galaxies (NLS1s) made it clear that there were active galactic nuclei (AGN) other than blazars and radio galaxies that can eject powerful relativistic jets. In…

High Energy Astrophysical Phenomena · Physics 2020-09-01 Luigi Foschini

We present new HST NICMOS observations of NGC 4945, a starburst galaxy hosting a highly obscured active nucleus that is one of the brightest extragalactic sources at 100 keV. The HST data are complemented with ground based [FeII] line and…

We present new mid-infrared (N-band) images of a sample of eight nearby Seyfert galaxies. In all of our targets, we detect a central unresolved source, which in some cases has been identified for the first time. In particular, we have…

Astrophysics · Physics 2009-10-31 Alfred Krabbe , Torsten Boeker , R. Maiolino

We present a large sample which contains 45 Seyfert 1 galaxies (Sy1s), 46 hidden broad-line region (HBLR) Seyfert 2 galaxies (Sy2s), 57 non-HBLR Sy2s, and 22 starburst galaxies to distinguish their properties and to seek the possible…

High Energy Astrophysical Phenomena · Physics 2015-05-28 Yu-Zhong Wu , Yong-Heng Zhao , Xian-Min Meng

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

NGC 4945 harbors one of the nearest active galactic nuclei (AGN), which allows reaching high spatial resolution with the current observational facilities. The Seyfert 2 nucleus is deeply obscured by an edge-on disk with $A_V\sim14$,…

We present Spitzer high-resolution spectra of off-nuclear regions in the central cluster galaxies NGC 1275 and NGC 4696 in the Perseus and Centaurus clusters, respectively. Both objects are surrounded by extensive optical emission-line…

Astrophysics · Physics 2009-11-13 R. Johnstone , N. Hatch , G. Ferland , A. Fabian , C. Crawford , R. Wilman

We are conducting a search for supermassive black holes (SMBHs) with masses below 10^7 M_sun by looking for signs of extremely low-level nuclear activity in nearby galaxies that are not known to be AGNs. Our survey has the following…

Astrophysics · Physics 2009-11-13 Himel Ghosh , Smita Mathur , Fabrizio Fiore , Laura Ferrarese

In this paper we present INTEGRAL observations of 7 AGNs: two newly discovered type 1 Seyferts, IGR J18027-1455 and IGR J21247+5058, and five well known Seyferts, NGC 6814 (type 1.5), Cyg A (Type 2), MCG-05-23-16 (type 2), ESO 103-G035…

We introduce the Keck Osiris Nearby AGN survey (KONA), a new adaptive optics-assisted integral-field spectroscopic survey of Seyfert galaxies. KONA permits at ~0.1" resolution a detailed study of the nuclear kinematic structure of gas and…

Astrophysics of Galaxies · Physics 2018-05-04 F. Müller-Sánchez , E. K. S. Hicks , M. Malkan , R. Davies , P. C. Yu , S. Shaver , B. Davis

The Fermi/LAT collaboration recently reported the detection of starburt galaxies in the high energy gamma-ray domain, as well as radio-loud narrow-line Seyfert 1 objects, which were previously unusual extragalactic suspects for high energy…

High Energy Astrophysical Phenomena · Physics 2011-02-28 Jean-Philippe Lenain , Claudio Ricci , Marc Türler , Daniela Dorner , Roland Walter

We present XMM-Newton observations of three AGN taken as part of a hunt to find very heavily obscured Compton-thick AGN. For obscuring columns greater than 10^25 cm^-2, AGN are only visible at energies below 10 keV via reflected/scattered…

High Energy Astrophysical Phenomena · Physics 2015-05-28 M. L. Trippe , C. S. Reynolds , M. Koss , R. F. Mushotzky , L. M. Winter