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相关论文: X-ray spectral complexity in narrow-line Seyfert 1…

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(abridged) With the commissioning of XMM came the discovery of 2.5-10 keV spectral complexity in some narrow-line Seyfert 1 galaxies (NLS1). In this work, we define two samples of NLS1: a complex sample whose members exhibit high-energy…

天体物理学 · 物理学 2009-11-11 L. C. Gallo

The soft (\approx 0.1--2.0 keV) X-ray spectra of narrow-line Seyfert 1 galaxies are known to be generally steeper than those of Seyfert 1 galaxies with broader optical permitted lines. This has been attributed to the presence of strong soft…

天体物理学 · 物理学 2016-01-13 W. N. Brandt , S. Mathur , M. Elvis

We have used the ROSAT Bright Source Catalogue to extract a complete sample of sources selected in the band from 0.1-0.4 keV. This 1/4 keV-selected sample is comprised of 54 Seyfert galaxies, 25 BL Lacertae objects, 4 clusters and 27…

天体物理学 · 物理学 2008-11-26 S. Vaughan , R. Edelson , R. S. Warwick , M. A. Malkan , M. R. Goad

We report on AGN with extremely soft X-ray spectra observed with ROSAT. From their optical emission lines these objects are classified as narrow-line Seyfert 1 galaxies (NLS1), almost all with extremely large Fe II/H-beta ratios and…

天体物理学 · 物理学 2007-05-23 Th. Boller , W. N. Brandt , H. Fink

We present results from an analysis of the broad-band, 0.3-195 keV, X-ray spectra of 48 Seyfert 1-1.5 sources detected in the very hard X-rays with the Swift Burst Alert Telescope (BAT). This sample is selected in an all-sky survey…

高能天体物理现象 · 物理学 2015-06-03 Lisa M. Winter , Sylvain Veilleux , Barry McKernan , Tim Kallman

We present the first in a series of papers describing the X-ray properties of a sample of 18 Seyfert 1 galaxies, using data obtained by \asca. The imaging data reveal a number of serendipitous hard X-ray sources in some source fields, but…

天体物理学 · 物理学 2008-11-26 K. Nandra , I. M. George , R. F. Mushotzky , T. J. Turner , T. Yaqoob

A sample of narrow-line (NLS1) and broad-line Seyfert 1 (BLS1) galaxies observed with Suzaku is presented. The final sample consists of 22 NLS1s and 47 BLS1s, for a total of 69 AGN that are all at low redshift (z<0.5) and exhibit low host…

高能天体物理现象 · 物理学 2020-10-07 Sophia G. H. Waddell , Luigi C. Gallo

The study of NLS1s using ASCA has many advantages. A representative sample can be studied; to date, observations of more than 30 NLS1s have been made. ASCA observations are conducted contiguously, so their X-ray variability properties can…

天体物理学 · 物理学 2009-10-31 Karen M. Leighly

The excellent soft X-ray sensitivity of the PSPC detector onboard the ROSAT satellite provided the first chance to study precisely the spectral and timing properties of Narrow-Line Seyfert 1 galaxies. ROSAT observations of Narrow-Line…

天体物理学 · 物理学 2009-10-31 Th. Boller

Narrow-line Seyfert\,1 galaxies (NLS1s) with very small broad-line widths (say, FWHM(\hb) $\la $ 1200\,\kms) represent the extreme type of Seyfert\,1 galaxies that have small black hole masses (\mbh) and/or high Eddington ratios (\redd).…

高能天体物理现象 · 物理学 2015-05-20 Y. L. Ai , W. Yuan , H. Y. Zhou , T. G. Wang , S. H. Zhang

This paper presents a quantification of the X-ray variability amplitude for 79 ASCA observations of 36 Seyfert 1 galaxies. We find that consideration of sources with the narrowest permitted lines in the optical band introduces scatter into…

天体物理学 · 物理学 2009-10-31 T. J. Turner , I. M. George , K. Nandra , D. Turcan

An analysis was made of 0.3-15 keV X-ray spectra of a Narrow-Line Seyfert 1 Galaxy, Ton S180, using archival data from ASCA, RXTE, and XMM-Newton. At energies above 2.5 keV, a power-law with a photon index of ~ 2.3 successfully and…

天体物理学 · 物理学 2015-06-24 Mio Murashima , Aya Kubota , Kazuo Makishima , Motohide Kokubun , Soojing Hong , Hitoshi Negoro

We present the optical spectra and simple statistical analysis for a complete sample of 110 soft X-ray selected AGN. About half of the sources are Narrow-Line Seyfert 1 galaxies (NLS1s), which have the steepest X-ray spectra, strongest FeII…

天体物理学 · 物理学 2016-08-30 D. Grupe , B. J. Wills , K. M. Leighly , H. Meusinger

We present the results of a detailed multi-wavelength study of a sample of sixteen narrow-line Seyfert 1 (NLSy1) galaxies known in $\gamma$-rays so far. This includes a focused X-ray spectral analysis, to compare them with a more general…

高能天体物理现象 · 物理学 2019-02-27 Vaidehi S. Paliya , M. L. Parker , J. Jiang , A. C. Fabian , L. Brenneman , M. Ajello , D. Hartmann

We present an analysis of spectrum and variability of the bright reddened narrow line Seyfert 1 galaxy Was~61 using 90 ks archival {\it XMM-Newton} data. The X-ray spectrum in 0.2-10 keV can be characterized by an absorbed power-law plus…

高能天体物理现象 · 物理学 2016-03-11 Liming Dou , Ting-Gui Wang , Yanli Ai , Weimin Yuan , Hongyan Zhou , Xiao-Bo Dong

We present an analysis of six 12 um selected Seyfert 2 galaxies that have been reported to be unabsorbed in the X-ray. By comparing the luminosities of these galaxies in the mid-IR (12um), optical ([O III]) and hard X-ray (2-10 keV), we…

天体物理学 · 物理学 2009-11-13 Murray Brightman , Kirpal Nandra

We present results from spectral analysis of ASCA data on the NLS1 Mrk 507. This galaxy was found to have an exceptionally flat ROSAT spectrum among the NLS1s. The ASCA spectrum however shows a clear absorption feature in the energy band…

天体物理学 · 物理学 2009-10-30 K. Iwasawa , W. N. Brandt , A. C. Fabian

In order to understand how the soft X-ray spectra vary we present the Hardness Ratio 1 versus Count Rates (HR1-CTs) correlation of 8 Narrow-line Seyfert 1 Galaxies (NLS1s) and 14 Broad-line Seyfert1 Galaxies (BLS1s) obtained during the…

天体物理学 · 物理学 2017-11-01 Linpeng Cheng , Jianyan Wei , Yongheng Zhao

We present a catalogue of ROSAT detected sources in the sample of spectroscopically selected Seyfert 1 and Seyfert 2 galaxies of Rafanelli et al. (1995). The catalogue contains 102 Seyfert 1 and 36 Seyfert 2 galaxies. The identification is…

天体物理学 · 物理学 2009-11-06 F. Pfefferkorn , Th. Boller , P. Rafanelli

Narrow Line Seyfert 1 galaxies represent a distinct category in the larger family of Type 1 Active Galactic Nuclei. The occurrence of emission line profiles not broader than 2000 km/s, combined with luminosity estimates comparable to those…

高能天体物理现象 · 物理学 2011-06-14 G. La Mura , S. Ciroi , V. Cracco , D. Ilić , L. Č. Popović , P. Rafanelli
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