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相关论文: First high energy observations of Narrow Line Seyf…

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Narrow-Line Seyfert 1 galaxies (NLS1s) are generally believed to be radio-quiet Active Galactic Nuclei (AGN) with relatively less-massive (10$^{5}$$-$10$^{8}$~M$_{\odot}$) Super-Massive Black Holes (SMBH). Using the FIRST radio detections…

星系天体物理 · 物理学 2018-07-16 Veeresh Singh , Hum Chand , C. H. Ishwara-Chandra , Preeti Kharb

We present an analysis of 22,656 narrow-line Seyfert 1 galaxies (NLSy1s) from Sloan Digital Sky Survey (SDSS) DR17 ($0.1\leq z\leq 0.9$), identifying a sample of spectroscopically anomalous sources. These anomalies were detected via the…

星系天体物理 · 物理学 2026-01-30 Arihant Tiwari , Rachana , Vivek M , Suvendu Rakshit

$\gamma$-ray-emitting narrow-line Seyfert 1 galaxies ($\gamma$-NLS1) constitute an intriguing small population of Active Galactic Nuclei with $\gamma$-ray emission resembling low power flat-spectrum radio quasars (FSRQ), but with differing…

高能天体物理现象 · 物理学 2023-05-31 Anna Luashvili , Catherine Boisson , Andreas Zech , Maialen Arrieta-Lobo , Daniel Kynoch

We propose two statistical tests to investigate how we see the nuclear region (r < 0.1 pc) of Narrow-Line Seyfert 1 galaxies (NLS1s). 1) The high-ionization nuclear emission-line region (HINER) test: Seyfert 1 galaxies (S1s) have…

天体物理学 · 物理学 2009-10-31 T. Murayama , T. Nagao , Y. Taniguchi

The study of narrow-line Seyfert 1 galaxies (NLS1s) is now mostly limited to low redshift ($z<0.8$) because their definition requires the presence of the H$\beta$ emission line, which is redshifted out of the spectral coverage of major…

星系天体物理 · 物理学 2021-06-04 Suvendu Rakshit , C. S. Stalin , Jari Kotilainen , Jaejin Shin

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…

天体物理学 · 物理学 2009-06-23 Volker Beckmann , Neil Gehrels , Jack Tueller

Recently growing evidence has been accumulated that the NLS1s are viewed from nearly pole-on viewing angles. However, there has been no theoretical model which explains the following important correlations; 1) weaker optical Fe II emitters…

天体物理学 · 物理学 2007-05-23 Yoshiaki Taniguchi , Takashi Murayama , Tohru Nagao

The recent observations of highly accreting supermassive black holes (SMBH) at very high redshift ($>$4) with the James Webb Space Telescope (JWST) allowed us to shed light for the very first time on the early evolutionary phases of active…

星系天体物理 · 物理学 2025-09-05 M. Berton , E. Järvelä , A. Tortosa , C. Mazzucchelli

We present radio spectral analyses for a sample of 29 radio-quiet (RQ) and three radio-loud (RL) narrow-line Seyfert 1 galaxies (NLS1s) detected with the Australia Telescope Compact Array at both 5.5 GHz and 9.0 GHz. The sample is…

We present multi-frequency radio data for a sample of narrow-line Seyfert 1 galaxies. We first focus on the sub-class of gamma-ray emitting narrow-line Seyfert 1 galaxies, studying the long-term radio variability of five sources and…

星系天体物理 · 物理学 2024-12-10 Xi Shao , Philip G. Edwards , Jamie Stevens , Minfeng Gu , Timothy J. Galvin , Minh T. Huynh

It is arguably in the X-ray regime that Narrow-line Seyfert 1 galaxies (NLS1s) exhibit the most extreme behaviour. Spectral complexity, rapid and large amplitude flux variations, and exceptional spectral variability are well known…

高能天体物理现象 · 物理学 2018-07-27 L. C. Gallo

We study the UV spectra of narrow-line Seyfert~1 (NLSy1) galaxies and compare them with ``normal'' AGN. Similar to their optical lines, the NLSy1s show narrower UV lines. They are also characterized by weaker CIV 1549, CIII] 1909, and…

天体物理学 · 物理学 2009-10-31 J. Kuraszkiewicz , B. J. Wilkes , B. Czerny , S. Mathur

We have studied the location of narrow-line Seyfert 1 (NLS1) galaxies and broad-line Seyfert 1 (BLS1) galaxies on the M_BH - sigma relation of non-active galaxies. We find that NLS1 galaxies as a class - as well as the BLS1 galaxies of our…

天体物理学 · 物理学 2009-11-13 S. Komossa , D. Xu

We performed phase-reference very long baseline interferometry (VLBI) observations on five radio-loud narrow-line Seyfert 1 galaxies (NLS1s) at 8.4 GHz with the Japanese VLBI Network (JVN). Each of the five targets (RXS J08066+7248, RXS…

We present results on the hard X-ray emission of NGC 5506, the brightest narrow line Seyfert 1 galaxy above 20 keV. All the recent observations by INTEGRAL, Swift and Suzaku have been analysed and spectral analysis during nine separated…

宇宙学与河外天体物理 · 物理学 2011-05-31 S. Soldi , V. Beckmann , N. Gehrels , S. De Jong , P. Lubinski

We use publicly available XMM-Newton data to systematically compare the hard X-ray photon indices, $\Gamma_{\rm 2-10\ keV}$ and the iron K$\alpha$ emission lines of narrow-line (NL) and broad-line Seyfert 1 (BLS1) galaxies. We compile a…

星系天体物理 · 物理学 2010-11-29 Xin-Lin Zhou , Shuang-Nan Zhang

For 3 radio-loud $\gamma$-ray detected Narrow-Line Seyfert 1 ($\gamma$-ray NLSy1) galaxies, we report optical variability on intra-night and/or week-like time scales, based on five $\geq$ 3 hours long monitoring sessions for each galaxy.…

星系天体物理 · 物理学 2018-12-12 Vineet Ojha , Gopal-Krishna , Hum Chand

This paper discusses the optical spectroscopic properties of the IRAS 1-Jy sample of ultraluminous infrared galaxies (ULIGs). One hundred and eight of the 118 1-Jy ULIGs have been observed at dlambda = 8.3 AA resolution over the wavelength…

天体物理学 · 物理学 2008-11-26 S. Veilleux , D. -C. Kim , D. B. Sanders

1H0323+342 is one of narrow-line radio-loud Seyfert 1 galaxies (RL-NLS1), which is a new class of gamma-ray emitting AGNs. Narrow-line Seyfert 1 galaxies (NLS1) have a small-mass black hole, but its mass accretion rate is almost as high as…

高能天体物理现象 · 物理学 2015-03-12 H. Shirakawa , Y. Fukazawa , Y. Tanaka , R. Itoh , K. Kawaguchi

We present spectra of 6 type 1 Seyfert galaxies, 2 Seyfert 2, a starburst galaxy and a compact narrow line radiogalaxy, taken in two spectral ranges centered around the near--IR CaII triplet (CaT) (at ~8600 Angstroms), and the Mgb stellar…

天体物理学 · 物理学 2009-10-31 L. Jimenez-Benito , A. I. Diaz , R. Terlevich , E. Terlevich