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相关论文: Magellan Spectroscopy of Low-Redshift Active Galac…

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We queried the Spitzer archive for high-resolution observations with the Infrared Spectrograph of optically selected active galactic nuclei (AGN) for the purpose of identifying sources with resolved fine-structure lines that would enable…

宇宙学与河外天体物理 · 物理学 2011-10-21 K. M. Dasyra , L. C. Ho , H. Netzer , F. Combes , B. Trakhtenbrot , E. Sturm , L. Armus , D. Elbaz

We study the large-scale spatial distribution of low-redshift quasars and Seyfert~1 galaxies using a sample of 106 luminous emission-line objects ($\bar{M}_{B} \approx -23$) selected by their H$\alpha$ emission lines in a far-red objective…

Several studies indicate that radio-loud (RL) Active Galactic Nuclei (AGN) are produced only by the most massive black holes (BH), $M_{\rm BH} \sim 10^8$-$10^{10} M_\odot$. This idea has been challenged by the discovery of RL Narrow Line…

星系天体物理 · 物理学 2016-03-09 Ranieri D. Baldi , Alessandro Capetti , Andrew Robinson , Ari Laor , Ehud Behar

We present XMM-Newton observations of four low-redshift Seyfert galaxies selected to have low host luminosities (M_g>-20 mag) and small stellar velocity dispersions (sigma_star<45 km/s), which are among the smallest stellar velocity…

宇宙学与河外天体物理 · 物理学 2014-11-20 C. E. Thornton , A. J. Barth , L. C. Ho , J. E. Greene

The cosmological evolution of X-ray-selected and optically selected Active Galactic Nuclei (AGNs) show different behaviours interpreted in terms of two different populations. The difference is evident mainly for low luminosity AGNs…

天体物理学 · 物理学 2009-11-13 D. Trevese , V. Zitelli , F. Vagnetti , K. Boutsia , G. M. Stirpe

We analyze Hubble Space Telescope (HST) optical imaging of eight low-mass galaxies hosting active galactic nuclei (AGN) identified via their photometric variability in \cite{baldassare_search_2020}. We use GALFIT to model the 2D galaxy…

星系天体物理 · 物理学 2025-02-06 Erin Kimbro , Vivienne Baldassare , Guy Worthey , Marla Geha , Jenny Greene

We quadruple the number of quasars known behind the Large Magellanic Cloud (LMC) from 55 (42 in the LMC fields of the third phase of the Optical Gravitational Lensing Experiment (OGLE)) to 200 by spectroscopically confirming 169 (144 new)…

We analyze an X-ray flux-limited, complete sample of 93 AGN at z< 0.1, selected from the ROSAT Bright Survey. Two thirds of the sample are Seyfert 1 galaxies (Sy1) and one third are Narrow-Line Seyfert 1 galaxies (NLSy1). We have obtained…

天体物理学 · 物理学 2009-11-10 M. Salvato , J. Greiner , B. Kuhlbrodt

We report the results of a pilot study that searched for dual active galactic nuclei (AGN) in local ($z<$0.25) galaxies hosting double-peaked narrow emission lines in their optical spectra. We present high-resolution $L-$band (1.5 GHz or 18…

Narrow-line Seyfert 1 galaxies (NLS1s) are a subclass of active galactic nuclei (AGN). It is often believed that these AGN have small black hole mass, which is responsible for the narrowness of the permitted lines. They are also…

星系天体物理 · 物理学 2018-09-27 A. Vietri , M. Berton , S. Ciroi , E. Congiu , G. La Mura , V. Cracco , M. Frezzato , S. Chen , A. Cattapan , T. Peruzzi , P. Rafanelli

We present an updated and revised analysis of the relationship between the Hbeta broad-line region (BLR) radius and the luminosity of the active galactic nucleus (AGN). Specifically, we have carried out two-dimensional surface brightness…

We present a measure of the hard (2-8 keV) X-ray luminosity function (XLF) of Active Galactic Nuclei up to z~5. At high redshifts, the wide area coverage of the Chandra Multiwavength Project is crucial to detect rare and luminous (Lx >…

Near infrared spectra with resolution R ~ 1100 in the rest wavelength range 1.8-2.2 microns have been obtained for a complete sample of 33 ultraluminous infrared galaxies. Of the 33 objects observed, 2 show evidence of a central AGN through…

天体物理学 · 物理学 2012-08-27 T. W. Murphy, , B. T. Soifer , K. Matthews , J. R. Kiger , L. Armus

We have conducted a new Arecibo survey for H I emission for 113 galaxies with broad-line (type 1) active galactic nuclei (AGNs) out to recession velocities as high as 35,000 km/s. The primary aim of the study is to obtain sensitive H I…

天体物理学 · 物理学 2009-11-13 Luis C. Ho , Jeremy Darling , Jenny E. Greene

With the aim of studying the influence of environment on the nuclear activity of galaxies, we have selected a well defined sample of 65 Compact Groups of galaxies with concordant redshift in the Hickson Catalog. In this proceeding, we…

天体物理学 · 物理学 2015-06-24 M. A. Martinez , A. del Olmo , J. Perea , R. Coziol

We present a high-quality, homogeneous sample of 157 H$\beta$ reverberation-mapped active galactic nuclei (RM AGNs) spanning redshifts $0.00308 \leq z \leq 0.8429$, which is approximately 3.8 times larger than the previously available…

星系天体物理 · 物理学 2025-07-30 Shulei Cao , Amit Kumar Mandal , Michal Zajaček , Bharat Ratra

We have started automatized photometric monitoring of active galactic nuclei using the 46 cm telescope of the Wise Observatory in Israel. The telescope is specially equipped with narrow-band filters to perform high-fidelity photometric…

星系天体物理 · 物理学 2018-07-10 F. Pozo Nuñez , D. Chelouche , S. Kaspi

In this paper, we present new determinations of redshifts on a sample of gravitational arclets identified in the cluster of galaxies Abell 2390. The arclets candidates were selected from their elongated morphology as seen in recent deep HST…

天体物理学 · 物理学 2007-05-23 J. Bezecourt , G. Soucail

From a parent catalog of 561 changing-look active galactic nuclei (CL-AGNs) identified by Guo et al. (2025), we investigate the evolutionary sequence of broad emission lines using a redshift-selected subset (0.35 < z < 0.45) of 54 CL-AGNs…