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Related papers: Active Galactic Nuclei with Candidate Intermediate…

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We present deep Near-infrared (NIR) images of a sample of 19 intermediate-redshift ($0.3<z<1.0$) radio-loud active galactic nuclei (AGN) with powerful relativistic jets ($L_{1.4GHz} >10^{27}$ WHz$^{-1}$), previously classified as…

We present an atlas of moderate-resolution (R ~ 1200-1600) optical spectra of 94 low-redshift (z < 0.5) active galactic nuclei taken with the Magellan 6.5 m Clay Telescope. The spectra mostly cover the rest-frame region 3600-6000 Ang. All…

Astrophysics of Galaxies · Physics 2014-11-20 Luis C. Ho , Minjin Kim

Observational searches for intermediate-mass black holes (IMBHs; $10^2 - 10^6$ $M_\odot$) include relatively isolated dwarf galaxies. For those that host active galactic nuclei (AGNs), the IMBH nature may be discerned through the accretion…

Astrophysics of Galaxies · Physics 2022-12-21 Xiaolong Yang , Prashanth Mohan , Jun Yang , Luis C. Ho , J. N. H. S. Aditya , Shaohua Zhang , Sumit Jaiswal , Xiaofeng Yang

We present a sample of 252 broad-line Active Galactic Nuclei (BLAGNs), incorporating 171 newly identified sources, spanning a redshift interval from $z$ = 0.8 to 7.2. We have analyzed spectroscopic data from the NIRSpec instrument aboard…

Astrophysics of Galaxies · Physics 2025-12-04 Caroline Baccus , Xinfeng Xu

We present new multi-wavelength observations of the dwarf Seyfert 1 galaxy POX 52 in order to investigate the properties of the host galaxy and the active nucleus, and to examine the mass of its black hole, previously estimated to be ~ 10^5…

Astrophysics · Physics 2009-11-13 C. E. Thornton , A. J. Barth , L. C. Ho , R. E. Rutledge , J. E. Greene

We present new Gemini-North/NIRI and VLT/SINFONI H-band spectroscopy for a flux limited sample of 40 z~4.8 active galactic nuclei, selected from the Sloan Digital Sky Survey. The sample probably contains the most massive active black holes…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 Benny Trakhtenbrot , Hagai Netzer , Paulina Lira , Ohad Shemmer

We analyse star formation in the nuclei of 9 Seyfert galaxies at spatial resolutions down to 0.085arcsec, corresponding to length scales of less than 10pc in some objects. Our data were taken mostly with the near infrared adaptive optics…

Astrophysics · Physics 2009-11-13 R. Davies , F. Mueller Sanchez , R. Genzel , L. Tacconi , E. Hicks , S. Friedrich , A. Sternberg

In this work, we test the hypothesis that narrow-line Seyfert 1 galaxies (NSL1s) are active galactic nuclei in their early phase and are therefore younger and more active than the more common broad-line Seyfert 1 galaxies (BLS1s). If that…

High Energy Astrophysical Phenomena · Physics 2018-07-17 James K. Williams , Mario Gliozzi , Ross V. Rudzinsky

In the last decade, there have been several discoveries of Active Galactic Nuclei (AGN) in dwarf galaxies including an AGN in an ultra-compact dwarf galaxy with a Black Hole mass $>$10$^{6}$ M$_{\odot}$. However, finding a Supermassive…

Astrophysics of Galaxies · Physics 2024-08-21 Abhishek Paswan , Mousumi Das , K Rubinur

The physics of active super massive black holes (BHs) is governed by their mass (M_BH), spin (a*) and accretion rate ($\dot{M}$). This work is the first in a series of papers with the aim of testing how these parameters determine the…

Astrophysics of Galaxies · Physics 2015-06-23 Daniel M. Capellupo , Hagai Netzer , Paulina Lira , Benny Trakhtenbrot , Julían Mejía-Restrepo

Ultra-luminous X-ray sources are extragalactic objects located outside the nucleus of the host galaxy with bolometric luminosities >10^39 erg s^-1. These extreme luminosities - if the emission is isotropic and below the theoretical (i.e.…

High Energy Astrophysical Phenomena · Physics 2010-01-06 Sean Farrell , Natalie Webb , Didier Barret , Olivier Godet , Joana Rodrigues

This study aims to characterise, for the first time, intranight optical variability (INOV) of low-mass active galactic nuclei (LMAGN) which host a black hole (BH) of mass $M_{BH} \sim 10^6 M_{\odot}$, i.e., even less massive than the…

High Energy Astrophysical Phenomena · Physics 2022-10-26 Gopal-Krishna , Krishan Chand , Hum Chand , Vibhore Negi , Sapna Mishra , S. Britzen , P. S. Bisht

We investigate the relation between the X-ray nuclear emission, optical emission line, radio luminosity and black hole mass for a sample of nearby Seyfert galaxies. Strong linear correlations between the 2-10 keV and [OIII], radio…

Astrophysics · Physics 2008-11-26 F. Panessa , L. Bassani , M. Cappi , M. Dadina , X. Barcons , F. J. Carrera , L. C. Ho , K. Iwasawa , S. Pellegrini

We have completed two years of photometric and spectroscopic monitoring of a large number of active galactic nuclei (AGNs) with very high accretion rates. In this paper, we report on the result of the second phase of the campaign, during…

We present inferences on the geometry and kinematics of the broad-Hbeta line-emitting region in four active galactic nuclei monitored as a part of the fall 2010 reverberation mapping campaign at MDM Observatory led by the Ohio State…

Astrophysics of Galaxies · Physics 2017-11-15 C. J. Grier , A. Pancoast , A. J. Barth , M. M. Fausnaugh , B. J. Brewer , T. Treu , B. M. Peterson

We present the results from performing spectral energy distribution (SED) fitting on 121 variable active galactic nuclei (AGN) candidates in the Hubble Ultra Deep Field (HUDF) using photometry from both the Hubble Space Telescope (HST) and…

We report the discovery using Spitzers high resolution spectrograph of 7 Active Galactic Nuclei (AGN) in a sample of 32 late-type galaxies that show no definitive signatures of AGN in their optical spectra. Our observations suggest that the…

Astrophysics · Physics 2009-11-13 S. Satyapal , D. Vega , R. P. Dudik , N. P. Abel , T. Heckman

We investigate the host galaxy luminosities of BL Lac Objects (BLLs) and Radio Loud Quasars (RLQs) at z<0.5 imaged with the Hubble Space Telescope (HST). From a homogeneous treatment of the data we construct the host galaxy luminosity…

Astrophysics · Physics 2009-11-07 Renato Falomo , Nicoletta Carangelo , Aldo Treves

JWST observations have unveiled faint active galactic nuclei (AGN) at high-redshift that provide insights on the formation of supermassive black holes (SMBHs) and their coevolution with galaxies. However, disentangling stellar from AGN…

The masses of the central black holes of Active Galactic Nuclei estimated by the reverberation virial technique seem to be significantly smaller than predicted from the black hole mass-bulge luminosity relation for massive black holes…

Astrophysics · Physics 2007-05-23 Amri Wandel
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