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It is shown that 21 cm intensity mapping could be used in the near term to make cosmologically useful measurements. Large scale structure could be detected using existing radio telescopes, or using prototypes for dedicated redshift survey…

宇宙学与河外天体物理 · 物理学 2010-10-13 Kiyoshi Wesley Masui , Patrick McDonald , Ue-Li Pen

We explore how the local environment is related to the redshift, type, and luminosity of active galactic nuclei (AGN). Recent simulations and observations are converging on the view that the extreme luminosity of quasars is fueled in major…

天体物理学 · 物理学 2009-11-13 Natalie E. Strand , Robert J. Brunner , Adam D. Myers

X-ray variability is a well-established characteristic of active galactic nuclei (AGN), known to correlate inversely with both the supermassive black hole mass and luminosity, although the degree of each remains a topic of debate. The…

We present a sample of 40 AGN in dwarf galaxies at redshifts $z \lesssim$ 2.4. The galaxies are drawn from the \textit{Chandra} COSMOS-Legacy survey as having stellar masses $10^{7}\leq M_{*}\leq3 \times 10^{9}$ M$_{\odot}$. Most of the…

星系天体物理 · 物理学 2018-05-16 M. Mezcua , F. Civano , S. Marchesi , H. Suh , G. Fabbiano , M. Volonteri

The properties of the host galaxies of a well-defined sample of 2215 radio-loud AGN with redshifts 0.03 < z < 0.3, defined from the SDSS, are investigated. These are predominantly low radio luminosity sources, with 1.4GHz luminosities of…

天体物理学 · 物理学 2008-11-26 P. N. Best , G. Kauffmann , T. M. Heckman , J. Brinchmann , S. Charlot , Z. Ivezic , S. D. M. White

We test the standardizability of a homogeneous sample of 41 lower-redshift ($0.00415\leq z \leq 0.474$) active galactic nuclei (AGNs) reverberation-mapped (RM) using the broad H$\alpha$ and H$\beta$ emission lines. We find that these…

星系天体物理 · 物理学 2025-04-07 Shulei Cao , Amit Kumar Mandal , Michal Zajaček , Bożena Czerny , Bharat Ratra

We present medium resolution near infrared spectroscopic observations of 41 obscured and intermediate class AGN (type 2, 1.9 and 1.8; AGN2) with redshift $z \lesssim$0.1, selected from the Swift/BAT 70-month catalogue. The observations have…

星系天体物理 · 物理学 2016-10-21 F. Onori , F. La Franca , F. Ricci , M. Brusa , E. Sani , R. Maiolino , S. Bianchi , A. Bongiorno , F. Fiore , A. Marconi , C. Vignali

JWST observations have uncovered a new population of red, compact objects at high redshifts dubbed `Little Red Dots' (LRDs), which typically show broad emission lines and are thought to be dusty Active Galactic Nuclei (AGN). Some of their…

Abstract abridged. The eROSITA X-ray telescope aboard the SRG orbital observatory, in the course of its all-sky survey, is expected to detect about three million active galactic nuclei (AGN) and hundred thousand clusters and groups of…

高能天体物理现象 · 物理学 2023-01-11 S. D. Bykov , M. R. Gilfanov , R. A. Sunyaev

In the Hubble Deep Field (HDF), twelve candidate sources of high-redshift (z > 3.5) AGN activity have been identified. The color selection criteria were established by passing spectra of selected quasars and Seyfert galaxies (appropriately…

天体物理学 · 物理学 2009-10-31 R. Michael Jarvis , Gordon M. MacAlpine

Context: Variations in the mass accretion rate appear to be responsible for the rapid transitions in spectral type that are observed in increasingly more active galactic nuclei (AGNs). These objects are now labeled "changing-look" AGNs and…

星系天体物理 · 物理学 2020-04-15 F. Marin , D. Hutsemékers

For measurement of the AGN luminosity function and its evolution, X-ray selection samples all types of AGN and provides reduced obscuration bias in comparison with UV-excess or optical surveys. The apparent decline in optically-selected…

We study the host galaxies and black holes of typical X-ray selected AGN at intermediate redshifts (z~0.5-1.4). The AGN are selected such that their spectral energy distributions are dominated by stellar emission, i.e., they show a…

天体物理学 · 物理学 2009-11-13 Almudena Alonso-Herrero

The possibility of a correlation between the radio (cm)- and $\gamma$-ray luminosity of variable AGN seen by EGRET is investigated. We performed Monte-Carlo simulations of typical data sets and applied different correlation techniques…

We show that individual (single-epoch) spectra of AGN can constrain some of the geometry and dynamics of the AGN broad line region. Studies of the cosmic influence of supermassive black holes are limited by the current large uncertainties…

星系天体物理 · 物理学 2019-08-21 S. I. Raimundo , A. Pancoast , M. Vestergaard , M. R. Goad , A. J. Barth

We have previously shown that the linewidth distribution in AGN can be accounted for by an axisymmetric broad emission line region. In this paper we show that the linewidth distribution changes with redshift and that these changes are…

天体物理学 · 物理学 2009-10-31 C. M. Rudge , D. J. Raine

We select a sample of radio galaxies at high redshifts (z>~1) in the COSMOS field, by cross-matching optical/infrared images with the FIRST radio data. The aim of this study is to explore the high-z radio-loud (RL) AGN population at much…

星系天体物理 · 物理学 2014-09-05 Ranieri D. Baldi , Alessandro Capetti , Marco Chiaberge , Annalisa Celotti

We discuss a sample of 29 AGN (16 narrow-lined and 13 broad-lined) discovered in a spectroscopic survey of ~1000 star-forming Lyman-break galaxies (LBGs) at z~3. Reaching apparent magnitudes of R_{AB}=25.5, the sample includes broad-lined…

天体物理学 · 物理学 2009-11-07 C. Steidel , M. Hunt , A. Shapley , K. Adelberger , M. Pettini , M. Dickinson , M. Giavalisco

A catalogue of 14453 radio-loud AGN with 1.4 GHz fluxes above 3.5 mJy in the redshift range 0.4<z<0.8, has been constructed from the cross-correlation of the NVSS and FIRST radio surveys with the MegaZ-LRG catalogue of luminous red galaxies…

天体物理学 · 物理学 2010-11-30 E. Donoso , P. N. Best , G. Kauffmann

Context: A long-standing challenge of observational AGN research is to find type 2 quasars, the luminous analogues of Seyfert-2 galaxies. Aims: We search for luminous narrow-line type 2 AGN, characterise their properties, and compare them…