Radio and spectroscopic properties of miniature radio- galaxies: revealing the bulk of radio-loud AGN population Ranieri D. Baldi 1, and Alessandro Capetti.

Slides:

Advertisements

Similar presentations

The accretion mechanism in low power radio-galaxies Ranieri D. Baldi 1, Barbara Balmaverde 2 & Alessandro Capetti 2 1: Università degli Studi di Torino.

Advertisements

AGN Feedback at the Parsec Scale Feng Yuan Shanghai Astronomical Observatory, CAS with: F. G. Xie (SHAO) J. P. Ostriker (Princeton University) M. Li (SHAO)

The ubiquitous UV murmurs of sleeping supermassive BHs Dani Maoz With: Neil Nagar, Heino Falcke, Andrew Wilson.

JVN observations of (NLS1s and) BAL quasars 2009Mar18-20 EAVN-WS Seoul Akihiro Doi ( 土居明広 ) （ ASTRO-G/JAXA ） Keiichi Asada, Kenta Fujisawa, Noriyuki.

Radio and X-ray emission in radio-quiet quasars Katrien C. Steenbrugge, Katherine M. Blundell and Zdenka Kuncic Instituto de Astronomía, UCN Department.

AGN Eddington Ratio Distributions

Spitzer Reveals Activities of Supermassive Black Holes in Elliptical Galaxies Qiusheng Gu Nanjing University in collaboration with J.-S. Huang (CfA), G.

The Radio-Loud/Radio-Quiet Dichotomy of AGN Brandon Kelly Astro 596.

AGN in hierarchical galaxy formation models Nikos Fanidakis and C.M. Baugh, R.G. Bower, S. Cole, C. Done, C. S. Frenk Accretion and ejection in AGN, Como,

Discovery of an FRII microquasar Manfred Pakull (Strasbourg Observatory) Jess Broderick (Southampton) Stephane Corbel (Université Paris 7 and CEA Saclay.

Bulges are some of the densest stellar systems. They can be flattened, ellipsoidal or bar-like. The surface brightness of a bulge is often approximated.

AGN-controlled gas cooling in elliptical galaxies and galaxy clusters Christian R. Kaiser, Edward C.D. Pope, Georgi Pavlovski, Hans Fangohr, Southampton.

Review of Radio Observations Tiziana Venturi Bologna, 5 Novembre 2009 Galaxy Evolution and Environment.

Quasar Clustering from SDSS DR7: Dependencies on FIRST Radio Magnitudes Andria C. Schwortz, Sarah Eftekharzadeh, Adam D. Myers, Yue Shen Clustering is.

Low-Luminosity AGN Heino Falcke Max-Planck Institut für Radioastronomie, Bonn Neil Nagar, Andrew S. Wilson Sera Markoff, Feng Yuan.

ACCRETION AND JET POWERS IN NEARBY ACCRETION AND JET POWERS IN NEARBY UNOBSCURED RADIO GALAXIES UNOBSCURED RADIO GALAXIES E. Trussoni (1), S. Vattakunnel.

Active Galactic Nuclei Very small angular size: point like High luminosity: compared to host galaxies Broad-band continuum emission: radio to TeV Strong.

USING LOW POWER RADIO GALAXIES AS BEACONS FOR CLUSTERS TO “FILL THE GAP” AT 1

Active Galactic Nuclei Astronomy 315 Professor Lee Carkner Lecture 19.

Weak-Lensing selected, X-ray confirmed Clusters and the AGN closest to them Dara Norman NOAO/CTIO 2006 November 6-8 Boston Collaborators: Deep Lens Survey.

Jets in Low Power Compact Radio Galaxies Marcello Giroletti Department of Astronomy, University of Bologna INAF Institute of Radio Astronomy & G. Giovannini.

Statistical Properties of Radio Galaxies in the local Universe Yen-Ting Lin Princeton University Pontificia Universidad Católica de Chile Yue Shen, Michael.

AGN in hierarchical galaxy formation models Nikos Fanidakis and C.M. Baugh, R.G. Bower, S. Cole, C. Done, C. S. Frenk Physics of Galactic Nuclei, Ringberg.

Low frequency radio observations of galaxy groups With acknowledgements to: R. Athreya, P. Mazzotta, T. Clarke, W. Forman, C. Jones, T. Ponman S.Giacintucci.

Dusty star formation at high redshift Chris Willott, HIA/NRC 1. Introductory cosmology 2. Obscured galaxy formation: the view with current facilities,

Optical Spectroscopy of Distant Red Galaxies Stijn Wuyts 1, Pieter van Dokkum 2 and Marijn Franx 1 1 Leiden Observatory, P.O. Box 9513, 2300RA Leiden,

1 The Fundamental Plane Relationship of Astrophysical Black Holes Ran Wang Supervisor: Xuebing Wu Peking University Ran Wang Supervisor: Xuebing Wu Peking.

The Evolution of Quasars and Massive Black Holes “Quasar Hosts and the Black Hole-Spheroid Connection”: Dunlop 2004 “The Evolution of Quasars”: Osmer 2004.

A spectroscopic survey of the 3CR sample of radio galaxies Authors: Sara Buttiglione (SISSA - Trieste), Alessandro Capetti (INAF – Osservatorio Astronomico.

Unravelling the formation and evolutionary histories of the most massive galaxies Ilani Loubser (Univ. of the Western Cape)

Jet/environment interactions in FR-I and FR-II radio galaxies Judith Croston with Martin Hardcastle, Mark Birkinshaw and Diana Worrall.

THE HST VIEW OF LINERS AND OTHER LOCAL AGN MARCO CHIABERGE CNR - Istituto di Radioastronomia - Bologna Alessandro Capetti (INAF-OATo) Duccio Macchetto.

Low Power Compact radio galaxies at high angular resolution Marcello Giroletti INAF Istituto di Radioastronomia & G. Giovannini (UniBO, IRA) G. B. Taylor.

I.Introduction  Recent evidence from Fermi and the VLBA has revealed a strong connection between ɣ -ray emission in AGNs and their parsec-scale radio.

High-resolution observations of powerful radio sources Monica Orienti Almudena Prieto 13/12/2007 Monica Orienti – IAC.

The Large Scale Structure of Seyferts and LINERs and Implications for their Central Engines Anca Constantin Drexel University AGN are not unbiased tracers.

Properties of the point-like sources in the XMM-LSS field Olga Melnyk and XMM-LSS collaboration N. Clerc, L. Chiappetti, A. Elyiv, P.Gandhi, E.Gosset,

The Environmental Effect on the UV Color-Magnitude Relation of Early-type Galaxies Hwihyun Kim Journal Club 10/24/2008 Schawinski et al. 2007, ApJS 173,

The MOJAVE Program: Studying the Relativistic Kinematics of AGN Jets Jansky Postdoctoral Fellow National Radio Astronomy Observatory Matthew Lister.

University of Leicester, UK X-ray and Observational Astronomy (XROA) Group Estelle Pons - The X-ray Universe June 2014.

FRI RADIO GALAXIES AT z > 1 STUDYING THE BUILDING BLOCKS OF TODAY'S MOST MASSIVE GALAXIES AND CLUSTERS Marco Chiaberge Space Telescope Science Institute.

Galactic Astronomy 銀河物理学特論 I Lecture 2-1: Active galaxies and super massive black holes in the local universe Seminar: Gultekin et al. 2009, ApJ, 698,

Joint formation and evolution of SMBHs and their host galaxies: How do the Quasar-Spheroid correlations change with the Cosmic Time? A. Treves Università.

Astrophysics from Space Lecture 6: Supermassive black holes Prof. Dr. M. Baes (UGent) Prof. Dr. C. Waelkens (KUL) Academic year

USING LOW POWER RADIO GALAXIES AS BEACONS FOR CLUSTERS AT 1

On the spectro-photometric properties of the bulk of Radio-Loud AGN population Ranieri D. Baldi 1, Alessandro Capetti 2 1: SISSA, Trieste 2: Osservatorio.

Radio Galaxies part 4. Apart from the radio the thin accretion disk around the AGN produces optical, UV, X-ray radiation The optical spectrum emitted.

21 Aug 2014HEAD Meeting Chicago Revealing the heavily obscured AGN population with radio selection Wilkes, Kuraszkiewicz, Atanas, Haas, Barthel, Willner,

The dependence on redshift of quasar black hole masses from the SLOAN survey R. Decarli Università dell’Insubria, Como, Italy A. Treves Università dell’Insubria,

Multiwavelength Properties of the SDSS Galaxies in Various Classes Feb 19, 2008 Joon Hyeop Lee 1, Myung Gyoon Lee 1, Changbom Park 2, Yun-Young Choi 2.

The History of Active Galaxies A.Barger, P. Capak, L. Cowie, RFM, A. Steffen, and Y. Yang Active Galaxies (AKA quasars, Seyfert galaxies etc) are radiating.

The University of Sheffield Joanna Holt 20 th October 2006 Emission line outflows: the evidence for AGN-induced feedback Clive Tadhunter.

Unification -- 2 Where next?. Recap of current status Emission from nuclear relativistic jets is important in all radio-loud objects. Axisymmetric dust.

The luminosity-dependent evolution of the radio luminosity function Emma Rigby University of Nottingham Collaborators: P. Best, M. Brookes, J. Dunlop,

Brigthest Cluster Galaxies Unique class of objects  most luminous  most massive  extended source  some BCG shows multiple nuclei → galaxy merger →

Tools for computing the AGN feedback: radio-loudness and the kinetic luminosity function Gabriele Melini Fabio La Franca Fabrizio Fiore Active Galactic.

X-RAY PROPERTIES OF FR II/NLRG X-RAY PROPERTIES OF FR II/NLRG E. Trussoni 1, A. Capetti 1, B. Balmaverde 2 1 INAF – Osservatorio Astronomico di Torino,

The Radio Properties of Type II Quasars PLAN Type II quasars Motivations Our sample Radio observations Basic radio properties Compare our results with.

High Redshift Galaxies/Galaxy Surveys ALMA Community Day April 18, 2011 Neal A. Miller University of Maryland.

The optical morphologies of the 2Jy sample of southern radio galaxies Cristina Ramos Almeida & Clive N. Tadhunter University of Sheffield.

1 Lei Bai George Rieke Marcia Rieke Steward Observatory Infrared Luminosity Function of the Coma Cluster.

AGN in the VVDS (Bongiorno, Gavignaud, Zamorani et al.) 1.What has been done: main results on Type 1 AGN evolution and accretion properties of faint AGN.

A spectroscopic study of the 3CR sample of radio galaxies

Radio Loud and Radio Quiet AGN

A Survey of Starburst Galaxies An effort to help understand the starburst phenomenon and its importance to galaxy evolution Megan Sosey & Duilia deMello.

Radio Galaxies Part 5.

The origin nuclear X-ray emission in the nuclei of radio galaxy-FR Is

Group Nov. 01, USTC 4/18/2019 Group Nov. 01, USTC AGN-dominated SFG-dominated.

Galaxies With Active Nuclei

Metallicity Evolution of Active Galactic Nuclei

Presentation transcript:

Radio and spectroscopic properties of miniature radio- galaxies: revealing the bulk of radio-loud AGN population Ranieri D. Baldi 1, and Alessandro Capetti 2 1: University of Torino, INAF 2: Astronomical Observatory of Torino, INAF 2009arXiv B

Baldi Ranieri D. Leiden, 25/11/2009 The Core Galaxies are miniature radio-galaxies. (Balmaverde & Capetti 06 and Balmaverde,Baldi & Capetti 08). CoreG 3CR/FRI

The aim of this presentation is: 1.The Optical spectroscopic identification of Core Galaxies. 2.Analysis of Radio properties. 3.Comparison with samples of Radio Loud AGN at higher power. Baldi Ranieri D. Leiden, 25/11/2009

The properties of the radio emission are similar to those of 3C/FRI. UGC 8745 = 0.7 ~20kpc

Baldi Ranieri D. Leiden, 25/11/2009 The CoreG show a Core Dominance of a factor 100 larger than the classical 3C/FRI. CoreG 3CR

Baldi Ranieri D. Leiden, 25/11/2009 The Core Galaxies are Low Excitation Galaxies (LEG) like 3C/FRI. 3CR/LEG Kewley et al. (2006)

Baldi Ranieri D. Leiden, 25/11/2009 The nuclear properties of CoreG are similar to those of FRI. CoreG show a genuine extended radio emission deficit of a factor 100.

Baldi Ranieri D. Leiden, 25/11/2009 Deficit in radio extended emission?? But, their radio core is fainter than that typical of FRI/LEG. Let us look for other core dominated sources in sample of higher power.

Baldi Ranieri D. Leiden, 25/11/2009 High core dominated sources with higher radio core power! From Giovannini et al. (1988) B2 sample, 11 objects with core dominance > 0.1 B2 CoreG 3CR/FRI B2

Baldi Ranieri D. Leiden, 25/11/2009 Our interpretation: The prevalence of low core dominance sources in low frequency flux limited samples is due to a selection bias. To test this scenario.. Best et al (2005) of RL AGN: crossmatching the galaxies drawn from the SDSS DR2 with the NVSS and FIRST radio surveys. Selection: > 5 mJy

Baldi Ranieri D. Leiden, 25/11/2009 The bulk of the population of this SDSS/NVSS AGN sample shows a large deficit of total radio emission, similar to that observed in CoreG. 3CR correlation Seyfert > 5 mJy At z=0.1 L r = erg s -1 CoreG

Baldi Ranieri D. Leiden, 25/11/2009 If we use the B2 sample flux selection criterion, low core dominance radio galaxies are the dominant population. 3CR correlation

Baldi Ranieri D. Leiden, 25/11/2009 Extended radio emission is indipendent of the AGN power. FWHM = 5 arcsec

Baldi Ranieri D. Leiden, 25/11/2009 Are there differences between core dominated sources and FRI? 1.Spectral classification 2.Host mass, morphology and colors 3.Black hole mass distribution

Baldi Ranieri D. Leiden, 25/11/2009 Most of the radio-loud AGN of the SDSS/NVSS sample are low excitation galaxies (LEG). LEG HEG SFG AGN

Baldi Ranieri D. Leiden, 25/11/2009 The radio sources of Best et al (2005) sample have nuclei with properties analogous with those of radio-loud LEG.

Baldi Ranieri D. Leiden, 25/11/2009 The popoulation of SDSS/NVSS AGN sample is flux-limited. The density of objects grows with L down to the completeness limit. Completeness limit

Baldi Ranieri D. Leiden, 25/11/ Most of the radio sources are highly core dominated. 2.Selection bias in radio flux-limited sample causes the inclusion only of radio-galaxies with well developped extended structures. 2.The bulk of RL AGN population is virtually unexplored. 4.Radio extended emission loses its fundamental role of “calorimeter” of the jet power! 5.the SDSS/NVSS AGN sample is composed of quiescent giant elliptical, M BH ~ , LEG, with nuclei similar to those of 3C FRI/LEG. Possible interpretations for low extended power: 1. Link between age and radio extended emission. Young, recurrent? 2.Influence of environment on the jets properties.