STATUS (structure): STATUS (structure):

Slides:



Advertisements
Similar presentations
X-ray jets from B : A Middle-aged Pulsar's New Trick Q. Daniel Wang & Seth Johnson University of Massachusetts.
Advertisements

X-ray and optical detection of the radio bent jet in 3C 17 Radio Galaxies in the Chandra Era F. Massaro & D. E. Harris, M. Chiaberge, P. Grandi, F. D.
Mapping HI absorption at z=0.026 against a resolved background CSO Andy Biggs, Martin Zwaan, Jochen Liske European Southern Observatory Frank Briggs Australian.
Radio properties of BAL quasars Takayuki HAYASHI (Univ. Tokyo, NAOJ/VLBI) Akihiro Doi (ISAS/JAXA) Hiroshi Nagai (ALMA/NAOJ)
Cyclotron & Synchrotron Radiation
Multi-Wavelength Polarizations of Western Hotspot of Pictor A Mahito Sasada (Kyoto University) S. Mineshige (Kyoto Univ.), H. Nagai (NAOJ), M. Kino (JAXA),
Particle acceleration in active galaxies – the X-ray view Martin Hardcastle (U. Herts) Thanks to many co-authors including Ralph Kraft (CfA), Judith Croston.
It’s Anybody’s Guess Welcome to. Question 1: B. C. D. A. Next question.
Compact Steep-Spectrum and Gigahertz Peaked-Spectrum Radio Sources Reviews: O’Dea 1998 PASP 110:493 Third Workshop on CSS/GPS Radio Sources 2003 PASA Vol.
X-ray synchrotron radiation and particle acceleration Martin Hardcastle University of Bristol, UK with Diana Worrall & Mark Birkinshaw (Bristol), Dan Harris.
GLAST Collab Mtg 08/05- 1 Getting IDs for the GLAST Catalog: Blazar FoM analysis Looking Under the Lamppost –The bright 3EG blazars share common characteristics.
Ultra Relativisitic Jets in Astrophysics, Banff, July 2005Gelbord et al.: Deep Observations of Quasar Jets Deep X-Ray and Optical Observations of Quasar.
Jets in Low Power Compact Radio Galaxies Marcello Giroletti Department of Astronomy, University of Bologna INAF Institute of Radio Astronomy & G. Giovannini.
L. Rudnick - Krakow - June 2006 Particle distributions in large scale radio jets Lawrence Rudnick University of Minnesota.
Astrophysical Jets Robert Laing (ESO). Galactic black-hole binary system Gamma-ray burst Young stellar object Jets are everywhere.
Sites of Particle Acceleration in Quasar Jets Alan Marscher Boston University Research Web Page:
Synchrotron Radiation, continued Rybicki & Lightman Chapter 6 Also Course notes for “Essential Radio Astronomy” at NRAO, Condon & Ransom
8th EVN Symposium 2006 Exploring the Universe with the real-time VLBI Toruń, Poland, September 2006 Carlo Stanghellini Istituto di Radioastronomia.
Star Formation Research Now & With ALMA Debra Shepherd National Radio Astronomy Observatory ALMA Specifications: Today’s (sub)millimeter interferometers.
Molecular absorption in Cen A on VLBI scales Huib Jan van Langevelde, JIVE Ylva Pihlström, NRAO Tony Beasley, CARMA.
Imaging Compact Supermassive Binary Black Holes with VLBI G. B. Taylor (UNM), C. Rodriguez (UNM), R. T. Zavala (USNO) A. B. Peck (CfA), L. K. Pollack (UCSC),
A study of a ULIRG-to-QSO transition object: possibly another gas-rich/gas-poor merger and a serendipitous line detection Manuel Aravena, Jeff Wagg, Padelis.
Low Power Compact radio galaxies at high angular resolution Marcello Giroletti INAF Istituto di Radioastronomia & G. Giovannini (UniBO, IRA) G. B. Taylor.
Gabriele Giovannini Dipartimento di Astronomia, Bologna University Istituto di Radioastronomia - INAF Low Luminosity Radio Loud AGNs In collaboration with.
This composite X-ray (blue)/radio (pink) image of the galaxy cluster Abell 400 shows radio jets immersed in a vast cloud of multimillion degree X-ray emitting.
EVN observations of GPS radio sources Liu X. Urumqi Observatory, NAOC.
Political Parties. Activity: Canada's Federal Political Parties Canada has five major political parties Check out the information about parties on
FRI RADIO GALAXIES AT z > 1 STUDYING THE BUILDING BLOCKS OF TODAY'S MOST MASSIVE GALAXIES AND CLUSTERS Marco Chiaberge Space Telescope Science Institute.
8/13/101 Updates on the simulation. 8/13/102 Some news I finally have the event generator working, for which the ‘physics’ event has 5 D D 0 bar,
Gabriele Giovannini Marcello Giroletti Gregory B. Taylor Dipartimento di Astronomia, Bologna University Istituto di Radioastronomia, INAF Bologna Dept.
USING LOW POWER RADIO GALAXIES AS BEACONS FOR CLUSTERS AT 1
40 Minutes Left.
Minutes Left:
The University of Sheffield Joanna Holt 20 th October 2006 Emission line outflows: the evidence for AGN-induced feedback Clive Tadhunter.
A USAGE OF THE VLBA: GRAVITATIONAL LENSING AND COMPACT/MEDIUM SYMMETRIC OBJECTS Pedro Augusto 1 (et al. 2 ) 1 Departamento de Matemática e Centro.
Challenging the merger/sloshing cold front paradigm: A2142 revisited by XMM Mariachiara Rossetti (Università degli Studi di Milano & IASF Milano) D. Eckert,
Experimental vs. Theoretical Probability. Theoretical vs. Experimental Probability Objectives: (1)(2) Essential Questions: (1)(2)
Personal Injury Lawyer Niagara Falls - KPC Personal Injury Lawyer (800)
بسم الله الرحمن الرحیم. Jet grouting.
David By michelangelo. Statue.
HomePlug Overview and Motorola Status
A spectroscopic study of the 3CR sample of radio galaxies
Locked.
Using the GAVRT Radio Telescope: The SETI Project
THE X-RAY PROPERTIES OF TYPICAL HIGH-REDSHIFT RADIO-LOUD QUASARS
Air Canada Customer Service Phone Number USA
SLOT Week 1 Day 1 1. When light from a star produces a line spectrum similar to that produced by a particular element, what should we conclude about that.
Robert Johnson W. Atwood, M. Ziegler, B. Baughman U.C. Santa Cruz and
A 325 MHz Radio Survey of M31 Yosi Gelfand (CfA) Joseph Lazio (NRL) Bryan Gaensler (CfA) Using the VLA A-array, we imaged 405 radio sources.
7.2 Fractions, Decimals, and Percents
معاًً من اجل بيئة مرورية آمنه
How to classify a Gamma -ray source as a Blazar
The origin nuclear X-ray emission in the nuclei of radio galaxy-FR Is
Galaxies.
Name: ________________________________________ Period: _____
What is a political party?
Reading a Vernier.
? Q: There are 2 candies in left hand.
Welcome to It’s Anybody’s Guess.
Guess the letter!.
AIDA Asic Heatsinks Prototype received, and approved.
4-H Status All members on this screen are “Pending,” because they are awaiting your confirmation. Confirming the member does not change their status from.
Properties of Normal Distributions
EXAMPLE.
÷ 5 = 29 How many 5s are there in 1? Great!
÷ 2 = 24 How many 2s are there in 4?
X-shaped radio sources as the core-dominated triple blazars
Time Approval Overview March 27, 2003
Cosmological parameters with radio galaxies
Modeling Sgr A* Flares: Nonthermal Processes in an Outflow
Presentation transcript:

STATUS (structure): STATUS (structure): 157 resolved flat-spectrum radio sources 61 sources rejected 12 CSO/MSOs 1 MSO candidate must be at z<0.09 83 sources left 12 have part of available data reduced 19 have no data reduced yet STATUS (structure): 4 anybody’s guess 4 probable core-jets 2 probable FRIIs 1 probable MSO 1 MSO 52 have all data available reduced STATUS (structure): 5 anybody’s guess 17 probable core-jets 2 probable FRIIs 13 probable CSO/MSOs 2 MSOs (if z<0.14; z<0.3) 4 core-jets 2 FRIIs (25 kpc; 570 kpc) 7 CSO/MSOs (two: 3.3 kpc; 13 kpc)