Radio flux density monitoring: recent MERLIN results Andy Biggs (Joint Institute for VLBI in Europe)

Slides:



Advertisements
Similar presentations
Jeroen Stil Department of Physics & Astronomy University of Calgary Stacking of Radio Surveys.
Advertisements

Kinematic Studies of the IDV Quasar S. Bernhart T. P. Krichbaum L. Fuhrmann Max-Planck-Institut fϋr Radioastronomie, Bonn.
Detection and Photometric Monitoring of QSOs and AGN with COROT J. Surdej, J.Poels, J.-F. Claeskens, E. Gosset Institut d’Astrophysique et de Géophysique,
Radio and X-ray emission in radio-quiet quasars Katrien C. Steenbrugge, Katherine M. Blundell and Zdenka Kuncic Instituto de Astronomía, UCN Department.
Gabriele Giovannini Dipartimento di Astronomia, Bologna University Istituto di Radioastronomia - INAF EVN observations of M87 as follow-up on a recent.
An Introduction to Gravitational Lensing Ian Browne, Jodrell Bank Observatory (Thanks to Andy Biggs and Neal Jackson for pictures and slides)
Mapping HI absorption at z=0.026 against a resolved background CSO Andy Biggs, Martin Zwaan, Jochen Liske European Southern Observatory Frank Briggs Australian.
A rough guide to radio astronomy and its use in lensing studies Simple stuff other lecturers may assume you know (and probably do)
On the origin of color anomaly between multiple images of lensed quasars Atsunori Yonehara (Univ. Tokyo, Inoue Fellow) (Univ. Tokyo, Inoue Fellow) Hiroyuki.
High-Resolution Radio Observations of the Scintillating Extragalactic Source J Brian Moloney 1, Denise Gabuzda 1, A. G. De Bruyn 2,3, J.P. Macquart.
25 YEARS AFTER THE DISCOVERY: SOME CURRENT TOPICS ON LENSED QSOs Santander (Spain), 15th-17th December 2004 CLASS B and the Hubble Constant Tom.
VLBI Imaging of a High Luminosity X-ray Hotspot Leith Godfrey Research School of Astronomy & Astrophysics Australian National University Geoff Bicknell,
Radio Astronomy And The Spiral Structure Of The Milky Way Jess Broderick Supervisor: Dr George Warr.
SLAC, 7 October Multifrequency Strategies for the Identification of Gamma-Ray Sources Marcus Ziegler Santa Cruz Institute for Particle Physics Gamma-ray.
25 YEARS AFTER THE DISCOVERY: SOME CURRENT TOPICS ON LENSED QSOs Santander (Spain), 15th-17th December 2004 FLUX RATIO ANOMALY by Luis J. Goicoechea (UC)
Physics 133: Extragalactic Astronomy and Cosmology Lecture 13; February
PX269 Galaxies Part 4: Galactic nuclei 4.1 Active galaxies.
SLAC, 7 October Multifrequency Strategies for the Identification of Gamma-Ray Sources Marcus Ziegler Santa Cruz Institute for Particle Physics Gamma-ray.
A Primer on SZ Surveys Gil Holder Institute for Advanced Study.
SLAC, 7 October Multifrequency Strategies for the Identification of Gamma-Ray Sources Marcus Ziegler Santa Cruz Institute for Particle Physics Gamma-ray.
25 YEARS AFTER THE DISCOVERY: SOME CURRENT TOPICS ON LENSED QSOs Santander (Spain), 15th-17th December 2004 Monitoring Projects: Introduction Dan Maoz,
Variable SiO Maser Emission from V838 Mon Mark Claussen May 16, 2006 Nature of V838 Mon and its Light Echo.
The Transient Universe: AY 250 Spring 2007 Existing Transient Surveys: Radio II: Interferometric Surveys Geoff Bower.
Deep, wide-field global VLBI observations of HDF-N Deep, wide-field global VLBI observations of HDF-N Seungyoup Chi Kapteyn Institute (RuG) / JIVE Collaborators.
VSOP-2 Detection of Faraday screen? Inoue M., Asada K.*, and Nagai H. National Astronomical Obs. of Japan * Institute of Space and Astronautical Science.
Survey Quality Jim Condon NRAO, Charlottesville. Survey Qualities Leiden 2011 Feb 25 Point-source detection limit S lim Resolution Ω s Brightness sensitivity.
RTS Manchester Two special radio AGN: BL Lac and J Ger de Bruyn + work with J-P. Macquart ASTRON, Dwingeloo & Kapteyn Institute,
11/12/03 5th COROT Week Detection and Photometric Monitoring of QSOs and AGN with COROT J. Surdej, J.-F. Claeskens, E. Gosset, J. Poels, P. Riaud, A. Smette,
Intraday variability of Sgr A* at radio wavelengths: A Day in the Life of Sgr A* Doug Roberts Northwestern University Adler Planetarium & Astronomy Museum.
The luminous X-ray hotspot in 4C 74.26: jet dynamics at work Mary Erlund Institute of Astronomy, Cambridge, UK A.C. Fabian, K.M. Blundell, C. Moss and.
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),
Observations of Intra-Hour Variable Quasars Hayley Bignall (JIVE) Dave Jauncey, Jim Lovell, Tasso Tzioumis (ATNF) Jean-Pierre Macquart (NRAO/Caltech) Lucyna.
Gravitational lensing and the problem of faint galaxies Alicia Berciano Alba (JIVE / Kapteyn institute) Mike Garret (JIVE) Leon Koopmans (Kapteyn institute)
Radio flux density monitoring: a practical guide Andy Biggs (Joint Institute for VLBI in Europe)
Beyond VLBI Micro-arcsecond Resolution with Inter-Stellar Scintillation D.L. Jauncey 1,2, J.E.J. Lovell 3, J.Y. Koay 4, J-P. Macquart 4, B.J. Rickett 5,
Academia Sinica National Taiwan University AMiBA System Performance Kai-yang Lin 1,2 and AMiBA Team 1,2,3 1 Institute of Astronomy and Astrophysics, Academia.
SUNYAEV-ZELDOVICH EFFECT. OUTLINE  What is SZE  What Can we learn from SZE  SZE Cluster Surveys  Experimental Issues  SZ Surveys are coming: What.
EVN observations of GPS radio sources Liu X. Urumqi Observatory, NAOC.
VLBI Observations of IDV Sources Brian Moloney Dr. Denise Gabuzda University College Cork.
5 GHz observations of intraday variability in some AGNs  Huagang Song & Xiang Liu  Urumqi Observation, NAOCAS.
The MOJAVE Program: Studying the Relativistic Kinematics of AGN Jets Jansky Postdoctoral Fellow National Radio Astronomy Observatory Matthew Lister.
E-MERLIN : a pathfinder for the SKA (a summary of the e-MERLIN talk given at the Berkeley SKA meeting) e-MERLIN : a pathfinder for the SKA (a summary of.
December 17, 2008 The EVLA Vision Galaxies Through CosmicTime 1 Microjansky Radio Sources: AGN or Star Formation? Ken Kellermann & EdFomalont NRAO in collaboration.
Aristeidis Noutsos University of Manchester. The LOFAR Ionosphere See Ger’s talk, in Hamburg last year. Variations of ~3 rad m –2 were observed in the.
Fig. Blazar Sequence ( Fossati et al ) Blazar ・・・ ⇛ Blazar Sequence( Fossati et al ) This characteristic was discovered among bright blazars.
Multi-Frequency Observations of the Gravitational Lens B Anupreeta More Max-Planck-Institut fuer Radioastronomie, Bonn Supervisor : Richard Porcas.
Photometric Redshifts of objects in B field Sanhita Joshi ANGLES Workshop, Crete 07/04/2005.
PHY306 1 Modern cosmology 2: More about Λ Distances at z ~1 Type Ia supernovae SNe Ia and cosmology Results from the Supernova Cosmology Project, the High.
Strong Lensing Surveys and Statistics Dan Maoz. zqzq Survey strategies: Search among source population for lensed cases or Search behind potential lenses.
E-MERLIN & EVLA P.J.DiamondP.J.Diamond MERLIN/VLBI National Facility Jodrell Bank Observatory University of Manchester MERLIN/VLBI National Facility Jodrell.
Gravitational lensing: surveys and studies with new instruments.
The Character of High Energy Emission From The Galactic Binary LS Andy Smith Smithsonian Astrophysical Observatory (for the VERITAS collaboration)
GBT Future Instrumentation Workshop Fixing the frequency coverage hole in C-Band Jagadheep D. Pandian Cornell University.
Dependence of the Integrated Faraday Rotations on Total Flux Density in Radio Sources Chen Y.J, Shen Z.-Q.
Impact of Interstellar Scintillation on Astrometric VLBI Dave Jauncey 1, Jim Lovell 1, Roopesh Ojha 1, Alan Fey 2, Yasuhiro Koyama 3, Hayley Bignall 4,
A Chandra Survey of Quasar Jets: Latest Results Jonathan Gelbord H.L. Marshall (MIT); D.A. Schwartz (SAO); D.M. Worrall & M. Birkinshaw (U. Bristol); J.E.J.
Sébastien Muller (ASIAA, Taiwan) M. Guélin (IRAM) M. Dumke (ESO) R. Lucas (IRAM) Probing isotopic ratios at z=0.89 Molecular line absorptions in front.
VLBA Observations of AU- scale HI Structures Crystal Brogan (NRAO/NAASC) W. M. Goss (NRAO), T. J. W. Lazio (NRL) SINS Meeting, Socorro, NM, May 21, 2006.
W.Becker 1, M.C.Weisskopf 2, Z.Arzoumanian 3, D.Lorimer 4, F.Camilo 5, R.F.Elsner 2, G.Kanbach 1, O.Reimer 6, D.A.Swartz 2, A.F.Tennant 2, S.L.O’Dell 2.
Variability of a Sample of Potential meerKAT/SKA Calibrators Faith Hungwe – RU/HartRAO Advisers: R.Ojha – United States Naval Observatory (USNO)‏ (Alan.
A smoothed hardness map of the hotspots of Cygnus A (right) reveals previously unknown structure around the hotspots in the form of outer and inner arcs.
32 nd ICRC –Beijing – August 11-18, 2011 Silvia Vernetto IFSI-INAF Torino, ITALY On behalf of the ARGO-YBJ collaboration Observation of MGRO J with.
AIPS.
K(2 m) Version of JASMINE and its Science
Observing Strategies for the Compact Array
The First Aperture Synthesis Images of the Galactic Centre
J : a peculiar quasar behind a fast-moving very local screen
“Intermediate” Scale Structure in Cold, Galactic HI Detected with the MERLIN Array Michael Faison (Yale), Miller Goss (NRAO), and Tom Muxlow (Jodrell.
What is the scattering screen in front of quasar PKS B ?
Towards a determination of H0 in JVAS B :
Presentation transcript:

Radio flux density monitoring: recent MERLIN results Andy Biggs (Joint Institute for VLBI in Europe)

Monitoring in the radio Radio monitoring has some advantages over the optical –High and consistent resolution –No extinction due to dust –No microlensing (?) –24 hour per day observing –365 day a year observing were good years for radio time delay determinations –PKS (Lovell et al. 1998) –JVAS B (Biggs et al. 1999) –CLASS (Fassnacht et al. 1999) –QSO (Haarsma et al. 1999) –CLASS (Koopmans et al. 2000)

What has happened since 2000? Only one radio time delay since 2000 –JVAS (Patnaik & Narasimha 2001) Most JVAS/CLASS lenses checked for variability –Results have been disappointing (images don’t vary) –Fassnacht talk Southern lenses as well –e.g. PMN J (Winn et al. 2004) Extrinsic variability detected in CLASS –Koopmans & de Bruyn 2000 –Microlensing or scintillation or both? Largest systematic search has been MERLIN “Key Project”

Extrinsic variability in Right: VLA monitoring revealed uncorrelated variability in A and B – probably microlensing Below: total flux has been monitored with the WSRT at 6, 13 and 21 cm Work by L. Koopmans & G. de Bruyn

MERLIN “Key Project” Monitored 8 JVAS/CLASS lens systems at 5 GHz – – – – – – – – February – November of 2001 (41 epochs) Main goal of project was to detect microlensing Results are preliminary –More work needed to better quantify flux density uncertainties –Assume 2% accuracy for the present –Flux ratios should be more reliable (Koopmans et al., 2003)

A B C D

A B

A B C D E

WSRT follow-up of (5 GHz) Error bars = thermal noise combined with 1% of flux density

VLA archival data of (8.4 GHz) Flux calibrator stability VLA map of

VLA archival data of Error bars = thermal noise combined with 0.5% of flux density

Summary 2 lenses show significant variability with MERLIN – Mainly intrinsic variability Some evidence for extrinsic effects – Clearest detection of extrinsic variability WSRT and VLA support MERLIN results Low Galactic latitude (  10  ) argues in favour of Galactic scintillation Cygnus superbubble lies close to 2045 line of sight No clear detections of microlensing effects seen in MERLIN data Radio time delay success is now lagging behind optical –Why don’t the radio sources vary? –Many appear to have low-frequency turnovers –How can the radio community deliver more time delays?