8thEVN - (other evn conferences)
September 26-29, 2006
Torun, Poland
published November 22, 2007
Torun, Poland
published November 22, 2007
This is the eighth in a series of biennial European VLBI Network (EVN)
Symposia devoted to reviewing new developments in Very Long Baseline
Interferometry (VLBI) science and technology. VLBI provides astronomers
with their sharpest view of the most energetic phenomena in the universe,
including expanding supernovae, pulsars, flare stars, star-forming regions
in molecular clouds, the environment surrounding nearby and distant
galaxies, gravitational lenses, starburst galaxies and distant active
galactic nuclei. The EVN is an interferometric array of radio telescopes spread throughout Europe and beyond, which conducts unique, high resolution, radio astronomical observations of cosmic radio sources; it often observes with other radio telescopes around the world making VLBI a truly global endeavour. The EVN is the most sensitive VLBI array in the world, thanks to the collection of extremely large telescopes that contribute to the network. After the first successes in real-time VLBI (e-VLBI), the EVN continues to make rapid progress in this and other areas of VLBI technological development. Among others, the results obtained using the e-VLBI state-of-the-art technique have been presented.
Editorial Board
Baan Willem, Bachiller Rafael, Booth Roy, Charlot Patrick, Diamond Phil, Garrett Mike, Hong Xiaoyu, Jonas Justin, Kus Andrzej, Mantovani Franco, Marecki Andrzej (chairman), Olofsson Hans, Schlueter Wolfgang, Tornikoski Merja, Wang Na, Zensus Anton
| VLBI Surveys |
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VLBI surveys
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VLBI at the highest frequencies - AGN studied with micro-arcsecond resolution
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Compact radio jets and nuclear regions in active galaxies
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| VLBI at high frequencies |
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A global 86-GHz VLBI survey of compact radio sources
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Deep, wide-field global VLBI observations of the HDF-N
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“Oscillating” components in the BL Lac object 0716+714?
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The kinematics of S5 1803+784
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Effects of the turbulent ISM on radio observations of quasars
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Intraday variability of AGNs in the southern hemisphere: the strange case of PMN J1326-5256
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VLBA observations of Intraday Variable Sources
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| VLBI polarisation studies |
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The compact polarised emission of AGN - do many AGN jets have helical magnetic fields?
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Searching for helical magnetic fields in BL Lac objects
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Kinematic studies of the IDV quasar 0917+624
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Using Faraday rotation sign-reversals to study magnetic fields in AGN jets
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Imaging of quasars and active galactic nuclei. Fine-scale structure evolution
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Constraining IMBH black hole masses with VLBI
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e-VLBI observations of a microquasar in outburst
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| CSS and GPS radio sources |
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Compact Steep Spectrum and GHz-Peaked Spectrum radio sources
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Multi-frequency radio observations of BAL quasar 1045+352
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Multi-frequency VSOP and VLBI observations of the quasar 3C309.1
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Low-luminosity radio-loud active galactic nuclei
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Low-power compact radio galaxies at high angular resolution
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| BL Lac objects |
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Towards a kinematic model of the Local Group
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BL Lac objects
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EVN & MERLIN studies of a new sample of BL Lac objects
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Multi-wavelength polarization VLBI observations of two BL Lac objects
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Rapid and correlated variability of blazar S5 0716+71 from radio- to sub-mm bands
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| Gravitational lensing |
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Gravitational lensing
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Multi-frequency VLBI observations of the gravitational lens B2016+112
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| Starburst galaxies |
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Starburst galaxies
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Supernova remnants in the central starburst region of M82
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Multiwavelength radio observations of the compact starburst in Arp 220
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| Megamasers and young stellar masers |
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Megamasers
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Molecular tori in AGN: a search using excited states of OH
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The role of magneticfieldsin massive star-formation
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EVN imaging of methanol masers towards massive protostars
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Water masers in NGC7538 region
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Parallax measurements of water maser sources beyond 5 kpc with VERA
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| Old stellar masers |
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Beaming in on some stimulating issues in stellar evolution
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The magnetically collimated jet of the evolved star W43A
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Spatio-kinematics and distance of water masers in the pre-planetary nebula IRAS 19134+2131
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OH26.5+0.6: insight into the circumstellar structure of an extreme OH/IR star
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EVN observations of OH maser burst in OH17.7-2.0
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Circumstellar SiO masers in the long-period variable star TXCam
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| Active stars |
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Winds in collision: high energy particles in massive binary systems
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Parallax measurements of the Mira-type star UX Cygni with phase-referenced VLBI
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Radio supernovae
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The 2006 explosion of the recurrent nova RS Ophiuchi
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| Recent e-EVN developments |
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Recent e-EVN developments
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Developments at the EVN MkIV data processor at JIVE
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Data processing software for radio astronomy
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On-demand radio imaging: access to calibrated data for all astronomers
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| VLBI hard- and software developments |
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The Swinburne distributed FX (DiFX) software correlator for astronomical and geodetic VLBI
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Phase correction of VLBI with water vapour radiometry
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VLBI observations of spacecraft
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The Long Wavelength Array
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Recent progress in Korean VLBI Network (KVN) project
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| Posters |
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Prospects for Weak Lensing surveys with next-generation arrays
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Main line OH masers in M82
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AU-scale collimation of protostellar outflows from water masers
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Analysing very large datasets with ParselTongue
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Maser observation in VY CMa with VERA
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VLBI data record/playback systems and correlators for Radioastron project
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EXPReS SA2: Network provision for a global e-VLBI array
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The VSOP Survey: Final individual results
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Japanese VLBI Network
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Comparing the SDSS and VLBI quasar and galaxy positions
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Millimeter VLBI detection of the TeV blazar Markarian 501
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EVN and MERLIN observations of nearby BL Lac objects and multiwavelength analysis
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Water masers in the star forming region in L1287
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Phase-delay astrometry of the polar-cap sample at 43 GHz
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Living life on the edge - wide-field VLBI at 90 cm!
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VLBI observations of blazar 0716+714 during the outburst in spring 2004
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Results from e-EVN observations of GRS 1915+105
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Description of moving plasma blob
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VSOP and VLBA Observations of EGRET-Identified Active Galactic Nuclei
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Dual-frequency VSOP imaging of a high-redshift radio quasar PKS 1402+044
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