BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:Gravitational Redshift Experiment with RadioAstron DTSTART;VALUE=DATE-TIME:20150617T081500Z DTEND;VALUE=DATE-TIME:20150617T083000Z DTSTAMP;VALUE=DATE-TIME:20260307T235712Z UID:indico-contribution-7-1@cern.ch DESCRIPTION:Speakers: Prof. BARTEL\, Norbert (York University)\nRadioAstro n on its eccentric orbit around Earth allows a unique test of the gravitat ional redshift predicted by general relativity. Large gravitational potent ial variations cause large variations of the on-board hydrogen maser clock rate\, which can be detected with ground radio telescopes. We report on r ecent results and possible improvements.\n\nhttps://events.mpifr-bonn.mpg. de/indico/event/7/session/0/contribution/1 LOCATION:Max-Planck-Institut für Radioastronomie 0.02 URL:https://events.mpifr-bonn.mpg.de/indico/event/7/session/0/contribution /1 END:VEVENT BEGIN:VEVENT SUMMARY:Introduction to RadioAstron DTSTART;VALUE=DATE-TIME:20150617T080000Z DTEND;VALUE=DATE-TIME:20150617T081500Z DTSTAMP;VALUE=DATE-TIME:20260307T235712Z UID:indico-contribution-7-0@cern.ch DESCRIPTION:Speakers: Prof. KARDASHEV\, Nikolay (Astro Space Center\, Lebe dev Physical Institue (ASC LPI))\, Dr. KOVALEV\, Yuri (Astro Space Center of Lebedev Physical Institute)\nhttps://events.mpifr-bonn.mpg.de/indico/ev ent/7/session/0/contribution/0 LOCATION:Max-Planck-Institut für Radioastronomie 0.02 URL:https://events.mpifr-bonn.mpg.de/indico/event/7/session/0/contribution /0 END:VEVENT BEGIN:VEVENT SUMMARY:Compact structures in cosmic masers DTSTART;VALUE=DATE-TIME:20150617T084500Z DTEND;VALUE=DATE-TIME:20150617T090000Z DTSTAMP;VALUE=DATE-TIME:20260307T235712Z UID:indico-contribution-7-3@cern.ch DESCRIPTION:Speakers: Dr. ALAKOZ\, Alexey (ASC LPI)\nThe first time space- VLBI detections of water maser emission have been obtained for the Megamas er galaxy NGC 4258 and several Galactic star-forming regions. In W3 IRS5 fringes were successfully detected on baselines of up to 6 Earth Diameter s delivering a record angular resolution of 36 microarcseconds. Linear re solution of better than 4 million kilometers has been achieved in observat ions of the water maser in Orion.\n\nhttps://events.mpifr-bonn.mpg.de/indi co/event/7/session/0/contribution/3 LOCATION:Max-Planck-Institut für Radioastronomie 0.02 URL:https://events.mpifr-bonn.mpg.de/indico/event/7/session/0/contribution /3 END:VEVENT BEGIN:VEVENT SUMMARY:Pulsars & Interstellar Scattering Results DTSTART;VALUE=DATE-TIME:20150617T083000Z DTEND;VALUE=DATE-TIME:20150617T084500Z DTSTAMP;VALUE=DATE-TIME:20260307T235712Z UID:indico-contribution-7-2@cern.ch DESCRIPTION:Speakers: Prof. GWINN\, Carl (Univ California\, Santa Barbara) \nhttps://events.mpifr-bonn.mpg.de/indico/event/7/session/0/contribution/2 LOCATION:Max-Planck-Institut für Radioastronomie 0.02 URL:https://events.mpifr-bonn.mpg.de/indico/event/7/session/0/contribution /2 END:VEVENT BEGIN:VEVENT SUMMARY:RadioAstron Nearby AGN Key Science Program DTSTART;VALUE=DATE-TIME:20150617T091500Z DTEND;VALUE=DATE-TIME:20150617T093000Z DTSTAMP;VALUE=DATE-TIME:20260307T235712Z UID:indico-contribution-7-5@cern.ch DESCRIPTION:Speakers: Prof. GIOVANNINI\, Gabriele (Bologna University and IRA/INAF)\nI will present preliminary results on the RadioAstron observati ons of three nearby AGN. Images at 5 and 22 GHz of 3C84 are available and will be presented and shortly discussed in comparison with ground VLBI res ults. We obtained high resolution images (about 50 micro-arcsec) showing a complex nuclear structure\, and a limb-brighted jet with a possible shor t counter-jet structure.\n\nhttps://events.mpifr-bonn.mpg.de/indico/event/ 7/session/0/contribution/5 LOCATION:Max-Planck-Institut für Radioastronomie 0.02 URL:https://events.mpifr-bonn.mpg.de/indico/event/7/session/0/contribution /5 END:VEVENT BEGIN:VEVENT SUMMARY:RadioAstron AGN Survey DTSTART;VALUE=DATE-TIME:20150617T090000Z DTEND;VALUE=DATE-TIME:20150617T091500Z DTSTAMP;VALUE=DATE-TIME:20260307T235712Z UID:indico-contribution-7-4@cern.ch DESCRIPTION:Speakers: Dr. KOVALEV\, Yuri (Astro Space Center of Lebedev Ph ysical Institute)\nhttps://events.mpifr-bonn.mpg.de/indico/event/7/session /0/contribution/4 LOCATION:Max-Planck-Institut für Radioastronomie 0.02 URL:https://events.mpifr-bonn.mpg.de/indico/event/7/session/0/contribution /4 END:VEVENT BEGIN:VEVENT SUMMARY:RadioAstron Strong AGN Key Science Program DTSTART;VALUE=DATE-TIME:20150617T094500Z DTEND;VALUE=DATE-TIME:20150617T100000Z DTSTAMP;VALUE=DATE-TIME:20260307T235712Z UID:indico-contribution-7-7@cern.ch DESCRIPTION:Speakers: LOBANOV\, Andrei ()\nhttps://events.mpifr-bonn.mpg.d e/indico/event/7/session/0/contribution/7 LOCATION:Max-Planck-Institut für Radioastronomie 0.02 URL:https://events.mpifr-bonn.mpg.de/indico/event/7/session/0/contribution /7 END:VEVENT BEGIN:VEVENT SUMMARY:Probing the innermost regions of AGN jets and their magnetic field s with RadioAstron DTSTART;VALUE=DATE-TIME:20150617T093000Z DTEND;VALUE=DATE-TIME:20150617T094500Z DTSTAMP;VALUE=DATE-TIME:20260307T235712Z UID:indico-contribution-7-6@cern.ch DESCRIPTION:Speakers: Dr. GÓMEZ\, Jose L. (Instituto de Astrofísica de A ndalucía - CSIC)\nWe present an update of the results from our RadioAstro n Key Science Project on polarization. These include successful polarizati on observations of BL Lac at 18 and 1.3 cm with ground-space fringe detect ions up to a projected baseline distance of 7.9 Earth diameters in length\ , revealing the innermost magnetic field structure with an angular resolut ion of 21 microarcseconds\, the highest achieved to date.\n\nhttps://event s.mpifr-bonn.mpg.de/indico/event/7/session/0/contribution/6 LOCATION:Max-Planck-Institut für Radioastronomie 0.02 URL:https://events.mpifr-bonn.mpg.de/indico/event/7/session/0/contribution /6 END:VEVENT END:VCALENDAR