Presentation by Karl Menten - aerap

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VLBI from the mid1960s on: ActiveGalactic Nucleiand their jets3C279v ~ 3.5 cA. Wehrle

Presentation on the GO-SKA project by Viola Tegethoff - aerap

VLBI Sources must have non-thermalradio emission• Active Galactic Nuclei• Radio “active” stars• Cosmic masersMicrowaveAmplification <strong>by</strong>StimulatedEmission ofRadiationWehrle et al. 1998

VLBI from the mid1960s on: ActiveGalactic Nucleiand their jets3C279v ~ 3.5 cA. Wehrle

Page 1: VLBI Today - Science andTechnical I
Page 6: MERLINRedshift 0.88582 absorption i
Page 9 and 10: VLBI Trigonometric Parallaxesradio
Page 16 and 17: GLOSTAR: A Global View of Star Form
Page 18 and 19: Inner Perseus Arm (Zhang et al. 201
Page 21 and 22: Cape VerdeanIslandsMauritius
Page 23 and 24: European VLBI Network
Page 25 and 26: VERAhttp://veraserver.mtk.nao.ac.jp
Page 27 and 28: Global VLBI Network
Page 29 and 30: The Very Long Baseline Array (VLBA)
Page 32 and 33: e-VLBI• connects VLBI radio teles

Presentation by Karl Menten - aerap

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