Presentation by Karl Menten - aerap

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Phase referencingTargetsourcea fewdegreesBackgroundquasarVLBA: Switch every 15second between maserand quasar. 50% duty cycle•• Allows imaging of weaksources• Provides excellentastrometric accuracy(down to 10 µarcsec)

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

VLBI Trigonometric Parallaxesradio sourcehttp://veraserver.mtk.nao.ac.jp/outline/vera2-e.html

Page 1 and 2: VLBI Today - Science andTechnical I
Page 3: VLBI from the mid1960s on: ActiveGa
Page 6: MERLINRedshift 0.88582 absorption i
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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