Presentation by Karl Menten - aerap

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e-VLBI• connects VLBI radio telescopes in realtime,while still employing the local timereferences of the VLBI technique.• Gigabit per second links via• their National Research Networksand• the Pan-European researchnetwork GEANT2IRC+10420
Modern VLBI requires:• Broad receiver bandwidths. Gives:• Good continuum sensitivity• Frequency agility (e.g, for redshiftedspectral line)• Fast switching• A dedicated network, allowing repeatedobservations• Broad bandwidth connectivity• Appreciable collecting area• A really good science case!
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 9 and 10: VLBI Trigonometric Parallaxesradio
Page 11: K-band image©M. McCaughrean
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)

Presentation by Karl Menten - aerap

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