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information_for_astronomers:user_guide:eb-hsa [2021/08/23 11:03]
ubach
information_for_astronomers:user_guide:eb-hsa [2022/07/20 10:28] (current)
ubach
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 ===== Using Effelsberg as part of the High Sensitivity Array (HSA) ===== ===== Using Effelsberg as part of the High Sensitivity Array (HSA) =====
  
-The Effelsberg 100m radio telescope takes part in observations scheduled as part of the VLBI "High Sensitivity Array" (HSA). These are observations together with the NRAO VLBA and at least 2 of the following additional telescope: Effelsberg 100m, VLA (phased array), GBT, ARECIBO.\\+The Effelsberg 100m radio telescope takes part in observations scheduled as part of the VLBI "High Sensitivity Array" (HSA). These are observations together with the NRAO VLBA and at least 2 of the following additional telescope: Effelsberg 100m, VLA (phased array), GBT.\\
 Effelsberg can be used at the HSA observing frequencies of  1.4/1.6, 5, 8.4, 15, 22 and 43 GHz. All these receivers have dual circular polarization. A 2.3 GHz receiver (RCP only) for geodetic S/X band observations is available as well. One can also propose Eb together with VLBA-only (using the same "​instructions"​) under an older agreement. Effelsberg can be used at the HSA observing frequencies of  1.4/1.6, 5, 8.4, 15, 22 and 43 GHz. All these receivers have dual circular polarization. A 2.3 GHz receiver (RCP only) for geodetic S/X band observations is available as well. One can also propose Eb together with VLBA-only (using the same "​instructions"​) under an older agreement.
  
information_for_astronomers/user_guide/eb-hsa.txt ยท Last modified: 2022/07/20 10:28 by ubach