Expanding New Zealand VLBI capability and the 30m dish

aut.researcherWeston, Stuart
dc.contributor.authorWeston, S
dc.date.accessioned2014-11-23T22:17:52Z
dc.date.available2014-11-23T22:17:52Z
dc.date.copyright2014-11-13
dc.date.issued2014-11-13
dc.description.abstractWe describe our current VLBI activities with the 12m dish; but also with the conversion of a former 100-foot (30-m) telecommunication antenna in New Zealand into a radio telescope show the future capabilities. Provide a brief of the specifications of the 30m and describe the telescope control system, telescope networking for VLBI, and telescope maintenance. Plans for RF, front-end and back-end developments based on radio astronomical and VLBI priorities will be outlined.
dc.identifier.citationThe Third International VLBI Technology Workshop held at Dwingeloo, where the headquarters of JIVE and its host insitute ASTRON are located, Groningen, Netherlands, 2014-11-10 to 2014-11-13
dc.identifier.urihttps://hdl.handle.net/10292/7971
dc.publisherJoint Institute for VLBI in Europe (JIVE)
dc.relation.urihttp://www.jive.nl/jivewiki/doku.php?id=various:t3rdivtw_presentations
dc.rightsExcept where otherwise noted, content on this wiki is licensed under the following license: CC Attribution-Share Alike 3.0 Unported.
dc.rights.accessrightsOpenAccess
dc.titleExpanding New Zealand VLBI capability and the 30m dish
dc.typeConference Contribution
pubs.elements-id173438
pubs.organisational-data/AUT
pubs.organisational-data/AUT/Design & Creative Technologies
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