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APP2 Status Summary: Proposed New VLBI Capabilities for Cycle 8

Author(s)
Matthews, Lynn D.; Crew, Geoffrey B.
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DownloadAPP2_Review_Nov2019_compwabs.pdf (3.323Mb)
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Abstract
This document contains material regarding the new capabilities proposed for ALMA Cycle 8. These included a passive phasing mode (for weaker sources), an ALMA Band 3 pulsar observing mode, a prototype spectral line mode, also for Band 3, and minor improvements to the code for operational reasons. In the event, the first two were accepted for a Cycle 8 that was delayed by the COVID-19 pandemic. The spectral line capability was deferred until Cycle 9. In response to reviewer questions, a modified figure was prepared and presented as an addendum. Both documents are presented here as a single PDF.
Description
This report was prepared for the formal acceptance of the software required for Cycle 8. Notionally it is ALMA Technical Note #21, but not (yet) published as such.
Date issued
2019-11-21
URI
https://hdl.handle.net/1721.1/164885
Keywords
Radio Astronomy, ALMA Observatory, Very Long Baseline Interferometry

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