Accession Number N20130009623
Title Haystack Observatory VLBI Correlator.
Publication Date Jun 2012
Media Count 4p
Personal Author A. Niell A. Whitney B. Corey K. Dudevoir M. Titus R. Cappallo
Abstract This report summarizes the activities of the Haystack Correlator during 2011. Highlights include acquisition of new hardware for a DiFX cluster, development and improvement of tools to facilitate DiFX production, more u-VLBI Galactic Center observations, Mark 6 recording system testing, and various other continuing projects. Non-real-time e-VLBI transfers and engineering support of other correlators continued. The Mark IV and DiFX VLBI correlators of the MIT Haystack Observatory, located in Westford, Massachusetts, are supported by the NASA Space Geodesy Program and the National Science Foundation. They are dedicated mainly to the pursuits of the IVS, with a smaller fraction of time allocated to processing radio astronomy observations for the Ultra High Sensitivity VLBI (u-VLBI) project. The Haystack correlators serve as a development system for testing new correlation modes, for hardware improvements such as the Mark 6 system, and in the case of the Mark IV, for diagnosing correlator problems encountered at Haystack and at the identical correlator at the U.S. Naval Observatory. This flexibility is made possible by the presence on-site of the team that designed the Mark IV correlator hardware and software. Some software support is provided to the Max Planck Institute for Radioastronomy (MPI) in Bonn, Germany for DiFX processing of IVS experiments.
Keywords Correlators
Nasa space programs
Radio astronomy
Real time operation
Very long base interferometry

Source Agency National Aeronautics and Space Administration
NTIS Subject Category 55A - Aeronomy
54B - Astronomy & Celestial Mechanics
Corporate Author Massachusetts Inst. of Tech., Cambridge.
Document Type Technical report
Title Note N/A
NTIS Issue Number 1319
Contract Number N/A

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