Details
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Feature
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Not Assigned
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None
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Data Processing
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-
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3
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3
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3.333
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Team_YANDA
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Sprint 5
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3.6
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Team_YANDA
Description
There is a requirement to form tied-array beams (for pulsar search and timing or VLBI) anywhere in the LOW field of view. Because of ionospheric anisoplanatism, this will require direction-dependent corrections in addition to the standard direction-independent complex gain solutions. At present, only direction-independent calibration against a known global sky model is envisaged.
LEAP (Rioja, Dodson & Franzen 2018; MN 478, 2337) is a method for evaluating delays for a grid of sources across the sky, from which solutions can be interpolated to arbitrary directions and provided to CSP for beam-forming. It is embarrassingly parallel, and therefore has the potential to run on ionospheric variation timescales, at least for compact configurations.
This feature is to evaluate the potential of LEAP for real-time beamforming.