SWIN files contain the VLBI fringe visibilities of an observing session (24 hours long or 1 hour long). The files are created by International VLBI Service (IVS) correlation centers and constitute the raw correlator output of the Distributed FX-style (DiFX) software correlator. These data form the basis for the fringe fitting process and can also be used to make source maps of the observed quasars.
|Temporal Extent:||Platform(s):||GROUND-BASED OBSERVATIONS|
|Data Center(s):||NASA/GSFC/SED/ESD/GGL/CDDIS||Instrument(s):||VLBI Station|
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