Pulsar Observations

All special processing required for pulsar observations is supported within the correlator. Details of the available gating and binning options, and their impact on the output data rate, are presented in the pulsar modes and output rate subsections of the DiFX section, respectively.

Connect with NRAO

The National Radio Astronomy Observatory and Green Bank Observatory are facilities of the U.S. National Science Foundation operated under cooperative agreement by Associated Universities, Inc.