June 2012 B-configuration

Each link in the list below presents scalar-averaged cross correlation spectra using several baselines in the B-configuration for each respective receiver band obtained in June 2012. The channel separation is 125 kHz. Hanning smoothing has been applied to minimize Gibbs ringing. The scale is logarithmic with arbitrary offset. The scale can be roughly calibrated by noting that the mean power level is roughly equal to the antenna SEFD in Jy. There is no bandpass calibration, so the downturns at the edges are due to the analog and/or digital filters. All plots are from the RCP correlation - the LCP looks very similar.

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.