Correlated with 64 spectral channels/subband, 2s integration.
Parkes: The main clock computer got stuck at 01:10UT halting the telescope, it came back into operation at 01:45UT
ATCA: CAOBS died 05:00-05:10.
Tied antennas 4-5 only until UT 0905. Then tied 1,3,4,5 and ran continuous CACAL for phase (changed local schedule to flag all sources as calibrators).
May need to flag ~1 minute of data at beginning of each scan (while CACAL adjusts phase).
Examine ATCA amplitudes
Output file: v252g.rpf (converted to v252g.uvfits at PI request)
ATCA reference: CA04 on pad W104
Correlation: 64 spectral points/IF, 1s integration, compute cross pols
Ceduna and Hobart record first two freq bands only.
Output file: v257a.rpf
Data verified by: Jeff Hodgson
Plots of the autocorrelations
Plots of the uncalibrated amplitude and phase against time
Plots of the uncalibrated amplitude and phase against frequency
Fringe-fit phase solutions
Fringe-fit delay solutions
Fringe-fit rate solutions
Amplitude and phase against time with fringe-fit solutions applied
Amplitude and phase against frequency with fringe-fit solutions applied