|File name||Description||Start date, UT range||Polarizations||# subbands (AIPS IFs)||Bandwidth per IF (MHz)||Spectral channels per IF/pol||Corr. int. time (s)|
|V469A.FITS||2012-09-14, 0/19:00:01 - 1/18:59:59||RR||32||8.0 MHz||16||2.0|
General comments: Correlation was done using 8 MHz subbands (use of “zoom bands” smaller than “parent bands” is required when different telescopes record different bandwidths).
Tid recorded an inverted band; the fix to this in correlation means that alternate empty subbands are created (i.e. there are twice as many subbands/AIPS IFs as expected, but only the odd-numbered IFs contain data).
Tid observed with two antennas at the start and end, respectively:
TD = DSS34
TI = DSS45
Ceduna maser/phase stability problem has been fixed!
ATCA has a fairly large delay offset between frequencies (~0.1 mus), but data should be OK after fringe-fitting.
Plots of autocorrelations
Plots of cross-polarization amplitude and phase against frequency (not always available)
Amplitude corrections from ACCOR
Fringe-fit delay solutions
Comments: Strong fringes found to all 10 stations in all bands recorded.
Fringe-fit phase solutions
Fringe-fit rate solutions