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: http://www.atnf.csiro.au/vlbi/dokuwiki/doku.php/correlator/records/v277b
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ToO experiment.
ATCA reference station is W104 (CA02).
Correlated with 64 spectral channels per 16 MHz subband, 2s integration, 4 polarizations.
Target source: 1550-5418 (magnetar)
Calibrators: 1531-5108, 1515-5559 (phase-reference calibrator)
Output files:
First observing block: 1400-1710 UT (DOY 57)
Second observing block: 2130-0029 UT
Verified by: Aquib
Date: July 24th, 2009
First observing block:
Ungated pass:
Comments: Similar sort of dip in ATCA baselines as in some previous experiments?
Plots of uncalibrated amplitude and phase against frequency
Comments: A very clear bumpy structure in ATCA baselines, there also seems to be a band inversion?
Plots of uncalibrated amplitude and phase against time
Comments: Ok
Comments: Ok
Comments: Ok
Comments: Ok
Plots of Amplitude and phase against frequency with fringe-fitted solutions applied
Comments: Same features in ATCA baselines as the uncalibrated data
Plots of Amplitude and phase against time with fringe-fitted solutions applied
Comments: Looks Ok
Second observing block:
Ungated pass:
Comments: Same as above
Plots of uncalibrated amplitude and phase against frequency
Comments: Same is above
Plots of uncalibrated amplitude and phase against time
Comments: Ok
Comments: Ok
Comments: Ok
Comments: Ok
Plots of Amplitude and phase against frequency with fringe-fitted solutions applied
Comments: Same as above
Plots of Amplitude and phase against time with fringe-fitted solutions applied
Comments: Looks Ok