User Tools

Site Tools


correlator:records:v191b

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
correlator:records:v191b [2009/04/11 16:09]
chotan
correlator:records:v191b [2014/11/11 18:08] (current)
Line 28: Line 28:
 **Output files:** **Output files:**
  
-[[ftp://​cira.ivec.org/​v191b/​v191b.DTSUM.txt|Brief data summary]]+[[http://​cira.ivec.org/pipeline/​v191b/​v191b.DTSUM.txt|Brief data summary]]
  
-[[ftp://​cira.ivec.org/​v191b/​v191b.SCAN.txt|Scan listing]]+[[http://​cira.ivec.org/pipeline/​v191b/​v191b.SCAN.txt|Scan listing]]
  
-[[ftp://​cira.ivec.org/​v191b/​v191b_POSSM_AUTOCORR.pdf|Plots of the autocorrelations]]\\+[[http://​cira.ivec.org/pipeline/​v191b/​v191b_POSSM_AUTOCORR.pdf|Plots of the autocorrelations]]\\
 **Comments:​** Hobart bandpasses exhibit apparent severe interference - strangely peaked autocorrelations,​ particularly in LHC.\\ **Comments:​** Hobart bandpasses exhibit apparent severe interference - strangely peaked autocorrelations,​ particularly in LHC.\\
 ATCA known spikes at band edges (tied array?).\\ ATCA known spikes at band edges (tied array?).\\
 Ceduna bandpasses not always flat. Ceduna bandpasses not always flat.
  
-[[ftp://​cira.ivec.org/​v191b/​v191b_VPLOT_UNCAL.pdf|Plots of the uncalibrated amplitude and phase against time]]\\+[[http://​cira.ivec.org/pipeline/​v191b/​v191b_VPLOT_UNCAL.pdf|Plots of the uncalibrated amplitude and phase against time]]\\
 **Comments:​** From VPLOT uncalibrated plots we see CA is off-source for a short time at the start of the experiment, Hobart takes longer to come on (Mopra may be slow too). Ceduna data is no good for almost half the experiment. Parkes comes online late but the source (and most calibrators) set very early. **Comments:​** From VPLOT uncalibrated plots we see CA is off-source for a short time at the start of the experiment, Hobart takes longer to come on (Mopra may be slow too). Ceduna data is no good for almost half the experiment. Parkes comes online late but the source (and most calibrators) set very early.
  
-[[ftp://​cira.ivec.org/​v191b/​v191b_POSSM_UNCAL.pdf|Plots of the uncalibrated amplitude and phase against frequency]]\\+[[http://​cira.ivec.org/pipeline/​v191b/​v191b_POSSM_UNCAL.pdf|Plots of the uncalibrated amplitude and phase against frequency]]\\
 **Comments:​** As expected then, POSSM uncalibrated plots show lots of rubbish to Ceduna and Parkes, Ceduna more or less throughout the entire experiment. **Comments:​** As expected then, POSSM uncalibrated plots show lots of rubbish to Ceduna and Parkes, Ceduna more or less throughout the entire experiment.
  
-[[ftp://​cira.ivec.org/​v191b/​v191b_FRING_DELAY2.pdf|Fringe-fit delay solutions]]\\+[[http://​cira.ivec.org/pipeline/​v191b/​v191b_FRING_DELAY2.pdf|Fringe-fit delay solutions]]\\
 **Comments:​** Sorry the first page is in landscape while the rest are portrait. I don't know why.\\ **Comments:​** Sorry the first page is in landscape while the rest are portrait. I don't know why.\\
 Note output\\ Note output\\
Line 49: Line 49:
 CUPPA0> FRING2: Failed on      336 solutions CUPPA0> FRING2: Failed on      336 solutions
  
-[[ftp://​cira.ivec.org/​v191b/​v191b_FRING_PHASE.pdf|Fringe-fit phase solutions]]\\ +[[http://​cira.ivec.org/pipeline/​v191b/​v191b_FRING_PHASE.pdf|Fringe-fit phase solutions]]\\ 
-Comments:+**Comments:** Ceduna looks a bit rubbish here again.
  
-[[ftp://​cira.ivec.org/​v191b/​v191b_FRING_RATE.pdf|Fringe-fit rate solutions]]\\ +[[http://​cira.ivec.org/pipeline/​v191b/​v191b_FRING_RATE.pdf|Fringe-fit rate solutions]]\\
-Comments:+
  
-[[ftp://​cira.ivec.org/​v191b/​v191b_VPLOT_FRING.pdf|Amplitude and phase against time with fringe-fit solutions applied]]\\ +[[http://​cira.ivec.org/pipeline/​v191b/​v191b_VPLOT_FRING.pdf|Amplitude and phase against time with fringe-fit solutions applied]]\\
-Comments:+
  
-[[ftp://​cira.ivec.org/​v191b/​v191b_POSSM_FRING.pdf|Amplitude and phase against frequency with fringe-fit solutions applied]]\\+[[http://​cira.ivec.org/pipeline/​v191b/​v191b_POSSM_FRING.pdf|Amplitude and phase against frequency with fringe-fit solutions applied]]\\
 **Comments:​** Note the scale on phase here is reduced, so apparent variability is typically small, not as significant as it first appears!\\ **Comments:​** Note the scale on phase here is reduced, so apparent variability is typically small, not as significant as it first appears!\\
 Remember we are interested in phase connection in the LL and RR bands, not cross-pols, so the not-rubbish data here all appears fine. Remember we are interested in phase connection in the LL and RR bands, not cross-pols, so the not-rubbish data here all appears fine.
  
correlator/records/v191b.txt · Last modified: 2014/11/11 18:08 (external edit)