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lbaops:lbamarch2005:v162d1 [2005/03/05 21:46]
chris.phillips
lbaops:lbamarch2005:v162d1 [2015/12/18 16:38] (current)
Line 1: Line 1:
-===== v162d1 Setup:\\ =====+===== v162d1 Setup: ===== 
 + 
 +^Antennas ​          | Mp-At-Ho-Pa-Ti | 
 +^Start ​             | 71 07:​00:​00 ​  | 
 +^Stop               | 71 13:​50:​00 ​  | 
 +^Channel 1          | 1634 - 1650 MHz USB LCP  | 
 +^Channel 2          | 1650 - 1666 MHz USB LCP  | 
 +^Bandwidth ​         | 16 MHz         | 
 +^Recorder ​          | S2             | 
 +^S2 Mode            | 32x4-2 ​        | 
 +^DAS Mode           | vsop.pro ​     | 
 +^Buggary Cable      | out             | 
 +^Tape Change ​       | 71 10:​01:​00 ​  | 
 + 
 +---- 
 + 
 +===== Comments: ===== 
 +Dodson 
 + 
 +CJP: Note early tape change time!!!!! 
 +  
 +RGD: Therefore one can use old tapes with tape density "​lp"​ (as opposed to "​slp"​). The tape lengths required are 3 hours and 4 hours. Not sure if this is a consideration anymore? 
 + 
 +This experiment observes PSR 1048-5832 so I will need to generate a polyco fit. However the recent solutions are really poor. So PKS will need to collect the timing data to generate a new timing solution. 
 + 
 + 
 +Emailed comments (repeating stuff): 
 + 
 +Files at ftp://​ftp.atnf.csiro.au/​pub/​people/​vlbi/​v162/​v162d1 (NOT INCOMING!!!) 
 + 
 +  Exp. Code:  v162d1 
 + 
 +   ​Notes: ​   PSR B1046-58 observation No 4. 
 +            7 hrs & 2 tape set 
 +            position & pulsar bin from ATCA obs 
 +            standard freq & setup 
 + 
 + 
 +  L hand polarisation (to match Tid) only.  
 +    
 +  The experiment is short (~ 7 hours) so two sets of tapes are needed 
 +but they can be the old 4 hour tapes (if there are any still). 
 +  Tape change is at ~10UT  
 + 
 +  ATCA has a pulsar polyco -- but I think it is duff (it has glitched I 
 +think and there have not been enough observations to solve the current 
 +fit).  
 + 
 +  So Parkes will have to collect the filter bank so we can find the 
 +solution. 
 + 
 +  Parkes also has a rest after the fringe finder (7UT to 7:15UT) till 
 +8:05UT. 
 +   
 +  No Ceduna
  
-^Antennas ​          | Mp-At-Ho-Pa-Ti |\\ 
-^Start ​             | 71 07:​00:​00 ​  |\\ 
-^Stop               | 71 13:​50:​00 ​  |\\ 
-^Channel 1          | 1634 - 1650 MHz USB LCP  |\\ 
-^Channel 2          | 1650 - 1666 MHz USB LCP  |\\ 
-^Bandwidth ​         | 16 MHz         |\\ 
-^Recorder ​          | S2             |\\ 
-^S2 Mode            | 32x4-2 ​        |\\ 
-^DAS Mode           | vsop.pro ​     |\\ 
-^Buggary Cable      | out             |\\ 
-^Tape Change ​       | 71 10:​01:​00 ​  |\\ 
-\\ 
-----\\ 
-\\ 
-===== Comments:\\ ===== 
-Dodson\\ 
-\\ 
-CJP: Note early tape change time!!!!!\\ 
- \\ 
-RGD: Therefore one can use old tapes with tape density "​lp"​ (as opposed to "​slp"​). The tape lengths required are 3 hours and 4 hours. Not sure if this is a consideration anymore?\\ 
-\\ 
-This experiment observes PSR 1048-5832 so I will need to generate a polyco fit. However the recent solutions are really poor. So PKS will need to collect the timing data to generate a new timing solution.\ 
lbaops/lbamarch2005/v162d1.txt · Last modified: 2015/12/18 16:38 (external edit)