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lbaops:lbadec2009:v316b [2005/04/07 08:23]
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lbaops:lbadec2009:v316b [2015/12/18 16:38] (current)
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 ===== Comments: ===== ===== Comments: =====
 +
 +The purpose of these observations is to obtain the final epoch for proper motion observations of IRAS05011-6815 strongest methanol maser in the LMC.  Previous observations were made under the (now lapsed) v135 experiment code.  We are using the same observing mode as the v255 experiments,​ although there are no setup changes required for this experiment. ​ The maser has a peak flux density of about 3.5 Jy and should be at a frequency of 6662.49 MHz, but probably wont be visible online (except perhaps at Parkes and the ATCA).
  
 ===== Observing comments for each antenna: ===== ===== Observing comments for each antenna: =====
 +
 +==== Hobart, Ceduna :  ====
 +
 +The setup requires only a single LO split and feed into IFP#1 and #2 on the DAS/​frequency translator. For Hobart the LO should be set to 810 MHz (as for the higher frequency band for the v255h). ​ For Ceduna, if you set the agilent to 11.1 GHz rather than 11.4 GHz, then you can use the same LO as at Hobart.
 +
 +==== Parkes, ATCA, Mopra :  ====
 +
 +Parkes and ATCA install "​straight through"​ cables from pkvsi1/2 to the two DAS. You will need to reinstall the Huygens cable before v289s. ATCA will record F2/DAS2 onto cavsi1. Parkes tune DAS1 to 6658  MHz and DAS2 to 6316.
 +
 +====  ATNF recording ====
 +
 +|       ^ Recorder ^ Remote Host ^ TCP Window ^ Port |
 +| Mopra | mpvsi2 | local |  |  |
 +| ATCA | cavsi1 | local |   ​| ​  |
 +| Parkes | pkvsi1 | local |  |  |
 +
  
 | [[.:​v316batlog | At]] | [[.:​v316bcdlog | Cd]] | [[.:​v316bholog | Ho]] | [[.:​v316bmplog | Mp]] | [[.:​v316bpalog | Pa]] | | [[.:​v316batlog | At]] | [[.:​v316bcdlog | Cd]] | [[.:​v316bholog | Ho]] | [[.:​v316bmplog | Mp]] | [[.:​v316bpalog | Pa]] |
lbaops/lbadec2009/v316b.txt · Last modified: 2015/12/18 16:38 (external edit)