|
Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://www.atnf.csiro.au/vlbi/wiki/index.php?n=LBAOct2010.V316D
Дата изменения: Unknown Дата индексирования: Tue Apr 12 15:02:59 2016 Кодировка: Поисковые слова: http www.astronomy.com |
V316Dv316d
Setup v316d.5cm: nif=2
Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v316/v316d The frequency setup is the same as for the maser observation sections of the v255 experiments. Break down of the schedule1230 - 1245 : Fringe finder 0208-512 1245 - 1901 : Target sources (also one fringe finder at 1755 UT for 15 min) 1901 - 1913 : Fringe finder 0208-512 (Hart joins experiment) 1913 - 2249 : Target sources 2249 - 2300 : Fringe finder 0637-752 Once Hart joins the experiment there are 30 second gaps in the schedule every 15-20 minutes to keep the Mark IV/V system happy. This will have no effect on the LBA telescopes. Comments:Observing comments for each antenna:
Observing LogsParkes onsource flagging Weather |