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lbaops:lbajun2007:v235a

v235a Setup:

Description The search for superluminal motion in the nearby proto-quasar candidate
Antennas At-Mp-Pa-Ho-Cd-Ti-Hh
Start 174 06:00:00
Stop 174 18:00:00
PI Morganti
Channel 1 DAS #1 IFP#1-LO 2268 - 2284 MHz USB RCP
Channel 2 DAS #1 IFP#1-HI 2284 - 2300 MHz USB RCP
Channel 3 DAS #1 IFP#2-LO 2268 - 2284 MHz USB LCP
Channel 4 DAS #1 IFP#2-HI 2284 - 2300 MHz USB LCP
Channel 5 DAS #2 IFP#1-LO 2300 - 2316 MHz USB RCP
Channel 6 DAS #2 IFP#1-HI 2316 - 2332 MHz USB RCP
Channel 7 DAS #2 IFP#2-LO 2300 - 2316 MHz USB LCP
Channel 8 DAS #2 IFP#2-HI 2316 - 2332 MHz USB LCP
DAS 1 Skyfreq 2284.00 MHz
DAS 2 Skyfreq 2316.00 MHz
Bandwidth 16 MHz
DAS Mode vsop.pro (telescope)

Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v235/v235a


Comments:

Schedule has changed from original (CJP 20 June 08:00 UT)

Please note disks recorded in observatory links below

Parkes, Mopra, ATCA

  • Connect DAS to VSIC using “Huygens” Cable
  • Both DAS units are used to give 2 x 256 Mbps = 512 Mbps recording over 8 x 16 MHz channels

Hobart, Ceduna

  • Connect DAS directly to VSIC
  • One DAS unit is used to give 1 x 256 Mbps recording over 4 x 16 MHz channels.
  • Recorded data will match the frequencies/polarisations listed in the table for DAS1.

Tibinbilla

  • Connect DAS directly to VSIC
  • One DAS unit is used to give 1 x 256 Mbps recording over 4 x 16 MHz channels.
  • Record frequencies listed at RCP for both DAS1 and DAS2 in the table above.

Tibdinbilla uses a different setup compared to Hobart and Ceduna

Hart

Vex schedule assume you will record all 8 channels

Observing comments for each antenna:

Observing Logs

lbaops/lbajun2007/v235a.txt · Last modified: 2015/12/18 16:38 (external edit)