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lbaops:lbajun2016:v537b

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v537b

Description Resolving Vela pulsars emission region directly via scintellometry
Antennas Pa-At-Ho-Ti-Mp
Start 177 22:00:00
Stop 178 02:00:00
PI Jean-Pierre Macquart

Setup lba18cm-2p-4IF:

Station Modes Pa At Mp
Channel 1 DAS #1 IFP#1-LO 1634 - 1650 MHz USB RCP
Channel 2 DAS #1 IFP#1-HI 1650 - 1666 MHz USB RCP
Channel 3 DAS #1 IFP#2-LO 1634 - 1650 MHz USB LCP
Channel 4 DAS #1 IFP#2-HI 1650 - 1666 MHz USB LCP
Channel 5 DAS #2 IFP#1-LO 1666 - 1682 MHz USB RCP
Channel 6 DAS #2 IFP#1-HI 1682 - 1698 MHz USB RCP
Channel 7 DAS #2 IFP#2-LO 1666 - 1682 MHz USB LCP
Channel 8 DAS #2 IFP#2-HI 1682 - 1698 MHz USB LCP
DAS 1 Skyfreq 1650 MHz
DAS 2 Skyfreq 1682 MHz
Bandwidth 16 MHz
DAS Mode vsop.pro (telescope)
Station Modes Ho
Channel 1 IFP#1-LO 1634 - 1650 MHz USB RCP
Channel 2 IFP#1-HI 1650 - 1666 MHz USB RCP
Channel 3 IFP#2-LO 1634 - 1650 MHz USB LCP
Channel 4 IFP#2-HI 1650 - 1666 MHz USB LCP
DAS 1 Skyfreq 1650 MHz
Bandwidth 16 MHz
DAS Mode vsop.pro (telescope)
Station Modes Ti
Channel 1 IFP#1-LO 1634 - 1650 MHz USB LCP
Channel 2 IFP#1-HI 1650 - 1666 MHz USB LCP
Channel 3 IFP#2-LO 1666 - 1682 MHz USB LCP
Channel 4 IFP#2-HI 1682 - 1698 MHz USB LCP
DAS 1 Skyfreq 1650 & 1682 MHz
Bandwidth 16 MHz
DAS Mode vsop.pro (telescope)

Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v537/v537b


Comments:

Observing comments for each antenna:

Observing Logs

Weather

Monica log information - EXPERIMENTAL:

lbaops/lbajun2016/v537b.1465885551.txt.gz · Last modified: 2016/06/14 16:25 by vlbi