vt001i DOY 322, 64 MHz test for disk-based recording systems
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From: <stingay_at_email.protected>
Date: Mon, 8 Nov 2004 12:37:08 +1100 (EST)
Dear All,
The schedules for vt001i can be found at:
ftp://ftp.atnf.csiro.au/pub/people/vlbi/vt001/vt001i
ATCA: vt001i_At.com (command file for AT sched)
MOPRA: vt001i_Mp.com (command file for AT sched)
Parkes: vt001i.psn
Ceduna: VEX file vt001i.skd appropriate for making schedule
The centre frequency for the observation is 6500 MHz. This experiment
will attempt to use the BG3 cables produced in Hobart to obtain dual
polarisation 64 MHz data from the DAS at each telescope, giving a data
rate of 512 Mbps recorded to disk.
The bands will be 6468 - 6532 MHz.
We will have to distribute the appropriate DAS profile for this test
sometime in the next week. Or instructions on manual setup of the DAS.
The source we will track is 2255-282.
More details in the lead-up to the observation......
Cheers, Steven
##=====================================================##
Dr Steven Tingay stingay_at_astro.swin.edu.au
Swinburne SKA Project Leader
Centre for Astrophysics and Supercomputing
Swinburne University of Technology
Mail No 31
P.O. Box 218, Hawthorn, Vic. 3122, Australia
ph: +61 3 9214 8758
fax: +61 3 9214 8797
http://astronomy.swin.edu.au/ska
##=====================================================##
Received on 2004-11-08 12:37:29
Date: Mon, 8 Nov 2004 12:37:08 +1100 (EST)
Dear All,
The schedules for vt001i can be found at:
ftp://ftp.atnf.csiro.au/pub/people/vlbi/vt001/vt001i
ATCA: vt001i_At.com (command file for AT sched)
MOPRA: vt001i_Mp.com (command file for AT sched)
Parkes: vt001i.psn
Ceduna: VEX file vt001i.skd appropriate for making schedule
The centre frequency for the observation is 6500 MHz. This experiment
will attempt to use the BG3 cables produced in Hobart to obtain dual
polarisation 64 MHz data from the DAS at each telescope, giving a data
rate of 512 Mbps recorded to disk.
The bands will be 6468 - 6532 MHz.
We will have to distribute the appropriate DAS profile for this test
sometime in the next week. Or instructions on manual setup of the DAS.
The source we will track is 2255-282.
More details in the lead-up to the observation......
Cheers, Steven
##=====================================================##
Dr Steven Tingay stingay_at_astro.swin.edu.au
Swinburne SKA Project Leader
Centre for Astrophysics and Supercomputing
Swinburne University of Technology
Mail No 31
P.O. Box 218, Hawthorn, Vic. 3122, Australia
ph: +61 3 9214 8758
fax: +61 3 9214 8797
http://astronomy.swin.edu.au/ska
##=====================================================##
Received on 2004-11-08 12:37:29