vt01i1 schedules
- Contemporary messages sorted: [ by date ] [ by thread ] [ by subject ] [ by author ] [ by messages with attachments ]
From: <stingay_at_email.protected>
Date: Sat, 30 Apr 2005 23:25:10 +1000 (EST)
Dear All,
The schedules for vt01i1 are now available (again sorry they are late) at:
ftp://ftp.atnf.csiro.au/pub/people/vlbi/vt01i1
This experiment is a disk-based imaging test. Further details for the
disk-based recording (DAS setup and recorder setup) will be sent around
closer to the experiment and posted to the wiki. As far as the
frequency/polarisation setups are concerned, they will be exactly the same
as for the previous experiments, v179/v181, except that both LCP and RCP
should be fed to the DAS, where possible. Please see my recent email for
details regarding v179/v181.
One other note for vt01i1 is that, for the purposes of setting up, I have
started the schedule at 11:00 UT, rather than the 11:30 UT listed in Jim's
block schedule on the web. Since all that will change between v179/v181
and vt01i is the recorder, and the PCFS is not needed for vt01i1, it is
more efficient to start vt01i1 at 11:00 UT, at the time that v179/v181
ends.
The ATCA and Mopra schedules are in place for vt01i1. The Parkes .psn
file is ready to collect via ftp and the VEX file is available via ftp for
Ceduna and Hobart.
Full information on the wiki soon.
Cheers, Steven
##=====================================================##
Dr Steven Tingay stingay_at_astro.swin.edu.au
Swinburne SKA Project Leader
Senior Lecturer
Centre for Astrophysics and Supercomputing
Swinburne University of Technology
Mail No H39
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 2005-04-30 23:25:32
Date: Sat, 30 Apr 2005 23:25:10 +1000 (EST)
Dear All,
The schedules for vt01i1 are now available (again sorry they are late) at:
ftp://ftp.atnf.csiro.au/pub/people/vlbi/vt01i1
This experiment is a disk-based imaging test. Further details for the
disk-based recording (DAS setup and recorder setup) will be sent around
closer to the experiment and posted to the wiki. As far as the
frequency/polarisation setups are concerned, they will be exactly the same
as for the previous experiments, v179/v181, except that both LCP and RCP
should be fed to the DAS, where possible. Please see my recent email for
details regarding v179/v181.
One other note for vt01i1 is that, for the purposes of setting up, I have
started the schedule at 11:00 UT, rather than the 11:30 UT listed in Jim's
block schedule on the web. Since all that will change between v179/v181
and vt01i is the recorder, and the PCFS is not needed for vt01i1, it is
more efficient to start vt01i1 at 11:00 UT, at the time that v179/v181
ends.
The ATCA and Mopra schedules are in place for vt01i1. The Parkes .psn
file is ready to collect via ftp and the VEX file is available via ftp for
Ceduna and Hobart.
Full information on the wiki soon.
Cheers, Steven
##=====================================================##
Dr Steven Tingay stingay_at_astro.swin.edu.au
Swinburne SKA Project Leader
Senior Lecturer
Centre for Astrophysics and Supercomputing
Swinburne University of Technology
Mail No H39
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 2005-04-30 23:25:32