V156G1
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From: <rdodson_at_email.protected>
Date: Wed, 09 Mar 2005 12:38:50 +0100 (JST)
Hi All
Antennas Mp-At-Cd-Ho-Pa
Start 72 10:00:00
Stop 72 21:48:00
Channel 1 4808 - 4824 MHz USB RCP
Channel 2 4808 - 4824 MHz USB LCP
Bandwidth 16 MHz
Recorder S2
S2 Mode 32x4-2
DAS Mode xx16s.pro
Buggary Cable in
Tape Change 72 15:59:00
Files at ftp://ftp.atnf.csiro.au/pub/people/vlbi/v156/v156g1
Exp. Code: v156g1
Notes: PSR B1259-63 observation No 7. Part 1 @ 4816MHz
Full pol. obs, i.e. both L&RCP. i.e buggery cable in
Pulsar binned at AT (unless a problem). All in CATIE.
CA CCC mode psr16_128-64. 12 hrs & 2 tape sets.
Both polarisations centred at 4816.
The experiment is ~ 12 hours so two sets of tapes are needed
Tape change is at ~16UT
ATCA has a pulsar polyco but it maybe out of date.
So Parkes will have to collect the filter bank so we can find the
solution.
From the wiki:
Status: O
1302-638 has recently gone through it's eclipse, and it is known that
there are frequency jumps when this occurs. Therefore timing
observations of 1302-638 are worthwhile.
Received on 2005-03-09 12:38:51
Date: Wed, 09 Mar 2005 12:38:50 +0100 (JST)
Hi All
Antennas Mp-At-Cd-Ho-Pa
Start 72 10:00:00
Stop 72 21:48:00
Channel 1 4808 - 4824 MHz USB RCP
Channel 2 4808 - 4824 MHz USB LCP
Bandwidth 16 MHz
Recorder S2
S2 Mode 32x4-2
DAS Mode xx16s.pro
Buggary Cable in
Tape Change 72 15:59:00
Files at ftp://ftp.atnf.csiro.au/pub/people/vlbi/v156/v156g1
Exp. Code: v156g1
Notes: PSR B1259-63 observation No 7. Part 1 @ 4816MHz
Full pol. obs, i.e. both L&RCP. i.e buggery cable in
Pulsar binned at AT (unless a problem). All in CATIE.
CA CCC mode psr16_128-64. 12 hrs & 2 tape sets.
Both polarisations centred at 4816.
The experiment is ~ 12 hours so two sets of tapes are needed
Tape change is at ~16UT
ATCA has a pulsar polyco but it maybe out of date.
So Parkes will have to collect the filter bank so we can find the
solution.
From the wiki:
Status: O
1302-638 has recently gone through it's eclipse, and it is known that
there are frequency jumps when this occurs. Therefore timing
observations of 1302-638 are worthwhile.
Received on 2005-03-09 12:38:51