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LBA Observing Roster Dec 2009

Roster for December 2009 LBA Session

The LBA session schedule is at http://www.atnf.csiro.au/vlbi/wiki/index.php?n=Main.LBADec2009

Day & DateStart Time (EDT)End Time (EDT)ExperimentsFrequency & ProposerVolunteer
Thursday 10/1206000900CRF57

v289q
S/X, IVS

1.4 GHz, Moin
Warren
Thursday 10/1209001600vt10h

vc094

v310a
4.8 GHz, CdHoTest

4.8 GHz, test

4.8 GHz, Ellingsen
Brett, Eric & Jamie
Thursday 10/1216000900v310a

vc095

v318a
4.8 Ghz, Ellingsen

1.4 GHz, test

1.4 GHz, Hotan
Jamie
Friday 11/1209001600vc096

v255h
6.7 GHz, test

6.7 GHz, Ellingsen
Brett, Eric & Jamie
Friday 11/1216000900v255h

vc097

v316b

vc098

v289r
6.7 GHz, Ellingsen

6.7 GHz, test

6.7 GHz, Beasley

1.4 GHz, test

1.4 GHz, Moin
Jamie
Saturday 12/1209002100vc099

v277c

vc100

v190m
8.4 GHz, test

8.4 GHz, Deller

8.4 GHz, test

8.4 GHz, Deller
John
Saturday 12/1221000900v190m

vc101

v271d
8.4 GHz, Deller

8.4 GHz, test

8.4 GHz, Petrov
Jay
Sunday 13/1209002100v271d8.4 GHz, PetrovDave Horsley
Sunday 13/1221000900v271d

vc102

v252n
8.4 GHz, Petrov

8.4 GHz, test

8.4 GHz, Ojha
Jim L.
Monday 14/1209001600v252n8.4 GHz, OjhaBrett & Eric
Monday 14/1216000900v252n

vc103

v289s
8.4 GHz, Ojha

1.4 GHz, test

1.4 GHz, Moin
Warren

If the observers want to adjust the start and stop times of the shifts, please update this page.

LBA disk schedule.

This has been revised as an a fit of muppetry I didn’t remember that 64 MHz experiments are 512 Mbps. The revised schedule requires a disk change to be made during the v271d experiment, which uses the Mk5 recorder.

LBA Disk setStart Time (EDT)End Time (EDT)ExperimentsObserverChange required at the end?
ATNF V016B and CURT V003BThursday 10/12, 6 amFriday 11/12 8amvt10i, vc095, v318a

vc094, v310a
JMcSwap disks
CURT V001BFriday 11/12 8amSaturday 12/12 5amvc096, v255h, vc097, v316bJaycdisko - switch to UTAS V001A
UTAS V001ASaturday 12/12 5amSunday 13/12 4amvc099, v277c, vc100, v190mJim Lchange disk for UTAS V002A
MPI-0609 (Mk5)Sunday 13/12 4amMonday 14/12 5 amvc101, v271dJay, Dave, Jim LUse Mk5 for this experiment
UTAS V002AMonday 14/12 6amTuesday 15/12 5amvc102, v252oJim L, Warren
No diskTuesday 15/12 5amTuesday 15/12 9amvc103, v289sWarreneVLBI and end of LBA week!

All disks have been checked and cleaned. ATNF V016B still has ~10 hours spare capacity.

Experiment Summary

ExperimentRxAgilentPol.DAS profileSecond LO(s)Coherence ToneNota bene
v289rL-band (2)4.1 GHzRCP, LCPVSOP_HO3.PRO852 MHz694.5eVLBI
vt10i4.8 (4)10.5 GHzRCP, LCPVSOP.PRO676 MHz962.6 
v310a4.8 (4)10.5 GHzRCP,LCP?????????668 MHz951.464 MHz bandwidth. DAS profile TBA
v318aL-band (2)4.1 GHzRCP, LCPPSR64_N.pro836 MHz678.564 MHz bandwidth. No AGC
v255h6.7 (5)12.2 GHzRCP, LCPVSOP.PRO468 & 810 MHz

810 MHz
788.125 & 830.875

830.875
Frequency changes required during experiment. This has been automated but requires SMY01 → IF1.
v316b6.7 (5)12.2 GHzRCP, LCPVSOP.PRO810 MHz830.875 
v289sL-band (2)4.1 GHzRCP, LCPVSOP_HO3.PRO852 MHz694.5eVLBI
v277c8.4 (6)14 GHzRCP,LCPVSOP.PRO777 MHz841.4 
v190m8.4 (6)14 GHzRCP,LCPVSOP.PRO777 MHz841.4 
v271d      Using the Mk5
v252o8.4 (6)14 GHzRCP, RCPVSOP.PRO777 & 809 MHz841.4 & 844.6 
v289tL-band (2)4.1 GHzRCP, LCPVSOP_HO3.PRO852 MHz694.5eVLBI

Note that the frequency for the coherence tone refers to the output of the CH 1 band splitter beneath the frequency translator (rack 6). A tone at the given frequency should return a 5 MHz coherence signal from the CH 1 band splitter.

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Page last modified on December 10, 2009, at 08:58 PM