LBA Observing Roster Jul 2010
Roster for March 2010LBA Session
The LBA session schedule is at http://www.atnf.csiro.au/vlbi/wiki/index.php?n=Main.LBAMar2010
Day & Date | Start Time (EDT) | End Time (EDT) | Experiments | Frequency & Proposer | Note | Volunteer |
---|---|---|---|---|---|---|
Thursday 22/7 | 1600 | 0900 | vc117a,b v255j vc118 v389a | 6.7 GHz, test 6.7 GHz, Ellingsen 1.4 GHz, test 1.4 GHz, Zanardo | 3am change from 8.4 to 1.4 GHz (Circ pol). Hobart only. | Jamie M |
Friday 23/7 | 0900 | 1600 | v389a | 1.4 GHz, Zanardo | Brett & Eric | |
Friday 23/7 | 1600 | 0900 | vc119a,b v255k | 6.7 GHz, test 6.7 GHz, Ellingsen | Experiment starts at 4pm | Claire |
Saturday 24/7 | 0900 | 2100 | vc121 v252s | 8.4 GHz, test 8.4 GHz, Ojha | Rx change needed before experiment start at 10 am. | Jamie M. |
Saturday 24/7 | 2100 | 0900 | v252s | 8.4 GHz, Ojha | Jay | |
Sunday 25/7 | 0900 | 2100 | v252s vc122 v271f | 8.4 GHz, Ojha 8.4 GHz, test 8.4 GHz, Petrov | v271f uses the S/X and Mark5A recorder | Warren |
Sunday 25/7 | 2100 | 0900 | v271f | 8.4 GHz, Petrov | John | |
Monday 26/7 | 0900 | 1600 | v271f vc123 vx016b | 8.4 GHz, Petrov 8.4 GHz, test 8.4 GHz, Moin | Brett & Eric | |
Monday 26/7 | 1600 | 0200 | vx016b | 8.4 GHz, Moin | Experiment followed by IVS - R1441 | Anita |
If the observers want to adjust the start and stop times of the shifts, please update this page.
LBA disk schedule - Hobart
LBA Disk set | Start Time (EDT) | End Time (EDT) | Experiments | Observer | Change required at the end? |
---|---|---|---|---|---|
ATNF V009A | Thursday 1600 | Friday 1600 | vc117, v255j, vc118, v389a | Brett/Claire | cDisko change to CURT V003B |
CURT V003B | Friday 1600 | Saturday 0300 | vc119, v255k | Claire | Unmount the ATNF V009A set and load the CURT V001B set |
CURT V001B | Saturday 1000 | Sunday 1100 | vc121, v252s | No change - the next experiments use Mk5A and CURT V003B again | |
Mk5A - PKS+0010 | Sunday 1100 | Monday 1200 | vc122, v271f | Use cDisko to select CURT V003B set. Unmount the disk module. | |
CURT V003B | Monday 1200 | Tuesday 0200 | vc123, vx016b | Anita | End o' LBA week. Load in a fresh IVS module for R1441. |
Spare sets are in abundance this run and are UTAS V001A, UTAS V002A, HOB HO and ATNF V016B. All sets (except ATNF V016B) are empty and xfs formatted.
LBA disk schedule - Ceduna
LBA Disk set | Start Time (EDT) | End Time (EDT) | Experiments | Observer | Change required at the end? |
---|---|---|---|---|---|
ATNF V007A | Thursday 1600 | Saturday 0300 | vc117, v255j, vc119, v255k | Claire(?) | Unmount ATNF V007A and replace with ATNF V010A |
CURT V006A | Saturday 1000 | Sunday 1100 | vc121,v252s | cDisko - Switch to ATNF V010A | |
ATNF V010A | Sunday 1100 | Monday 1200 | vc122, v271f | Unmount both sets, load in ATNF V010B and CURT V007B | |
ATNF V010B | Monday 1200 | Tuesday 0200 | vc123,vx016b | Anita | End of LBA Week. Unmount drives so that Bev can remove them for shipping. |
Spare sets - CURT V007B & ATNF V012A
Experiment Summary - Hobart
Experiment | Rx | Agilent | Pol. | DAS profile | Second LO(s) | Coherence Tone | Nota bene |
v255j | 6.7 (5) | 12.2 GHz | RCP, LCP | VSOP.PRO | 468 & 810 MHz 810 & 810 MHz | 788.125 830.875 | Two frequency setups. Changes can be automated in the snap file. |
v389a | 1.4 (2) | 4.15 GHz | RCP, LCP | VSOP_HO.PRO | 802 MHz | 694.5 | See http://www-ra.phys.utas.edu.au/wiki/index.php?n=MtPleasant26m.Lbandcircular for instructions on getting Circular polarisation |
v255k | 6.7 (5) | 12.2 GHz | RCP, LCP | VSOP.PRO | 468 & 810 MHz 810 & 810 MHz | 788.125 830.875 | Two frequency setups. Changes can be automated in the snap file. |
v252s | 8.4 (6) | 14 GHz | RCP only (RF switches at XOXX on the Folly Interface ) | VSOP.PRO | 777 & 809 | 841.4 & 844.6 | |
v271f | S/X (1) | N/A | RCP only | N/A | N/A | Test using the vertex radiator - should appear as steady sine wave on CRO above the DAS PC 821.601 MHz for vc01 USB 824.801 MHz for vc02 USB 828.001 MHz for vc03 USB 832.801 MHz for vc04 USB 836.001 MHz for vc05 USB 844.001 MHz for vc06 USB 847.201 MHz for vc07 USB 850.401 MHz for vc08 USB | The experiment only uses vc01-08. |
vx016b | 8.4 (5) | 14 GHz | RCP,LCP | 64MHZ_N.PRO | 793 MHz | 843.0 | Needs BG3 cable (currently installed) |
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.
SMY01 should be used for the channel 1 LO of the frequency translator and the SML for channel 2. The upper SMX is used for the tone.
Experiment Summary - Ceduna
Experiment | Rx | Agilent | Pol. | DAS profile | Second LO(s) | Coherence Tone | Nota bene |
v255j | 6.7 | 11.1 GHz | RCP, LCP | VSOP.PRO | 468 & 810 MHz 810 & 810 MHz | 788.125 830.875 | Two frequency setups. Changes can be automated in the snap file. |
v255k | 6.7 | 11.1 GHz | RCP, LCP | VSOP.PRO | 468 & 810 MHz 810 & 810 MHz | 788.125 830.875 | Two frequency setups. Changes can be automated in the snap file. |
v252s | 8.4 | 13.04 GHz | RCP only | VSOP.PRO | 637 & 669 | 841.4 & 844.6 | |
v271f | 8.4 | 13.04 GHz | RCP only | VSOPX0Y0.PRO(?) | 428 & 684 MHz | 820.5 | Change the frequencies through rs.tcl - SMY01 should be 428 and SMY02 should be 684. VSOP profile needs checking. |
vx016b | 8.4 | 13.04 GHz | RCP,LCP | 64MHZ_F.PRO | 653 MHz | 843.0 | Needs BG3 cable (currently installed) |
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.
For the v271f & v252s experiments, we need to be able to change these remotely. If we use SMY01 and SMY02 then Bev doesn't need to make an extra trip out to the station. This does mean that we won't be able to check coherence though.