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COVER INFORMATION

Station: ATCA (Code At )
Experiment: VSOP observation of J1316-33 at 5 GHz
Exp. Code: w060d


Schedule Version: 1.00
Processed by SCHED version: Release of 1 Dec. 1998

PI: J. Lovell

Address: ATNF, c/o COSSA
GPO Box 3023, Canberra 2601, ACT
Australia


Phone: +61-2-6216-7234
EMAIL: jlovell@atnf.csiro.au
Fax: +61-2-6216-7222
Phone during observation:

Observing mode: VSOP, 5 GHz continuum, 128-2-2

Notes: Fringe finder : J1337-12
BR not used



Schedule for ATCA (Code At ) Page 2
VSOP observation of J1316-33 at 5 GHz
UP: D => Below limits; H => Below horizon mask. blank => Up.
Early: Seconds between end of slew and start. Dwell: On source seconds.
Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
-------------------------------------------------------------------------------
Start UT Source Start / Stop Early Tapes
Stop UT LST EL AZ HA UP ParA Dwell (see above)
-------------------------------------------------------------------------------

--- Mon 19 Jul 1999 Day 200 ---

Next scan frequencies: 4800.00 4816.00
Next BBC frequencies: 300.00 316.00
Next scan bandwidths: 16.00 16.00

01 15 00 J1316-33 06 58 53 13.0 121.6 -6.3 -117.9 0 1 1 52
01 37 00 --- 07 20 57 17.1 119.4 -5.9 -115.4 1320 F 1 515

01 37 00 J1316-33 07 20 57 17.1 119.4 -5.9 -115.4 -2 1 1 515
02 00 00 --- 07 44 01 21.5 117.3 -5.5 -112.9 1378 F 1 998

02 00 00 J1316-33 07 44 01 21.5 117.3 -5.5 -112.9 -2 1 1 998
02 05 00 --- 07 49 01 22.5 116.9 -5.5 -112.4 298 F 1 1103

02 05 00 J1316-33 07 49 01 22.5 116.9 -5.5 -112.4 -2 1 1 1103
02 25 00 --- 08 09 05 26.4 115.2 -5.1 -110.3 1198 F 1 1523

02 25 00 J1316-33 08 09 05 26.4 115.2 -5.1 -110.3 -2 1 1 1523
03 00 00 --- 08 44 10 33.3 112.6 -4.5 -106.7 2098 F 1 2258

03 00 00 J1316-33 08 44 10 33.3 112.6 -4.5 -106.7 -2 1 1 2258
03 40 00 --- 09 24 17 41.4 109.9 -3.9 -102.8 2398 F 1 3098

03 42 00 J1337-12 09 26 17 29.8 87.9 -4.2 -117.7 83 1 1 3140
03 47 00 --- 09 31 18 30.9 87.3 -4.1 -117.8 300 F 1 3245

03 49 00 J1316-33 09 33 18 43.2 109.4 -3.7 -101.9 81 1 1 3287
04 14 00 --- 09 58 23 48.3 108.0 -3.3 -99.4 1500 F 1 3812

04 14 00 J1316-33 09 58 23 48.3 108.0 -3.3 -99.4 -2 1 1 3812
04 24 00 --- 10 08 24 50.4 107.5 -3.1 -98.4 598 F 1 4022

04 24 00 J1316-33 10 08 24 50.4 107.5 -3.1 -98.4 -2 1 1 4022
04 39 00 --- 10 23 27 53.5 106.8 -2.9 -96.9 898 F 1 4337

04 41 00 J1337-12 10 25 27 42.5 79.4 -3.2 -119.4 77 1 1 4379
04 46 00 --- 10 30 28 43.6 78.6 -3.1 -119.7 300 F 1 4484

04 48 00 J1316-33 10 32 28 55.4 106.4 -2.7 -95.9 76 1 1 4526
05 00 00 --- 10 44 30 57.9 106.0 -2.5 -94.6 720 F 1 4778


SETUP FILE INFORMATION:
NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings.


Setup file: /home/sched/short-term/progs/sched_jul99/setups/vsop4800.set
Matches group at6cm in /home/sched/short-term/progs/sched_jul99/catalogs/freq.dat

Setup group: 2 Station: ATCA Total bit rate: 128
Format: S2 Bits per sample: 2 Sample rate: 32.000
Number of channels: 2 Passes/head pos: 1 Speedup factor: 1.00

Tape speeds: Low density - 6.300 ips, High density - 4.20 ips
Time per pass for 17600 ft, High density tapes is: 13:58:06

LO sum= 4800.00 4816.00
1st LO= 4500.00 4500.00
Net SB= U U
Pol. = LCP LCP
BBC fr= 300.00 316.00
Bandwd= 16.00 16.00
BBC = 0 0
BBC SB= U U
IF = C C

Track assignments are:
track1= 0, 0
barrel=roll_off
 SOURCE LIST -- VSOP observation of J1316-33 at 5 GHz
Catalog positions marked with *.
Position of date is for stop time of first scan.
Names used in schedule marked with *.
Short names used in VLA and SNAP files marked with +.

Source Source position (RA/Dec)
(B1950) (J2000) (Date)

J1316-3338 13 13 20.042358 * 13 16 07.985938 13 16 05.812344
1313-333 -33 23 09.68779 *-33 38 59.17250 -33 38 52.03654
* J1316-33 /home/sched/short-term/progs/sched_jul99/catalogs/sources.vlba
USNO - Ref Frame 1998-6, Eubanks June 1998

J1337-1257 13 34 59.803871 * 13 37 39.782776 13 37 37.683466
1334-127 -12 42 09.74295 *-12 57 24.69323 -12 57 10.44967
* J1337-12 /home/sched/short-term/progs/sched_jul99/catalogs/sources.vlba
USNO - Ref Frame 1998-6, Eubanks June 1998



The solar corona can cause unstable phases for sources too close to the Sun.
SCHED provides warnings at individual scans for distances less than 10 degrees.
The distance from the Sun to each source in this schedule is:
Source Sun distance (deg)
J1316-33 94.4
J1337-12 91.3

Barry Clark estimates from predictions by Ketan Desai of IPM scattering sizes
that the Sun will cause amplitude reductions on the longest VLBA baselines
at a solar distance of 60deg F^(-0.6) where F is in GHz.
For common VLBI bands, this is:
327 MHz 117. deg
610 MHz 81. deg
1.6 GHz 45. deg
2.3 GHz 36. deg
5.0 GHz 23. deg
8.4 GHz 17. deg
15.0 GHz 12. deg
22.0 GHz 9. deg
43.0 GHz 6. deg