COVER INFORMATION Station: WSTRBORK (Code Wb ) Experiment: GD017 format, 18 cm, Arp 220, Phil Diamond, November 2003 Exp. Code: GD017B Schedule Version: 1.00 Processed by SCHED version: NRAO internal release of 4 October 2004 PI: Phil Diamond Address: MERLIN/VLBI National Facility Jodrell Bank, Macclesfield Cheshire, SK11 9DL England Phone: (+44) (0)1477 572625 EMAIL: pdiamond@jb.man.ac.uk Fax: (+44) (0)1477 571618 Phone during observation: (+44) (0)1477 572625 Observing mode: 256-8-2 Notes: Primary fringe finder 1613+341 Schedule for WSTRBORK (Code Wb ) Page 2 GD017 format, 18 cm, Arp 220, Phil Diamond, November 2003 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. TPStart: Tape motion start time. Frequencies are LO sum (band edge). ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) ---------------------------------------------------------------------------------------- --- Sun 6 Mar 2005 Day 65 --- Next scan frequencies: 1633.99 1633.99 1641.99 1641.99 1649.99 1649.99 1657.99 1657.99 Next BBC frequencies: 123.99 123.99 131.99 131.99 139.99 139.99 147.99 147.99 Next scan bandwidths: 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 21 00 00 1613+341 08 25 17 12.8 49.0 -7.8 D 0.0 0 1 1 0 21 00 00 21 06 00 --- 08 31 18 13.4 50.1 -7.7 D 0.0 0 F 1 4800 21 06 00 ARP220 08 31 18 9.5 63.4 -7.1 D 0.0 -10 1 1 4800 21 06 00 21 22 00 --- 08 47 21 11.7 66.4 -6.8 D 0.0 0 F 1 17600 21 35 00 ARP220 09 00 23 13.5 68.8 -6.6 D 0.0 770 1 2 17600 21 35 00 21 57 00 --- 09 22 27 16.7 72.9 -6.2 D 0.0 0 R 1 0 22 10 00 ARP220 09 35 29 18.6 75.4 -6.0 0.0 545 1 3 0 22 10 00 22 32 00 --- 09 57 33 21.8 79.5 -5.6 0.0 1320 F 1 17600 22 45 00 ARP220 10 10 35 23.8 82.0 -5.4 0.0 756 1 4 17600 22 45 00 23 07 00 --- 10 32 38 27.1 86.2 -5.0 0.0 1320 R 1 0 23 20 00 1613+341 10 45 40 31.2 73.2 -5.5 0.0 731 1 5 0 23 20 00 23 26 00 --- 10 51 41 32.0 74.2 -5.4 0.0 360 F 1 4800 23 26 00 ARP220 10 51 41 29.9 90.0 -4.7 0.0 -49 1 5 4800 23 26 00 23 42 00 --- 11 07 44 32.4 93.2 -4.5 0.0 911 F 1 17600 --- Mon 7 Mar 2005 Day 66 --- 00 01 00 ARP220 11 26 47 35.2 97.2 -4.1 0.0 1111 1 6 17600 00 01 00 00 23 00 --- 11 48 51 38.5 102.0 -3.8 0.0 1320 R 1 0 00 30 00 ARP220 11 55 52 39.5 103.6 -3.7 0.0 401 1 7 0 00 30 00 00 52 00 --- 12 17 56 42.7 108.8 -3.3 0.0 1320 F 1 17600 01 05 00 ARP220 12 30 58 44.6 112.1 -3.1 0.0 756 1 8 17600 01 05 00 01 27 00 --- 12 53 01 47.6 117.9 -2.7 0.0 1320 R 1 0 01 40 00 1613+341 13 06 03 52.1 100.5 -3.1 0.0 731 1 9 0 01 40 00 01 46 00 --- 13 12 04 53.0 101.9 -3.0 0.0 360 F 1 4800 Schedule for WSTRBORK (Code Wb ) Page 3 GD017 format, 18 cm, Arp 220, Phil Diamond, November 2003 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. TPStart: Tape motion start time. Frequencies are LO sum (band edge). ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) ---------------------------------------------------------------------------------------- --- Mon 7 Mar 2005 Day 66 --- 01 46 00 ARP220 13 12 04 50.0 123.4 -2.4 0.0 -49 1 9 4800 01 46 00 02 02 00 --- 13 28 07 52.0 128.3 -2.1 0.0 911 F 1 17600 02 15 00 ARP220 13 41 09 53.5 132.6 -1.9 0.0 756 1 10 17600 02 15 00 02 37 00 --- 14 03 13 55.8 140.4 -1.5 0.0 1320 R 1 0 02 45 00 ARP220 14 11 14 56.5 143.4 -1.4 0.0 460 1 11 0 02 45 00 03 07 00 --- 14 33 18 58.3 152.2 -1.0 0.0 1320 F 1 17600 03 15 00 ARP220 14 41 19 58.8 155.6 -0.9 0.0 460 1 12 17600 03 15 00 03 37 00 --- 15 03 23 60.0 165.3 -0.5 0.0 1320 R 1 0 03 45 00 1613+341 15 11 24 68.2 143.1 -1.0 0.0 431 1 13 0 03 45 00 03 51 00 --- 15 17 25 68.8 146.2 -0.9 0.0 360 F 1 4800 03 51 00 ARP220 15 17 25 60.4 171.7 -0.3 0.0 -49 1 13 4800 03 51 00 04 07 00 --- 15 33 28 60.6 179.2 0.0 0.0 911 F 1 17600 04 15 00 ARP220 15 41 29 60.5 182.9 0.1 0.0 460 1 14 17600 04 15 00 04 37 00 --- 16 03 33 60.1 193.1 0.5 0.0 1320 R 1 0 ----------- Tape Change ------------ 05 00 00 1613+341 16 26 36 71.1 188.2 0.2 0.0 1331 1 1 0 05 00 00 05 06 00 --- 16 32 37 71.0 192.0 0.3 0.0 360 F 1 4800 05 06 00 ARP220 16 32 37 58.6 205.9 1.0 0.0 -49 1 1 4800 05 06 00 05 22 00 --- 16 48 40 57.4 212.5 1.2 0.0 911 F 1 17600 05 30 00 1613+341 16 56 41 69.8 206.4 0.7 0.0 431 1 2 17600 05 30 00 05 33 00 --- 16 59 42 69.6 208.1 0.8 0.0 180 R 1 15200 05 33 00 ARP220 16 59 42 56.5 216.8 1.4 0.0 -49 1 2 15200 05 33 00 05 52 00 --- 17 18 45 54.6 223.8 1.7 0.0 1091 R 1 0 05 53 00 ARP220 17 19 45 54.5 224.1 1.7 0.0 47 1 3 0 05 53 00 06 15 00 --- 17 41 49 52.1 231.5 2.1 0.0 1320 F 1 17600 06 17 00 ARP220 17 43 49 51.8 232.2 2.1 0.0 106 1 4 17600 06 17 00 06 39 00 --- 18 05 53 49.1 238.8 2.5 0.0 1320 R 1 0 06 41 00 ARP220 18 07 53 48.8 239.4 2.5 0.0 106 1 5 0 06 41 00 07 03 00 --- 18 29 57 45.9 245.5 2.9 0.0 1320 F 1 17600 Schedule for WSTRBORK (Code Wb ) Page 4 GD017 format, 18 cm, Arp 220, Phil Diamond, November 2003 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. TPStart: Tape motion start time. Frequencies are LO sum (band edge). ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) ---------------------------------------------------------------------------------------- --- Mon 7 Mar 2005 Day 66 --- 07 10 00 1516+193 18 36 58 39.2 248.6 3.3 0.0 386 1 6 17600 07 10 00 07 13 00 --- 18 39 58 38.8 249.3 3.4 0.0 180 R 1 15200 07 13 00 ARP220 18 39 58 44.5 248.1 3.1 0.0 -28 1 6 15200 07 13 00 07 32 00 --- 18 59 01 41.8 252.8 3.4 0.0 1112 R 1 0 07 35 00 ARP220 19 02 02 41.3 253.5 3.4 0.0 165 1 7 0 07 35 00 07 57 00 --- 19 24 05 38.1 258.6 3.8 0.0 1320 F 1 17600 08 00 00 ARP220 19 27 06 37.7 259.2 3.9 0.0 165 1 8 17600 08 00 00 08 22 00 --- 19 49 09 34.4 264.0 4.2 0.0 1320 R 1 0 08 25 00 ARP220 19 52 10 33.9 264.6 4.3 0.0 165 1 9 0 08 25 00 08 47 00 --- 20 14 14 30.6 269.1 4.7 0.0 1320 F 1 17600 08 50 00 1516+193 20 17 14 24.4 270.4 5.0 0.0 149 1 10 17600 08 50 00 09 00 00 --- 20 27 16 22.9 272.4 5.2 0.0 600 R 1 9600 09 00 00 ARP220 20 27 16 28.6 271.7 4.9 0.0 -28 1 10 9600 09 00 00 09 12 00 --- 20 39 18 26.8 274.1 5.1 0.0 692 R 1 0 09 15 00 ARP220 20 42 18 26.4 274.7 5.1 0.0 165 1 11 0 09 15 00 09 37 00 --- 21 04 22 23.1 278.9 5.5 0.0 1320 F 1 17600 09 40 00 ARP220 21 07 22 22.6 279.5 5.5 0.0 165 1 12 17600 09 40 00 10 02 00 --- 21 29 26 19.4 283.6 5.9 0.0 1320 R 1 0 10 05 00 1613+341 21 32 26 32.5 285.1 5.3 0.0 131 1 13 0 10 05 00 10 08 00 --- 21 35 27 32.1 285.7 5.4 0.0 180 F 1 2400 10 08 00 ARP220 21 35 27 18.5 284.7 6.0 D 0.0 -199 1 13 2400 10 08 00 10 27 00 --- 21 54 30 15.7 288.3 6.3 D 0.0 0 F 1 17600 10 30 00 ARP220 21 57 31 15.3 288.8 6.4 D 0.0 170 1 14 17600 10 30 00 10 52 00 --- 22 19 34 12.2 292.9 6.7 D 0.0 0 R 1 0 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: arp220.set Matches group wb18cm in /usr/local/vlbi_sched/catalogs/freq.dat E-mail Foley 22Jan97 MFFE, must be using Low patch Setup group: 6 Station: WSTRBORK Total bit rate: 256 Format: MKIV1:2 Bits per sample: 2 Sample rate: 16.000 Number of channels: 8 Passes/head pos: 1 Speedup factor: 1.00 Tape speeds: Low density - 270.000 ips, High density - 160.00 ips Time per pass for 17600 ft, High density tapes is: 00:22:00 1st LO= 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 1510.00 Net SB= U U U U U U U U Pol. = RCP LCP RCP LCP RCP LCP RCP LCP BBC = 2 1 4 3 6 5 8 7 BBC SB= U U U U U U U U IF = 2N 1N 2N 1N 2N 1N 2N 1N The following frequency sets based on this setup were used. Frequency Set: 6 Setup file default. No pcal detection. LO sum= 1633.99 1633.99 1641.99 1641.99 1649.99 1649.99 1657.99 1657.99 BBC fr= 123.99 123.99 131.99 131.99 139.99 139.99 147.99 147.99 Bandwd= 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 Track assignments are: track1= 2, 10, 18, 26, 3, 11, 19, 27 barrel=roll_off SOURCE LIST -- GD017 format, 18 cm, Arp 220, Phil Diamond, November 2003 Catalog positions marked with *. Precession of date coordinates is based on stop time of first scan. Names used in schedule marked with *. Short names used in VLA and SNAP files marked with +. Observation date used in B1950/J2000 coordinate conversion (PRECDATE): 1979.900 No adjustments are made for rates (DRA, DDEC). Scan hours are for recording scans only. Baseline hours are only counted for scans above horizon at both ends. Source Source position (RA/Dec) (B1950) (J2000) (Date) * ARP220 15 32 46.880196 * 15 34 57.224670 15 35 11.038195 23 40 07.99276 * 23 30 11.56400 23 28 50.20626 From catalog imbedded in main SCHED input file. 14.333 scan hours, 933.144 baseline hours above horizon. * 1516+193 15 14 40.987286 * 15 16 56.797600 15 17 11.234204 19 43 10.96935 * 19 32 13.01900 19 30 46.99831 From catalog imbedded in main SCHED input file. 0.217 scan hours, 32.847 baseline hours above horizon. * 1613+341 16 11 47.914510 * 16 13 41.064500 16 13 52.969205 34 20 19.83496 * 34 12 47.91000 34 11 37.69314 From catalog imbedded in main SCHED input file. 0.900 scan hours, 40.750 baseline hours above horizon. * 3C286 13 28 49.657708 * 13 31 08.288000 13 31 23.761925 30 45 58.64136 * 30 30 32.96000 30 28 43.26779 From catalog imbedded in main SCHED input file. 0.000 scan hours, 0.000 baseline hours above horizon. 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) ARP220 114.1 1516+193 118.6 1613+341 104.8 3C286 138.5 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