COVER INFORMATION Station: JODRELL1 (Code Jb ) Experiment: 3C48 6cm Exp. Code: GA025B Schedule Version: 1.00 Processed by SCHED version: 8.10 Bug fixs and minor enhancements PI: Tao An Address: Shanghai Astronomical Observatory 80 Nandan Road Shanghai, 200030 China Phone: +86 21 64386191 EMAIL: antao@shao.ac.cn Fax: +86 21 64386191 Phone during observation: +86 21 64386191 Observing mode: 3C48 dual pol at 6cm (1024 Mb/s) Notes: COVER LETTER: ! From block schedule. allocated ! ! Eb, Wb, Jb1, Mc, Nt, Tr, + VLBA(-MK) ! This schedule file is for EVN antennas 1024Mbps ! ! day 80, March 21th Sunday, EU 1200 - 2000, 1024Mbps ! US 1200 - 2000, 512Mbps 5GHz global network observation of 3C48. Since the different data recording rate of the EVN and VLBA, two different schedule files are made for EVN and VLBA respectively. The correlation position is 120 mas north of the active nucleus, at a component B2, RA 01 37 41.29949, DEC +33 09 35.1338. This setup enables to less degradation of flux density in both VLBI core region and shock-induced blobs in the north jet. One correlation pass is sufficient. A dual polarisation mode is used and cross-correlation products requested. The sources 3C138 is used as EVPA calibrator, will be observed 2 scans DA193 is used as D-term calibrator, will be observed 6 scans Schedule for JODRELL1 (Code Jb ) Page 2 3C48 6cm 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. For disks, the footages are really the GBytes TPStart: Tape motion start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Sun 21 Mar 2010 Day 80 --- Next scan frequencies: 4942.49 4942.49 4942.49 4942.49 4974.49 4974.49 4974.49 4974.49 5006.49 5006.49 5006.49 5006.49 5038.49 5038.49 5038.49 5038.49 Next BBC frequencies: 102.49 102.49 102.49 102.49 134.49 134.49 134.49 134.49 166.49 166.49 166.49 166.49 198.49 198.49 198.49 198.49 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 12 00 00 3C345 23 46 21 22.8 -53.4 7.1 38.7 0 1 1 0 12 00 00 12 05 00 --- 23 51 22 22.2 -52.5 7.1 38.2 300 F 1 39 12 00 04 12 07 00 3C48 23 53 22 62.6 126.5 -1.7 -35.1 -616 1 1 39 12 07 00 12 12 00 --- 23 58 23 63.2 128.4 -1.7 -34.1 -316 F 1 77 12 07 04 12 12 20 3C48 23 58 43 63.3 128.5 -1.7 -34.0 6 1 1 77 12 12 20 12 22 00 --- 00 08 25 64.4 132.4 -1.5 -31.9 580 F 1 152 12 12 24 12 22 00 3C48 00 08 25 64.4 132.4 -1.5 -31.9 -10 1 1 152 No stop 12 32 00 --- 00 18 26 65.4 136.6 -1.3 -29.4 590 F 1 230 12 22 04 12 32 20 3C48 00 18 46 65.5 136.8 -1.3 -29.3 5 1 1 230 12 32 20 12 44 00 --- 00 30 28 66.6 142.1 -1.1 -26.1 700 F 1 320 12 32 24 12 44 00 3C48 00 30 28 66.6 142.1 -1.1 -26.1 -10 1 1 320 No stop 12 54 00 --- 00 40 30 67.5 147.0 -1.0 -22.9 590 F 1 397 12 44 04 12 54 20 3C48 00 40 50 67.5 147.2 -1.0 -22.8 5 1 1 397 12 54 20 13 06 00 --- 00 52 32 68.4 153.3 -0.8 -18.8 700 F 1 488 12 54 24 13 08 00 3C454.3 00 54 32 46.2 223.9 2.0 25.6 -182 1 1 488 13 08 00 13 12 00 --- 00 58 33 45.7 225.2 2.1 26.2 58 F 1 519 13 08 04 13 14 00 3C48 01 00 33 68.9 157.7 -0.6 -15.8 -170 1 1 519 13 14 00 13 28 00 --- 01 14 36 69.5 165.7 -0.4 -10.2 670 F 1 627 13 14 04 13 28 20 3C48 01 14 56 69.5 165.9 -0.4 -10.0 4 1 1 627 13 28 20 13 38 00 --- 01 24 37 69.8 171.7 -0.2 -5.9 580 F 1 702 13 28 24 13 38 20 3C48 01 24 57 69.8 171.9 -0.2 -5.8 4 1 1 702 13 38 20 13 50 00 --- 01 36 39 70.0 179.0 -0.0 -0.7 700 F 1 792 13 38 24 Schedule for JODRELL1 (Code Jb ) Page 3 3C48 6cm 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. For disks, the footages are really the GBytes TPStart: Tape motion start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Sun 21 Mar 2010 Day 80 --- 13 50 00 3C48 01 36 39 70.0 179.0 -0.0 -0.7 -10 1 1 792 No stop 14 00 00 --- 01 46 41 69.9 185.1 0.1 3.7 590 F 1 870 13 50 04 14 00 20 3C48 01 47 01 69.9 185.3 0.1 3.8 4 1 1 870 14 00 20 14 12 00 --- 01 58 43 69.6 192.4 0.3 8.8 700 F 1 960 14 00 24 14 12 00 3C48 01 58 43 69.6 192.4 0.3 8.8 -10 1 1 960 No stop 14 22 00 --- 02 08 44 69.2 198.2 0.5 12.9 590 F 1 1037 14 12 04 14 22 20 3C48 02 09 05 69.2 198.4 0.5 13.1 5 1 1 1037 14 22 20 14 34 00 --- 02 20 46 68.6 205.0 0.7 17.6 700 F 1 1128 14 22 24 14 34 00 3C48 02 20 46 68.6 205.0 0.7 17.6 -10 1 1 1128 No stop 14 44 00 --- 02 30 48 67.9 210.3 0.9 21.2 590 F 1 1205 14 34 04 14 44 20 3C48 02 31 08 67.9 210.5 0.9 21.3 5 1 1 1205 14 44 20 14 56 00 --- 02 42 50 66.9 216.4 1.1 25.1 700 F 1 1295 14 44 24 14 56 00 3C48 02 42 50 66.9 216.4 1.1 25.1 -10 1 1 1295 No stop 15 06 00 --- 02 52 52 66.0 221.0 1.2 28.0 590 F 1 1373 14 56 04 15 06 20 3C48 02 53 12 65.9 221.2 1.2 28.1 5 1 1 1373 15 06 20 15 18 00 --- 03 04 54 64.7 226.3 1.4 31.1 700 F 1 1463 15 06 24 15 18 00 3C48 03 04 54 64.7 226.3 1.4 31.1 -10 1 1 1463 No stop 15 28 00 --- 03 14 55 63.6 230.4 1.6 33.4 590 F 1 1541 15 18 04 15 28 20 3C48 03 15 15 63.6 230.5 1.6 33.5 6 1 1 1541 15 28 20 15 40 00 --- 03 26 57 62.2 234.9 1.8 35.8 700 F 1 1631 15 28 24 15 40 00 3C48 03 26 57 62.2 234.9 1.8 35.8 -10 1 1 1631 No stop 15 50 00 --- 03 36 59 60.9 238.4 2.0 37.6 590 F 1 1708 15 40 04 15 50 20 3C48 03 37 19 60.9 238.6 2.0 37.6 6 1 1 1708 15 50 20 16 02 00 --- 03 49 01 59.3 242.4 2.2 39.3 700 F 1 1799 15 50 24 16 04 00 DA193 03 51 01 64.9 109.6 -2.1 -47.2 -431 1 1 1799 16 04 00 16 08 00 --- 03 55 02 65.5 110.9 -2.0 -46.7 -191 F 1 1830 16 04 04 16 10 00 3C48 03 57 02 58.3 244.9 2.3 40.4 -436 1 1 1830 16 10 00 16 24 00 --- 04 11 04 56.3 249.0 2.5 41.9 404 F 1 1938 16 10 04 16 24 20 3C48 04 11 25 56.3 249.1 2.6 41.9 6 1 1 1938 16 24 20 16 34 20 --- 04 21 26 54.9 251.8 2.7 42.8 600 F 1 2015 16 24 24 Schedule for JODRELL1 (Code Jb ) Page 4 3C48 6cm 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. For disks, the footages are really the GBytes TPStart: Tape motion start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Sun 21 Mar 2010 Day 80 --- 16 34 20 3C48 04 21 26 54.9 251.8 2.7 42.8 -10 1 1 2015 No stop 16 46 00 --- 04 33 08 53.2 254.8 2.9 43.7 690 F 1 2106 16 34 24 16 46 20 3C48 04 33 28 53.2 254.9 2.9 43.7 6 1 1 2106 16 46 20 16 53 00 --- 04 40 09 52.2 256.6 3.0 44.1 400 F 1 2157 16 46 24 16 55 00 DA193 04 42 10 71.6 129.4 -1.2 -37.0 -409 1 1 2157 16 55 00 16 59 00 --- 04 46 10 72.1 131.4 -1.2 -35.8 -169 F 1 2188 16 55 04 17 01 00 3C48 04 48 11 51.0 258.5 3.2 44.5 -408 1 1 2188 17 01 00 17 08 00 --- 04 55 12 50.0 260.2 3.3 44.8 12 F 1 2242 17 01 04 17 08 00 3C48 04 55 12 50.0 260.2 3.3 44.8 -10 1 1 2242 No stop 17 18 00 --- 05 05 13 48.5 262.4 3.4 45.2 590 F 1 2320 17 08 04 17 18 20 3C48 05 05 33 48.4 262.5 3.5 45.2 7 1 1 2320 17 18 20 17 30 00 --- 05 17 15 46.7 265.1 3.6 45.5 700 F 1 2410 17 18 24 17 30 00 3C48 05 17 15 46.7 265.1 3.6 45.5 -10 1 1 2410 No stop 17 40 00 --- 05 27 17 45.2 267.2 3.8 45.6 590 F 1 2488 17 30 04 17 40 20 3C48 05 27 37 45.2 267.2 3.8 45.6 7 1 1 2488 17 40 20 17 52 00 --- 05 39 19 43.4 269.6 4.0 45.7 700 F 1 2578 17 40 24 17 54 00 DA193 05 41 19 76.3 167.8 -0.2 -9.5 -307 1 1 2578 17 54 00 17 58 00 --- 05 45 20 76.5 171.0 -0.2 -7.0 -67 F 1 2609 17 54 04 18 00 00 3C48 05 47 20 42.2 271.2 4.2 45.7 -300 1 1 2609 18 00 00 18 14 00 --- 06 01 23 40.1 274.0 4.4 45.5 540 F 1 2717 18 00 04 18 14 20 3C48 06 01 43 40.1 274.0 4.4 45.5 7 1 1 2717 18 14 20 18 24 20 --- 06 11 44 38.6 275.9 4.6 45.4 600 F 1 2795 18 14 24 18 24 20 3C48 06 11 44 38.6 275.9 4.6 45.4 -10 1 1 2795 No stop 18 36 00 --- 06 23 26 36.8 278.1 4.8 45.1 690 F 1 2885 18 24 24 18 36 20 3C48 06 23 46 36.8 278.2 4.8 45.1 7 1 1 2885 18 36 20 18 51 00 --- 06 38 29 34.6 280.9 5.0 44.6 880 F 1 2999 18 36 24 18 53 00 DA193 06 40 29 74.6 213.7 0.7 25.6 -168 1 1 2999 18 53 00 18 58 00 --- 06 45 30 74.2 216.9 0.8 27.9 132 F 1 3037 18 53 04 19 00 00 3C48 06 47 30 33.3 282.5 5.2 44.3 -162 1 1 3037 19 00 00 19 06 00 --- 06 53 31 32.4 283.5 5.3 44.1 198 F 1 3084 19 00 04 Schedule for JODRELL1 (Code Jb ) Page 5 3C48 6cm 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. For disks, the footages are really the GBytes TPStart: Tape motion start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Sun 21 Mar 2010 Day 80 --- 19 08 00 3C138 06 55 31 49.1 215.6 1.6 21.3 -171 1 1 3084 19 08 00 19 14 00 --- 07 01 32 48.5 217.6 1.7 22.4 189 F 1 3130 19 08 04 19 16 00 3C48 07 03 33 31.0 285.3 5.4 43.6 -170 1 1 3130 19 16 00 19 20 00 --- 07 07 33 30.4 286.0 5.5 43.4 70 F 1 3161 19 16 04 19 20 00 3C48 07 07 33 30.4 286.0 5.5 43.4 -10 1 1 3161 No stop 19 33 00 --- 07 20 36 28.5 288.3 5.7 42.8 770 F 1 3262 19 20 04 19 35 00 3C138 07 22 36 46.5 224.4 2.0 25.9 -155 1 1 3262 19 35 00 19 41 00 --- 07 28 37 45.8 226.3 2.1 26.8 205 F 1 3308 19 35 04 19 43 00 3C48 07 30 37 27.1 290.1 5.9 42.2 -155 1 1 3308 19 43 00 19 53 00 --- 07 40 39 25.7 291.8 6.0 41.6 445 F 1 3386 19 43 04 19 55 00 DA193 07 42 39 67.5 244.1 1.8 44.5 -148 1 1 3386 19 55 00 20 00 00 --- 07 47 40 66.8 245.9 1.9 45.3 152 F 1 3424 19 55 04 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: ga025b.6cm Matches group j1b6cm in /home/antao/sched/catalogs/freq.dat LO from Spencer 05Jun96, must be using Low patch Setup group: 1 Station: JODRELL1 Total bit rate: 1024 Format: MKIV1:2 Bits per sample: 2 Sample rate: 32.000 Number of channels: 16 Speedup factor: 0.50 Disk used to record data. 1st LO= 4840.00 4840.00 4840.00 4840.00 4840.00 4840.00 4840.00 4840.00 4840.00 4840.00 4840.00 4840.00 4840.00 4840.00 4840.00 4840.00 Net SB= L L U U L L U U L L U U L L U U Pol. = RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP BBC = 2 1 2 1 4 3 4 3 6 5 6 5 8 7 8 7 BBC SB= L L U U L L U U L L U U L L U U IF = 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N The following frequency sets based on this setup were used. Frequency Set: 1 Setup file default. LO sum= 4942.49 4942.49 4942.49 4942.49 4974.49 4974.49 4974.49 4974.49 5006.49 5006.49 5006.49 5006.49 5038.49 5038.49 5038.49 5038.49 BBC fr= 102.49 102.49 102.49 102.49 134.49 134.49 134.49 134.49 166.49 166.49 166.49 166.49 198.49 198.49 198.49 198.49 Bandwd= 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 Track assignments are: track1= 2, 10, 18, 26, 3, 11, 19, 27, 66, 74, 82, 90, 67, 75, 83, 91 barrel=roll_off SOURCE LIST -- 3C48 6cm 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) Error (B1950) (J2000) (Date) (mas) * 3C48 01 34 49.826424 * 01 37 41.299490 01 38 16.031371 0.00 32 54 20.25962 * 33 09 35.13380 33 12 46.21950 0.00 From catalog imbedded in main SCHED input file. 6.656 scan hours, 88.593 baseline hours above horizon. J0521+1638 05 18 16.514010 * 05 21 09.885892 05 21 46.222045 0.34 0518+165 16 35 26.83441 * 16 38 22.05188 16 38 58.16839 0.27 * 3C138 /home/antao/sched/catalogs/sources.vlba J0521+16 VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 0.200 scan hours, 2.346 baseline hours above horizon. J0555+3948 05 52 01.407173 * 05 55 30.805615 05 56 14.928309 0.26 0552+398 39 48 21.94585 * 39 48 49.16500 39 49 02.08506 0.40 * DA193 /home/antao/sched/catalogs/sources.vlba J0555+39 VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 0.367 scan hours, 2.527 baseline hours above horizon. J1642+3948 16 41 17.606227 * 16 42 58.809964 16 43 20.734855 0.26 * 3C345 39 54 10.81495 * 39 48 36.99401 39 47 06.63547 0.40 1641+399 /home/antao/sched/catalogs/sources.vlba J1642+39 VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 0.083 scan hours, 0.500 baseline hours above horizon. J2253+1608 22 51 29.519743 * 22 53 57.747942 22 54 27.680805 0.31 * 3C454.3 15 52 54.34806 * 16 08 53.56089 16 12 05.89703 0.20 2251+158 /home/antao/sched/catalogs/sources.vlba J2253+16 VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 0.067 scan hours, 0.643 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) 3C48 39.7 3C138 79.9 DA193 88.4 3C345 105.0 3C454.3 23.2 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