COVER INFORMATION Station: SHANGHAI (Code Sh ) Experiment: Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam Exp. Code: EG037A Schedule Version: 1.00 Processed by SCHED version: 6.05 June 2006 PI: M. Giroletti Address: INAF Istituto di Radioastronomia Via Gobetti 101 40129 Bologna Italy Phone: +39 051 639 9394 EMAIL: giroletti@ira.inaf.it Fax: +39 051 639 9431 Phone during observation: +39 347 906 6221 Observing mode: Phase-referencing of three sources at 6cm (1 Gb/s) Notes: Schedule for SHANGHAI (Code Sh ) Page 2 Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam 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 ---------------------------------------------------------------------------------------- --- Fri 1 Jun 2007 Day 152 --- 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: 742.49 742.49 742.49 742.49 774.49 774.49 774.49 774.49 806.49 806.49 806.49 806.49 838.49 838.49 838.49 838.49 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 15 30 00 J1221+4411 16 13 45 43.3 -56.7 3.9 85.7 0 1 1 0 15 30 00 15 31 30 =1218+444 16 15 15 43.0 -56.6 3.9 85.5 90 F 1 12 15 30 01 15 31 30 NGC4051 16 15 15 39.8 -55.8 4.2 82.9 -7 1 1 12 15 31 30 15 34 00 --- 16 17 46 39.4 -55.7 4.2 82.5 143 F 1 31 15 31 31 15 34 00 J1221+4411 16 17 46 42.6 -56.6 3.9 85.1 -7 1 1 31 15 34 00 15 35 30 =1218+444 16 19 16 42.3 -56.6 4.0 84.8 83 F 1 43 15 34 01 15 35 30 NGC4051 16 19 16 39.1 -55.6 4.3 82.2 -7 1 1 43 15 35 30 15 38 00 --- 16 21 46 38.6 -55.6 4.3 81.9 143 F 1 62 15 35 31 15 38 00 J1221+4411 16 21 46 41.8 -56.5 4.0 84.4 -7 1 1 62 15 38 00 15 39 30 =1218+444 16 23 16 41.6 -56.5 4.0 84.2 83 F 1 74 15 38 01 15 39 30 NGC4051 16 23 16 38.4 -55.5 4.3 81.6 -7 1 1 74 15 39 30 15 42 00 --- 16 25 47 37.9 -55.4 4.4 81.2 143 F 1 93 15 39 31 15 42 00 J1221+4411 16 25 47 41.1 -56.4 4.1 83.8 -7 1 1 93 15 42 00 15 43 30 =1218+444 16 27 17 40.9 -56.4 4.1 83.6 83 F 1 105 15 42 01 15 45 30 J1308+3546 16 29 17 48.4 -69.6 3.3 81.5 105 1 1 105 15 45 30 15 47 00 --- 16 30 48 48.0 -69.6 3.4 81.3 90 F 1 116 15 45 31 15 47 00 NGC5033 16 30 48 49.2 -68.5 3.3 82.8 -4 1 1 116 15 47 00 15 49 30 --- 16 33 18 48.7 -68.4 3.3 82.5 146 F 1 135 15 47 01 15 49 30 J1308+3546 16 33 18 47.5 -69.4 3.4 81.0 -4 1 1 135 15 49 30 15 51 00 --- 16 34 48 47.2 -69.4 3.4 80.8 86 F 1 147 15 49 31 15 51 00 NGC5033 16 34 48 48.4 -68.4 3.3 82.3 -4 1 1 147 15 51 00 15 53 30 --- 16 37 19 47.9 -68.3 3.4 82.0 146 F 1 166 15 51 01 Schedule for SHANGHAI (Code Sh ) Page 3 Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam 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 ---------------------------------------------------------------------------------------- --- Fri 1 Jun 2007 Day 152 --- 15 53 30 J1308+3546 16 37 19 46.7 -69.2 3.5 80.6 -4 1 1 166 15 53 30 15 55 00 --- 16 38 49 46.4 -69.2 3.5 80.4 86 F 1 178 15 53 31 15 55 00 NGC5033 16 38 49 47.6 -68.2 3.4 81.8 -4 1 1 178 15 55 00 15 57 30 --- 16 41 19 47.1 -68.1 3.5 81.6 146 F 1 197 15 55 01 15 57 30 J1308+3546 16 41 19 45.9 -69.1 3.5 80.1 -4 1 1 197 15 57 30 15 59 00 --- 16 42 50 45.6 -69.0 3.6 80.0 86 F 1 209 15 57 31 16 00 00 J1340+3754 16 43 50 52.1 -66.9 3.1 86.2 47 1 1 209 16 00 00 16 01 30 =1338+381 16 45 20 51.8 -66.9 3.1 86.0 90 F 1 221 16 00 01 16 01 30 NGC5273 16 45 20 51.9 -70.6 3.0 83.3 -6 1 1 221 16 01 30 16 04 00 --- 16 47 50 51.4 -70.5 3.1 83.0 144 F 1 240 16 01 31 16 04 00 J1340+3754 16 47 50 51.3 -66.8 3.1 85.6 -6 1 1 240 16 04 00 16 05 30 =1338+381 16 49 21 51.0 -66.8 3.1 85.4 84 F 1 252 16 04 01 16 05 30 NGC5273 16 49 21 51.1 -70.4 3.1 82.9 -6 1 1 252 16 05 30 16 08 00 --- 16 51 51 50.6 -70.3 3.2 82.6 144 F 1 271 16 05 31 16 08 00 J1340+3754 16 51 51 50.5 -66.7 3.2 85.1 -6 1 1 271 16 08 00 16 09 30 =1338+381 16 53 21 50.2 -66.7 3.2 84.9 84 F 1 283 16 08 01 16 09 30 NGC5273 16 53 21 50.3 -70.2 3.2 82.4 -6 1 1 283 16 09 30 16 12 00 --- 16 55 52 49.8 -70.1 3.2 82.1 144 F 1 302 16 09 31 16 12 00 J1340+3754 16 55 52 49.7 -66.6 3.3 84.6 -6 1 1 302 16 12 00 16 13 30 =1338+381 16 57 22 49.4 -66.5 3.3 84.4 84 F 1 314 16 12 01 16 15 30 J1221+4411 16 59 22 35.2 -55.2 4.6 78.7 94 1 1 314 16 15 30 16 17 00 =1218+444 17 00 53 34.9 -55.2 4.7 78.4 90 F 1 325 16 15 31 16 17 00 NGC4051 17 00 53 31.8 -53.9 5.0 75.9 -7 1 1 325 16 17 00 16 19 30 --- 17 03 23 31.4 -53.8 5.0 75.6 143 F 1 344 16 17 01 16 19 30 J1221+4411 17 03 23 34.5 -55.1 4.7 78.1 -7 1 1 344 16 19 30 16 21 00 =1218+444 17 04 53 34.2 -55.0 4.7 77.8 83 F 1 356 16 19 31 16 21 00 NGC4051 17 04 53 31.1 -53.7 5.0 75.4 -7 1 1 356 16 21 00 16 23 30 --- 17 07 24 30.7 -53.6 5.1 75.0 143 F 1 375 16 21 01 16 23 30 J1221+4411 17 07 24 33.8 -54.9 4.8 77.5 -7 1 1 375 16 23 30 16 25 00 =1218+444 17 08 54 33.5 -54.8 4.8 77.3 83 F 1 387 16 23 31 Schedule for SHANGHAI (Code Sh ) Page 4 Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam 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 ---------------------------------------------------------------------------------------- --- Fri 1 Jun 2007 Day 152 --- 16 25 00 NGC4051 17 08 54 30.4 -53.5 5.1 74.8 -7 1 1 387 16 25 00 16 27 30 --- 17 11 24 30.0 -53.4 5.1 74.4 143 F 1 406 16 25 01 16 27 30 J1221+4411 17 11 24 33.1 -54.7 4.8 76.9 -7 1 1 406 16 27 30 16 29 00 =1218+444 17 12 55 32.8 -54.6 4.9 76.7 83 F 1 418 16 27 31 16 31 00 J1308+3546 17 14 55 39.3 -67.2 4.1 76.5 105 1 1 418 16 31 00 16 32 30 --- 17 16 25 39.0 -67.1 4.1 76.3 90 F 1 430 16 31 01 16 32 30 NGC5033 17 16 25 40.2 -66.3 4.0 77.5 -4 1 1 430 16 32 30 16 35 00 --- 17 18 56 39.7 -66.2 4.1 77.3 146 F 1 449 16 32 31 16 35 00 J1308+3546 17 18 56 38.5 -66.9 4.2 76.1 -4 1 1 449 16 35 00 16 36 30 --- 17 20 26 38.2 -66.8 4.2 75.9 86 F 1 461 16 35 01 16 36 30 NGC5033 17 20 26 39.4 -66.1 4.1 77.1 -4 1 1 461 16 36 30 16 39 00 --- 17 22 56 38.9 -66.0 4.2 76.8 146 F 1 480 16 36 31 16 39 00 J1308+3546 17 22 56 37.7 -66.7 4.2 75.6 -4 1 1 480 16 39 00 16 40 30 --- 17 24 26 37.4 -66.6 4.3 75.5 86 F 1 492 16 39 01 16 40 30 NGC5033 17 24 26 38.6 -65.9 4.2 76.6 -4 1 1 492 16 40 30 16 43 00 --- 17 26 57 38.1 -65.7 4.2 76.4 146 F 1 511 16 40 31 16 43 00 J1308+3546 17 26 57 36.9 -66.4 4.3 75.2 -4 1 1 511 16 43 00 16 44 30 --- 17 28 27 36.6 -66.3 4.3 75.0 86 F 1 523 16 43 01 16 45 30 J1340+3754 17 29 27 43.1 -65.3 3.8 80.3 47 1 1 523 16 45 30 16 47 00 =1338+381 17 30 58 42.8 -65.3 3.8 80.1 90 F 1 534 16 45 31 16 47 00 NGC5273 17 30 58 42.7 -68.4 3.8 78.3 -5 1 1 534 16 47 00 16 49 30 --- 17 33 28 42.2 -68.2 3.8 78.0 145 F 1 554 16 47 01 16 49 30 J1340+3754 17 33 28 42.3 -65.1 3.9 79.8 -5 1 1 554 16 49 30 16 51 00 =1338+381 17 34 58 42.0 -65.1 3.9 79.6 85 F 1 565 16 49 31 16 51 00 NGC5273 17 34 58 41.9 -68.1 3.9 77.9 -5 1 1 565 16 51 00 16 53 30 --- 17 37 29 41.5 -68.0 3.9 77.6 145 F 1 584 16 51 01 16 53 30 J1340+3754 17 37 29 41.6 -64.9 3.9 79.3 -5 1 1 584 16 53 30 16 55 00 =1338+381 17 38 59 41.3 -64.9 4.0 79.2 85 F 1 596 16 53 31 16 55 00 NGC5273 17 38 59 41.2 -67.9 3.9 77.4 -5 1 1 596 16 55 00 16 57 30 --- 17 41 29 40.7 -67.8 4.0 77.2 145 F 1 615 16 55 01 Schedule for SHANGHAI (Code Sh ) Page 5 Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam 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 ---------------------------------------------------------------------------------------- --- Fri 1 Jun 2007 Day 152 --- 16 57 30 J1340+3754 17 41 29 40.8 -64.8 4.0 78.9 -5 1 1 615 16 57 30 16 59 00 =1338+381 17 43 00 40.5 -64.7 4.0 78.7 85 F 1 627 16 57 31 17 01 00 J1221+4411 17 45 00 27.3 -52.8 5.4 72.0 96 1 1 627 17 01 00 17 02 30 =1218+444 17 46 30 27.0 -52.7 5.4 71.8 90 F 1 639 17 01 01 17 02 30 NGC4051 17 46 30 24.0 -51.2 5.7 69.2 -7 1 1 639 17 02 30 17 05 00 --- 17 49 01 23.6 -51.0 5.8 68.9 143 F 1 658 17 02 31 17 05 00 J1221+4411 17 49 01 26.6 -52.6 5.5 71.4 -7 1 1 658 17 05 00 17 06 30 =1218+444 17 50 31 26.3 -52.5 5.5 71.2 83 F 1 670 17 05 01 17 06 30 NGC4051 17 50 31 23.4 -50.9 5.8 68.6 -7 1 1 670 17 06 30 17 09 00 --- 17 53 01 23.0 -50.7 5.8 68.3 143 F 1 689 17 06 31 17 09 00 J1221+4411 17 53 01 25.9 -52.3 5.5 70.8 -7 1 1 689 17 09 00 17 10 30 =1218+444 17 54 31 25.6 -52.2 5.5 70.6 83 F 1 701 17 09 01 17 10 30 NGC4051 17 54 31 22.7 -50.6 5.8 68.1 -7 1 1 701 17 10 30 17 13 00 --- 17 57 02 22.3 -50.4 5.9 67.7 143 F 1 720 17 10 31 17 13 00 J1221+4411 17 57 02 25.2 -52.0 5.6 70.2 -7 1 1 720 17 13 00 17 14 30 =1218+444 17 58 32 25.0 -51.9 5.6 70.0 83 F 1 732 17 13 01 17 16 30 J1308+3546 18 00 32 30.4 -64.1 4.9 71.6 106 1 1 732 17 16 30 17 18 00 --- 18 02 03 30.1 -64.0 4.9 71.4 90 F 1 743 17 16 31 17 18 00 NGC5033 18 02 03 31.3 -63.4 4.8 72.4 -4 1 1 743 17 18 00 17 20 30 --- 18 04 33 30.8 -63.3 4.8 72.2 146 F 1 763 17 18 01 17 20 30 J1308+3546 18 04 33 29.6 -63.8 4.9 71.1 -4 1 1 763 17 20 30 17 22 00 --- 18 06 03 29.3 -63.7 5.0 71.0 86 F 1 774 17 20 31 17 22 00 NGC5033 18 06 03 30.5 -63.1 4.9 72.0 -4 1 1 774 17 22 00 17 24 30 --- 18 08 34 30.1 -63.0 4.9 71.7 146 F 1 793 17 22 01 17 24 30 J1308+3546 18 08 34 28.8 -63.5 5.0 70.7 -4 1 1 793 17 24 30 17 26 00 --- 18 10 04 28.5 -63.4 5.0 70.5 86 F 1 805 17 24 31 17 26 00 NGC5033 18 10 04 29.8 -62.9 4.9 71.5 -4 1 1 805 17 26 00 17 28 30 --- 18 12 34 29.3 -62.7 5.0 71.3 146 F 1 824 17 26 01 17 28 30 J1308+3546 18 12 34 28.1 -63.2 5.1 70.3 -4 1 1 824 17 28 30 17 30 00 --- 18 14 05 27.8 -63.0 5.1 70.1 86 F 1 836 17 28 31 Schedule for SHANGHAI (Code Sh ) Page 6 Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam 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 ---------------------------------------------------------------------------------------- --- Fri 1 Jun 2007 Day 152 --- 17 31 00 J1340+3754 18 15 05 34.3 -62.9 4.6 74.9 47 1 1 836 17 31 00 17 32 30 =1338+381 18 16 35 34.0 -62.8 4.6 74.7 90 F 1 848 17 31 01 17 32 30 NGC5273 18 16 35 33.8 -65.5 4.6 73.4 -5 1 1 848 17 32 30 17 35 00 --- 18 19 05 33.3 -65.3 4.6 73.1 145 F 1 867 17 32 31 17 35 00 J1340+3754 18 19 05 33.6 -62.6 4.6 74.4 -5 1 1 867 17 35 00 17 36 30 =1338+381 18 20 36 33.3 -62.5 4.7 74.2 85 F 1 879 17 35 01 17 36 30 NGC5273 18 20 36 33.0 -65.2 4.6 73.0 -5 1 1 879 17 36 30 17 39 00 --- 18 23 06 32.5 -65.0 4.7 72.7 145 F 1 898 17 36 31 17 39 00 J1340+3754 18 23 06 32.8 -62.3 4.7 73.9 -5 1 1 898 17 39 00 17 40 30 =1338+381 18 24 36 32.5 -62.2 4.7 73.7 85 F 1 910 17 39 01 17 40 30 NGC5273 18 24 36 32.2 -64.9 4.7 72.6 -5 1 1 910 17 40 30 17 43 00 --- 18 27 07 31.7 -64.7 4.7 72.3 145 F 1 929 17 40 31 17 43 00 J1340+3754 18 27 07 32.0 -62.1 4.8 73.4 -5 1 1 929 17 43 00 17 44 30 =1338+381 18 28 37 31.8 -62.0 4.8 73.3 85 F 1 941 17 43 01 17 46 30 J1221+4411 18 30 37 19.6 -49.6 6.1 65.3 98 1 1 941 17 46 30 17 48 00 =1218+444 18 32 08 19.4 -49.5 6.2 65.1 90 F 1 952 17 46 31 17 48 00 NGC4051 18 32 08 16.6 -47.6 6.5 62.5 -7 1 1 952 17 48 00 17 50 30 --- 18 34 38 16.2 -47.4 6.5 62.1 143 F 1 972 17 48 01 17 50 30 J1221+4411 18 34 38 19.0 -49.3 6.2 64.7 -7 1 1 972 17 50 30 17 52 00 =1218+444 18 36 08 18.8 -49.1 6.2 64.5 83 F 1 983 17 50 31 17 52 00 NGC4051 18 36 08 16.0 -47.3 6.5 61.9 -7 1 1 983 17 52 00 17 54 30 --- 18 38 39 15.6 -47.0 6.6 61.5 143 F 1 1003 17 52 01 17 54 30 J1221+4411 18 38 39 18.3 -48.9 6.3 64.1 -7 1 1 1003 17 54 30 17 56 00 =1218+444 18 40 09 18.1 -48.8 6.3 63.9 83 F 1 1014 17 54 31 17 56 00 NGC4051 18 40 09 15.4 -46.9 6.6 61.2 -7 1 1 1014 17 56 00 17 58 30 --- 18 42 39 15.0 -46.7 6.7 60.9 143 F 1 1033 17 56 01 17 58 30 J1221+4411 18 42 39 17.7 -48.6 6.3 63.5 -7 1 1 1033 17 58 30 18 00 00 =1218+444 18 44 10 17.5 -48.5 6.4 63.3 83 F 1 1045 17 58 31 18 02 00 J1308+3546 18 46 10 21.7 -60.4 5.6 66.5 106 1 1 1045 18 02 00 18 03 30 --- 18 47 40 21.4 -60.3 5.6 66.4 90 F 1 1057 18 02 01 Schedule for SHANGHAI (Code Sh ) Page 7 Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam 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 ---------------------------------------------------------------------------------------- --- Fri 1 Jun 2007 Day 152 --- 18 03 30 NGC5033 18 47 40 22.7 -59.9 5.6 67.2 -4 1 1 1057 18 03 30 18 06 00 --- 18 50 11 22.2 -59.7 5.6 67.0 146 F 1 1076 18 03 31 18 06 00 J1308+3546 18 50 11 21.0 -60.0 5.7 66.1 -4 1 1 1076 18 06 00 18 07 30 --- 18 51 41 20.7 -59.9 5.7 65.9 86 F 1 1088 18 06 01 18 07 30 NGC5033 18 51 41 22.0 -59.6 5.6 66.8 -4 1 1 1088 18 07 30 18 10 00 --- 18 54 11 21.5 -59.3 5.7 66.5 146 F 1 1107 18 07 31 18 10 00 J1308+3546 18 54 11 20.2 -59.7 5.8 65.6 -4 1 1 1107 18 10 00 18 11 30 --- 18 55 41 20.0 -59.6 5.8 65.4 86 F 1 1119 18 10 01 18 11 30 NGC5033 18 55 41 21.2 -59.2 5.7 66.3 -4 1 1 1119 18 11 30 18 14 00 --- 18 58 12 20.8 -59.0 5.7 66.0 146 F 1 1138 18 11 31 18 14 00 J1308+3546 18 58 12 19.5 -59.3 5.8 65.1 -4 1 1 1138 18 14 00 18 15 30 --- 18 59 42 19.2 -59.2 5.8 65.0 86 F 1 1150 18 14 01 18 16 30 J1340+3754 19 00 42 25.8 -59.7 5.3 69.4 47 1 1 1150 18 16 30 18 18 00 =1338+381 19 02 12 25.5 -59.6 5.4 69.3 90 F 1 1161 18 16 31 18 18 00 NGC5273 19 02 12 25.0 -62.0 5.3 68.5 -4 1 1 1161 18 18 00 18 20 30 --- 19 04 43 24.5 -61.8 5.4 68.2 146 F 1 1181 18 18 01 18 20 30 J1340+3754 19 04 43 25.0 -59.4 5.4 69.0 -4 1 1 1181 18 20 30 18 22 00 =1338+381 19 06 13 24.7 -59.2 5.4 68.8 86 F 1 1192 18 20 31 18 22 00 NGC5273 19 06 13 24.2 -61.7 5.4 68.0 -4 1 1 1192 18 22 00 18 24 30 --- 19 08 44 23.8 -61.5 5.4 67.7 146 F 1 1212 18 22 01 18 24 30 J1340+3754 19 08 44 24.3 -59.0 5.5 68.5 -4 1 1 1212 18 24 30 18 26 00 =1338+381 19 10 14 24.0 -58.9 5.5 68.3 86 F 1 1223 18 24 31 18 26 00 NGC5273 19 10 14 23.5 -61.4 5.5 67.6 -4 1 1 1223 18 26 00 18 28 30 --- 19 12 44 23.0 -61.1 5.5 67.3 146 F 1 1243 18 26 01 18 28 30 J1340+3754 19 12 44 23.5 -58.7 5.5 68.0 -4 1 1 1243 18 28 30 18 30 00 =1338+381 19 14 14 23.3 -58.6 5.6 67.8 86 F 1 1254 18 28 31 18 42 00 3C345 19 26 16 56.0 -63.7 2.7 91.9 663 1 1 1254 18 42 00 18 53 00 --- 19 37 18 53.9 -63.8 2.9 90.1 660 F 1 1339 18 42 01 18 59 00 J1308+3546 19 43 19 11.4 -54.9 6.6 59.7 287 1 1 1339 18 59 00 19 01 00 --- 19 45 20 11.0 -54.7 6.6 59.5 120 F 1 1355 18 59 01 Schedule for SHANGHAI (Code Sh ) Page 8 Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam 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 ---------------------------------------------------------------------------------------- --- Fri 1 Jun 2007 Day 152 --- 19 01 00 NGC5033 19 45 20 12.3 -54.5 6.5 60.2 -4 1 1 1355 19 01 00 19 03 30 --- 19 47 50 11.9 -54.3 6.6 59.9 146 F 1 1374 19 01 01 19 03 30 J1308+3546 19 47 50 10.6 -54.5 6.7 59.1 -4 1 1 1374 19 03 30 19 05 00 --- 19 49 20 10.3 -54.3 6.7 59.0 86 F 1 1386 19 03 31 19 05 00 NGC5033 19 49 20 11.6 -54.1 6.6 59.7 -4 1 1 1386 19 05 00 19 07 30 --- 19 51 51 11.2 -53.9 6.6 59.4 146 F 1 1405 19 05 01 19 07 30 J1308+3546 19 51 51 9.9 -54.0 6.7 58.6 -4 1 1 1405 19 07 30 19 09 00 --- 19 53 21 9.6 -53.9 6.7 58.4 86 F 1 1417 19 07 31 19 09 00 NGC5033 19 53 21 10.9 -53.7 6.7 59.2 -4 1 1 1417 19 09 00 19 11 30 --- 19 55 51 10.5 -53.4 6.7 58.9 146 F 1 1436 19 09 01 19 11 30 J1308+3546 19 55 51 9.2 -53.6 6.8 58.1 -4 1 1 1436 19 11 30 19 13 00 --- 19 57 22 8.9 -53.4 6.8 57.9 86 F 1 1448 19 11 31 19 15 00 J1340+3754 19 59 22 15.2 -54.6 6.3 62.2 108 1 1 1448 19 15 00 19 17 00 =1338+381 20 01 22 14.9 -54.4 6.3 61.9 120 F 1 1463 19 15 01 19 17 00 NGC5273 20 01 22 14.1 -56.6 6.3 61.6 -4 1 1 1463 19 17 00 19 19 30 --- 20 03 53 13.6 -56.4 6.4 61.3 146 F 1 1482 19 17 01 19 19 30 J1340+3754 20 03 53 14.4 -54.2 6.4 61.6 -4 1 1 1482 19 19 30 19 21 00 =1338+381 20 05 23 14.2 -54.0 6.4 61.4 86 F 1 1494 19 19 31 19 21 00 NGC5273 20 05 23 13.4 -56.2 6.4 61.1 -4 1 1 1494 19 21 00 19 23 30 --- 20 07 53 12.9 -56.0 6.4 60.8 146 F 1 1513 19 21 01 19 23 30 J1340+3754 20 07 53 13.7 -53.8 6.5 61.1 -4 1 1 1513 19 23 30 19 25 00 =1338+381 20 09 24 13.5 -53.6 6.5 60.9 86 F 1 1525 19 23 31 19 25 00 NGC5273 20 09 24 12.7 -55.8 6.4 60.6 -4 1 1 1525 19 25 00 19 27 30 --- 20 11 54 12.2 -55.6 6.5 60.3 146 F 1 1544 19 25 01 19 27 30 J1340+3754 20 11 54 13.0 -53.4 6.5 60.6 -4 1 1 1544 19 27 30 19 29 00 =1338+381 20 13 24 12.8 -53.2 6.5 60.4 86 F 1 1556 19 27 31 19 31 00 J1308+3546 20 15 24 5.9 -51.4 7.1 55.6 107 1 1 1556 19 31 00 19 32 30 --- 20 16 55 5.6 -51.2 7.1 55.4 90 F 1 1568 19 31 01 19 32 30 NGC5033 20 16 55 6.9 -51.1 7.1 56.1 -4 1 1 1568 19 32 30 19 35 00 --- 20 19 25 6.5 -50.9 7.1 55.8 146 F 1 1587 19 32 31 Schedule for SHANGHAI (Code Sh ) Page 9 Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam 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 ---------------------------------------------------------------------------------------- --- Fri 1 Jun 2007 Day 152 --- 19 35 00 J1308+3546 20 19 25 5.2 -51.0 7.2 55.0 -4 1 1 1587 19 35 00 19 36 30 --- 20 20 55 5.0 -50.8 7.2 D 54.8 0 F 1 1599 19 35 01 19 36 30 NGC5033 20 20 55 6.3 -50.7 7.1 55.6 -4 1 1 1599 19 36 30 19 39 00 --- 20 23 26 5.9 -50.4 7.2 55.2 146 F 1 1618 19 36 31 19 40 30 NGC5033 20 24 56 5.6 -50.2 7.2 55.0 88 1 1 1618 19 40 30 19 43 00 --- 20 27 26 5.2 -49.9 7.2 54.7 150 F 1 1637 19 40 31 19 46 30 J1340+3754 20 30 57 9.8 -51.4 6.8 58.0 200 1 1 1637 19 46 30 19 48 00 =1338+381 20 32 27 9.5 -51.3 6.9 57.8 90 F 1 1649 19 46 31 19 48 00 NGC5273 20 32 27 8.6 -53.4 6.8 57.7 -4 1 1 1649 19 48 00 19 50 30 --- 20 34 58 8.2 -53.1 6.9 57.4 146 F 1 1668 19 48 01 19 50 30 J1340+3754 20 34 58 9.1 -51.0 6.9 57.5 -4 1 1 1668 19 50 30 19 52 00 =1338+381 20 36 28 8.9 -50.8 6.9 57.3 86 F 1 1680 19 50 31 19 52 00 NGC5273 20 36 28 8.0 -53.0 6.9 57.2 -4 1 1 1680 19 52 00 19 54 30 --- 20 38 58 7.5 -52.7 6.9 56.9 146 F 1 1699 19 52 01 19 54 30 J1340+3754 20 38 58 8.5 -50.6 7.0 56.9 -4 1 1 1699 19 54 30 19 56 00 =1338+381 20 40 29 8.2 -50.4 7.0 56.7 86 F 1 1711 19 54 31 19 56 00 NGC5273 20 40 29 7.3 -52.5 7.0 56.7 -4 1 1 1711 19 56 00 19 58 30 --- 20 42 59 6.8 -52.2 7.0 56.4 146 F 1 1730 19 56 01 19 58 30 J1340+3754 20 42 59 7.8 -50.1 7.0 56.4 -4 1 1 1730 19 58 30 20 00 00 =1338+381 20 44 29 7.6 -50.0 7.1 56.2 86 F 1 1742 19 58 31 21 46 00 3C345 22 30 47 21.5 -55.5 5.8 66.8 6335 1 1 1742 21 46 00 21 57 00 --- 22 41 48 19.6 -54.6 6.0 65.3 660 F 1 1827 21 46 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: eg037a.6cm Matches group sh6cm in /irasoft/sched/catalogs/freq.dat Dual-pol available since summer 2005 (CR 051122). Setup group: 7 Station: SHANGHAI 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= 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 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 = 1 2 1 2 3 4 3 4 5 6 5 6 7 8 7 8 BBC SB= L L U U L L U U L L U U L L U U IF = C A C A C A C A C A C A C A C A The following frequency sets based on this setup were used. Frequency Set: 7 Setup file default. Used pcal sets: 1 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= 742.49 742.49 742.49 742.49 774.49 774.49 774.49 774.49 806.49 806.49 806.49 806.49 838.49 838.49 838.49 838.49 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 The following pulse cal sets were used with this setup: Pulse cal detection set: 1 PCAL = 1MHZ PCALXB1= S1 S3 S5 S7 S9 S11 S13 S15 PCALXB2= S2 S4 S6 S8 S10 S12 S14 S16 PCALFR1= 490 510 490 510 490 510 490 510 PCALFR2= 490 510 490 510 490 510 490 510 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 -- Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam 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) * NGC4051 12 00 36.396526 * 12 03 09.613000 12 03 33.683915 0.00 44 48 34.49046 * 44 31 52.65000 44 29 33.48252 0.00 From catalog imbedded in main SCHED input file. 1.250 scan hours, 29.525 baseline hours above horizon. * NGC5033 13 11 09.172609 * 13 13 27.475000 13 13 49.569781 0.00 36 51 30.38369 * 36 35 37.94000 36 33 20.07013 0.00 From catalog imbedded in main SCHED input file. 1.333 scan hours, 35.439 baseline hours above horizon. * NGC5273 13 39 55.142349 * 13 42 08.370000 13 42 29.824721 0.00 35 54 21.44090 * 35 39 15.33000 35 37 02.38011 0.00 From catalog imbedded in main SCHED input file. 1.333 scan hours, 34.865 baseline hours above horizon. * J1221+4411 12 18 59.032728 * 12 21 27.044650 12 21 50.467548 0.42 1218+444 44 28 07.64767 * 44 11 29.67155 44 09 10.01409 0.60 /irasoft/sched/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 1.000 scan hours, 22.003 baseline hours above horizon. * J1308+3546 13 06 03.930616 * 13 08 23.709146 13 08 45.976769 0.27 36 02 36.26229 * 35 46 37.16399 35 44 18.39533 0.45 /irasoft/sched/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 1.083 scan hours, 26.565 baseline hours above horizon. * J1340+3754 13 38 11.121586 * 13 40 22.951814 13 40 44.250726 0.33 1338+381 38 09 53.16408 * 37 54 43.83329 37 52 31.03015 0.49 J1340+37 /irasoft/sched/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 1.083 scan hours, 27.754 baseline hours above horizon. J1642+3948 16 41 17.606231 * 16 42 58.809968 16 43 15.877211 0.26 1641+399 39 54 10.81494 * 39 48 36.99400 39 47 37.94371 0.40 * 3C345 /irasoft/sched/catalogs/sources.vlba J1642+39 VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.367 scan hours, 13.200 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) NGC4051 88.8 NGC5033 104.2 NGC5273 109.0 J1221+4411 91.7 J1308+3546 104.0 J1340+3754 107.1 3C345 118.1 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