COVER INFORMATION Station: SHANGHAI (Code Sh ) Experiment: VLBI observations at 18 cm of faint nuclear sources in the BCS Sample. Exp. Code: EL040A Schedule Version: 2.00 Processed by SCHED version: 9.30 Release near March 23, 2010 PI: Elisabetta Liuzzo Address: IRA-INAF via Piero Gobetti, 101 Bologna Italy Phone: +39-051-6399364 EMAIL: liuzzo@ira.inaf.it Fax: Phone during observation: +39-339-4697414 Observing mode: Continuum Notes: Schedule for SHANGHAI (Code Sh ) Page 2 VLBI observations at 18 cm of faint nuclear sources in the BCS Sample. 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 6 Jun 2010 Day 157 --- Next scan frequencies: 1610.49 1610.49 1610.49 1610.49 1642.49 1642.49 1642.49 1642.49 1674.49 1674.49 1674.49 1674.49 1706.49 1706.49 1706.49 1706.49 Next BBC frequencies: 689.51 689.51 689.51 689.51 657.51 657.51 657.51 657.51 625.51 625.51 625.51 625.51 593.51 593.51 593.51 593.51 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 14 00 00 J1249+2817 15 04 18 60.8 273.1 2.2 76.1 0 1 1 0 14 00 00 14 01 30 =1246+285 15 05 48 60.4 273.2 2.3 76.0 90 F 1 12 14 00 01 14 01 58 1256 15 06 16 62.4 271.4 2.1 75.5 20 1 1 12 14 01 58 14 05 28 --- 15 09 46 61.7 271.8 2.2 75.5 210 F 1 39 14 01 59 14 05 56 J1249+2817 15 10 15 59.5 273.7 2.3 75.9 21 1 1 39 14 05 56 14 07 26 =1246+285 15 11 45 59.2 273.9 2.4 75.9 90 F 1 50 14 05 57 14 07 54 1256 15 12 13 61.1 272.1 2.2 75.4 20 1 1 50 14 07 54 14 11 24 --- 15 15 44 60.4 272.5 2.3 75.4 210 F 1 77 14 07 55 14 11 53 J1249+2817 15 16 12 58.2 274.3 2.4 75.7 21 1 1 77 14 11 53 14 13 23 =1246+285 15 17 42 57.9 274.5 2.5 75.7 90 F 1 89 14 11 54 14 13 51 1256 15 18 10 59.9 272.7 2.3 75.3 20 1 1 89 14 13 51 14 17 21 --- 15 21 41 59.1 273.1 2.4 75.3 210 F 1 116 14 13 52 14 17 49 J1249+2817 15 22 10 56.9 274.9 2.5 75.5 21 1 1 116 14 17 49 14 19 19 =1246+285 15 23 40 56.6 275.1 2.6 75.5 90 F 1 128 14 17 50 14 19 47 1256 15 24 08 58.6 273.4 2.4 75.2 20 1 1 128 14 19 47 14 23 17 --- 15 27 38 57.8 273.8 2.5 75.1 210 F 1 155 14 19 48 14 24 13 J1342+2709 15 28 35 66.6 266.9 1.8 73.8 38 1 1 155 14 24 13 14 25 43 =1339+274 15 30 05 66.3 267.1 1.8 73.9 90 F 1 166 14 24 14 14 26 13 1347 15 30 35 68.2 268.8 1.7 76.3 22 1 1 166 14 26 13 14 29 43 --- 15 34 05 67.4 269.3 1.7 76.4 210 F 1 194 14 26 14 14 30 14 J1342+2709 15 34 36 65.3 267.8 1.9 74.0 23 1 1 194 14 30 14 14 31 44 =1339+274 15 36 06 65.0 268.0 1.9 74.0 90 F 1 205 14 30 15 Schedule for SHANGHAI (Code Sh ) Page 3 VLBI observations at 18 cm of faint nuclear sources in the BCS Sample. 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 6 Jun 2010 Day 157 --- 14 32 13 1347 15 36 36 66.9 269.6 1.8 76.4 22 1 1 205 14 32 13 14 35 43 --- 15 40 07 66.1 270.1 1.8 76.4 210 F 1 232 14 32 14 14 36 14 J1342+2709 15 40 37 64.0 268.7 2.0 74.1 23 1 1 232 14 36 14 14 37 44 =1339+274 15 42 08 63.7 268.9 2.0 74.1 90 F 1 244 14 36 15 14 38 14 1347 15 42 38 65.6 270.4 1.9 76.4 23 1 1 244 14 38 14 14 41 44 --- 15 46 08 64.8 270.9 1.9 76.3 210 F 1 271 14 38 15 14 42 15 J1342+2709 15 46 39 62.7 269.5 2.1 74.1 23 1 1 271 14 42 15 14 43 45 =1339+274 15 48 09 62.4 269.7 2.1 74.1 90 F 1 283 14 42 16 14 44 14 1347 15 48 39 64.3 271.2 2.0 76.3 23 1 1 283 14 44 14 14 47 44 --- 15 52 10 63.5 271.6 2.0 76.3 210 F 1 310 14 44 15 14 49 00 J1443+2501 15 53 26 73.6 252.4 1.1 64.2 52 1 1 310 14 49 00 14 50 30 =1441+252 15 54 56 73.3 252.9 1.2 64.5 90 F 1 321 14 49 01 14 51 00 1430 15 55 26 70.8 256.1 1.4 66.4 22 1 1 321 14 51 00 14 54 30 --- 15 58 56 70.1 257.1 1.4 66.9 210 F 1 348 14 51 01 14 54 59 J1443+2501 15 59 25 72.4 254.3 1.2 65.4 21 1 1 348 14 54 59 14 56 29 =1441+252 16 00 56 72.1 254.8 1.3 65.7 90 F 1 360 14 55 00 14 56 59 1430 16 01 25 69.6 257.7 1.5 67.3 21 1 1 360 14 56 59 15 00 29 --- 16 04 56 68.9 258.6 1.5 67.7 210 F 1 387 14 57 00 15 00 57 J1443+2501 16 05 25 71.2 256.1 1.3 66.5 21 1 1 387 15 00 57 15 02 27 =1441+252 16 06 55 70.8 256.5 1.4 66.7 90 F 1 399 15 00 58 15 02 57 1430 16 07 25 68.3 259.2 1.6 68.0 21 1 1 399 15 02 57 15 06 27 --- 16 10 56 67.6 260.0 1.6 68.3 210 F 1 426 15 02 58 15 06 56 J1443+2501 16 11 25 69.9 257.7 1.4 67.4 21 1 1 426 15 06 56 15 08 26 =1441+252 16 12 55 69.6 258.1 1.5 67.6 90 F 1 437 15 06 57 15 08 56 1430 16 13 25 67.1 260.5 1.7 68.6 21 1 1 437 15 08 56 15 12 26 --- 16 16 55 66.3 261.2 1.7 68.9 210 F 1 464 15 08 57 15 14 31 J1249+2817 16 19 00 44.9 280.3 3.5 73.0 85 1 1 464 15 14 31 15 16 01 =1246+285 16 20 31 44.6 280.4 3.5 72.9 90 F 1 476 15 14 32 15 16 28 1256 16 20 59 46.5 279.0 3.4 73.0 21 1 1 476 15 16 28 15 19 58 --- 16 24 29 45.8 279.4 3.4 72.9 210 F 1 503 15 16 29 Schedule for SHANGHAI (Code Sh ) Page 4 VLBI observations at 18 cm of faint nuclear sources in the BCS Sample. 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 6 Jun 2010 Day 157 --- 15 20 27 J1249+2817 16 24 58 43.6 280.9 3.6 72.7 21 1 1 503 15 20 27 15 21 57 =1246+285 16 26 28 43.3 281.0 3.6 72.6 90 F 1 515 15 20 28 15 22 25 1256 16 26 56 45.2 279.6 3.5 72.7 21 1 1 515 15 22 25 15 25 55 --- 16 30 27 44.5 279.9 3.5 72.6 210 F 1 542 15 22 26 15 26 24 J1249+2817 16 30 56 42.4 281.4 3.7 72.3 21 1 1 542 15 26 24 15 27 54 =1246+285 16 32 26 42.1 281.5 3.7 72.2 90 F 1 554 15 26 25 15 28 22 1256 16 32 54 44.0 280.1 3.5 72.4 21 1 1 554 15 28 22 15 31 52 --- 16 36 24 43.2 280.5 3.6 72.2 210 F 1 581 15 28 23 15 32 20 J1249+2817 16 36 53 41.1 281.9 3.8 72.0 21 1 1 581 15 32 20 15 33 50 =1246+285 16 38 23 40.8 282.1 3.8 71.9 90 F 1 592 15 32 21 15 34 18 1256 16 38 51 42.7 280.7 3.6 72.1 21 1 1 592 15 34 18 15 37 48 --- 16 42 22 42.0 281.0 3.7 71.9 210 F 1 619 15 34 19 15 38 46 J1342+2709 16 43 20 50.6 276.0 3.0 73.1 39 1 1 619 15 38 46 15 40 16 =1339+274 16 44 50 50.3 276.1 3.0 73.0 90 F 1 631 15 38 47 15 40 47 1347 16 45 21 52.2 277.1 2.9 74.7 23 1 1 631 15 40 47 15 44 17 --- 16 48 52 51.5 277.4 3.0 74.5 210 F 1 658 15 40 48 15 44 49 J1342+2709 16 49 24 49.3 276.6 3.1 72.9 24 1 1 658 15 44 49 15 46 19 =1339+274 16 50 54 49.0 276.7 3.1 72.8 90 F 1 670 15 44 50 15 46 50 1347 16 51 25 50.9 277.7 3.0 74.4 24 1 1 670 15 46 50 15 50 20 --- 16 54 55 50.2 278.0 3.1 74.2 210 F 1 697 15 46 51 15 50 51 J1342+2709 16 55 27 48.0 277.2 3.2 72.6 24 1 1 697 15 50 51 15 52 21 =1339+274 16 56 58 47.7 277.3 3.2 72.6 90 F 1 708 15 50 52 15 52 53 1347 16 57 29 49.6 278.2 3.1 74.1 24 1 1 708 15 52 53 15 56 23 --- 17 00 59 48.9 278.6 3.2 73.9 210 F 1 735 15 52 54 15 56 54 J1342+2709 17 01 31 46.7 277.8 3.3 72.4 24 1 1 735 15 56 54 15 58 24 =1339+274 17 03 02 46.4 277.9 3.3 72.3 90 F 1 747 15 56 55 15 58 56 1347 17 03 33 48.3 278.8 3.2 73.8 24 1 1 747 15 58 56 16 02 26 --- 17 07 03 47.6 279.1 3.3 73.6 210 F 1 774 15 58 57 16 03 44 J1443+2501 17 08 22 57.8 268.1 2.4 70.8 57 1 1 774 16 03 44 16 05 14 =1441+252 17 09 52 57.5 268.4 2.4 70.8 90 F 1 786 16 03 45 Schedule for SHANGHAI (Code Sh ) Page 5 VLBI observations at 18 cm of faint nuclear sources in the BCS Sample. 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 6 Jun 2010 Day 157 --- 16 05 44 1430 17 10 22 54.9 269.8 2.6 70.7 22 1 1 786 16 05 44 16 09 14 --- 17 13 53 54.2 270.2 2.7 70.7 210 F 1 813 16 05 45 16 09 43 J1443+2501 17 14 22 56.5 269.0 2.5 70.8 21 1 1 813 16 09 43 16 11 13 =1441+252 17 15 52 56.2 269.2 2.5 70.8 90 F 1 824 16 09 44 16 11 44 1430 17 16 23 53.6 270.5 2.7 70.7 22 1 1 824 16 11 44 16 15 14 --- 17 19 53 52.9 271.0 2.8 70.7 210 F 1 852 16 11 45 16 15 43 J1443+2501 17 20 23 55.2 269.8 2.6 70.9 21 1 1 852 16 15 43 16 17 13 =1441+252 17 21 53 54.9 270.0 2.6 70.9 90 F 1 863 16 15 44 16 17 43 1430 17 22 23 52.4 271.3 2.8 70.7 22 1 1 863 16 17 43 16 21 13 --- 17 25 54 51.6 271.7 2.9 70.6 210 F 1 890 16 17 44 16 21 43 J1443+2501 17 26 24 53.9 270.5 2.7 70.8 21 1 1 890 16 21 43 16 23 13 =1441+252 17 27 54 53.6 270.7 2.7 70.8 90 F 1 902 16 21 44 16 23 43 1430 17 28 24 51.1 272.0 2.9 70.6 22 1 1 902 16 23 43 16 27 13 --- 17 31 55 50.3 272.4 3.0 70.6 210 F 1 929 16 23 44 16 29 44 3C345 17 34 26 76.5 313.5 0.9 126.0 103 1 1 929 16 29 44 16 39 44 --- 17 44 28 74.9 309.2 1.0 120.3 600 F 1 1006 16 29 45 16 43 38 J1249+2817 17 48 22 26.4 288.5 5.0 67.2 149 1 1 1006 16 43 38 16 45 08 =1246+285 17 49 52 26.1 288.7 5.0 67.1 90 F 1 1018 16 43 39 16 45 37 1256 17 50 22 27.9 287.4 4.8 67.6 22 1 1 1018 16 45 37 16 49 07 --- 17 53 53 27.2 287.7 4.9 67.3 210 F 1 1045 16 45 38 16 49 38 J1249+2817 17 54 24 25.2 289.1 5.1 66.7 24 1 1 1045 16 49 38 16 51 08 =1246+285 17 55 54 24.9 289.2 5.1 66.6 90 F 1 1057 16 49 39 16 51 38 1256 17 56 24 26.6 287.9 4.9 67.1 23 1 1 1057 16 51 38 16 55 08 --- 17 59 55 25.9 288.3 5.0 66.9 210 F 1 1084 16 51 39 16 55 40 J1249+2817 18 00 26 23.9 289.7 5.2 66.2 24 1 1 1084 16 55 40 16 57 10 =1246+285 18 01 57 23.6 289.8 5.2 66.1 90 F 1 1095 16 55 41 16 57 40 1256 18 02 27 25.4 288.5 5.0 66.7 23 1 1 1095 16 57 40 17 01 10 --- 18 05 58 24.7 288.9 5.1 66.4 210 F 1 1123 16 57 41 17 01 42 J1249+2817 18 06 30 22.7 290.3 5.3 65.7 24 1 1 1123 17 01 42 17 03 12 =1246+285 18 08 00 22.4 290.4 5.3 65.6 90 F 1 1134 17 01 43 Schedule for SHANGHAI (Code Sh ) Page 6 VLBI observations at 18 cm of faint nuclear sources in the BCS Sample. 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 6 Jun 2010 Day 157 --- 17 03 43 1256 18 08 31 24.2 289.1 5.1 66.2 24 1 1 1134 17 03 43 17 07 13 --- 18 12 01 23.5 289.4 5.2 66.0 210 F 1 1161 17 03 44 17 08 10 J1342+2709 18 12 58 31.7 284.6 4.5 68.6 39 1 1 1161 17 08 10 17 09 40 =1339+274 18 14 29 31.4 284.8 4.5 68.5 90 F 1 1173 17 08 11 17 10 13 1347 18 15 02 33.4 285.3 4.4 69.6 26 1 1 1173 17 10 13 17 13 43 --- 18 18 32 32.7 285.6 4.5 69.4 210 F 1 1200 17 10 14 17 14 18 J1342+2709 18 19 07 30.5 285.2 4.6 68.2 27 1 1 1200 17 14 18 17 15 48 =1339+274 18 20 37 30.2 285.4 4.6 68.1 90 F 1 1212 17 14 19 17 16 21 1347 18 21 11 32.1 285.9 4.5 69.2 26 1 1 1212 17 16 21 17 19 51 --- 18 24 41 31.4 286.2 4.6 69.0 210 F 1 1239 17 16 22 17 20 26 J1342+2709 18 25 16 29.2 285.8 4.7 67.7 27 1 1 1239 17 20 26 17 21 56 =1339+274 18 26 47 28.9 286.0 4.7 67.6 90 F 1 1250 17 20 27 17 22 29 1347 18 27 20 30.9 286.4 4.6 68.8 26 1 1 1250 17 22 29 17 25 59 --- 18 30 51 30.1 286.8 4.7 68.5 210 F 1 1277 17 22 30 17 26 35 J1342+2709 18 31 26 27.9 286.4 4.8 67.3 27 1 1 1277 17 26 35 17 28 05 =1339+274 18 32 56 27.6 286.6 4.8 67.2 90 F 1 1289 17 26 36 17 28 39 1347 18 33 30 29.6 287.0 4.7 68.3 27 1 1 1289 17 28 39 17 32 09 --- 18 37 01 28.9 287.3 4.8 68.1 210 F 1 1316 17 28 40 17 33 27 J1443+2501 18 38 20 38.6 278.6 3.9 69.1 58 1 1 1316 17 33 27 17 34 57 =1441+252 18 39 50 38.3 278.8 3.9 69.0 90 F 1 1328 17 33 28 17 35 29 1430 18 40 22 35.8 279.8 4.1 68.4 24 1 1 1328 17 35 29 17 38 59 --- 18 43 53 35.0 280.2 4.2 68.3 210 F 1 1355 17 35 30 17 39 30 J1443+2501 18 44 24 37.3 279.2 4.0 68.8 23 1 1 1355 17 39 30 17 41 00 =1441+252 18 45 54 37.0 279.4 4.0 68.8 90 F 1 1366 17 39 31 17 41 33 1430 18 46 27 34.5 280.5 4.2 68.1 24 1 1 1366 17 41 33 17 45 03 --- 18 49 57 33.7 280.8 4.3 68.0 210 F 1 1393 17 41 34 17 45 34 J1443+2501 18 50 29 36.0 279.9 4.1 68.6 24 1 1 1393 17 45 34 17 47 04 =1441+252 18 51 59 35.7 280.0 4.1 68.5 90 F 1 1405 17 45 35 17 47 37 1430 18 52 32 33.2 281.1 4.3 67.9 24 1 1 1405 17 47 37 17 51 07 --- 18 56 03 32.5 281.4 4.4 67.7 210 F 1 1432 17 47 38 Schedule for SHANGHAI (Code Sh ) Page 7 VLBI observations at 18 cm of faint nuclear sources in the BCS Sample. 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 6 Jun 2010 Day 157 --- 17 51 39 J1443+2501 18 56 34 34.8 280.5 4.2 68.3 24 1 1 1432 17 51 39 17 53 09 =1441+252 18 58 05 34.4 280.6 4.2 68.2 90 F 1 1444 17 51 40 17 53 42 1430 18 58 38 31.9 281.7 4.4 67.5 25 1 1 1444 17 53 42 17 57 12 --- 19 02 08 31.2 282.1 4.5 67.4 210 F 1 1471 17 53 43 17 59 13 J1249+2817 19 04 10 11.4 296.2 6.2 60.7 84 1 1 1471 17 59 13 18 00 43 =1246+285 19 05 40 11.1 296.4 6.3 60.5 90 F 1 1482 17 59 14 18 01 18 1256 19 06 15 12.7 295.0 6.1 61.3 28 1 1 1482 18 01 18 18 04 48 --- 19 09 46 12.1 295.4 6.2 61.0 210 F 1 1510 18 01 19 18 05 26 J1249+2817 19 10 24 10.2 296.9 6.3 60.1 30 1 1 1510 18 05 26 18 06 56 =1246+285 19 11 54 9.9 297.1 6.4 59.9 90 F 1 1521 18 05 27 18 07 32 1256 19 12 30 11.5 295.7 6.2 60.8 29 1 1 1521 18 07 32 18 11 02 --- 19 16 01 10.8 296.1 6.3 60.4 210 F 1 1548 18 07 33 18 11 40 J1249+2817 19 16 39 9.0 297.6 6.4 59.4 31 1 1 1548 18 11 40 18 13 10 =1246+285 19 18 09 8.7 297.8 6.5 59.3 90 F 1 1560 18 11 41 18 13 47 1256 19 18 46 10.3 296.4 6.3 60.2 30 1 1 1560 18 13 47 18 17 17 --- 19 22 16 9.6 296.8 6.4 59.8 210 F 1 1587 18 13 48 18 17 56 J1249+2817 19 22 55 7.8 298.4 6.6 58.8 32 1 1 1587 18 17 56 18 19 26 =1246+285 19 24 26 7.5 298.5 6.6 58.6 90 F 1 1599 18 17 57 18 20 03 1256 19 25 03 9.1 297.1 6.4 59.5 30 1 1 1599 18 20 03 18 23 33 --- 19 28 34 8.5 297.5 6.5 59.2 210 F 1 1626 18 20 04 18 24 44 J1342+2709 19 29 45 16.2 292.3 5.8 62.9 54 1 1 1626 18 24 44 18 26 14 =1339+274 19 31 15 15.9 292.4 5.8 62.8 90 F 1 1637 18 24 45 18 26 50 1347 19 31 52 17.8 292.7 5.7 63.7 29 1 1 1637 18 26 50 18 30 20 --- 19 35 22 17.1 293.1 5.7 63.4 210 F 1 1664 18 26 51 18 30 59 J1342+2709 19 36 01 14.9 293.0 5.9 62.3 31 1 1 1664 18 30 59 18 32 29 =1339+274 19 37 31 14.6 293.1 5.9 62.2 90 F 1 1676 18 31 00 18 33 06 1347 19 38 08 16.6 293.4 5.8 63.1 30 1 1 1676 18 33 06 18 36 36 --- 19 41 39 15.9 293.7 5.8 62.8 210 F 1 1703 18 33 07 18 37 15 J1342+2709 19 42 18 13.7 293.6 6.0 61.8 31 1 1 1703 18 37 15 18 38 45 =1339+274 19 43 48 13.4 293.8 6.0 61.7 90 F 1 1715 18 37 16 Schedule for SHANGHAI (Code Sh ) Page 8 VLBI observations at 18 cm of faint nuclear sources in the BCS Sample. 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 6 Jun 2010 Day 157 --- 18 39 22 1347 19 44 26 15.4 294.0 5.9 62.6 30 1 1 1715 18 39 22 18 42 52 --- 19 47 56 14.7 294.4 6.0 62.3 210 F 1 1742 18 39 23 18 43 31 J1342+2709 19 48 36 12.5 294.3 6.1 61.2 31 1 1 1742 18 43 31 18 45 01 =1339+274 19 50 06 12.2 294.5 6.1 61.1 90 F 1 1753 18 43 32 18 45 39 1347 19 50 44 14.1 294.7 6.0 62.0 30 1 1 1753 18 45 39 18 49 09 --- 19 54 14 13.5 295.1 6.1 61.7 210 F 1 1781 18 45 40 18 50 24 J1443+2501 19 55 29 22.5 286.5 5.2 64.9 56 1 1 1781 18 50 24 18 51 54 =1441+252 19 56 59 22.2 286.7 5.2 64.8 90 F 1 1792 18 50 25 18 52 30 1430 19 57 36 19.7 287.8 5.4 64.0 28 1 1 1792 18 52 30 18 56 00 --- 20 01 06 19.0 288.2 5.5 63.7 210 F 1 1819 18 52 31 18 56 35 J1443+2501 20 01 41 21.2 287.1 5.3 64.5 27 1 1 1819 18 56 35 18 58 05 =1441+252 20 03 12 20.9 287.3 5.3 64.4 90 F 1 1831 18 56 36 18 58 42 1430 20 03 48 18.5 288.5 5.5 63.5 28 1 1 1831 18 58 42 19 02 12 --- 20 07 19 17.7 288.8 5.6 63.3 210 F 1 1858 18 58 43 19 02 47 J1443+2501 20 07 54 20.0 287.8 5.4 64.1 28 1 1 1858 19 02 47 19 04 17 =1441+252 20 09 25 19.7 288.0 5.4 64.0 90 F 1 1870 19 02 48 19 04 54 1430 20 10 02 17.2 289.1 5.6 63.1 29 1 1 1870 19 04 54 19 08 24 --- 20 13 32 16.5 289.5 5.7 62.8 210 F 1 1897 19 04 55 19 09 00 J1443+2501 20 14 08 18.7 288.5 5.5 63.6 28 1 1 1897 19 09 00 19 10 30 =1441+252 20 15 38 18.4 288.6 5.5 63.5 90 F 1 1908 19 09 01 19 11 07 1430 20 16 16 15.9 289.8 5.7 62.6 29 1 1 1908 19 11 07 19 14 37 --- 20 19 46 15.2 290.2 5.8 62.4 210 F 1 1935 19 11 08 19 17 52 3C345 20 23 01 45.1 297.0 3.7 83.3 140 1 1 1935 19 17 52 19 27 52 --- 20 33 03 43.2 297.3 3.8 82.0 600 F 1 2013 19 17 53 22 17 42 3C345 23 23 21 12.5 309.2 6.7 59.7 10135 1 1 2013 22 17 42 22 27 42 --- 23 33 23 10.8 310.2 6.8 58.3 600 F 1 2090 22 17 43 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: kvsr.L1024 Matching groups in /irasoft/sched/catalogs/freq.dat: sh18cm Huang Xinyong 27Sept05 ****** Only 244.98 of 256.00 MHz total bandwidth is within the IFs in the setup file before any FREQ or DOPPLER shifts. 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= 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 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= U U L L U U L L U U L L U U L L 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: 10 Setup file default. Used pcal sets: 1 LO sum= 1610.49 1610.49 1610.49 1610.49 1642.49 1642.49 1642.49 1642.49 1674.49 1674.49 1674.49 1674.49 1706.49 1706.49 1706.49 1706.49 BBC fr= 689.51 689.51 689.51 689.51 657.51 657.51 657.51 657.51 625.51 625.51 625.51 625.51 593.51 593.51 593.51 593.51 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 -- VLBI observations at 18 cm of faint nuclear sources in the BCS Sample. 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) * 1347 13 47 56.361186 * 13 50 13.580000 13 50 44.107367 0.00 28 31 35.46424 * 28 16 44.90000 28 13 38.58214 0.00 From catalog imbedded in main SCHED input file. 1.517 scan hours, 73.499 baseline hours above horizon. * 1430 14 30 26.985300 * 14 32 41.600000 14 33 11.725403 0.00 25 08 29.68707 * 24 55 19.00000 24 52 32.08137 0.00 From catalog imbedded in main SCHED input file. 1.400 scan hours, 68.483 baseline hours above horizon. * 1256 12 56 58.532285 * 12 59 23.360000 12 59 55.235063 0.00 28 10 51.32460 * 27 54 41.50000 27 51 19.36311 0.00 From catalog imbedded in main SCHED input file. 1.517 scan hours, 73.499 baseline hours above horizon. * J1249+2817 12 46 52.177719 * 12 49 18.409281 12 49 50.527333 0.56 1246+285 28 34 03.57796 * 28 17 43.61456 28 14 19.62141 0.78 /irasoft/sched/catalogs/sources.vlba Petrov Dec. 2009 Solution 2009c_astro 51 Observations 0.650 scan hours, 28.473 baseline hours above horizon. * J1342+2709 13 39 49.302022 * 13 42 08.376682 13 42 39.249746 0.30 1339+274 27 24 36.85831 * 27 09 30.61728 27 06 20.88231 0.53 /irasoft/sched/catalogs/sources.vlba Petrov Dec. 2009 Solution 2009c_astro 73 Observations 0.650 scan hours, 28.473 baseline hours above horizon. * J1443+2501 14 41 43.558261 * 14 43 56.892198 14 44 26.786912 0.04 1441+252 25 14 23.98283 * 25 01 44.49069 24 59 03.93840 0.04 J1443+25 /irasoft/sched/catalogs/sources.vlba GSFC Nov. 2009 Solution 2009a 561 Observations 0.600 scan hours, 26.724 baseline hours above horizon. J1642+3948 16 41 17.606229 * 16 42 58.809967 16 43 22.325984 0.01 * 3C345 39 54 10.81492 * 39 48 36.99398 39 47 24.11512 0.01 1641+399 /irasoft/sched/catalogs/sources.vlba J1642+39 GSFC Nov. 2009 Solution 2009a 52093 Observations 0.500 scan hours, 25.833 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) 1347 111.8 1430 120.7 1256 103.3 J1249+2817 101.3 J1342+2709 111.2 J1443+2501 122.2 3C345 117.4 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