COVER INFORMATION Station: SHANGHAI (Code Sh ) Experiment: Dominant heating mechanism in ULIRGs Exp. Code: EP064N Schedule Version: 1.00 Processed by SCHED version: 8.10 Bug fixs and minor enhancements PI: Miguel A. Perez-Torres Address: IAA - CSIC Glorieta de la Astronomia s/n 18008 Granada, Spain Phone: +34-958230644 EMAIL: torres@iaa.es Fax: +34-958814530 Phone during observation: +34-665252538 Observing mode: 1024 Mbps Notes: 6-hr of 1-Gb/s, phase-ref of IRAS 19542+1110 with EVN+MERLIN Fourth epoch obs-ns at 6cm Schedule for SHANGHAI (Code Sh ) Page 2 Dominant heating mechanism in ULIRGs 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 ---------------------------------------------------------------------------------------- --- Sat 29 May 2010 Day 149 --- 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 21 40 00 J2001+1027 22 14 01 53.1 243.3 2.2 51.1 0 1 1 0 21 40 00 21 44 00 =1958+103 22 18 01 52.3 244.3 2.3 51.7 240 F 1 31 21 40 01 21 44 00 IRAS1954 22 18 01 51.9 246.6 2.3 53.2 -4 1 1 31 No stop 21 47 30 --- 22 21 32 51.3 247.4 2.4 53.7 206 F 1 58 21 44 01 21 47 30 J2001+1027 22 21 32 51.6 245.2 2.3 52.2 -4 1 1 58 No stop 21 49 00 =1958+103 22 23 02 51.3 245.6 2.4 52.5 86 F 1 70 21 47 31 21 49 00 IRAS1954 22 23 02 51.0 247.7 2.4 53.9 -4 1 1 70 No stop 21 52 30 --- 22 26 33 50.3 248.5 2.5 54.4 206 F 1 97 21 49 01 21 53 30 J2001+1027 22 27 33 50.5 246.6 2.4 53.1 56 1 1 97 21 53 30 21 55 00 =1958+103 22 29 03 50.2 247.0 2.5 53.3 90 F 1 108 21 53 31 21 55 00 IRAS1954 22 29 03 49.8 249.1 2.5 54.7 -4 1 1 108 No stop 21 58 30 --- 22 32 34 49.1 249.8 2.6 55.1 206 F 1 135 21 55 01 21 58 30 J2001+1027 22 32 34 49.5 247.8 2.5 53.7 -4 1 1 135 No stop 22 00 00 =1958+103 22 34 04 49.2 248.1 2.5 53.9 86 F 1 147 21 58 31 22 00 00 IRAS1954 22 34 04 48.8 250.2 2.6 55.2 -4 1 1 147 No stop 22 03 30 --- 22 37 35 48.0 250.9 2.7 55.6 206 F 1 174 22 00 01 22 03 30 J2001+1027 22 37 35 48.5 248.9 2.6 54.3 -4 1 1 174 No stop 22 05 00 =1958+103 22 39 05 48.2 249.2 2.6 54.5 86 F 1 186 22 03 31 22 05 00 IRAS1954 22 39 05 47.7 251.2 2.7 55.8 -4 1 1 186 No stop 22 08 30 --- 22 42 35 47.0 251.9 2.8 56.1 206 F 1 213 22 05 01 22 09 30 J2001+1027 22 43 36 47.3 250.2 2.7 55.0 56 1 1 213 22 09 30 22 11 00 =1958+103 22 45 06 47.0 250.5 2.7 55.2 90 F 1 225 22 09 31 Schedule for SHANGHAI (Code Sh ) Page 3 Dominant heating mechanism in ULIRGs 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 ---------------------------------------------------------------------------------------- --- Sat 29 May 2010 Day 149 --- 22 11 00 IRAS1954 22 45 06 46.5 252.4 2.8 56.4 -4 1 1 225 No stop 22 14 30 --- 22 48 36 45.8 253.1 2.9 56.7 206 F 1 252 22 11 01 22 15 30 J2001+1027 22 49 37 46.1 251.4 2.8 55.6 56 1 1 252 22 15 30 22 17 00 =1958+103 22 51 07 45.7 251.7 2.8 55.8 90 F 1 263 22 15 31 22 17 00 IRAS1954 22 51 07 45.3 253.6 2.9 56.9 -4 1 1 263 No stop 22 20 30 --- 22 54 37 44.6 254.2 3.0 57.2 206 F 1 290 22 17 01 22 20 30 J2001+1027 22 54 37 45.0 252.4 2.9 56.1 -4 1 1 290 No stop 22 22 00 =1958+103 22 56 08 44.7 252.7 2.9 56.2 86 F 1 302 22 20 31 22 22 00 IRAS1954 22 56 08 44.3 254.5 3.0 57.3 -4 1 1 302 No stop 22 25 30 --- 22 59 38 43.5 255.2 3.0 57.6 206 F 1 329 22 22 01 22 25 30 J2001+1027 22 59 38 44.0 253.3 3.0 56.5 -4 1 1 329 No stop 22 27 00 =1958+103 23 01 08 43.7 253.6 3.0 56.7 86 F 1 341 22 25 31 22 27 00 IRAS1954 23 01 08 43.2 255.4 3.1 57.7 -4 1 1 341 No stop 22 30 30 --- 23 04 39 42.5 256.1 3.1 58.0 206 F 1 368 22 27 01 22 31 30 J2001+1027 23 05 39 42.8 254.4 3.1 57.0 56 1 1 368 22 31 30 22 33 00 =1958+103 23 07 09 42.5 254.7 3.1 57.1 90 F 1 379 22 31 31 22 33 00 IRAS1954 23 07 09 42.0 256.5 3.2 58.1 -4 1 1 379 No stop 22 36 30 --- 23 10 40 41.2 257.1 3.2 58.4 206 F 1 406 22 33 01 22 36 30 J2001+1027 23 10 40 41.7 255.3 3.1 57.4 -4 1 1 406 No stop 22 38 00 =1958+103 23 12 10 41.4 255.6 3.2 57.5 86 F 1 418 22 36 31 22 38 00 IRAS1954 23 12 10 40.9 257.4 3.3 58.4 -4 1 1 418 No stop 22 41 30 --- 23 15 41 40.2 257.9 3.3 58.7 206 F 1 445 22 38 01 22 41 30 J2001+1027 23 15 41 40.7 256.2 3.2 57.8 -4 1 1 445 No stop 22 43 00 =1958+103 23 17 11 40.4 256.5 3.3 57.9 86 F 1 457 22 41 31 22 43 00 IRAS1954 23 17 11 39.9 258.2 3.3 58.7 -4 1 1 457 No stop 22 46 30 --- 23 20 42 39.1 258.8 3.4 58.9 206 F 1 484 22 43 01 22 47 30 J2001+1027 23 21 42 39.4 257.2 3.3 58.1 56 1 1 484 22 47 30 22 49 00 =1958+103 23 23 12 39.1 257.5 3.4 58.2 90 F 1 495 22 47 31 22 49 00 IRAS1954 23 23 12 38.6 259.2 3.4 59.1 -4 1 1 495 No stop 22 52 30 --- 23 26 43 37.9 259.7 3.5 59.2 206 F 1 523 22 49 01 Schedule for SHANGHAI (Code Sh ) Page 4 Dominant heating mechanism in ULIRGs 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 ---------------------------------------------------------------------------------------- --- Sat 29 May 2010 Day 149 --- 22 52 30 J2001+1027 23 26 43 38.4 258.1 3.4 58.4 -4 1 1 523 No stop 22 54 00 =1958+103 23 28 13 38.1 258.3 3.4 58.5 86 F 1 534 22 52 31 22 54 00 IRAS1954 23 28 13 37.6 260.0 3.5 59.3 -4 1 1 534 No stop 22 57 30 --- 23 31 43 36.8 260.5 3.6 59.5 206 F 1 561 22 54 01 22 57 30 J2001+1027 23 31 43 37.3 258.9 3.5 58.7 -4 1 1 561 No stop 22 59 00 =1958+103 23 33 14 37.0 259.1 3.5 58.8 86 F 1 573 22 57 31 22 59 00 IRAS1954 23 33 14 36.5 260.8 3.6 59.5 -4 1 1 573 No stop 23 02 30 --- 23 36 44 35.8 261.3 3.7 59.7 206 F 1 600 22 59 01 23 03 30 J2001+1027 23 37 44 36.1 259.8 3.6 59.0 57 1 1 600 23 03 30 23 05 00 =1958+103 23 39 15 35.8 260.1 3.6 59.1 90 F 1 612 23 03 31 23 05 00 IRAS1954 23 39 15 35.2 261.7 3.7 59.8 -4 1 1 612 No stop 23 08 30 --- 23 42 45 34.5 262.2 3.8 59.9 206 F 1 639 23 05 01 23 08 30 J2001+1027 23 42 45 35.0 260.6 3.7 59.2 -4 1 1 639 No stop 23 10 00 =1958+103 23 44 15 34.7 260.9 3.7 59.3 86 F 1 650 23 08 31 23 10 00 IRAS1954 23 44 15 34.2 262.4 3.8 60.0 -4 1 1 650 No stop 23 13 30 --- 23 47 46 33.4 263.0 3.8 60.1 206 F 1 677 23 10 01 23 13 30 J2001+1027 23 47 46 34.0 261.4 3.8 59.4 -4 1 1 677 No stop 23 15 00 =1958+103 23 49 16 33.6 261.6 3.8 59.5 86 F 1 689 23 13 31 23 15 00 IRAS1954 23 49 16 33.1 263.2 3.9 60.1 -4 1 1 689 No stop 23 18 30 --- 23 52 47 32.3 263.7 3.9 60.2 206 F 1 716 23 15 01 23 19 30 J2001+1027 23 53 47 32.7 262.3 3.9 59.6 57 1 1 716 23 19 30 23 21 00 =1958+103 23 55 17 32.4 262.5 3.9 59.7 90 F 1 728 23 19 31 23 21 00 IRAS1954 23 55 17 31.8 264.0 4.0 60.3 -4 1 1 728 No stop 23 24 30 --- 23 58 48 31.1 264.5 4.0 60.4 206 F 1 755 23 21 01 23 24 30 J2001+1027 23 58 48 31.6 263.0 4.0 59.8 -4 1 1 755 No stop 23 26 00 =1958+103 00 00 18 31.3 263.2 4.0 59.9 86 F 1 766 23 24 31 23 26 00 IRAS1954 00 00 18 30.7 264.7 4.1 60.4 -4 1 1 766 No stop 23 29 30 --- 00 03 49 30.0 265.2 4.1 60.5 206 F 1 793 23 26 01 23 29 30 J2001+1027 00 03 49 30.6 263.7 4.0 60.0 -4 1 1 793 No stop 23 31 00 =1958+103 00 05 19 30.2 264.0 4.1 60.0 86 F 1 805 23 29 31 Schedule for SHANGHAI (Code Sh ) Page 5 Dominant heating mechanism in ULIRGs 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 ---------------------------------------------------------------------------------------- --- Sat 29 May 2010 Day 149 --- 23 31 00 IRAS1954 00 05 19 29.7 265.4 4.1 60.5 -3 1 1 805 No stop 23 34 30 --- 00 08 50 28.9 265.9 4.2 60.6 207 F 1 832 23 31 01 23 35 30 J2001+1027 00 09 50 29.3 264.6 4.1 60.1 57 1 1 832 23 35 30 23 37 00 =1958+103 00 11 20 29.0 264.8 4.2 60.1 90 F 1 844 23 35 31 23 37 00 IRAS1954 00 11 20 28.4 266.3 4.2 60.6 -3 1 1 844 No stop 23 40 30 --- 00 14 50 27.6 266.8 4.3 60.7 207 F 1 871 23 37 01 23 40 30 J2001+1027 00 14 50 28.2 265.3 4.2 60.2 -3 1 1 871 No stop 23 42 00 =1958+103 00 16 21 27.9 265.5 4.2 60.2 87 F 1 883 23 40 31 23 42 00 IRAS1954 00 16 21 27.3 267.0 4.3 60.7 -3 1 1 883 No stop 23 45 30 --- 00 19 51 26.6 267.4 4.4 60.7 207 F 1 910 23 42 01 23 45 30 J2001+1027 00 19 51 27.1 266.0 4.3 60.3 -3 1 1 910 No stop 23 47 00 =1958+103 00 21 22 26.8 266.2 4.3 60.3 87 F 1 921 23 45 31 23 47 00 IRAS1954 00 21 22 26.2 267.6 4.4 60.8 -3 1 1 921 No stop 23 50 30 --- 00 24 52 25.5 268.1 4.5 60.8 207 F 1 948 23 47 01 23 51 30 J2001+1027 00 25 52 25.8 266.8 4.4 60.4 57 1 1 948 23 51 30 23 53 00 =1958+103 00 27 23 25.5 267.0 4.4 60.4 90 F 1 960 23 51 31 23 53 00 IRAS1954 00 27 23 25.0 268.4 4.5 60.8 -3 1 1 960 No stop 23 56 30 --- 00 30 53 24.2 268.9 4.6 60.8 207 F 1 987 23 53 01 23 56 30 J2001+1027 00 30 53 24.8 267.5 4.5 60.5 -3 1 1 987 No stop 23 58 00 =1958+103 00 32 23 24.5 267.7 4.5 60.5 87 F 1 999 23 56 31 --- Start: Sat 29 May 2010 Day 149 -- Stop: Sun 30 May 2010 Day 150 --- 23 58 00 IRAS1954 00 32 23 23.9 269.1 4.6 60.8 -3 1 1 999 No stop 00 01 30 --- 00 35 54 23.1 269.5 4.6 60.8 207 F 1 1026 23 58 01 00 01 30 J2001+1027 00 35 54 23.7 268.1 4.6 60.5 -3 1 1 1026 No stop 00 03 00 =1958+103 00 37 24 23.4 268.3 4.6 60.5 87 F 1 1037 00 01 31 00 03 00 IRAS1954 00 37 24 22.8 269.7 4.7 60.8 -3 1 1 1037 No stop 00 06 30 --- 00 40 55 22.1 270.2 4.7 60.8 207 F 1 1064 00 03 01 00 07 30 J2001+1027 00 41 55 22.4 268.9 4.7 60.5 57 1 1 1064 00 07 30 00 09 00 =1958+103 00 43 25 22.1 269.1 4.7 60.5 90 F 1 1076 00 07 31 Schedule for SHANGHAI (Code Sh ) Page 6 Dominant heating mechanism in ULIRGs 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 30 May 2010 Day 150 --- 00 09 00 IRAS1954 00 43 25 21.5 270.5 4.8 60.8 -3 1 1 1076 No stop 00 12 30 --- 00 46 56 20.8 271.0 4.8 60.8 207 F 1 1103 00 09 01 00 12 30 J2001+1027 00 46 56 21.3 269.6 4.8 60.6 -3 1 1 1103 No stop 00 14 00 =1958+103 00 48 26 21.0 269.8 4.8 60.6 87 F 1 1115 00 12 31 00 14 00 IRAS1954 00 48 26 20.5 271.2 4.9 60.8 -3 1 1 1115 No stop 00 17 30 --- 00 51 57 19.7 271.6 4.9 60.8 207 F 1 1142 00 14 01 00 17 30 J2001+1027 00 51 57 20.3 270.2 4.8 60.6 -3 1 1 1142 No stop 00 19 00 =1958+103 00 53 27 19.9 270.4 4.9 60.6 87 F 1 1153 00 17 31 00 19 00 IRAS1954 00 53 27 19.4 271.8 4.9 60.8 -3 1 1 1153 No stop 00 22 30 --- 00 56 57 18.6 272.2 5.0 60.8 207 F 1 1181 00 19 01 00 23 30 J2001+1027 00 57 58 19.0 271.0 4.9 60.5 57 1 1 1181 00 23 30 00 25 00 =1958+103 00 59 28 18.7 271.2 5.0 60.5 90 F 1 1192 00 23 31 00 25 00 IRAS1954 00 59 28 18.1 272.6 5.0 60.7 -3 1 1 1192 No stop 00 28 30 --- 01 02 58 17.3 273.0 5.1 60.7 207 F 1 1219 00 25 01 00 28 30 J2001+1027 01 02 58 17.9 271.6 5.0 60.5 -3 1 1 1219 No stop 00 30 00 =1958+103 01 04 29 17.6 271.8 5.0 60.5 87 F 1 1231 00 28 31 00 30 00 IRAS1954 01 04 29 17.0 273.2 5.1 60.7 -3 1 1 1231 No stop 00 33 30 --- 01 07 59 16.3 273.6 5.2 60.6 207 F 1 1258 00 30 01 00 33 30 J2001+1027 01 07 59 16.8 272.3 5.1 60.5 -3 1 1 1258 No stop 00 35 00 =1958+103 01 09 29 16.5 272.5 5.1 60.5 87 F 1 1270 00 33 31 00 35 00 IRAS1954 01 09 29 16.0 273.8 5.2 60.6 -3 1 1 1270 No stop 00 38 30 --- 01 13 00 15.2 274.3 5.3 60.6 207 F 1 1297 00 35 01 00 39 30 J2001+1027 01 14 00 15.5 273.0 5.2 60.4 57 1 1 1297 00 39 30 00 41 00 =1958+103 01 15 30 15.2 273.2 5.2 60.4 90 F 1 1308 00 39 31 00 41 00 IRAS1954 01 15 30 14.7 274.6 5.3 60.5 -3 1 1 1308 No stop 00 44 30 --- 01 19 01 13.9 275.0 5.4 60.5 207 F 1 1335 00 41 01 00 44 30 J2001+1027 01 19 01 14.5 273.7 5.3 60.3 -3 1 1 1335 No stop 00 46 00 =1958+103 01 20 31 14.2 273.9 5.3 60.3 87 F 1 1347 00 44 31 00 46 00 IRAS1954 01 20 31 13.6 275.2 5.4 60.4 -3 1 1 1347 No stop 00 49 30 --- 01 24 02 12.8 275.6 5.4 60.4 207 F 1 1374 00 46 01 Schedule for SHANGHAI (Code Sh ) Page 7 Dominant heating mechanism in ULIRGs 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 30 May 2010 Day 150 --- 00 49 30 J2001+1027 01 24 02 13.4 274.3 5.4 60.3 -3 1 1 1374 No stop 00 51 00 =1958+103 01 25 32 13.1 274.5 5.4 60.2 87 F 1 1386 00 49 31 00 51 00 IRAS1954 01 25 32 12.5 275.8 5.5 60.3 -3 1 1 1386 No stop 00 54 30 --- 01 29 03 11.8 276.2 5.5 60.2 207 F 1 1413 00 51 01 00 55 30 J2001+1027 01 30 03 12.1 275.0 5.5 60.2 57 1 1 1413 00 55 30 00 57 00 =1958+103 01 31 33 11.8 275.2 5.5 60.1 90 F 1 1424 00 55 31 00 57 00 IRAS1954 01 31 33 11.2 276.6 5.6 60.2 -3 1 1 1424 No stop 01 00 30 --- 01 35 04 10.5 277.0 5.6 60.1 207 F 1 1452 00 57 01 01 00 30 J2001+1027 01 35 04 11.1 275.7 5.6 60.1 -3 1 1 1452 No stop 01 02 00 =1958+103 01 36 34 10.7 275.9 5.6 60.0 87 F 1 1463 01 00 31 01 02 00 IRAS1954 01 36 34 10.2 277.2 5.7 60.1 -3 1 1 1463 No stop 01 05 30 --- 01 40 04 9.4 277.6 5.7 60.0 207 F 1 1490 01 02 01 01 05 30 J2001+1027 01 40 04 10.0 276.3 5.6 59.9 -3 1 1 1490 No stop 01 07 00 =1958+103 01 41 35 9.7 276.5 5.7 59.9 87 F 1 1502 01 05 31 01 07 00 IRAS1954 01 41 35 9.1 277.8 5.7 59.9 -3 1 1 1502 No stop 01 10 30 --- 01 45 05 8.4 278.2 5.8 59.8 207 F 1 1529 01 07 01 01 11 30 J2001+1027 01 46 05 8.7 277.1 5.7 59.8 57 1 1 1529 01 11 30 01 13 00 =1958+103 01 47 36 8.4 277.2 5.8 59.8 90 F 1 1541 01 11 31 01 13 00 IRAS1954 01 47 36 7.8 278.6 5.8 59.7 -3 1 1 1541 No stop 01 16 30 --- 01 51 06 7.1 279.0 5.9 59.6 207 F 1 1568 01 13 01 01 16 30 J2001+1027 01 51 06 7.6 277.7 5.8 59.7 -3 1 1 1568 No stop 01 18 00 =1958+103 01 52 37 7.3 277.9 5.8 59.6 87 F 1 1579 01 16 31 01 18 00 IRAS1954 01 52 37 6.8 279.2 5.9 59.6 -3 1 1 1579 No stop 01 21 30 --- 01 56 07 6.0 279.6 6.0 59.4 207 F 1 1606 01 18 01 01 21 30 J2001+1027 01 56 07 6.6 278.3 5.9 59.5 -3 1 1 1606 No stop 01 23 00 =1958+103 01 57 37 6.3 278.5 5.9 59.5 87 F 1 1618 01 21 31 01 23 00 IRAS1954 01 57 37 5.7 279.8 6.0 59.4 -3 1 1 1618 No stop 01 26 30 --- 02 01 08 5.0 280.3 6.1 D 59.2 0 F 1 1645 01 23 01 01 28 30 2134+004 02 03 08 20.4 258.0 4.4 56.9 92 1 1 1645 01 28 30 01 34 30 --- 02 09 09 19.1 258.9 4.5 57.2 360 F 1 1692 01 28 31 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: ep064n.6cm Matches group sh6cm in /home/cristina/sched_8.1/catalogs/freq.dat Update freq. range AnTao 22Mar08 Setup group: 9 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: 10 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 -- Dominant heating mechanism in ULIRGs 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) * IRAS1954 19 54 13.636383 * 19 56 35.783458 19 57 07.118594 0.00 11 11 01.41913 * 11 19 05.01998 11 20 42.40276 0.00 From catalog imbedded in main SCHED input file. 3.675 scan hours, 139.713 baseline hours above horizon. J1331+3030 13 28 49.657764 * 13 31 08.288056 13 31 39.114706 0.36 * 3C286 30 45 58.64058 * 30 30 32.95922 30 27 18.96037 0.47 1328+307 /home/cristina/sched_8.1/catalogs/sources.vlba J1331+30 VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 0.083 scan hours, 3.000 baseline hours above horizon. * J2001+1027 19 58 47.472002 * 20 01 10.643445 20 01 42.174770 2.16 1958+103 10 19 37.10156 * 10 27 58.11707 10 29 39.41451 2.15 /home/cristina/sched_8.1/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 1.642 scan hours, 52.536 baseline hours above horizon. J2136+0041 21 34 05.207389 * 21 36 38.586324 21 37 11.804261 0.30 2134+00 00 28 25.08002 * 00 41 54.21285 00 44 44.27755 0.20 * 2134+004 /home/cristina/sched_8.1/catalogs/sources.vlba J2136+00 VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 0.100 scan hours, 4.441 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) IRAS1954 118.8 3C286 112.9 J2001+1027 118.3 2134+004 101.3 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