COVER INFORMATION Station: VLBA_NL (Code Nl ) Experiment: VLBA/VLTI/Keck Observations of AGB Stars Exp. Code: BC168C Schedule Version: 1.00 Processed by SCHED version: 6.05 June 2006 PI: W. D. Cotton Address: NRAO 520 Edgemont Road Charlottesville, VA 22903 Phone: (434) 2960319 EMAIL: bcotton@nrao.edu Fax: (434) 2960278 Phone during observation: (434) 2968266 Observing mode: Notes: BE SURE PULSE CAL IS OFF ON PROGRAM SOURCES. To be run around 1 October 2007 Schedule for VLBA_NL (Code Nl ) Page 2 VLBA/VLTI/Keck Observations of AGB Stars 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. Automatic tape allocation specified. Tape positions are just estimates. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Sun 24 Feb 2008 Day 55 --- Next scan frequencies: 43122.78 43122.78 42821.32 42821.32 Next BBC frequencies: 922.78 922.78 621.32 621.32 Next scan bandwidths: 4.00 4.00 4.00 4.00 09 57 49 J1613+3412 14 06 11 63.9 96.3 -2.1 -63.7 0 1 1 0 09 57 49 10 01 49 --- 14 10 11 64.6 97.2 -2.1 -63.4 239 F 1 2 09 58 12 10 02 49 S_SER 14 11 11 58.5 145.6 -1.2 -25.8 22 1 1 2 10 02 49 10 19 46 --- 14 28 11 60.1 153.0 -0.9 -20.4 1017 F 1 10 10 03 12 Next scan frequencies: 43131.74 43131.74 42830.22 42830.22 Next BBC frequencies: 931.74 931.74 630.22 630.22 10 21 45 J1751+0939 14 30 11 35.4 111.1 -3.4 -44.9 64 1 1 10 10 21 45 10 25 45 --- 14 34 11 36.1 112.0 -3.3 -44.6 239 F 1 12 10 22 08 10 26 45 RT_OPH 14 35 11 36.5 109.8 -3.4 -45.7 52 1 1 12 10 26 45 10 43 42 --- 14 52 11 39.5 113.5 -3.1 -44.2 1017 F 1 20 10 27 08 Next scan frequencies: 43122.78 43122.78 42821.32 42821.32 Next BBC frequencies: 922.78 922.78 621.32 621.32 10 45 41 J1613+3412 14 54 11 72.6 109.3 -1.3 -58.3 47 1 1 20 10 45 41 10 49 41 --- 14 58 11 73.3 110.8 -1.3 -57.4 239 F 1 22 10 46 04 10 50 41 S_SER 14 59 11 62.1 168.1 -0.4 -9.1 16 1 1 22 10 50 41 11 07 38 --- 15 16 11 62.5 176.9 -0.1 -2.4 1017 F 1 30 10 51 04 Next scan frequencies: 43130.30 43121.96 42820.50 42820.50 Next BBC frequencies: 930.30 921.96 620.50 620.50 11 09 38 J1743-0350 15 18 11 33.6 134.5 -2.4 -32.2 56 1 1 30 11 09 38 11 13 37 --- 15 22 11 34.1 135.5 -2.4 -31.6 239 F 1 32 11 10 01 11 14 37 T_OPH 15 23 11 29.8 160.3 -1.2 -15.2 37 1 1 32 11 14 37 11 31 34 --- 15 40 11 30.7 164.9 -0.9 -11.7 1017 F 1 41 11 15 00 Next scan frequencies: 43131.74 43131.74 42830.22 42830.22 Next BBC frequencies: 931.74 931.74 630.22 630.22 11 33 34 J1751+0939 15 42 11 47.1 129.1 -2.2 -36.0 81 1 1 41 11 33 34 11 37 33 --- 15 46 11 47.6 130.3 -2.1 -35.3 239 F 1 42 11 33 57 Schedule for VLBA_NL (Code Nl ) Page 3 VLBA/VLTI/Keck Observations of AGB Stars 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. Automatic tape allocation specified. Tape positions are just estimates. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Sun 24 Feb 2008 Day 55 --- 11 38 33 RT_OPH 15 47 11 48.3 127.7 -2.2 -37.0 52 1 1 42 11 38 33 11 55 30 --- 16 04 11 50.7 133.0 -1.9 -33.8 1017 F 1 51 11 38 56 Next scan frequencies: 43128.70 43128.70 42827.20 42827.20 Next BBC frequencies: 928.70 928.70 627.20 627.20 11 57 30 J2015+3710 16 06 11 42.7 73.8 -4.2 -64.1 74 1 1 51 11 57 30 12 01 29 --- 16 10 11 43.4 74.3 -4.1 -64.3 239 F 1 53 11 57 53 12 02 29 RT_AQL 16 11 11 35.9 108.1 -3.5 -46.4 31 1 1 53 12 02 29 12 19 26 --- 16 28 11 38.9 111.8 -3.2 -45.0 1017 F 1 61 12 02 52 Next scan frequencies: 43122.78 43122.78 42821.32 42821.32 Next BBC frequencies: 922.78 922.78 621.32 621.32 12 21 26 J1613+3412 16 30 11 81.8 204.1 0.3 21.6 28 1 1 61 12 21 26 12 25 25 --- 16 34 11 81.4 209.3 0.3 26.1 239 F 1 63 12 21 49 12 27 25 S_SER 16 36 11 58.2 215.7 1.2 26.7 67 1 1 63 12 27 25 12 44 22 --- 16 53 11 56.2 222.4 1.5 31.2 1017 F 1 71 12 27 48 Next scan frequencies: 43130.30 43121.96 42820.50 42820.50 Next BBC frequencies: 930.30 921.96 620.50 620.50 12 46 22 J1743-0350 16 55 11 43.0 163.1 -0.8 -12.6 74 1 1 71 12 46 22 12 50 21 --- 16 59 11 43.2 164.4 -0.8 -11.6 239 F 1 73 12 46 45 12 51 21 T_OPH 17 00 11 31.8 187.3 0.4 5.7 31 1 1 73 12 51 21 13 08 18 --- 17 17 11 31.2 192.1 0.7 9.4 1017 F 1 81 12 51 44 Next scan frequencies: 43128.70 43128.70 42827.20 42827.20 Next BBC frequencies: 928.70 928.70 627.20 627.20 13 10 18 J2015+3710 17 19 11 56.0 82.8 -2.9 -68.3 41 1 1 81 13 10 18 13 14 17 --- 17 23 11 56.7 83.3 -2.9 -68.4 239 F 1 83 13 10 41 13 15 17 RT_AQL 17 24 11 48.1 125.9 -2.2 -38.1 25 1 1 83 13 15 17 13 32 14 --- 17 41 11 50.6 131.0 -2.0 -35.1 1017 F 1 91 13 15 40 13 34 14 BLLAC 17 43 11 43.0 66.3 -4.3 -67.5 71 1 1 91 13 34 14 13 40 13 --- 17 49 11 44.0 66.9 -4.2 -68.1 359 F 1 94 13 34 37 Schedule for VLBA_NL (Code Nl ) Page 4 VLBA/VLTI/Keck Observations of AGB Stars 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. Automatic tape allocation specified. Tape positions are just estimates. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Sun 24 Feb 2008 Day 55 --- Next scan frequencies: 43130.30 43121.96 42820.50 42820.50 Next BBC frequencies: 930.30 921.96 620.50 620.50 13 42 12 J1743-0350 17 51 11 44.4 182.4 0.1 1.8 37 1 1 94 13 42 12 13 46 12 --- 17 55 11 44.3 183.8 0.2 2.8 239 F 1 96 13 42 35 13 47 12 T_OPH 17 56 11 29.1 202.6 1.4 17.4 23 1 1 96 13 47 12 14 04 09 --- 18 13 11 27.7 207.0 1.6 20.7 1017 F 1 104 13 47 35 Next scan frequencies: 43122.78 43122.78 42821.32 42821.32 Next BBC frequencies: 922.78 922.78 621.32 621.32 14 06 09 J1613+3412 18 15 11 65.1 262.3 2.0 63.3 39 1 1 104 14 06 09 14 10 08 --- 18 19 11 64.4 263.1 2.1 63.5 239 F 1 106 14 06 32 14 11 08 S_SER 18 20 11 42.8 247.9 3.0 45.5 11 1 1 106 14 11 08 14 28 05 --- 18 37 11 39.8 251.7 3.3 46.9 1017 F 1 114 14 11 31 Next scan frequencies: 43130.30 43121.96 42820.50 42820.50 Next BBC frequencies: 930.30 921.96 620.50 620.50 14 30 05 J1743-0350 18 39 11 42.7 198.7 0.9 13.9 78 1 1 114 14 30 05 14 34 04 --- 18 43 11 42.5 200.1 1.0 14.9 239 F 1 116 14 30 28 14 35 04 T_OPH 18 44 11 24.8 214.6 2.2 26.2 18 1 1 116 14 35 04 14 52 01 --- 19 01 11 22.9 218.6 2.4 29.0 1017 F 1 124 14 35 27 Next scan frequencies: 43131.74 43131.74 42830.22 42830.22 Next BBC frequencies: 931.74 931.74 630.22 630.22 14 55 01 J1751+0939 19 04 11 54.2 211.5 1.2 23.3 111 1 1 124 14 55 01 14 59 00 --- 19 08 11 53.8 213.0 1.3 24.3 239 F 1 126 14 55 24 15 00 00 RT_OPH 19 09 11 55.5 212.5 1.2 24.1 50 1 1 126 15 00 00 15 16 57 --- 19 26 11 53.7 219.0 1.5 28.6 1017 F 1 135 15 00 23 Next scan frequencies: 43128.70 43128.70 42827.20 42827.20 Next BBC frequencies: 928.70 928.70 627.20 627.20 15 18 57 J2015+3710 19 28 11 79.8 112.6 -0.8 -59.8 43 1 1 135 15 18 57 15 22 56 --- 19 32 11 80.4 115.0 -0.7 -58.1 239 F 1 137 15 19 20 Schedule for VLBA_NL (Code Nl ) Page 5 VLBA/VLTI/Keck Observations of AGB Stars 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. Automatic tape allocation specified. Tape positions are just estimates. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Sun 24 Feb 2008 Day 55 --- 15 23 56 RT_AQL 19 33 11 59.9 177.4 -0.1 -1.9 12 1 1 137 15 23 56 15 40 53 --- 19 50 11 59.9 185.7 0.2 4.4 1017 F 1 145 15 24 19 15 42 53 BLLAC 19 52 11 65.9 77.6 -2.2 -80.1 42 1 1 145 15 42 53 15 48 52 --- 19 58 11 66.9 78.1 -2.1 -80.7 359 F 1 148 15 43 16 Next scan frequencies: 43122.78 43122.78 42821.32 42821.32 Next BBC frequencies: 922.78 922.78 621.32 621.32 15 50 51 J1613+3412 20 00 11 45.6 -80.5 3.8 62.8 8 1 1 148 15 50 51 15 54 51 --- 20 04 11 44.9 -80.0 3.8 62.6 239 F 1 150 15 51 14 15 58 50 S_SER 20 08 11 23.2 268.7 4.8 50.3 1 1 1 150 15 58 50 16 15 47 --- 20 25 11 20.0 271.5 5.1 50.3 1017 F 1 158 15 59 13 Next scan frequencies: 43130.30 43121.96 42820.50 42820.50 Next BBC frequencies: 930.30 921.96 620.50 620.50 16 16 47 J1743-0350 20 26 11 31.4 229.3 2.7 34.5 26 1 1 158 16 16 47 16 20 46 --- 20 30 11 30.9 230.3 2.8 35.1 239 F 1 160 16 17 10 16 21 46 T_OPH 20 31 11 10.4 237.1 3.9 40.7 13 1 1 160 16 21 46 16 38 43 --- 20 48 11 7.7 240.2 4.2 42.3 1017 F 1 168 16 22 09 Next scan frequencies: 43131.74 43131.74 42830.22 42830.22 Next BBC frequencies: 931.74 931.74 630.22 630.22 16 41 43 J1751+0939 20 51 11 39.3 243.9 3.0 42.8 110 1 1 168 16 41 43 16 45 42 --- 20 55 11 38.6 244.8 3.1 43.2 239 F 1 170 16 42 06 16 46 42 RT_OPH 20 56 11 40.4 245.2 3.0 43.6 50 1 1 170 16 46 42 17 03 39 --- 21 13 11 37.5 249.0 3.3 45.2 1017 F 1 178 16 47 05 Next scan frequencies: 43128.70 43128.70 42827.20 42827.20 Next BBC frequencies: 928.70 928.70 627.20 627.20 17 05 39 J2015+3710 21 15 11 77.7 253.1 1.0 63.7 33 1 1 178 17 05 39 17 09 38 --- 21 19 11 77.0 254.7 1.1 64.6 239 F 1 180 17 06 02 17 12 08 RT_AQL 21 21 41 52.4 224.4 1.7 32.2 95 1 1 180 17 12 08 17 29 05 --- 21 38 41 50.1 229.9 2.0 35.7 1017 F 1 188 17 12 31 Schedule for VLBA_NL (Code Nl ) Page 6 VLBA/VLTI/Keck Observations of AGB Stars 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. Automatic tape allocation specified. Tape positions are just estimates. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Sun 24 Feb 2008 Day 55 --- 17 31 05 BLLAC 21 40 41 85.8 80.7 -0.4 -95.6 14 1 1 188 17 31 05 17 37 04 --- 21 46 41 86.9 78.5 -0.3 -98.8 359 F 1 191 17 31 28 Next scan frequencies: 43122.78 43122.78 42821.32 42821.32 Next BBC frequencies: 922.78 922.78 621.32 621.32 17 39 04 J1613+3412 21 48 41 26.3 -66.5 5.6 55.7 -8 1 1 191 17 39 04 17 43 03 --- 21 52 41 25.6 -65.9 5.6 55.4 232 F 1 193 17 39 27 17 44 03 S_SER 21 53 41 3.7 -74.1 6.5 47.8 10 1 1 193 17 44 03 18 01 00 --- 22 10 41 0.7 -71.3 6.8 D 46.8 0 F 1 201 17 44 26 Next scan frequencies: 43131.74 43131.74 42830.22 42830.22 Next BBC frequencies: 931.74 931.74 630.22 630.22 18 04 59 J1751+0939 22 14 41 24.5 260.8 4.4 48.3 12 1 1 201 18 04 59 18 08 59 --- 22 18 41 23.7 261.5 4.4 48.4 239 F 1 203 18 05 22 18 09 59 RT_OPH 22 19 41 25.5 262.1 4.4 48.8 50 1 1 203 18 09 59 18 26 56 --- 22 36 41 22.3 265.1 4.7 49.2 1017 F 1 211 18 10 22 Next scan frequencies: 43128.70 43128.70 42827.20 42827.20 Next BBC frequencies: 928.70 928.70 627.20 627.20 18 28 55 J2015+3710 22 38 41 62.3 272.5 2.4 69.3 34 1 1 211 18 28 55 18 32 55 --- 22 42 41 61.5 273.1 2.4 69.2 239 F 1 213 18 29 18 18 33 55 RT_AQL 22 43 41 39.8 247.1 3.1 44.6 10 1 1 213 18 33 55 18 50 52 --- 23 00 41 36.8 250.9 3.4 46.0 1017 F 1 221 18 34 18 18 52 51 BLLAC 23 02 41 78.9 277.8 1.0 87.8 29 1 1 221 18 52 51 18 58 50 --- 23 08 41 77.8 278.1 1.1 87.0 359 F 1 224 18 53 14 Next scan frequencies: 43131.74 43131.74 42830.22 42830.22 Next BBC frequencies: 931.74 931.74 630.22 630.22 19 00 50 J1751+0939 23 10 41 14.1 270.4 5.3 49.2 -14 1 1 224 19 00 50 19 04 49 --- 23 14 41 13.3 271.1 5.4 49.1 226 F 1 226 19 01 13 19 05 49 RT_OPH 23 15 41 15.1 271.6 5.3 49.5 50 1 1 226 19 05 49 19 22 47 --- 23 32 41 11.9 274.4 5.6 49.3 1017 F 1 235 19 06 12 Schedule for VLBA_NL (Code Nl ) Page 7 VLBA/VLTI/Keck Observations of AGB Stars 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. Automatic tape allocation specified. Tape positions are just estimates. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) SYNC ---------------------------------------------------------------------------------------- --- Sun 24 Feb 2008 Day 55 --- Next scan frequencies: 43128.70 43128.70 42827.20 42827.20 Next BBC frequencies: 928.70 928.70 627.20 627.20 19 24 46 J2015+3710 23 34 41 51.9 280.1 3.3 67.2 34 1 1 235 19 24 46 19 28 46 --- 23 38 41 51.2 280.6 3.4 67.0 239 F 1 236 19 25 09 19 29 45 RT_AQL 23 39 41 29.8 258.6 4.0 48.3 11 1 1 236 19 29 45 19 46 43 --- 23 56 41 26.7 261.7 4.3 48.9 1017 F 1 245 19 30 08 19 48 42 BLLAC 23 58 41 68.6 281.2 1.9 81.6 30 1 1 245 19 48 42 19 54 41 --- 00 04 41 67.5 281.7 2.0 81.0 359 F 1 248 19 49 05 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: bc161.vlba Matches group v7mm_b8 in /home/filehost/cwalker/sched/catalogs/freq.dat Setup group: 3 Station: VLBA_NL Total bit rate: 64 Format: VLBA1:2 Bits per sample: 2 Sample rate: 8.000 Number of channels: 4 Speedup factor: 2.00 Disk used to record data. 1st LO= 42200.00 42200.00 42200.00 42200.00 Net SB= U U U U Pol. = RCP LCP RCP LCP BBC = 1 2 3 4 BBC SB= U U U U IF = A C A C VLBA FE= 7mm omit 7mm omit VLBA Synth= 15.4 7.4 11.6 The following frequency sets based on this setup were used. Frequency Set: 3 Based on FREQ, BW, and/or DOPPLER in schedule. Used pcal sets: 1 LO sum= 43122.78 43122.78 42821.32 42821.32 BBC fr= 922.78 922.78 621.32 621.32 Bandwd= 4.000 4.000 4.000 4.000 Frequency Set: 13 Based on FREQ, BW, and/or DOPPLER in schedule. Used pcal sets: 1 LO sum= 43131.74 43131.74 42830.22 42830.22 BBC fr= 931.74 931.74 630.22 630.22 Bandwd= 4.000 4.000 4.000 4.000 Frequency Set: 22 Based on FREQ, BW, and/or DOPPLER in schedule. Used pcal sets: 1 LO sum= 43130.30 43121.96 42820.50 42820.50 BBC fr= 930.30 921.96 620.50 620.50 Bandwd= 4.000 4.000 4.000 4.000 Frequency Set: 32 Based on FREQ, BW, and/or DOPPLER in schedule. Used pcal sets: 1 LO sum= 43128.70 43128.70 42827.20 42827.20 BBC fr= 928.70 928.70 627.20 627.20 Bandwd= 4.000 4.000 4.000 4.000 The following pulse cal sets were used with this setup: Pulse cal detection set: 1 PCAL = OFF PCALXB1= S1 S2 S3 S4 OFF OFF OFF OFF PCALXB2= M1 M2 M3 M4 OFF OFF OFF OFF PCALFR1= 0 0 0 0 0 0 0 0 PCALFR2= 0 0 0 0 0 0 0 0 Track assignments are: track1= 2, 10, 18, 26 barrel=roll_off SOURCE LIST -- VLBA/VLTI/Keck Observations of AGB Stars 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) * BLLAC 22 00 39.362506 * 22 02 43.291373 22 03 01.825789 0.27 42 02 08.59079 * 42 16 39.97993 42 18 56.07631 0.40 From catalog imbedded in main SCHED input file. Doppler based on other sources. 0.499 scan hours, 21.527 baseline hours above horizon. * J1613+3412 16 11 47.914510 * 16 13 41.064500 16 14 00.090657 0.00 34 20 19.83496 * 34 12 47.91000 34 11 08.81893 0.00 From catalog imbedded in main SCHED input file. Doppler based on other sources. 0.399 scan hours, 17.252 baseline hours above horizon. * J1743-0350 17 41 20.616009 * 17 43 58.856133 17 44 24.754055 0.00 -03 48 48.89991 *-03 50 04.61671 -03 50 30.53308 0.00 From catalog imbedded in main SCHED input file. Doppler based on other sources. 0.332 scan hours, 13.658 baseline hours above horizon. * J1751+0939 17 49 10.387929 * 17 51 32.818572 17 51 56.035372 0.30 09 39 42.82589 * 09 39 00.72844 09 38 36.28048 0.20 From catalog imbedded in main SCHED input file. Doppler based on other sources. 0.399 scan hours, 14.946 baseline hours above horizon. * J2015+3710 20 13 37.014534 * 20 15 28.729820 20 15 45.723142 0.00 37 01 44.45892 * 37 10 59.51480 37 12 14.58913 0.00 From catalog imbedded in main SCHED input file. Doppler based on other sources. 0.399 scan hours, 16.754 baseline hours above horizon. * S_SER 15 19 18.922090 * 15 21 39.534426 15 22 03.377288 0.00 14 29 35.55464 * 14 18 53.12402 14 16 48.42951 0.00 From catalog imbedded in main SCHED input file. Hipparcos position Doppler based on LSR frame and radio definition. Velocities: 20.00 20.00 20.00 20.00 1.695 scan hours, 66.104 baseline hours above horizon. Proper motion used. Reference epoch: 1991.25000 At epoch: RA = 15 21 39.534100 Dec = 14 18 53.08600 Rates: RA = 0.28 mas/yr Dec = 2.25 mas/yr Paralax: 0.0000 mas. Planetary motion (includes proper motion). Ref. MJD: 54520.4179 Rates: RA = 0.52744E-07 s/day Dec = 0.61602E-05 arcsec/day * T_OPH 16 30 52.050129 * 16 33 43.700000 16 34 12.175375 0.00 -16 01 39.77807 *-16 07 54.00000 -16 09 04.75438 0.00 From catalog imbedded in main SCHED input file. ICRS position Doppler based on LSR frame and radio definition. Velocities: -29.00 29.00 29.00 29.00 1.413 scan hours, 56.229 baseline hours above horizon. * RT_OPH 17 54 11.440715 * 17 56 32.036574 17 56 54.916309 0.00 11 10 29.85519 * 11 10 09.62030 11 09 48.42258 0.00 From catalog imbedded in main SCHED input file. ICRS position Doppler based on LSR frame and radio definition. Velocities: -40.00 -40.00 -40.00 -40.00 1.695 scan hours, 63.858 baseline hours above horizon. Proper motion used. Reference epoch: 1991.25000 At epoch: RA = 17 56 32.036000 Dec = 11 10 09.72000 Rates: RA = 0.50 mas/yr Dec = -5.90 mas/yr Paralax: 0.0000 mas. Planetary motion (includes proper motion). Ref. MJD: 54520.4179 Rates: RA = 0.93024E-07 s/day Dec = -0.16153E-04 arcsec/day * RT_AQL 19 35 40.404073 * 19 38 01.612956 19 38 24.091919 0.00 11 36 26.98531 * 11 43 17.99549 11 44 10.41222 0.00 From catalog imbedded in main SCHED input file. Hipparcos position Doppler based on LSR frame and radio definition. Velocities: -28.00 -28.00 -28.00 -28.00 1.695 scan hours, 68.169 baseline hours above horizon. Proper motion used. Reference epoch: 1991.25000 At epoch: RA = 19 38 01.603200 Dec = 11 43 18.22800 Rates: RA = 8.48 mas/yr Dec = -13.76 mas/yr Paralax: 0.0000 mas. Planetary motion (includes proper motion). Ref. MJD: 54520.4179 Rates: RA = 0.15808E-05 s/day Dec = -0.37673E-04 arcsec/day 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) BLLAC 52.2 J1613+3412 98.4 J1743-0350 70.7 J1751+0939 71.5 J2015+3710 56.2 S_SER 108.4 T_OPH 86.1 RT_OPH 70.7 RT_AQL 47.4 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