COVER INFORMATION Station: HART (Code Hh ) Experiment: OH outburst in a proto-planetary nebula Exp. Code: es057b Schedule Version: 1.00 Processed by SCHED version: 6.04 March 2006 PI: M. Szymczak Address: Torun Centre for Astronomy ul. Gagarina 11, Torun, PL-87100 Poland Phone: +48 56 6113029 EMAIL: msz@astro.uni.torun.pl Fax: +48 56 6113009 Phone during observation: +48 56 6113010 Observing mode: VLBA/MKIV Notes: Please, make sure PHASE CAL is OFF. 0.5MHz filters Schedule for HART (Code Hh ) Page 2 OH outburst in a proto-planetary nebula 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 ---------------------------------------------------------------------------------------- --- Mon 2 Jun 2008 Day 154 --- Next scan frequencies: 1611.79 1611.79 1611.79 1611.79 Next BBC frequencies: 101.79 101.79 101.79 101.79 Next scan bandwidths: 0.50 0.50 0.50 0.50 19 00 00 3C286 13 37 12 33.6 358.5 0.1 0.0 0 1 1 0 19 00 00 19 10 00 --- 13 47 13 33.5 356.0 0.3 0.0 600 F 1 2 19 00 04 19 12 00 3C286 13 49 14 33.5 355.4 0.3 0.0 95 1 1 2 19 12 00 19 22 00 --- 13 59 15 33.3 352.9 0.5 0.0 600 F 1 5 19 12 04 19 24 00 3C286 14 01 16 33.2 352.3 0.5 0.0 95 1 1 5 19 24 00 19 34 00 --- 14 11 17 32.8 349.8 0.7 0.0 600 F 1 7 19 24 04 19 34 00 3C345 14 11 17 15.4 29.4 -2.5 0.0 -123 1 1 7 19 34 00 19 44 00 --- 14 21 19 16.5 27.7 -2.4 0.0 477 F 1 10 19 34 04 19 44 00 3C345 14 21 19 16.5 27.7 -2.4 0.0 -20 1 1 10 19 44 00 19 48 00 --- 14 25 20 16.9 27.0 -2.3 0.0 220 F 1 11 19 44 04 19 48 00 3C286 14 25 20 32.2 346.3 0.9 0.0 -123 1 1 11 19 48 00 19 58 00 --- 14 35 21 31.6 343.9 1.1 0.0 477 F 1 13 19 48 04 20 00 00 3C286 14 37 22 31.5 343.4 1.1 0.0 95 1 1 13 20 00 00 20 10 00 --- 14 47 23 30.8 341.0 1.3 0.0 600 F 1 15 20 00 04 20 12 00 3C286 14 49 24 30.6 340.5 1.3 0.0 95 1 1 15 20 12 00 20 22 00 --- 14 59 25 29.9 338.2 1.5 0.0 600 F 1 18 20 12 04 20 22 00 3C345 14 59 25 20.0 21.0 -1.7 0.0 -123 1 1 18 20 22 00 20 32 00 --- 15 09 27 20.8 19.1 -1.6 0.0 477 F 1 20 20 22 04 20 32 00 3C345 15 09 27 20.8 19.1 -1.6 0.0 -20 1 1 20 20 32 00 20 36 00 --- 15 13 28 21.1 18.3 -1.5 0.0 220 F 1 21 20 32 04 20 36 00 3C286 15 13 28 28.6 335.0 1.7 0.0 -123 1 1 21 20 36 00 20 46 00 --- 15 23 29 27.6 332.8 1.9 0.0 477 F 1 24 20 36 04 20 48 00 3C286 15 25 30 27.4 332.4 1.9 0.0 95 1 1 24 20 48 00 20 58 00 --- 15 35 31 26.3 330.3 2.1 0.0 600 F 1 26 20 48 04 21 00 00 3C286 15 37 32 26.1 329.9 2.1 0.0 95 1 1 26 21 00 00 21 10 00 --- 15 47 33 24.9 327.9 2.3 0.0 600 F 1 29 21 00 04 Schedule for HART (Code Hh ) Page 3 OH outburst in a proto-planetary nebula 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 ---------------------------------------------------------------------------------------- --- Mon 2 Jun 2008 Day 154 --- 21 10 00 3C345 15 47 33 23.0 11.6 -0.9 0.0 -123 1 1 29 21 10 00 21 20 00 --- 15 57 35 23.5 9.6 -0.8 0.0 477 F 1 31 21 10 04 21 20 00 3C345 15 57 35 23.5 9.6 -0.8 0.0 -20 1 1 31 21 20 00 21 24 00 --- 16 01 35 23.6 8.7 -0.7 0.0 220 F 1 32 21 20 04 21 25 30 OH17.7-2.0 16 03 06 53.6 79.0 -2.5 0.0 -46 1 1 32 21 25 30 21 35 30 --- 16 13 07 55.8 77.3 -2.3 0.0 554 F 1 34 21 25 34 21 37 00 OH17.7-2.0 16 14 38 56.1 77.0 -2.3 0.0 65 1 1 34 21 37 00 21 47 00 --- 16 24 39 58.3 75.1 -2.1 0.0 600 F 1 37 21 37 04 21 47 00 OH17.7-2.0 16 24 39 58.3 75.1 -2.1 0.0 -20 1 1 37 21 47 00 21 57 00 --- 16 34 41 60.5 72.9 -1.9 0.0 580 F 1 39 21 47 04 21 58 30 OH17.7-2.0 16 36 11 60.8 72.6 -1.9 0.0 65 1 1 39 21 58 30 22 06 30 --- 16 44 12 62.5 70.7 -1.8 0.0 480 F 1 41 21 58 34 22 08 00 J1733-1304 16 45 43 73.0 43.5 -0.8 0.0 33 1 1 41 22 08 00 22 14 00 =1730-130 16 51 44 73.9 39.5 -0.7 0.0 360 F 1 43 22 08 04 22 15 30 OH17.7-2.0 16 53 14 64.4 68.2 -1.6 0.0 35 1 1 43 22 15 30 22 25 30 --- 17 03 16 66.5 65.2 -1.5 0.0 600 F 1 45 22 15 34 22 27 00 OH17.7-2.0 17 04 46 66.8 64.7 -1.4 0.0 65 1 1 45 22 27 00 22 37 00 --- 17 14 47 68.8 61.1 -1.3 0.0 600 F 1 47 22 27 04 22 37 00 OH17.7-2.0 17 14 47 68.8 61.1 -1.3 0.0 -20 1 1 47 22 37 00 22 47 00 --- 17 24 49 70.8 56.8 -1.1 0.0 580 F 1 50 22 37 04 22 48 30 OH17.7-2.0 17 26 19 71.0 56.1 -1.1 0.0 65 1 1 50 22 48 30 22 56 30 --- 17 34 21 72.5 52.0 -0.9 0.0 480 F 1 52 22 48 34 22 58 00 J1733-1304 17 35 51 77.2 357.5 0.0 0.0 33 1 1 52 22 58 00 23 04 00 =1730-130 17 41 52 77.1 350.9 0.1 0.0 360 F 1 53 22 58 04 23 05 30 OH17.7-2.0 17 43 22 74.0 46.6 -0.8 0.0 35 1 1 53 23 05 30 23 15 30 --- 17 53 24 75.6 39.5 -0.6 0.0 600 F 1 56 23 05 34 23 17 00 OH17.7-2.0 17 54 54 75.8 38.3 -0.6 0.0 65 1 1 56 23 17 00 23 27 00 --- 18 04 56 77.1 29.4 -0.4 0.0 600 F 1 58 23 17 04 23 27 00 OH17.7-2.0 18 04 56 77.1 29.4 -0.4 0.0 -20 1 1 58 23 27 00 23 37 00 --- 18 14 57 78.0 19.0 -0.3 0.0 580 F 1 60 23 27 04 Schedule for HART (Code Hh ) Page 4 OH outburst in a proto-planetary nebula 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 ---------------------------------------------------------------------------------------- --- Mon 2 Jun 2008 Day 154 --- 23 38 30 OH17.7-2.0 18 16 28 78.1 17.3 -0.2 0.0 65 1 1 60 23 38 30 23 46 30 --- 18 24 29 78.5 8.0 -0.1 0.0 480 F 1 62 23 38 34 23 48 00 J1733-1304 18 25 59 72.2 313.6 0.9 0.0 33 1 1 62 23 48 00 23 54 00 =1730-130 18 32 00 71.2 310.2 1.0 0.0 360 F 1 64 23 48 04 --- Start: Mon 2 Jun 2008 Day 154 -- Stop: Tue 3 Jun 2008 Day 155 --- 23 55 30 OH17.7-2.0 18 33 30 78.6 357.0 0.0 0.0 35 1 1 64 23 55 30 00 05 30 --- 18 43 32 78.2 345.0 0.2 0.0 600 F 1 66 23 55 34 00 07 00 OH17.7-2.0 18 45 02 78.1 343.3 0.2 0.0 65 1 1 66 00 07 00 00 17 00 --- 18 55 04 77.3 332.6 0.4 0.0 600 F 1 69 00 07 04 00 17 00 OH17.7-2.0 18 55 04 77.3 332.6 0.4 0.0 -20 1 1 69 00 17 00 00 27 00 --- 19 05 06 76.1 323.4 0.6 0.0 580 F 1 71 00 17 04 00 28 30 OH17.7-2.0 19 06 36 75.9 322.2 0.6 0.0 65 1 1 71 00 28 30 00 36 30 --- 19 14 37 74.7 316.1 0.7 0.0 480 F 1 73 00 28 34 00 38 00 J1733-1304 19 16 07 62.7 293.1 1.7 0.0 33 1 1 73 00 38 00 00 44 00 =1730-130 19 22 08 61.5 291.5 1.8 0.0 360 F 1 75 00 38 04 00 45 30 OH17.7-2.0 19 23 39 73.2 310.3 0.9 0.0 35 1 1 75 00 45 30 00 55 30 --- 19 33 40 71.4 304.9 1.0 0.0 600 F 1 77 00 45 34 00 57 00 OH17.7-2.0 19 35 10 71.1 304.1 1.1 0.0 65 1 1 77 00 57 00 01 07 00 --- 19 45 12 69.2 299.7 1.2 0.0 600 F 1 79 00 57 04 01 07 00 OH17.7-2.0 19 45 12 69.2 299.7 1.2 0.0 -20 1 1 79 01 07 00 01 17 00 --- 19 55 14 67.2 296.0 1.4 0.0 580 F 1 82 01 07 04 01 18 30 OH17.7-2.0 19 56 44 66.9 295.5 1.4 0.0 65 1 1 82 01 18 30 01 26 30 --- 20 04 45 65.3 292.9 1.6 0.0 480 F 1 84 01 18 34 01 28 00 J1733-1304 20 06 16 52.0 282.2 2.5 0.0 33 1 1 84 01 28 00 01 34 00 =1730-130 20 12 17 50.6 281.2 2.6 0.0 360 F 1 85 01 28 04 01 35 30 OH17.7-2.0 20 13 47 63.4 290.4 1.7 0.0 35 1 1 85 01 35 30 01 45 30 --- 20 23 48 61.3 287.9 1.9 0.0 600 F 1 88 01 35 34 01 47 00 OH17.7-2.0 20 25 19 60.9 287.5 1.9 0.0 65 1 1 88 01 47 00 01 57 00 --- 20 35 20 58.8 285.3 2.1 0.0 600 F 1 90 01 47 04 Schedule for HART (Code Hh ) Page 5 OH outburst in a proto-planetary nebula 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 ---------------------------------------------------------------------------------------- --- Tue 3 Jun 2008 Day 155 --- 01 57 00 OH17.7-2.0 20 35 20 58.8 285.3 2.1 0.0 -20 1 1 90 01 57 00 02 07 00 --- 20 45 22 56.6 283.4 2.2 0.0 580 F 1 92 01 57 04 02 08 30 OH17.7-2.0 20 46 52 56.3 283.1 2.3 0.0 65 1 1 92 02 08 30 02 16 30 --- 20 54 54 54.5 281.7 2.4 0.0 480 F 1 94 02 08 34 02 18 00 J1733-1304 20 56 24 40.8 275.0 3.4 0.0 33 1 1 94 02 18 00 02 24 00 =1730-130 21 02 25 39.5 274.2 3.5 0.0 360 F 1 96 02 18 04 02 25 30 OH17.7-2.0 21 03 55 52.5 280.1 2.5 0.0 35 1 1 96 02 25 30 02 35 30 --- 21 13 57 50.3 278.6 2.7 0.0 600 F 1 98 02 25 34 02 37 00 OH17.7-2.0 21 15 27 50.0 278.4 2.7 0.0 65 1 1 98 02 37 00 02 47 00 --- 21 25 29 47.7 276.9 2.9 0.0 600 F 1 101 02 37 04 02 47 00 OH17.7-2.0 21 25 29 47.7 276.9 2.9 0.0 -20 1 1 101 02 47 00 02 57 00 --- 21 35 30 45.5 275.6 3.1 0.0 580 F 1 103 02 47 04 02 58 30 OH17.7-2.0 21 37 00 45.1 275.4 3.1 0.0 65 1 1 103 02 58 30 03 06 30 --- 21 45 02 43.3 274.4 3.2 0.0 480 F 1 105 02 58 34 03 08 00 J1733-1304 21 46 32 29.6 269.2 4.2 0.0 33 1 1 105 03 08 00 03 14 00 =1730-130 21 52 33 28.2 268.5 4.3 0.0 360 F 1 106 03 08 04 03 15 30 OH17.7-2.0 21 54 03 41.3 273.2 3.4 0.0 35 1 1 106 03 15 30 03 25 30 --- 22 04 05 39.1 272.1 3.6 0.0 600 F 1 109 03 15 34 03 27 00 OH17.7-2.0 22 05 35 38.7 271.9 3.6 0.0 65 1 1 109 03 27 00 03 37 00 --- 22 15 37 36.5 270.8 3.7 0.0 600 F 1 111 03 27 04 03 37 00 OH17.7-2.0 22 15 37 36.5 270.8 3.7 0.0 -20 1 1 111 03 37 00 03 47 00 --- 22 25 38 34.2 269.7 3.9 0.0 580 F 1 114 03 37 04 03 48 30 OH17.7-2.0 22 27 09 33.9 269.5 3.9 0.0 65 1 1 114 03 48 30 03 56 30 --- 22 35 10 32.1 268.6 4.1 0.0 480 F 1 116 03 48 34 03 58 00 J1733-1304 22 36 40 18.3 264.0 5.1 0.0 33 1 1 116 03 58 00 04 04 00 =1730-130 22 42 41 17.0 263.4 5.2 0.0 360 F 1 117 03 58 04 04 05 30 OH17.7-2.0 22 44 11 30.0 267.7 4.2 0.0 35 1 1 117 04 05 30 04 15 30 --- 22 54 13 27.8 266.7 4.4 0.0 600 F 1 120 04 05 34 04 17 00 OH17.7-2.0 22 55 43 27.5 266.5 4.4 0.0 65 1 1 120 04 17 00 04 27 00 --- 23 05 45 25.2 265.5 4.6 0.0 600 F 1 122 04 17 04 Schedule for HART (Code Hh ) Page 6 OH outburst in a proto-planetary nebula 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 ---------------------------------------------------------------------------------------- --- Tue 3 Jun 2008 Day 155 --- 04 27 00 OH17.7-2.0 23 05 45 25.2 265.5 4.6 0.0 -20 1 1 122 04 27 00 04 37 00 --- 23 15 47 23.0 264.5 4.7 0.0 580 F 1 124 04 27 04 04 38 30 OH17.7-2.0 23 17 17 22.6 264.3 4.8 0.0 65 1 1 124 04 38 30 04 46 30 --- 23 25 18 20.8 263.5 4.9 0.0 480 F 1 126 04 38 34 04 48 30 J2253+1608 23 27 18 47.2 348.3 0.5 0.0 -38 1 1 126 04 48 30 05 03 30 =2251+158 23 42 21 46.3 343.2 0.8 0.0 862 F 1 130 04 48 34 05 03 30 J2253+1608 23 42 21 46.3 343.2 0.8 0.0 -20 1 1 130 05 03 30 05 18 30 =2251+158 23 57 23 45.2 338.3 1.1 0.0 880 F 1 134 05 03 34 05 20 30 J2253+1608 23 59 24 45.0 337.6 1.1 0.0 95 1 1 134 05 20 30 05 35 30 =2251+158 00 14 26 43.6 333.0 1.3 0.0 900 F 1 137 05 20 34 05 37 30 J2253+1608 00 16 27 43.4 332.4 1.4 0.0 95 1 1 137 05 37 30 05 52 30 =2251+158 00 31 29 41.7 328.1 1.6 0.0 900 F 1 141 05 37 34 05 54 30 J2253+1608 00 33 29 41.5 327.5 1.7 0.0 95 1 1 141 05 54 30 06 09 30 =2251+158 00 48 32 39.6 323.5 1.9 0.0 900 F 1 144 05 54 34 06 11 30 J2253+1608 00 50 32 39.3 323.0 1.9 0.0 95 1 1 144 06 11 30 06 26 30 =2251+158 01 05 35 37.2 319.2 2.2 0.0 900 F 1 148 06 11 34 06 28 30 J2253+1608 01 07 35 36.9 318.8 2.2 0.0 95 1 1 148 06 28 30 06 43 30 =2251+158 01 22 37 34.6 315.3 2.5 0.0 900 F 1 152 06 28 34 06 45 30 J2253+1608 01 24 38 34.3 314.9 2.5 0.0 95 1 1 152 06 45 30 07 00 30 =2251+158 01 39 40 31.8 311.7 2.8 0.0 900 F 1 155 06 45 34 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: es057.set Matches group hh18cm in /usr/local/sched/catalogs/freq.dat Values confirmed by E-mail Jonathan Quick 291100 (CR) Setup group: 7 Station: HART Total bit rate: 32 Format: MKIV1:1 Bits per sample: 2 Sample rate: 4.000 Number of channels: 4 Speedup factor: 2.00 Disk used to record data. 1st LO= 1510.00 1510.00 1510.00 1510.00 Net SB= U U U U Pol. = LCP RCP LCP RCP BBC = 1 2 3 4 BBC SB= U U U U IF = 1N 2N 1N 2N The following frequency sets based on this setup were used. Frequency Set: 7 Based on FREQ, BW, and/or DOPPLER in schedule. No pcal detection. LO sum= 1611.79 1611.79 1611.79 1611.79 BBC fr= 101.79 101.79 101.79 101.79 Bandwd= 0.500 0.500 0.500 0.500 Track assignments are: track1= 2, 6, 10, 14 barrel=roll_off SOURCE LIST -- OH outburst in a proto-planetary nebula 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) * OH17.7-2.0 18 27 39.767201 * 18 30 30.695000 18 31 01.378577 0.00 -14 31 03.68772 *-14 28 56.82000 -14 28 40.73318 0.00 From catalog imbedded in main SCHED input file. Doppler based on LSR frame and radio definition. Velocities: 61.60 61.60 61.60 61.60 5.700 scan hours, 149.783 baseline hours above horizon. J1331+3030 13 28 49.657756 * 13 31 08.288048 13 31 33.354364 0.37 1328+307 30 45 58.64060 * 30 30 32.95924 30 27 57.09267 0.47 * 3C286 /usr/local/sched/catalogs/sources.vlba J1331+30 VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro Doppler based on other sources. 1.500 scan hours, 38.480 baseline hours above horizon. J1642+3948 16 41 17.606231 * 16 42 58.809968 16 43 18.088844 0.26 1641+399 39 54 10.81494 * 39 48 36.99400 39 47 32.56184 0.40 * 3C345 /usr/local/sched/catalogs/sources.vlba J1642+39 VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro Doppler based on other sources. 0.700 scan hours, 13.881 baseline hours above horizon. * J1733-1304 17 30 13.535187 * 17 33 02.705785 17 33 33.166595 0.21 1730-130 -13 02 45.83975 *-13 04 49.54823 -13 05 17.91153 0.30 J1733-13 /usr/local/sched/catalogs/sources.vlba NRAO530 VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro Doppler based on other sources. 0.900 scan hours, 20.600 baseline hours above horizon. * J2253+1608 22 51 29.519744 * 22 53 57.747943 22 54 23.142102 0.31 2251+158 15 52 54.34806 * 16 08 53.56089 16 11 29.12833 0.20 3C454.3 /usr/local/sched/catalogs/sources.vlba J2253+16 VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro Doppler based on other sources. 2.000 scan hours, 55.143 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) OH17.7-2.0 153.8 3C286 109.6 3C345 117.9 J1733-1304 165.3 J2253+1608 81.9 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