COVER INFORMATION Station: VLBA_OV (Code Ov ) Experiment: H2O masers in IRAS16342-3814 Exp. Code: bc184b Schedule Version: 1.00 Processed by SCHED version: 6.05 June 2006 PI: Mark Claussen Address: National Radio Astronomy Observatory P. O. Box O Socorro, New Mexico, 87801 U.S.A. Phone: 505 835 7284 EMAIL: mclausse@aoc.nrao.edu Fax: 505 835 7027 Phone during observation: 505 835 7284 Observing mode: 1.3 cm VLBA non-standard correlator setup Notes: Schedule for VLBA_OV (Code Ov ) Page 2 H2O masers in IRAS16342-3814 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 ---------------------------------------------------------------------------------------- --- Mon 7 Apr 2008 Day 98 --- Next scan frequencies: 22220.27 22226.80 22233.25 22239.70 Next BBC frequencies: 720.27 726.80 733.25 739.70 Next scan bandwidths: 8.00 8.00 8.00 8.00 07 38 40 J1626-2951 12 49 22 5.8 134.9 -3.6 -40.5 0 1 1 0 Stopped 07 40 20 =1622-297 12 51 02 6.0 135.2 -3.6 -40.3 100 S 1 2 07 40 24 J1626-2951 12 51 07 6.1 135.2 -3.6 -40.3 0 1 1 2 07 40 24 07 45 24 =1622-297 12 56 07 6.8 136.1 -3.5 -39.6 299 F 1 6 07 40 47 08 00 49 IRAS16342 13 11 34 0.7 142.0 -3.4 D -38.7 910 1 1 6 08 00 49 08 15 47 --- 13 26 34 2.5 144.4 -3.2 H -36.3 0 F 1 21 08 01 12 08 15 51 IRAS16342 13 26 39 2.5 144.4 -3.2 H -36.3 0 1 1 21 08 15 47 08 30 48 --- 13 41 39 4.2 146.8 -2.9 -33.8 0 F 1 35 08 15 47 08 30 53 IRAS16342 13 41 43 4.2 146.8 -2.9 -33.8 0 1 1 35 08 30 48 08 45 50 --- 13 56 43 5.7 149.3 -2.7 -31.2 898 F 1 50 08 30 48 08 46 50 J1733-1304 13 57 43 18.6 123.8 -3.6 -42.8 28 1 1 50 08 46 50 08 51 49 =1730-130 14 02 43 19.4 124.7 -3.5 -42.2 299 F 1 55 08 47 13 08 52 49 IRAS16342 14 03 43 6.4 150.5 -2.6 -30.0 28 1 1 55 08 52 49 09 07 46 --- 14 18 43 7.9 153.1 -2.3 -27.4 898 F 1 69 08 53 12 09 07 51 IRAS16342 14 18 47 7.9 153.1 -2.3 -27.4 0 1 1 69 09 07 46 09 22 48 --- 14 33 47 9.2 155.8 -2.1 -24.6 898 F 1 84 09 07 46 09 22 53 IRAS16342 14 33 51 9.2 155.8 -2.1 -24.6 0 1 1 84 09 22 48 09 37 50 --- 14 48 51 10.3 158.5 -1.8 -21.8 898 F 1 98 09 22 48 09 37 54 IRAS16342 14 48 56 10.3 158.5 -1.8 -21.8 0 1 1 98 09 37 50 09 52 52 --- 15 03 56 11.3 161.3 -1.6 -19.0 898 F 1 113 09 37 50 09 52 56 IRAS16342 15 04 00 11.4 161.4 -1.6 -18.9 0 1 1 113 09 52 52 10 07 54 --- 15 19 00 12.2 164.2 -1.3 -16.0 898 F 1 127 09 52 52 10 07 58 IRAS16342 15 19 05 12.2 164.2 -1.3 -16.0 0 1 1 127 10 07 54 10 22 56 --- 15 34 05 13.0 167.1 -1.1 -13.1 898 F 1 142 10 07 54 10 23 00 IRAS16342 15 34 09 13.0 167.2 -1.1 -13.0 0 1 1 142 10 22 56 10 37 58 --- 15 49 09 13.6 170.1 -0.8 -10.0 898 F 1 157 10 22 56 Schedule for VLBA_OV (Code Ov ) Page 3 H2O masers in IRAS16342-3814 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 ---------------------------------------------------------------------------------------- --- Mon 7 Apr 2008 Day 98 --- 10 38 02 IRAS16342 15 49 14 13.6 170.1 -0.8 -10.0 0 1 1 157 10 37 58 10 53 00 --- 16 04 14 14.0 173.1 -0.6 -7.0 898 F 1 171 10 37 58 10 53 04 IRAS16342 16 04 18 14.0 173.1 -0.6 -7.0 0 1 1 171 10 53 00 11 08 02 --- 16 19 18 14.3 176.2 -0.3 -3.9 898 F 1 186 10 53 00 11 08 06 IRAS16342 16 19 22 14.3 176.2 -0.3 -3.9 0 1 1 186 11 08 02 11 23 04 --- 16 34 22 14.4 179.2 -0.1 -0.8 898 F 1 200 11 08 02 11 23 08 IRAS16342 16 34 27 14.4 179.2 -0.1 -0.8 0 1 1 200 11 23 04 11 38 06 --- 16 49 27 14.4 182.3 0.2 2.3 898 F 1 215 11 23 04 11 38 10 IRAS16342 16 49 31 14.4 182.3 0.2 2.3 0 1 1 215 11 38 06 11 53 08 --- 17 04 31 14.2 185.3 0.4 5.4 898 F 1 229 11 38 06 11 53 12 IRAS16342 17 04 36 14.2 185.3 0.4 5.4 0 1 1 229 11 53 08 12 08 09 --- 17 19 36 13.8 188.3 0.7 8.5 898 F 1 244 11 53 08 12 08 14 IRAS16342 17 19 40 13.8 188.3 0.7 8.5 0 1 1 244 12 08 09 12 23 11 --- 17 34 40 13.3 191.3 0.9 11.5 898 F 1 258 12 08 09 12 24 13 J1733-1304 17 35 42 39.7 180.7 0.0 0.6 3 1 1 258 12 24 13 12 29 12 =1730-130 17 40 42 39.7 182.3 0.1 1.9 299 F 1 263 12 24 36 12 30 15 IRAS16342 17 41 44 13.0 192.7 1.1 12.9 3 1 1 263 12 30 15 12 45 12 --- 17 56 44 12.3 195.6 1.3 15.9 898 F 1 278 12 30 38 12 45 16 IRAS16342 17 56 49 12.3 195.6 1.3 15.9 0 1 1 278 12 45 12 13 00 14 --- 18 11 49 11.4 198.5 1.6 18.8 898 F 1 292 12 45 12 13 00 18 IRAS16342 18 11 53 11.4 198.5 1.6 18.8 0 1 1 292 13 00 14 13 15 16 --- 18 26 53 10.4 201.3 1.8 21.7 898 F 1 307 13 00 14 13 15 20 IRAS16342 18 26 57 10.4 201.4 1.8 21.7 0 1 1 307 13 15 16 13 30 18 --- 18 41 57 9.2 204.1 2.1 24.5 898 F 1 321 13 15 16 13 31 20 J1733-1304 18 42 59 37.1 201.4 1.2 17.3 0 1 1 321 13 31 20 13 36 19 =1730-130 18 47 59 36.7 202.8 1.2 18.5 299 F 1 326 13 31 43 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: bc184.set Matches group v1cm_b3 in /home/filehost/cwalker/sched/catalogs/freq.dat Setup group: 8 Station: VLBA_OV Total bit rate: 128 Format: VLBA1:4 Bits per sample: 2 Sample rate: 16.000 Number of channels: 4 Speedup factor: 2.00 Disk used to record data. 1st LO= 21500.00 21500.00 21500.00 21500.00 Net SB= U U U U Pol. = LCP LCP LCP LCP BBC = 1 2 3 4 BBC SB= U U U U IF = D D D D VLBA FE= omit 1cm omit 1cm VLBA Synth= 9.1 15.4 12.4 The following frequency sets based on this setup were used. Frequency Set: 8 Based on FREQ, BW, and/or DOPPLER in schedule. Used pcal sets: 1 LO sum= 22220.27 22226.80 22233.25 22239.70 BBC fr= 720.27 726.80 733.25 739.70 Bandwd= 8.000 8.000 8.000 8.000 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, 18, 3, 19 barrel=roll_off SOURCE LIST -- H2O masers in IRAS16342-3814 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) * IRAS16342 16 34 16.977557 * 16 37 40.003000 16 38 15.166071 0.00 -38 14 19.14315 *-38 20 18.47000 -38 21 22.20294 0.00 From catalog imbedded in main SCHED input file. Doppler based on LSR frame and radio definition. Velocities: 176.00 88.00 1.00 -86.00 5.485 scan hours, 134.381 baseline hours above horizon. * J1626-2951 16 22 57.242941 * 16 26 06.020847 16 26 38.757846 0.00 1622-297 -29 44 41.40057 *-29 51 26.97131 -29 52 41.24367 0.00 J1626-29 From catalog imbedded in main SCHED input file. USNO - Ref Frame 1998-6, Eubanks June 1998 Doppler based on other sources. 0.083 scan hours, 2.327 baseline hours above horizon. * J1733-1304 17 30 13.535185 * 17 33 02.705782 17 33 31.789612 0.00 1730-130 -13 02 45.83980 *-13 04 49.54828 -13 05 20.89665 0.00 J1733-13 From catalog imbedded in main SCHED input file. NRAO530 USNO - Ref Frame 1998-6, Eubanks June 1998 Doppler based on other sources. 0.249 scan hours, 8.311 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) IRAS16342 123.0 J1626-2951 127.8 J1733-1304 114.1 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