COVER INFORMATION Station: VLBA_KP (Code Kp ) Experiment: M87 multi-epoch at 90cm Exp. Code: BJ046B Schedule Version: 1.00 Processed by SCHED version: Release of 18 Sept. 2003 PI: Bill Junor Address: ISR-1, Space & Atmospheric Sciences MS D466, LANL, P.O. Box 1663 Los Alamos, New Mexico, 87545 U.S.A. Phone: 505 667 0788 EMAIL: bjunor@lanl.gov Fax: 505 665 7395 Phone during observation: 505 699 7692 Observing mode: 90cm 128-4-2 Notes: COVER LETTER: BJ046 SUMMARY: This project needs about 100 hours times 45 baselines to meet the sensitivity requirements. This time can be accumulated in many separated sessions. One session should be a full track with all antennas to set the calibration and ensure full uv coverage. The other sessions can involve as little as 2 hours and as few as 6 antennas. The sessions can be run as filler in gaps between other projects. This project can be run prior to Feb 1, 2004, to accumulate test data on baselines to MK. These test observations need not be long --- 2--4 hours but should include 3C147, 1148-001 and 3C274. Tropospheric weather is not a problem. The ionosphere will have a bigger impact. 3C274 is mostly a night-time object now. -------------------------------------------------------------------- Here is the official dynamic scheduling sheet: ================================================================ Preferred Dynamic Contraints. Alter [defaults] as desired. ================================================================ Equipment constraints: Stations. Below each station code, the "o" indicates an [optional] station that is to be used if it is available. Change "o" to "r" if the station is required or change "o" to "n" if the station is not to be used. SC HN NL FD LA PT KP OV BR MK o o o o o o o o o r Minimum number of stations [6]: May we swap PT for a single VLA antenna? [yes] Consult http://www.aoc.nrao.edu/~gtaylor/y1gotcha.html to decide. If you adopt the default, then both PT and VLA1 must be in the stations list in the keyin file. Bands and polarizations. Below each band code, insert "R" if the righthand polarization is to be used, "L" if the lefthand polarization is to be used, "d" if dual polarizations are to be used, or "o" if the band is in your setups but scheduling should not be constrained by its availability. 90cm 50cm 20cm 13cm 6cm 4cm 2cm 1cm 7mm 3mm d Weather constraints: [appropriate for bands marked "L", "R", or "d" above and for at least the minimum number of stations] Date constraints: Preferred date(s), usually a series start [none]: No earlier than Jan 15, 2004. Excluded dates plus reason [none]: Too close to Sun. Preferred interval between segments in days [none]: Special conditions (e.g., a series with different spacings in time) [See the comments at the top.]: Schedule for VLBA_KP (Code Kp ) Page 2 M87 multi-epoch at 90cm 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. TPStart: Tape motion start time. Frequencies are LO sum (band edge). 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) ---------------------------------------------------------------------------------------- --- Tue 3 Feb 2004 Day 34 --- Next scan frequencies: 324.49 324.49 332.49 332.49 Next BBC frequencies: 824.49 824.49 832.49 832.49 Next scan bandwidths: 8.00 8.00 8.00 8.00 04 51 35 3C147 06 16 02 71.1 -16.6 0.6 157.9 0 1 1 0 04 51 15 04 56 34 --- 06 21 02 70.7 -18.9 0.6 154.8 299 F 1 2128 04 58 34 3C147 06 23 02 70.6 -19.7 0.7 153.6 114 1 1 2128 04 58 14 05 03 33 --- 06 28 02 70.2 -21.9 0.8 150.6 299 F 1 4256 05 05 32 3C147 06 30 02 70.1 -22.7 0.8 149.5 114 1 1 4256 05 05 12 05 10 32 --- 06 35 02 69.6 -24.7 0.9 146.7 299 F 1 6384 05 49 39 3C274 07 14 15 15.6 84.9 -5.3 -59.9 2233 1 2 6384 05 49 19 06 19 34 --- 07 44 15 21.9 88.8 -4.8 -60.3 1795 R 1 16716 06 21 37 3C147 07 46 19 61.0 -42.9 2.1 116.4 30 1 2 16716 06 21 17 06 26 36 --- 07 51 19 60.2 -43.6 2.1 114.8 299 R 1 14588 06 28 48 1148-001 07 53 31 25.4 107.8 -4.0 -53.9 25 1 2 14588 06 28 28 06 33 47 --- 07 58 31 26.4 108.6 -3.9 -53.5 299 R 1 12460 06 34 47 3C274 07 59 31 25.2 90.8 -4.5 -60.3 42 1 2 12460 06 34 27 07 04 42 --- 08 29 31 31.5 95.0 -4.0 -59.9 1795 R 1 360 07 05 42 3C274 08 30 31 31.7 95.1 -4.0 -59.9 54 1 3 360 07 05 22 07 35 37 --- 09 00 31 38.1 99.7 -3.5 -58.9 1795 F 1 12460 07 37 42 3C147 09 02 36 49.2 -49.0 3.3 96.7 20 1 3 12460 07 37 22 07 42 41 --- 09 07 36 48.4 -49.1 3.4 95.7 299 F 1 14588 07 44 56 1148-001 09 09 52 40.1 122.4 -2.7 -45.8 15 1 3 14588 07 44 36 07 49 56 --- 09 14 52 40.9 123.5 -2.6 -45.0 299 F 1 16716 07 50 55 3C274 09 15 52 41.2 102.2 -3.3 -58.1 40 1 4 16716 07 50 35 08 20 50 --- 09 45 52 47.4 107.8 -2.8 -55.8 1795 R 1 6384 08 21 50 3C274 09 46 52 47.6 108.0 -2.7 -55.7 54 1 5 6384 08 21 30 08 51 45 --- 10 16 52 53.5 114.8 -2.2 -52.1 1795 F 1 5717 08 53 49 3C147 10 18 55 36.9 -48.8 4.6 82.2 8 1 5 5717 08 53 29 08 58 48 --- 10 23 55 36.1 -48.7 4.7 81.3 299 F 1 7845 Schedule for VLBA_KP (Code Kp ) Page 3 M87 multi-epoch at 90cm 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. TPStart: Tape motion start time. Frequencies are LO sum (band edge). 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) ---------------------------------------------------------------------------------------- --- Tue 3 Feb 2004 Day 34 --- 09 01 10 1148-001 10 26 18 51.9 144.2 -1.4 -29.8 8 1 5 7845 09 00 50 09 06 09 --- 10 31 18 52.5 145.9 -1.3 -28.4 299 F 1 9973 09 07 09 3C274 10 32 18 56.4 118.9 -2.0 -49.5 36 1 6 9973 09 06 49 09 37 04 --- 11 02 18 61.7 128.8 -1.5 -42.6 1795 R 1 13127 09 38 04 3C274 11 03 18 61.9 129.2 -1.5 -42.3 54 1 6 13127 09 37 44 10 07 59 --- 11 33 18 66.3 142.6 -1.0 -31.8 1795 R 1 1026 10 10 01 3C147 11 35 20 25.0 314.7 5.9 69.3 1 1 7 1026 10 09 41 10 15 00 --- 11 40 20 24.3 315.0 6.0 68.5 299 F 1 1102 10 16 44 1148-001 11 42 05 57.6 175.9 -0.1 -3.5 6 1 7 1102 10 16 24 10 21 43 --- 11 47 05 57.6 178.2 -0.1 -1.5 299 F 1 3230 10 22 43 3C274 11 48 05 68.1 150.8 -0.7 -25.0 33 1 7 3230 10 22 23 10 52 38 --- 12 18 05 70.2 170.6 -0.2 -8.1 1795 F 1 15330 10 53 38 3C274 12 19 05 70.2 171.3 -0.2 -7.5 54 1 8 15330 10 53 18 11 23 33 --- 12 49 05 70.0 193.0 0.3 11.2 1795 R 1 7769 11 25 33 3C147 12 51 05 14.1 320.5 7.1 56.8 2 1 8 7769 11 25 13 11 30 32 --- 12 56 05 13.5 321.0 7.2 55.9 299 R 1 5641 11 32 29 1148-001 12 58 02 53.9 209.4 1.1 24.6 30 1 8 5641 11 32 09 11 37 29 --- 13 03 02 53.4 211.3 1.2 26.1 299 R 1 3514 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: bw051.set Matches group v5090n in /home/filehost/cwalker/sched/catalogs/freq.dat Setup group: 1 Station: VLBA Total bit rate: 128 Format: VLBA1:4 Bits per sample: 2 Sample rate: 16.000 Number of channels: 4 Passes/head pos: 1 Speedup factor: 2.00 Tape speeds: Low density - 133.330 ips, High density - 80.00 ips Time per pass for 17600 ft, High density tapes is: 00:44:00 1st LO= -500.00 -500.00 -500.00 -500.00 Net SB= U U U U Pol. = RCP LCP RCP LCP BBC = 1 2 3 4 BBC SB= U U U U IF = B D B D VLBA FE= omit 90cm omit 90cm VLBA Synth= 15.4 15.4 15.4 The following frequency sets based on this setup were used. Frequency Set: 1 Setup file default. Used pcal sets: 1 LO sum= 324.49 324.49 332.49 332.49 BBC fr= 824.49 824.49 832.49 832.49 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 = 1MHZ PCALXB1= S1 S3 S1 S3 S1 S2 S3 S4 PCALXB2= S2 S4 S2 S4 M1 M2 M3 M4 PCALFR1= 510 510 6510 6510 0 0 0 0 PCALFR2= 510 510 6510 6510 0 0 0 0 Track assignments are: track1= 2, 18, 3, 19 barrel=roll_auto SOURCE LIST -- M87 multi-epoch at 90cm 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). Source Source position (RA/Dec) (B1950) (J2000) (Date) J0542+4951 05 38 43.517539 * 05 42 36.137917 05 42 55.605195 0538+498 49 49 42.83693 * 49 51 07.23356 49 51 26.49724 * 3C147 /home/filehost/cwalker/sched/catalogs/sources.vlba J0542+49 ICRF - Ext.1 Source - 1998 IERS Annual Report J1150-0023 11 48 10.124953 * 11 50 43.870762 11 50 56.694991 * 1148-001 -00 07 13.16375 *-00 23 54.20490 -00 25 17.14744 J1150-00 /home/filehost/cwalker/sched/catalogs/sources.vlba ICRF - Ext.1 Source - 1998 IERS Annual Report J1230+1223 12 28 17.569280 * 12 30 49.423382 12 31 02.023923 1228+126 12 40 01.74911 * 12 23 28.04393 12 22 01.08304 * 3C274 /home/filehost/cwalker/sched/catalogs/sources.vlba J1230+12 ICRF - Ext.1 Source - 1998 IERS Annual Report 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) 3C147 127.7 1148-001 135.7 3C274 130.1 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