COVER INFORMATION Station: TIANMA65 (Code T6 ) Experiment: Long overdue - Measuring the Parallax and proper motion of the Crab. Ste Exp. Code: EK036A Schedule Version: 2.00 Processed by SCHED version: 11.40 Release 11.4. March 14, 2015 PI: Franz Kirsten Address: Curtin Institute of Radio Astronomy Curtin University Perth Australia Phone: +61 8 9266 9103 EMAIL: franz.kirsten@curtin.edu.au Fax: +61 8 9266 9246 Phone during observation: +61 8 9266 9103 Observing mode: Continuum 18cm (1 Gb/s), pulsar gating Notes: Target pulsar bright enough to fringe on Fringe finder / bandpass cal: J0518+2054 / J0530+1331 PCAL off, AGC off at all stations Ef, Jb1, T6, Sr, Ro70 require extra attenuator due to high Tsys from Nebula. Schedule for TIANMA65 (Code T6 ) Page 2 Long overdue - Measuring the Parallax and proper motion of the Crab. Ste UP: D => Below limits; H => Below horizon mask; W => still slewing at end; blank => Up. Early: Seconds between end of slew and start. Dwell: On source seconds. Disk: GBytes recorded to this point. TPStart: Recording start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Disk TPStart Stop UT LST EL AZ HA UP ParA Dwell GBytes SYNC ---------------------------------------------------------------------------------------- --- Sun 18 Oct 2015 Day 291 --- Next scan frequencies: 1610.49 1610.49 1610.49 1610.49 1642.49 1642.49 1642.49 1642.49 1674.49 1674.49 1674.49 1674.49 1706.49 1706.49 1706.49 1706.49 Next BBC frequencies: 659.51 659.51 659.51 659.51 627.51 627.51 627.51 627.51 595.51 595.51 595.51 595.51 563.51 563.51 563.51 563.51 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 23 00 00 J0530+1331 08 53 00 40.8 260.9 3.4 60.4 0 0 23 00 00 23 10 00 =0528+134 09 03 01 38.6 262.4 3.5 60.8 600 77 23 00 01 23 11 05 CRAB 09 04 06 42.9 272.1 3.5 67.4 44 77 23 11 05 23 23 25 --- 09 16 28 40.3 273.6 3.7 67.2 740 172 23 11 06 23 23 45 CRAB 09 16 48 40.2 273.7 3.7 67.2 18 172 23 23 45 23 36 15 --- 09 29 20 37.5 275.1 3.9 66.9 750 268 23 23 46 23 36 55 J0518+2054 09 30 01 33.4 275.8 4.2 65.8 22 268 23 36 55 23 37 55 =0515+208 09 31 01 33.2 276.0 4.2 65.8 60 276 23 36 56 23 38 35 CRAB 09 31 41 37.0 275.4 3.9 66.9 22 276 23 38 35 23 51 05 --- 09 44 13 34.3 276.8 4.1 66.5 750 372 23 38 36 --- Start: Sun 18 Oct 2015 Day 291 -- Stop: Mon 19 Oct 2015 Day 292 --- 23 51 25 CRAB 09 44 33 34.3 276.8 4.2 66.5 18 372 23 51 25 00 03 55 --- 09 57 05 31.6 278.2 4.4 66.1 750 468 23 51 26 00 04 35 J0518+2054 09 57 45 27.5 279.0 4.6 64.9 22 468 00 04 35 00 05 35 =0515+208 09 58 45 27.3 279.1 4.7 64.9 60 476 00 04 36 00 06 15 CRAB 09 59 25 31.1 278.5 4.4 66.0 22 476 00 06 15 00 18 45 --- 10 11 57 28.5 279.9 4.6 65.5 750 572 00 06 16 00 19 05 CRAB 10 12 18 28.4 279.9 4.6 65.5 18 572 00 19 05 00 31 35 --- 10 24 50 25.8 281.3 4.8 65.0 750 668 00 19 06 00 32 15 J0518+2054 10 25 30 21.7 282.1 5.1 63.7 22 668 00 32 15 00 33 15 =0515+208 10 26 30 21.5 282.2 5.1 63.7 60 676 00 32 16 00 33 55 CRAB 10 27 10 25.3 281.5 4.9 64.8 23 676 00 33 55 00 46 25 --- 10 39 42 22.6 282.9 5.1 64.2 750 772 00 33 56 00 46 45 CRAB 10 40 02 22.6 282.9 5.1 64.2 18 772 00 46 45 00 59 15 --- 10 52 34 20.0 284.3 5.3 63.5 750 868 00 46 46 Schedule for TIANMA65 (Code T6 ) Page 3 Long overdue - Measuring the Parallax and proper motion of the Crab. Ste UP: D => Below limits; H => Below horizon mask; W => still slewing at end; blank => Up. Early: Seconds between end of slew and start. Dwell: On source seconds. Disk: GBytes recorded to this point. TPStart: Recording start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Disk TPStart Stop UT LST EL AZ HA UP ParA Dwell GBytes SYNC ---------------------------------------------------------------------------------------- --- Mon 19 Oct 2015 Day 292 --- 01 00 25 J0530+1331 10 53 44 15.0 277.0 5.4 61.0 49 868 01 00 25 01 05 00 =0528+134 10 58 20 14.0 277.5 5.4 60.8 275 903 01 00 26 01 06 10 CRAB 10 59 30 18.5 285.1 5.4 63.1 49 903 01 06 10 01 18 30 --- 11 11 52 16.0 286.4 5.6 62.4 740 998 01 06 11 01 18 50 CRAB 11 12 12 15.9 286.5 5.6 62.4 18 998 01 18 50 01 31 10 --- 11 24 34 13.4 287.9 5.8 61.6 740 1093 01 18 51 01 32 00 J0518+2054 11 25 25 9.3 288.9 6.1 60.2 32 1093 01 32 00 01 33 00 =0515+208 11 26 25 9.1 289.0 6.1 60.1 60 1101 01 32 01 01 33 50 CRAB 11 27 15 12.8 288.2 5.9 61.4 33 1101 01 33 50 01 46 10 --- 11 39 37 10.3 289.6 6.1 60.5 740 1196 01 33 51 01 46 30 CRAB 11 39 57 10.3 289.6 6.1 60.5 18 1196 01 46 30 01 58 50 --- 11 52 19 7.8 291.1 6.3 59.5 740 1290 01 46 31 02 01 30 CRAB 11 54 59 7.2 291.4 6.3 59.3 158 1290 02 01 30 02 13 50 --- 12 07 21 4.8 292.9 6.5 D 58.3 0 1385 02 01 31 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess315.L1024 --- WARNING --- This group does not match an entry in the frequency catalog. This might be ok because the catalog is not complete. But be very careful to be sure that the setup is correct. Setup group: 14 Station: TIANMA65 Total bit rate: 1024 Format: MARK5B Bits per sample: 2 Sample rate: 32.000 Number of channels: 16 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 2270.00 2270.00 2270.00 2270.00 2270.00 2270.00 2270.00 2270.00 2270.00 2270.00 2270.00 2270.00 2270.00 2270.00 2270.00 2270.00 Net SB= L L U U L L U U L L U U L L U U IF SB = L L L L L L L L L L L L L L L L Pol. = RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP BBC = 1 5 1 5 2 6 2 6 3 7 3 7 4 8 4 8 BBC SB= U U L L U U L L U U L L U U L L IF = A2 B1 A2 B1 A2 B1 A2 B1 A2 B1 A2 B1 A2 B1 A2 B1 The following frequency sets based on these setups were used. Frequency Set: 12 Setup file default. Used with PCAL = off LO sum= 1610.49 1610.49 1610.49 1610.49 1642.49 1642.49 1642.49 1642.49 1674.49 1674.49 1674.49 1674.49 1706.49 1706.49 1706.49 1706.49 BBC fr= 659.51 659.51 659.51 659.51 627.51 627.51 627.51 627.51 595.51 595.51 595.51 595.51 563.51 563.51 563.51 563.51 Bandwd= 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 Matching frequency sets: 12 Track assignments are: track1= 2, 10, 18, 26, 4, 12, 20, 28, 6, 14, 22, 30, 8, 16, 24, 32 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) * CRAB 05 31 31.388685 * 05 34 31.934000 05 35 29.692879 0.00 21 58 54.53487 * 22 00 52.19100 22 01 18.48119 0.00 From catalog imbedded in main SCHED input file. 0515+208 05 15 05.041798 * 05 18 03.824513 05 19 01.125354 0.02 * J0518+2054 20 51 43.76307 * 20 54 52.49736 20 55 41.97620 0.03 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc GSFC 2015a astro solution, unpublished 1774 observations. 0528+134 05 28 06.759216 * 05 30 56.416747 05 31 50.712033 0.21 * J0530+1331 13 29 42.28885 * 13 31 55.14952 13 32 29.02251 0.24 J0530+13 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc GSFC 2015a astro solution, unpublished 135789 observations. SOURCE SCAN SUMMARY FOR SOURCES LISTED ABOVE Scan hours are for recording scans only. Baseline hours are only counted for scans above horizon at both ends. Source Setup file Frequency sets Observing hours (duplicates not shown) Scan Baseline CRAB sess315.L1024 1 2 3 4 5 6 7 8 9 12 13 14 3.303 283.739 J0518+2054 sess315.L1024 1 2 3 4 5 6 7 8 9 12 13 14 0.100 8.453 J0530+1331 sess315.L1024 1 2 3 4 5 6 7 8 9 12 13 14 0.318 26.243 EFFECT OF SOLAR CORONA 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) CRAB 121.0 J0518+2054 124.9 J0530+1331 121.8 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