COVER INFORMATION Station: HART (Code Hh ) Experiment: Gamma-ray microquasars: radio pulsars in disguise? Exp. Code: EF018c Schedule Version: 1.00 Processed by SCHED version: 6.05 June 2006 PI: R. Fender Address: School of Physics & Astronomy University of Southampton SO17 1BJ Southampton UK Phone: +44 2380 592076 EMAIL: rpf@phys.soton.ac.uk Fax: +44 2380 593910 Phone during observation: Observing mode: Phase-referencing of LS 5039 at 6cm (512 Mb/s) Notes: Place additional information here (note2-4 available) Schedule for HART (Code Hh ) Page 2 Gamma-ray microquasars: radio pulsars in disguise? 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 5 Mar 2007 Day 64 --- Next scan frequencies: 4966.49 4966.49 4966.49 4966.49 4982.49 4982.49 4982.49 4982.49 4998.49 4998.49 4998.49 4998.49 5014.49 5014.49 5014.49 5014.49 Next BBC frequencies: 366.49 366.49 366.49 366.49 382.49 382.49 382.49 382.49 398.49 398.49 398.49 398.49 414.49 414.49 414.49 414.49 Next scan bandwidths: 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 03 00 00 3C345 15 40 41 22.7 13.0 -1.0 0.0 0 1 1 0 03 00 00 03 07 00 --- 15 47 43 23.1 11.6 -0.9 0.0 420 F 1 27 03 00 04 03 12 00 J1825-1718 15 52 43 53.5 84.3 -2.6 0.0 159 1 1 27 03 12 00 03 15 00 --- 15 55 44 54.2 83.9 -2.5 0.0 180 F 1 39 03 12 04 03 15 00 LS5039 15 55 44 53.1 80.1 -2.5 0.0 -32 1 1 39 03 15 00 03 20 00 --- 16 00 45 54.2 79.3 -2.4 0.0 268 F 1 58 03 15 04 03 20 00 J1825-1718 16 00 45 55.3 83.1 -2.4 0.0 -32 1 1 58 03 20 00 03 23 00 --- 16 03 45 56.0 82.7 -2.4 0.0 148 F 1 70 03 20 04 03 23 00 LS5039 16 03 45 54.9 78.8 -2.4 0.0 -32 1 1 70 03 23 00 03 28 00 --- 16 08 46 56.0 77.9 -2.3 0.0 268 F 1 89 03 23 04 03 29 00 J1825-1718 16 09 46 57.3 81.7 -2.3 0.0 28 1 1 89 03 29 00 03 32 00 --- 16 12 47 58.0 81.3 -2.2 0.0 180 F 1 101 03 29 04 03 32 00 LS5039 16 12 47 56.9 77.2 -2.2 0.0 -32 1 1 101 03 32 00 03 37 00 --- 16 17 47 58.0 76.2 -2.1 0.0 268 F 1 120 03 32 04 03 37 00 J1825-1718 16 17 47 59.1 80.4 -2.1 0.0 -32 1 1 120 03 37 00 03 40 00 --- 16 20 48 59.7 79.9 -2.1 0.0 148 F 1 132 03 37 04 03 40 00 LS5039 16 20 48 58.6 75.6 -2.1 0.0 -32 1 1 132 03 40 00 03 45 00 --- 16 25 49 59.7 74.6 -2.0 0.0 268 F 1 151 03 40 04 03 46 00 J1743-0350 16 26 49 61.2 43.4 -1.3 0.0 11 1 1 151 03 46 00 03 53 00 =1741-038 16 33 50 62.2 40.4 -1.2 0.0 420 F 1 178 03 46 04 03 55 00 J1825-1718 16 35 50 63.1 77.0 -1.8 0.0 66 1 1 178 03 55 00 03 58 00 --- 16 38 51 63.7 76.4 -1.8 0.0 180 F 1 190 03 55 04 Schedule for HART (Code Hh ) Page 3 Gamma-ray microquasars: radio pulsars in disguise? 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 5 Mar 2007 Day 64 --- 03 58 00 LS5039 16 38 51 62.5 71.6 -1.8 0.0 -32 1 1 190 03 58 00 04 03 00 --- 16 43 52 63.6 70.3 -1.7 0.0 268 F 1 209 03 58 04 04 03 00 J1825-1718 16 43 52 64.8 75.2 -1.7 0.0 -32 1 1 209 04 03 00 04 06 00 --- 16 46 52 65.5 74.5 -1.7 0.0 148 F 1 221 04 03 04 04 06 00 LS5039 16 46 52 64.2 69.5 -1.7 0.0 -32 1 1 221 04 06 00 04 11 00 --- 16 51 53 65.3 68.1 -1.6 0.0 268 F 1 240 04 06 04 04 12 00 J1825-1718 16 52 53 66.8 73.0 -1.6 0.0 28 1 1 240 04 12 00 04 15 00 --- 16 55 54 67.4 72.2 -1.5 0.0 180 F 1 252 04 12 04 04 15 00 LS5039 16 55 54 66.1 66.9 -1.5 0.0 -32 1 1 252 04 15 00 04 20 00 --- 17 00 55 67.1 65.3 -1.4 0.0 268 F 1 271 04 15 04 04 20 00 J1825-1718 17 00 55 68.5 70.8 -1.4 0.0 -32 1 1 271 04 20 00 04 23 00 --- 17 03 55 69.1 69.9 -1.4 0.0 148 F 1 283 04 20 04 04 23 00 LS5039 17 03 55 67.7 64.3 -1.4 0.0 -32 1 1 283 04 23 00 04 28 00 --- 17 08 56 68.7 62.5 -1.3 0.0 268 F 1 302 04 23 04 04 29 00 J1743-0350 17 09 56 66.5 22.0 -0.6 0.0 11 1 1 302 04 29 00 04 36 00 =1741-038 17 16 57 67.0 17.7 -0.5 0.0 420 F 1 329 04 29 04 04 38 00 J1825-1718 17 18 57 72.2 64.5 -1.1 0.0 66 1 1 329 04 38 00 04 41 00 --- 17 21 58 72.8 63.2 -1.1 0.0 180 F 1 341 04 38 04 04 41 00 LS5039 17 21 58 71.3 57.0 -1.1 0.0 -32 1 1 341 04 41 00 04 46 00 --- 17 26 59 72.2 54.5 -1.0 0.0 268 F 1 360 04 41 04 04 46 00 J1825-1718 17 26 59 73.8 60.9 -1.0 0.0 -32 1 1 360 04 46 00 04 49 00 --- 17 29 59 74.4 59.4 -0.9 0.0 148 F 1 372 04 46 04 04 49 00 LS5039 17 29 59 72.8 52.9 -0.9 0.0 -32 1 1 372 04 49 00 04 54 00 --- 17 35 00 73.6 50.1 -0.9 0.0 268 F 1 391 04 49 04 04 55 00 J1825-1718 17 36 00 75.6 56.0 -0.8 0.0 28 1 1 391 04 55 00 04 58 00 --- 17 39 01 76.1 54.2 -0.8 0.0 180 F 1 403 04 55 04 04 58 00 LS5039 17 39 01 74.3 47.6 -0.8 0.0 -32 1 1 403 04 58 00 05 03 00 --- 17 44 02 75.1 44.1 -0.7 0.0 268 F 1 422 04 58 04 05 03 00 J1825-1718 17 44 02 77.0 50.7 -0.7 0.0 -32 1 1 422 05 03 00 05 06 00 --- 17 47 02 77.5 48.5 -0.6 0.0 148 F 1 434 05 03 04 Schedule for HART (Code Hh ) Page 4 Gamma-ray microquasars: radio pulsars in disguise? 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 5 Mar 2007 Day 64 --- 05 06 00 LS5039 17 47 02 75.6 41.9 -0.7 0.0 -32 1 1 434 05 06 00 05 11 00 --- 17 52 03 76.3 37.9 -0.6 0.0 268 F 1 453 05 06 04 05 17 30 3C345 17 58 34 22.0 344.5 1.3 0.0 254 1 1 453 05 17 30 05 24 30 --- 18 05 35 21.6 343.1 1.4 0.0 420 F 1 480 05 17 34 05 30 30 J1825-1718 18 11 36 80.8 22.0 -0.2 0.0 219 1 1 480 05 30 30 05 33 30 --- 18 14 37 81.0 17.7 -0.2 0.0 180 F 1 492 05 30 34 05 33 30 LS5039 18 14 37 78.6 14.9 -0.2 0.0 -32 1 1 492 05 33 30 05 38 30 --- 18 19 37 78.8 8.8 -0.1 0.0 268 F 1 511 05 33 34 05 38 30 J1825-1718 18 19 37 81.3 10.1 -0.1 0.0 -32 1 1 511 05 38 30 05 41 30 --- 18 22 38 81.4 5.4 -0.1 0.0 148 F 1 523 05 38 34 05 41 30 LS5039 18 22 38 78.9 5.1 -0.1 0.0 -32 1 1 523 05 41 30 05 46 30 --- 18 27 39 79.0 358.8 0.0 0.0 268 F 1 542 05 41 34 05 47 30 J1825-1718 18 28 39 81.4 355.8 0.0 0.0 28 1 1 542 05 47 30 05 50 30 --- 18 31 39 81.3 351.1 0.1 0.0 180 F 1 554 05 47 34 05 50 30 LS5039 18 31 39 78.9 353.7 0.1 0.0 -32 1 1 554 05 50 30 05 55 30 --- 18 36 40 78.7 347.5 0.2 0.0 268 F 1 573 05 50 34 05 55 30 J1825-1718 18 36 40 81.1 343.4 0.2 0.0 -32 1 1 573 05 55 30 05 58 30 --- 18 39 41 80.9 339.0 0.2 0.0 148 F 1 584 05 55 34 05 58 30 LS5039 18 39 41 78.5 344.0 0.2 0.0 -32 1 1 584 05 58 30 06 03 30 --- 18 44 42 78.2 338.2 0.3 0.0 268 F 1 604 05 58 34 06 04 30 J1743-0350 18 45 42 63.5 323.8 1.0 0.0 11 1 1 604 06 04 30 06 11 30 =1741-038 18 52 43 62.5 320.5 1.1 0.0 420 F 1 631 06 04 34 06 13 30 J1825-1718 18 54 43 79.1 320.7 0.5 0.0 66 1 1 631 06 13 30 06 16 30 --- 18 57 44 78.7 317.8 0.5 0.0 180 F 1 643 06 13 34 06 16 30 LS5039 18 57 44 76.8 325.2 0.5 0.0 -32 1 1 643 06 16 30 06 21 30 --- 19 02 45 76.1 320.9 0.6 0.0 268 F 1 662 06 16 34 06 21 30 J1825-1718 19 02 45 77.9 313.4 0.6 0.0 -32 1 1 662 06 21 30 06 24 30 --- 19 05 45 77.4 311.0 0.7 0.0 148 F 1 674 06 21 34 06 24 30 LS5039 19 05 45 75.7 318.5 0.7 0.0 -32 1 1 674 06 24 30 06 29 30 --- 19 10 46 74.9 314.8 0.7 0.0 268 F 1 693 06 24 34 Schedule for HART (Code Hh ) Page 5 Gamma-ray microquasars: radio pulsars in disguise? 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 5 Mar 2007 Day 64 --- 06 30 30 J1825-1718 19 11 46 76.4 306.7 0.8 0.0 28 1 1 693 06 30 30 06 33 30 --- 19 14 46 75.8 304.7 0.8 0.0 180 F 1 704 06 30 34 06 33 30 LS5039 19 14 46 74.2 312.1 0.8 0.0 -32 1 1 704 06 33 30 06 38 30 --- 19 19 47 73.4 309.1 0.9 0.0 268 F 1 724 06 33 34 06 38 30 J1825-1718 19 19 47 74.9 301.8 0.9 0.0 -32 1 1 724 06 38 30 06 41 30 --- 19 22 48 74.3 300.2 0.9 0.0 148 F 1 735 06 38 34 06 41 30 LS5039 19 22 48 72.8 307.4 0.9 0.0 -32 1 1 735 06 41 30 06 46 30 --- 19 27 49 71.9 304.7 1.0 0.0 268 F 1 755 06 41 34 06 52 30 3C345 19 33 50 13.2 327.7 2.8 0.0 224 1 1 755 06 52 30 06 59 30 --- 19 40 51 12.4 326.6 3.0 0.0 420 F 1 782 06 52 34 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: ef018c.6cm Matches group hh6cm in /aps3/sched/catalogs/freq.dat Values confirmed by E-mail Jonathan Quick 221105 (CR) Setup group: 8 Station: HART Total bit rate: 512 Format: MKIV1:2 Bits per sample: 2 Sample rate: 16.000 Number of channels: 16 Speedup factor: 1.00 Disk used to record data. 1st LO= 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 Net SB= L L U U L L U U L L U U L L U U Pol. = RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP BBC = 2 1 2 1 4 3 4 3 6 5 6 5 8 7 8 7 BBC SB= L L U U L L U U L L U U L L U U IF = 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N The following frequency sets based on this setup were used. Frequency Set: 8 Setup file default. No pcal detection. LO sum= 4966.49 4966.49 4966.49 4966.49 4982.49 4982.49 4982.49 4982.49 4998.49 4998.49 4998.49 4998.49 5014.49 5014.49 5014.49 5014.49 BBC fr= 366.49 366.49 366.49 366.49 382.49 382.49 382.49 382.49 398.49 398.49 398.49 398.49 414.49 414.49 414.49 414.49 Bandwd= 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 Track assignments are: track1= 2, 10, 18, 26, 3, 11, 19, 27, 66, 74, 82, 90, 67, 75, 83, 91 barrel=roll_off SOURCE LIST -- Gamma-ray microquasars: radio pulsars in disguise? 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) * LS5039 18 23 23.640919 * 18 26 15.056600 18 26 39.431619 0.00 -14 52 42.60801 *-14 50 54.26100 -14 50 50.03872 0.00 From catalog imbedded in main SCHED input file. 1.667 scan hours, 54.567 baseline hours above horizon. J1642+3948 16 41 17.606231 * 16 42 58.809968 16 43 13.723290 0.26 1641+399 39 54 10.81494 * 39 48 36.99400 39 47 21.82974 0.40 * 3C345 /aps3/sched/catalogs/sources.vlba J1642+39 VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.350 scan hours, 13.650 baseline hours above horizon. * J1743-0350 17 41 20.616010 * 17 43 58.856134 17 44 21.540343 0.20 1741-038 -03 48 48.89989 *-03 50 04.61669 -03 50 30.71656 0.30 J1743-03 /aps3/sched/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.350 scan hours, 13.505 baseline hours above horizon. * J1825-1718 18 22 42.013830 * 18 25 36.532282 18 26 01.357293 1.29 -17 20 35.28894 *-17 18 49.84782 -17 18 45.21453 1.99 /aps3/sched/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 1.000 scan hours, 30.505 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) LS5039 68.0 3C345 97.6 J1743-0350 79.1 J1825-1718 68.1 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