COVER INFORMATION Station: SHANGHAI (Code Sh ) Experiment: Phase-referencing of lensed SMGs detected by HATLAS Exp. Code: EI011 Schedule Version: 2.00 Processed by SCHED version: 10.00 Release Sept. 15, 2011 PI: Eduardo Ibar Address: UK ATC The Royal Observatory Edinburgh UK Phone: +44 131 668 8441 EMAIL: ibar@roe.ac.uk Fax: Phone during observation: Observing mode: L-band Phase-referencing (512 Mb/s) Notes: PLEASE TURN OFF PHASE CAL TONES Schedule for SHANGHAI (Code Sh ) Page 2 Phase-referencing of lensed SMGs detected by HATLAS 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 ---------------------------------------------------------------------------------------- --- Thu 3 Nov 2011 Day 307 --- Next scan frequencies: 1634.49 1634.49 1634.49 1634.49 1650.49 1650.49 1650.49 1650.49 1666.49 1666.49 1666.49 1666.49 1682.49 1682.49 1682.49 1682.49 Next BBC frequencies: 665.51 665.51 665.51 665.51 649.51 649.51 649.51 649.51 633.51 633.51 633.51 633.51 617.51 617.51 617.51 617.51 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 02 30 00 0837+012 13 22 50 17.1 260.6 4.7 57.7 0 0 02 30 00 02 31 35 --- 13 24 26 16.7 260.8 4.7 57.7 95 6 02 30 01 02 31 35 G09V1908 13 24 26 18.4 261.9 4.7 58.1 -7 6 No stop 02 41 05 --- 13 33 57 16.3 263.3 4.8 58.4 563 43 02 31 36 02 41 05 0837+012 13 33 57 14.7 262.1 4.9 58.0 -7 43 No stop 02 42 50 --- 13 35 42 14.4 262.4 4.9 58.1 98 50 02 41 06 02 42 50 G09V1908 13 35 42 16.0 263.5 4.9 58.4 -7 50 No stop 02 52 20 --- 13 45 14 13.9 264.8 5.0 58.6 563 86 02 42 51 02 53 00 0837+012 13 45 54 12.2 263.8 5.1 58.4 33 86 02 53 00 02 54 40 --- 13 47 34 11.8 264.0 5.1 58.4 100 93 02 53 01 02 54 40 G09V1908 13 47 34 13.4 265.1 5.1 58.7 -7 93 No stop 03 03 40 --- 13 56 36 11.5 266.3 5.2 58.8 533 128 02 54 41 03 03 40 0837+012 13 56 36 9.9 265.2 5.3 58.6 -7 128 No stop 03 05 25 --- 13 58 21 9.5 265.4 5.3 58.6 98 135 03 03 41 03 05 25 G09V1908 13 58 21 11.1 266.5 5.2 58.8 -7 135 No stop 03 14 55 --- 14 07 53 9.1 267.8 5.4 58.9 563 171 03 05 26 03 16 55 OJ287 14 09 53 19.6 282.1 5.2 63.0 98 171 03 16 55 03 23 15 --- 14 16 14 18.3 282.8 5.3 62.7 380 196 03 16 56 03 25 40 0837+012 14 18 39 5.2 268.1 5.6 58.9 120 196 03 25 40 03 27 15 --- 14 20 15 4.9 268.3 5.7 D 58.9 0 202 03 25 41 03 27 15 G09V1908 14 20 15 6.4 269.4 5.6 59.0 -7 202 No stop 03 36 45 --- 14 29 46 4.4 270.6 5.8 D 59.0 0 239 03 27 16 Schedule for SHANGHAI (Code Sh ) Page 3 Phase-referencing of lensed SMGs detected by HATLAS 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 ---------------------------------------------------------------------------------------- --- Thu 3 Nov 2011 Day 307 --- 05 01 00 4C39.25 15 54 15 14.4 307.1 6.4 61.4 5010 239 05 01 00 05 07 20 --- 16 00 36 13.3 307.8 6.5 60.6 380 263 05 01 01 09 34 05 3C345 20 28 05 44.2 297.1 3.7 82.6 15893 263 09 34 05 09 40 30 --- 20 34 31 42.9 297.4 3.9 81.8 385 288 09 34 06 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: sess311.L512 Matching groups in /home/ibar/Programs/SCHED_10.0/catalogs/freq.dat: sh18cm Huang Xinyong 27Sept05 Setup group: 7 Station: SHANGHAI Total bit rate: 512 Format: MARK5B Bits per sample: 2 Sample rate: 16.000 Number of channels: 16 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 2300.00 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 = 1 2 1 2 3 4 3 4 5 6 5 6 7 8 7 8 BBC SB= U U L L U U L L U U L L U U L L IF = C A C A C A C A C A C A C A C A The following frequency sets based on these setups were used. Frequency Set: 11 Setup file default. Used pcal sets: 1 LO sum= 1634.49 1634.49 1634.49 1634.49 1650.49 1650.49 1650.49 1650.49 1666.49 1666.49 1666.49 1666.49 1682.49 1682.49 1682.49 1682.49 BBC fr= 665.51 665.51 665.51 665.51 649.51 649.51 649.51 649.51 633.51 633.51 633.51 633.51 617.51 617.51 617.51 617.51 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 Matching frequency sets: 11 The following pulse cal sets were used with this setup: Pulse cal detection set: 1 PCAL = OFF PCALXB1= S1 S2 S3 S4 S5 S6 S7 S8 PCALXB2= M1 M2 M3 M4 M5 M6 M7 M8 PCALFR1= 0 0 0 0 0 0 0 0 PCALFR2= 0 0 0 0 0 0 0 0 Track assignments are: track1= 2, 4, 6, 8, 10, 12, 14, 16, 18, 20, 22, 24, 26, 28, 30, 32 barrel=roll_off SOURCES USED IN RECORDING SCANS -- Phase-referencing of lensed SMGs detected by HATLAS 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) * G09V1908 08 40 23.646907 * 08 42 59.990000 08 43 38.009592 0.00 03 00 51.18593 * 02 50 01.40000 02 47 25.89930 0.00 From catalog imbedded in main SCHED input file. 1.250 scan and 72.714 baseline hours in setup: sess311.L512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 9 10 11 * G09_EVN1 09 02 17.413825 * 09 04 53.140000 09 05 30.884392 0.00 02 32 16.78217 * 02 20 17.20000 02 17 25.16659 0.00 From catalog imbedded in main SCHED input file. 1.250 scan and 57.231 baseline hours in setup: sess311.L512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 9 10 * G09V1326 09 16 05.022245 * 09 18 40.760000 09 19 18.427410 0.00 02 43 26.12810 * 02 30 45.90000 02 27 44.10219 0.00 From catalog imbedded in main SCHED input file. 1.250 scan and 46.124 baseline hours in setup: sess311.L512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 10 * G12V2319 11 35 59.570804 * 11 38 33.440000 11 39 09.952033 0.00 01 05 48.67336 * 00 49 11.50000 00 45 14.86041 0.00 From catalog imbedded in main SCHED input file. 1.250 scan and 50.082 baseline hours in setup: sess311.L512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 10 * G15V2258 14 17 21.506943 * 14 19 55.590000 14 20 31.748872 0.00 -00 21 04.33815 *-00 34 48.60000 -00 38 00.49239 0.00 From catalog imbedded in main SCHED input file. 1.258 scan and 56.809 baseline hours in setup: sess311.L512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 9 10 * BOOTES01 14 26 19.696736 * 14 28 25.380000 14 28 54.230304 0.00 35 09 08.97748 * 34 55 47.20000 34 52 38.22673 0.00 From catalog imbedded in main SCHED input file. 1.250 scan and 65.946 baseline hours in setup: sess311.L512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 9 10 J0839+0104 08 37 14.821382 * 08 39 49.611002 08 40 27.276565 0.17 * 0837+012 01 15 05.94720 * 01 04 26.73647 01 01 54.39615 0.37 /home/ibar/Programs/SCHED_10.0/catalogs/sources.vlba GSFC 2010a astro solution 127 Observations 0.225 scan and 12.142 baseline hours in setup: sess311.L512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 9 10 11 J0854+2006 08 51 57.250615 * 08 54 48.874927 08 55 30.477541 0.00 0851+202 20 17 58.41745 * 20 06 30.64090 20 03 39.73827 0.01 J0854+20 /home/ibar/Programs/SCHED_10.0/catalogs/sources.vlba * OJ287 GSFC 2010a astro solution 164475 Observations 0.106 scan and 6.967 baseline hours in setup: sess311.L512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 9 10 11 J0909+0121 09 06 35.181594 * 09 09 10.091600 09 09 47.616263 0.06 * 0906+015 01 33 48.12923 * 01 21 35.61775 01 18 40.84067 0.12 J0909+01 /home/ibar/Programs/SCHED_10.0/catalogs/sources.vlba GSFC 2010a astro solution 404 Observations 0.225 scan and 9.604 baseline hours in setup: sess311.L512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 9 10 J0914+0245 09 12 01.939424 * 09 14 37.913435 09 15 15.660542 0.01 * 0912+029 02 58 27.82034 * 02 45 59.24675 02 43 00.13889 0.02 J0914+02 /home/ibar/Programs/SCHED_10.0/catalogs/sources.vlba GSFC 2010a astro solution 4709 Observations 0.225 scan and 7.715 baseline hours in setup: sess311.L512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 10 J0927+3902 09 23 55.319213 * 09 27 03.013934 09 27 48.163586 0.29 0923+392 39 15 23.56646 * 39 02 20.85186 38 59 00.65660 0.16 * 4C39.25 /home/ibar/Programs/SCHED_10.0/catalogs/sources.vlba J0927+39 GSFC 2010a astro solution 231732 Observations 0.106 scan and 6.967 baseline hours in setup: sess311.L512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 9 10 11 J1133+0040 11 30 46.181479 * 11 33 20.055793 11 33 56.591504 0.04 * 1130+009 00 57 27.49183 * 00 40 52.83731 00 36 56.75833 0.06 J1133+00 /home/ibar/Programs/SCHED_10.0/catalogs/sources.vlba GSFC 2010a astro solution 871 Observations 0.225 scan and 8.365 baseline hours in setup: sess311.L512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 10 J1410+0203 14 07 32.231489 * 14 10 04.655971 14 10 40.410547 0.10 * 1407+022 02 17 14.85064 * 02 03 06.91228 01 59 48.94852 0.24 /home/ibar/Programs/SCHED_10.0/catalogs/sources.vlba GSFC 2010a astro solution 81 Observations 0.225 scan and 9.178 baseline hours in setup: sess311.L512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 9 10 J1426+3625 14 24 32.676805 * 14 26 37.087486 14 27 05.593978 0.05 * 1424+366 36 38 36.02444 * 36 25 09.57375 36 21 59.20161 0.06 /home/ibar/Programs/SCHED_10.0/catalogs/sources.vlba GSFC 2010a astro solution 738 Observations 0.225 scan and 10.937 baseline hours in setup: sess311.L512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 9 10 J1642+3948 16 41 17.606228 * 16 42 58.809965 16 43 21.840329 0.81 * 3C345 39 54 10.81494 * 39 48 36.99400 39 47 29.33393 0.54 1641+399 /home/ibar/Programs/SCHED_10.0/catalogs/sources.vlba J1642+39 GSFC 2010a astro solution 52595 Observations 0.107 scan and 7.058 baseline hours in setup: sess311.L512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 9 10 11 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) G09V1908 88.0 G09_EVN1 82.6 G09V1326 79.3 G12V2319 45.6 G15V2258 14.6 BOOTES01 49.9 0837+012 88.3 OJ287 89.9 0906+015 81.3 0912+029 80.4 4C39.25 89.0 1130+009 46.8 1407+022 17.8 1424+366 51.4 3C345 62.7 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