COVER INFORMATION Station: SHANGHAI (Code Sh ) Experiment: Network Monitoring Expt Exp. Code: N07L2 Schedule Version: 1.00 Processed by SCHED version: 6.05 June 2006 PI: Hayley Bignall Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31-521-596520 EMAIL: bignall@jive.nl Fax: Phone during observation: +31-521-596520 Observing mode: Notes: L-band NME (256 Mbps, 2-bit sampling, 8 MHz filters) for session Please send the disk pack by express to JIVE Schedule for SHANGHAI (Code Sh ) Page 2 Network Monitoring Expt 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 ---------------------------------------------------------------------------------------- --- Wed 6 Jun 2007 Day 157 --- Next scan frequencies: 1637.99 1637.99 1645.99 1645.99 1653.99 1653.99 1661.99 1661.99 Next BBC frequencies: 662.01 662.01 654.01 654.01 646.01 646.01 638.01 638.01 Next scan bandwidths: 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 10 00 00 DA193 11 02 33 28.9 -58.6 5.1 72.0 0 1 1 0 10 00 00 10 15 00 --- 11 17 36 26.1 -57.5 5.4 70.1 900 F 1 29 10 00 01 10 17 00 DA193 11 19 36 25.8 -57.4 5.4 69.9 117 1 1 29 10 17 00 10 27 00 --- 11 29 38 24.0 -56.6 5.6 68.6 600 F 1 48 10 17 01 10 29 00 DA193 11 31 38 23.6 -56.5 5.6 68.3 117 1 1 48 10 29 00 10 32 00 --- 11 34 39 23.1 -56.2 5.6 67.9 180 F 1 54 10 29 01 10 32 00 J0605+4030 11 34 39 25.2 -56.3 5.5 69.6 -5 1 1 54 10 32 00 10 38 00 =0602+405 11 40 40 24.1 -55.9 5.6 68.8 355 F 1 66 10 32 01 10 39 00 DA193 11 41 40 21.8 -55.7 5.8 67.0 54 1 1 66 10 39 00 10 42 00 --- 11 44 40 21.3 -55.4 5.8 66.6 180 F 1 72 10 39 01 10 42 00 J0624+3856 11 44 40 26.1 -58.6 5.3 69.9 -10 1 1 72 10 42 00 10 48 00 =0620+389 11 50 41 25.1 -58.1 5.4 69.2 350 F 1 83 10 42 01 10 49 00 DA193 11 51 42 20.1 -54.8 5.9 65.7 50 1 1 83 10 49 00 10 52 00 --- 11 54 42 19.5 -54.6 6.0 65.3 180 F 1 89 10 49 01 10 52 00 J0605+4030 11 54 42 21.6 -54.8 5.8 66.9 -5 1 1 89 10 52 00 10 58 00 =0602+405 12 00 43 20.6 -54.3 5.9 66.1 355 F 1 101 10 52 01 10 59 00 DA193 12 01 43 18.3 -54.0 6.1 64.4 54 1 1 101 10 59 00 11 02 00 --- 12 04 44 17.8 -53.7 6.1 64.0 180 F 1 106 10 59 01 11 02 00 J0624+3856 12 04 44 22.5 -57.0 5.7 67.4 -10 1 1 106 11 02 00 11 08 00 =0620+389 12 10 45 21.4 -56.5 5.8 66.7 350 F 1 118 11 02 01 11 09 00 DA193 12 11 45 16.6 -53.1 6.3 63.0 50 1 1 118 11 09 00 11 12 00 --- 12 14 45 16.1 -52.8 6.3 62.6 180 F 1 124 11 09 01 11 12 00 J0605+4030 12 14 45 18.2 -53.1 6.1 64.2 -5 1 1 124 11 12 00 11 18 00 =0602+405 12 20 46 17.1 -52.6 6.2 63.4 355 F 1 135 11 12 01 Schedule for SHANGHAI (Code Sh ) Page 3 Network Monitoring Expt 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 ---------------------------------------------------------------------------------------- --- Wed 6 Jun 2007 Day 157 --- 11 19 00 DA193 12 21 46 14.9 -52.2 6.4 61.7 54 1 1 135 11 19 00 11 22 00 --- 12 24 47 14.4 -51.9 6.5 61.3 180 F 1 141 11 19 01 11 22 00 J0624+3856 12 24 47 19.0 -55.3 6.0 64.9 -10 1 1 141 11 22 00 11 28 00 =0620+389 12 30 48 17.9 -54.8 6.1 64.1 350 F 1 153 11 22 01 11 29 00 DA193 12 31 48 13.2 -51.2 6.6 60.3 50 1 1 153 11 29 00 11 32 00 --- 12 34 49 12.7 -50.9 6.6 59.9 180 F 1 159 11 29 01 11 34 00 DA193 12 36 49 12.4 -50.7 6.7 59.6 117 1 1 159 11 34 00 11 44 00 --- 12 46 51 10.7 -49.7 6.8 58.2 600 F 1 178 11 34 01 11 46 00 DA193 12 48 51 10.4 -49.5 6.9 57.9 117 1 1 178 11 46 00 11 49 00 --- 12 51 51 9.9 -49.2 6.9 57.5 180 F 1 184 11 46 01 11 49 00 J0605+4030 12 51 51 11.9 -49.6 6.8 59.1 -5 1 1 184 11 49 00 11 55 00 =0602+405 12 57 52 11.0 -49.0 6.9 58.2 355 F 1 195 11 49 01 11 56 00 DA193 12 58 53 8.8 -48.4 7.0 56.5 54 1 1 195 11 56 00 11 59 00 --- 13 01 53 8.3 -48.1 7.1 56.1 180 F 1 201 11 56 01 11 59 00 J0624+3856 13 01 53 12.6 -51.9 6.6 60.0 -9 1 1 201 11 59 00 12 05 00 =0620+389 13 07 54 11.5 -51.2 6.7 59.2 351 F 1 213 11 59 01 12 06 30 DA193 13 09 24 7.1 -47.3 7.2 55.0 81 1 1 213 12 06 30 12 09 00 --- 13 11 55 6.7 -47.0 7.3 54.6 150 F 1 218 12 06 31 12 09 00 J0605+4030 13 11 55 8.7 -47.6 7.1 56.2 -5 1 1 218 12 09 00 12 15 00 =0602+405 13 17 56 7.8 -46.9 7.2 55.3 355 F 1 229 12 09 01 12 16 00 DA193 13 18 56 5.6 -46.2 7.4 53.6 54 1 1 229 12 16 00 12 19 00 --- 13 21 56 5.2 -45.9 7.4 53.1 180 F 1 235 12 16 01 12 19 00 J0624+3856 13 21 56 9.2 -49.8 7.0 57.2 -9 1 1 235 12 19 00 12 25 00 =0620+389 13 27 57 8.3 -49.1 7.1 56.4 351 F 1 247 12 19 01 12 29 00 J0605+4030 13 31 58 5.6 -45.3 7.4 53.2 234 1 1 247 12 29 00 12 35 00 =0602+405 13 37 59 4.7 -44.6 7.5 D 52.3 0 F 1 258 12 29 01 12 39 00 J0624+3856 13 42 00 6.0 -47.6 7.3 54.4 235 1 1 258 12 39 00 12 45 00 =0620+389 13 48 01 5.1 -46.9 7.4 53.5 360 F 1 270 12 39 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: NME.18CM Matches group sh18cm in /aps3/sched/catalogs/freq.dat Huang Xinyong 27Sept05 Setup group: 11 Station: SHANGHAI Total bit rate: 256 Format: MKIV1:2 Bits per sample: 2 Sample rate: 16.000 Number of channels: 8 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 Net SB= U U U U U U U U Pol. = RCP LCP RCP LCP RCP LCP RCP LCP BBC = 1 2 3 4 5 6 7 8 BBC SB= L L L L L L L L IF = C A C A C A C A The following frequency sets based on this setup were used. Frequency Set: 11 Setup file default. Used pcal sets: 1 LO sum= 1637.99 1637.99 1645.99 1645.99 1653.99 1653.99 1661.99 1661.99 BBC fr= 662.01 662.01 654.01 654.01 646.01 646.01 638.01 638.01 Bandwd= 8.000 8.000 8.000 8.000 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 S5 S7 S1 S3 S5 S7 PCALXB2= S2 S4 S6 S8 S2 S4 S6 S8 PCALFR1= 10 10 10 10 6010 6010 6010 6010 PCALFR2= 10 10 10 10 6010 6010 6010 6010 Track assignments are: track1= 2, 10, 18, 26, 3, 11, 19, 27 barrel=roll_off SOURCE LIST -- Network Monitoring Expt 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) J0555+3948 05 52 01.407172 * 05 55 30.805614 05 56 00.628040 0.26 0552+398 39 48 21.94585 * 39 48 49.16500 39 49 01.41499 0.40 * DA193 /aps3/sched/catalogs/sources.vlba J0555+39 VLBA Calib Srcs - GSFC sols. - catalog 2004f_astro 1.533 scan hours, 76.412 baseline hours above horizon. * J0605+4030 06 02 20.058848 * 06 05 50.855368 06 06 20.905881 0.28 0602+405 40 30 26.00793 * 40 30 08.10360 40 30 14.17401 0.42 /aps3/sched/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.900 scan hours, 39.326 baseline hours above horizon. * J0624+3856 06 20 51.522615 * 06 24 19.021309 06 24 48.681229 0.27 0620+389 38 58 27.34271 * 38 56 48.73590 38 56 43.45275 0.41 J0624+38 /aps3/sched/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.900 scan hours, 36.783 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) DA193 21.3 J0605+4030 23.1 J0624+3856 24.9 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