COVER INFORMATION Station: URUMQI (Code Ur ) Experiment: Locating AGN in local analogs of Lyman break galaxies Exp. Code: EO006C Schedule Version: 1.00 Processed by SCHED version: 6.05 June 2006 PI: R.A. Overzier Address: MPA Karl-Schwarzschildstr. 1 Garching Germany Phone: +49-89-300002216 EMAIL: overzier@mpa-garching.mpg.de Fax: Phone during observation: Observing mode: Phase-referencing of a source at 18cm (1 Gb/s) Notes: Target: J210358 Phase-reference calibrator: J2110-1020 Fringe finder: J2253+1608 Amplitude calibrator: J2110-1020 Schedule for URUMQI (Code Ur ) Page 2 Locating AGN in local analogs of Lyman break galaxies 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 ---------------------------------------------------------------------------------------- --- Sun 8 Jun 2008 Day 160 --- 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: 310.49 310.49 310.49 310.49 342.49 342.49 342.49 342.49 374.49 374.49 374.49 374.49 406.49 406.49 406.49 406.49 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 00 00 00 J2110-1020 22 55 42 31.1 210.6 1.8 22.1 0 1 1 0 00 00 00 00 02 00 =2107-105 22 57 42 30.9 211.1 1.8 22.4 120 F 1 15 00 00 04 00 02 37 J210358 22 58 20 32.9 214.3 1.9 24.3 28 1 1 15 00 02 37 00 07 17 --- 23 03 00 32.4 215.5 2.0 25.2 280 F 1 52 00 02 41 00 07 54 J2110-1020 23 03 37 30.4 212.7 1.9 23.5 28 1 1 52 00 07 54 00 09 34 =2107-105 23 05 18 30.2 213.1 1.9 23.8 100 F 1 65 00 07 58 00 10 11 J210358 23 05 55 32.1 216.3 2.0 25.7 29 1 1 65 00 10 11 00 14 51 --- 23 10 36 31.6 217.5 2.1 26.5 280 F 1 101 00 10 15 00 15 28 J2110-1020 23 11 13 29.6 214.7 2.0 24.8 28 1 1 101 00 15 28 00 17 08 =2107-105 23 12 53 29.4 215.1 2.0 25.1 100 F 1 114 00 15 32 00 17 45 J210358 23 13 30 31.3 218.3 2.2 27.0 29 1 1 114 00 17 45 00 22 25 --- 23 18 11 30.8 219.5 2.2 27.7 280 F 1 150 00 17 49 00 23 02 J2110-1020 23 18 48 28.8 216.6 2.1 26.1 28 1 1 150 00 23 02 00 24 42 =2107-105 23 20 28 28.6 217.0 2.2 26.4 100 F 1 163 00 23 06 00 25 19 J210358 23 21 05 30.4 220.2 2.3 28.2 29 1 1 163 00 25 19 00 29 59 --- 23 25 46 29.9 221.4 2.4 28.9 280 F 1 199 00 25 23 00 30 36 J2110-1020 23 26 23 28.0 218.5 2.3 27.3 29 1 1 199 00 30 36 00 32 16 =2107-105 23 28 03 27.8 218.9 2.3 27.6 100 F 1 212 00 30 40 00 32 53 J210358 23 28 41 29.5 222.1 2.4 29.4 29 1 1 212 00 32 53 00 37 33 --- 23 33 21 28.9 223.3 2.5 30.1 280 F 1 248 00 32 57 00 38 10 J2110-1020 23 33 58 27.1 220.4 2.4 28.5 29 1 1 248 00 38 10 00 39 50 =2107-105 23 35 39 26.9 220.8 2.4 28.8 100 F 1 261 00 38 14 Schedule for URUMQI (Code Ur ) Page 3 Locating AGN in local analogs of Lyman break galaxies 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 ---------------------------------------------------------------------------------------- --- Sun 8 Jun 2008 Day 160 --- 00 40 27 J210358 23 36 16 28.6 224.0 2.5 30.5 29 1 1 261 00 40 27 00 45 07 --- 23 40 57 28.0 225.1 2.6 31.2 280 F 1 297 00 40 31 00 45 44 J2110-1020 23 41 34 26.2 222.2 2.5 29.7 29 1 1 297 00 45 44 00 47 24 =2107-105 23 43 14 26.0 222.6 2.5 29.9 100 F 1 310 00 45 48 00 47 54 J2110-1020 23 43 44 25.9 222.7 2.6 30.0 28 1 1 310 00 47 54 00 53 54 =2107-105 23 49 45 25.2 224.1 2.7 30.9 360 F 1 356 00 47 58 00 56 54 J2253+1608 23 52 45 60.0 209.0 1.0 21.5 62 1 1 356 00 56 54 01 03 24 =2251+158 23 59 17 59.4 211.8 1.1 23.5 390 F 1 406 00 56 58 01 06 24 J2110-1020 00 02 17 23.5 227.0 2.9 32.6 58 1 1 406 01 06 24 01 08 04 =2107-105 00 03 57 23.3 227.4 2.9 32.9 100 F 1 419 01 06 28 01 08 41 J210358 00 04 34 24.8 230.6 3.0 34.4 29 1 1 419 01 08 41 01 13 21 --- 00 09 15 24.1 231.7 3.1 35.0 280 F 1 455 01 08 45 01 13 58 J2110-1020 00 09 52 22.5 228.7 3.0 33.6 29 1 1 455 01 13 58 01 15 38 =2107-105 00 11 33 22.3 229.1 3.0 33.9 100 F 1 468 01 14 02 01 16 15 J210358 00 12 10 23.7 232.3 3.1 35.4 29 1 1 468 01 16 15 01 20 55 --- 00 16 50 23.1 233.3 3.2 35.9 280 F 1 504 01 16 19 01 21 32 J2110-1020 00 17 28 21.5 230.3 3.1 34.6 29 1 1 504 01 21 32 01 23 12 =2107-105 00 19 08 21.2 230.7 3.1 34.8 100 F 1 517 01 21 36 01 23 49 J210358 00 19 45 22.6 234.0 3.3 36.3 29 1 1 517 01 23 49 01 28 29 --- 00 24 26 21.9 235.0 3.3 36.8 280 F 1 554 01 23 53 01 29 06 J2110-1020 00 25 03 20.4 232.0 3.2 35.5 29 1 1 554 01 29 06 01 30 46 =2107-105 00 26 43 20.2 232.3 3.3 35.7 100 F 1 566 01 29 10 01 31 23 J210358 00 27 20 21.5 235.6 3.4 37.1 29 1 1 566 01 31 23 01 36 03 --- 00 32 01 20.8 236.6 3.5 37.6 280 F 1 603 01 31 27 01 36 40 J2110-1020 00 32 38 19.3 233.6 3.4 36.4 29 1 1 603 01 36 40 01 38 20 =2107-105 00 34 18 19.1 233.9 3.4 36.6 100 F 1 615 01 36 44 01 38 57 J210358 00 34 55 20.4 237.2 3.5 38.0 29 1 1 615 01 38 57 01 43 37 --- 00 39 36 19.6 238.2 3.6 38.4 280 F 1 652 01 39 01 01 44 14 J2110-1020 00 40 13 18.2 235.2 3.5 37.3 29 1 1 652 01 44 14 01 45 54 =2107-105 00 41 54 17.9 235.5 3.5 37.4 100 F 1 664 01 44 18 Schedule for URUMQI (Code Ur ) Page 4 Locating AGN in local analogs of Lyman break galaxies 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 ---------------------------------------------------------------------------------------- --- Sun 8 Jun 2008 Day 160 --- 01 46 31 J210358 00 42 31 19.2 238.8 3.6 38.7 29 1 1 664 01 46 31 01 51 11 --- 00 47 11 18.5 239.7 3.7 39.2 280 F 1 701 01 46 35 01 51 48 J2110-1020 00 47 48 17.0 236.7 3.6 38.1 29 1 1 701 01 51 48 01 53 28 =2107-105 00 49 29 16.8 237.1 3.6 38.2 100 F 1 714 01 51 52 01 54 05 J210358 00 50 06 18.0 240.3 3.8 39.5 29 1 1 714 01 54 05 01 58 45 --- 00 54 47 17.3 241.2 3.8 39.9 280 F 1 750 01 54 09 01 59 22 J2110-1020 00 55 24 15.9 238.2 3.7 38.8 29 1 1 750 01 59 22 02 01 02 =2107-105 00 57 04 15.6 238.6 3.8 39.0 100 F 1 763 01 59 26 02 01 39 J210358 00 57 41 16.8 241.8 3.9 40.2 29 1 1 763 02 01 39 02 06 19 --- 01 02 22 16.0 242.7 4.0 40.6 280 F 1 799 02 01 43 02 06 56 J2110-1020 01 02 59 14.7 239.7 3.9 39.6 29 1 1 799 02 06 56 02 08 36 =2107-105 01 04 39 14.4 240.1 3.9 39.7 100 F 1 812 02 07 00 02 09 13 J210358 01 05 16 15.6 243.3 4.0 40.8 29 1 1 812 02 09 13 02 13 53 --- 01 09 57 14.8 244.2 4.1 41.2 280 F 1 848 02 09 17 02 14 30 J2110-1020 01 10 34 13.5 241.2 4.0 40.3 29 1 1 848 02 14 30 02 16 10 =2107-105 01 12 14 13.2 241.5 4.0 40.4 100 F 1 861 02 14 34 02 16 47 J210358 01 12 52 14.3 244.8 4.1 41.5 29 1 1 861 02 16 47 02 21 27 --- 01 17 32 13.6 245.7 4.2 41.8 280 F 1 897 02 16 51 02 22 04 J2110-1020 01 18 09 12.3 242.7 4.1 40.9 29 1 1 897 02 22 04 02 23 44 =2107-105 01 19 50 12.0 243.0 4.2 41.1 100 F 1 910 02 22 08 02 24 21 J210358 01 20 27 13.1 246.2 4.3 42.0 29 1 1 910 02 24 21 02 29 01 --- 01 25 08 12.3 247.1 4.3 42.4 280 F 1 946 02 24 25 02 29 38 J2110-1020 01 25 45 11.1 244.1 4.3 41.6 29 1 1 946 02 29 38 02 31 18 =2107-105 01 27 25 10.8 244.4 4.3 41.7 100 F 1 959 02 29 42 02 31 55 J210358 01 28 02 11.8 247.6 4.4 42.6 29 1 1 959 02 31 55 02 36 35 --- 01 32 43 11.0 248.5 4.5 42.9 280 F 1 995 02 31 59 02 37 12 J2110-1020 01 33 20 9.8 245.5 4.4 42.2 29 1 1 995 02 37 12 02 38 52 =2107-105 01 35 00 9.5 245.8 4.4 42.3 100 F 1 1008 02 37 16 02 39 29 J210358 01 35 37 10.5 249.0 4.5 43.1 29 1 1 1008 02 39 29 02 44 09 --- 01 40 18 9.7 249.9 4.6 43.4 280 F 1 1044 02 39 33 Schedule for URUMQI (Code Ur ) Page 5 Locating AGN in local analogs of Lyman break galaxies 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 ---------------------------------------------------------------------------------------- --- Sun 8 Jun 2008 Day 160 --- 02 44 46 J2110-1020 01 40 55 8.6 246.9 4.5 42.7 29 1 1 1044 02 44 46 02 46 26 =2107-105 01 42 35 8.3 247.2 4.5 42.8 100 F 1 1057 02 44 50 02 47 03 J210358 01 43 13 9.3 250.4 4.6 43.6 29 1 1 1057 02 47 03 02 51 43 --- 01 47 53 8.4 251.3 4.7 43.9 280 F 1 1093 02 47 07 02 52 20 J2110-1020 01 48 30 7.3 248.3 4.6 43.3 29 1 1 1093 02 52 20 02 54 00 =2107-105 01 50 11 7.0 248.6 4.7 43.4 100 F 1 1106 02 52 24 02 54 37 J210358 01 50 48 7.9 251.8 4.8 44.0 29 1 1 1106 02 54 37 02 59 17 --- 01 55 29 7.1 252.6 4.9 44.3 280 F 1 1142 02 54 41 02 59 54 J2110-1020 01 56 06 6.0 249.7 4.8 43.8 29 1 1 1142 02 59 54 03 01 34 =2107-105 01 57 46 5.7 249.9 4.8 43.9 100 F 1 1155 02 59 58 03 02 11 J210358 01 58 23 6.6 253.2 4.9 44.5 29 1 1 1155 03 02 11 03 06 51 --- 02 03 04 5.8 254.0 5.0 44.7 280 F 1 1191 03 02 15 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: eo006c.18cm Matches group ur18cm in /afs/mpa/home/overzier/SCHED/catalogs/freq.dat update L.Xiang 9Feb05 Setup group: 8 Station: URUMQI Total bit rate: 1024 Format: MKIV1:2 Bits per sample: 2 Sample rate: 32.000 Number of channels: 16 Speedup factor: 0.50 Disk used to record data. 1st LO= 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 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= 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= 310.49 310.49 310.49 310.49 342.49 342.49 342.49 342.49 374.49 374.49 374.49 374.49 406.49 406.49 406.49 406.49 Bandwd= 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 16.000 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 -- Locating AGN in local analogs of Lyman break galaxies 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) * J210358 21 01 18.743096 * 21 03 58.730000 21 04 27.101389 0.00 -07 39 59.00072 *-07 28 02.20000 -07 26 01.77313 0.00 From catalog imbedded in main SCHED input file. 3.422 scan hours, 143.261 baseline hours above horizon. * J2110-1020 21 07 18.816387 * 21 10 00.978983 21 10 29.715824 0.28 2107-105 -10 33 12.27643 *-10 20 57.31917 -10 18 52.73044 0.46 J2110-10 /afs/mpa/home/overzier/SCHED/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 1.411 scan hours, 55.222 baseline hours above horizon. * J2253+1608 22 51 29.519744 * 22 53 57.747943 22 54 23.350640 0.31 2251+158 15 52 54.34806 * 16 08 53.56089 16 11 30.40083 0.20 3C454.3 /afs/mpa/home/overzier/SCHED/catalogs/sources.vlba J2253+16 VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.108 scan hours, 5.958 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) J210358 121.0 J2110-1020 120.6 J2253+1608 86.5 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