COVER INFORMATION Station: SHANGHAI (Code Sh ) 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 SHANGHAI (Code Sh ) 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: 689.51 689.51 689.51 689.51 657.51 657.51 657.51 657.51 625.51 625.51 625.51 625.51 593.51 593.51 593.51 593.51 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 00 00 00 J2110-1020 01 11 47 18.9 244.7 4.0 51.9 0 1 1 0 00 00 00 00 02 00 =2107-105 01 13 48 18.6 245.0 4.1 52.1 120 F 1 15 00 00 01 00 02 37 J210358 01 14 25 19.0 248.4 4.2 53.4 32 1 1 15 00 02 37 00 07 17 --- 01 19 05 18.1 249.2 4.2 53.8 280 F 1 52 00 02 38 00 07 54 J2110-1020 01 19 43 17.4 245.9 4.2 52.6 32 1 1 52 00 07 54 00 09 34 =2107-105 01 21 23 17.1 246.2 4.2 52.8 100 F 1 65 00 07 55 00 10 11 J210358 01 22 00 17.5 249.6 4.3 54.0 32 1 1 65 00 10 11 00 14 51 --- 01 26 41 16.5 250.3 4.4 54.4 280 F 1 101 00 10 12 00 15 28 J2110-1020 01 27 18 15.9 247.1 4.3 53.3 32 1 1 101 00 15 28 00 17 08 =2107-105 01 28 58 15.6 247.3 4.3 53.4 100 F 1 114 00 15 29 00 17 45 J210358 01 29 35 15.9 250.8 4.4 54.6 32 1 1 114 00 17 45 00 22 25 --- 01 34 16 15.0 251.5 4.5 55.0 280 F 1 150 00 17 46 00 23 02 J2110-1020 01 34 53 14.4 248.2 4.4 53.9 32 1 1 150 00 23 02 00 24 42 =2107-105 01 36 33 14.1 248.5 4.4 54.1 100 F 1 163 00 23 03 00 25 19 J210358 01 37 10 14.4 251.9 4.5 55.2 32 1 1 163 00 25 19 00 29 59 --- 01 41 51 13.5 252.6 4.6 55.5 280 F 1 199 00 25 20 00 30 36 J2110-1020 01 42 28 12.9 249.4 4.5 54.5 32 1 1 199 00 30 36 00 32 16 =2107-105 01 44 09 12.6 249.6 4.6 54.7 100 F 1 212 00 30 37 00 32 53 J210358 01 44 46 12.9 253.0 4.7 55.7 32 1 1 212 00 32 53 00 37 33 --- 01 49 26 11.9 253.7 4.7 56.0 280 F 1 248 00 32 54 00 38 10 J2110-1020 01 50 04 11.4 250.5 4.7 55.1 32 1 1 248 00 38 10 00 39 50 =2107-105 01 51 44 11.0 250.7 4.7 55.2 100 F 1 261 00 38 11 Schedule for SHANGHAI (Code Sh ) 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 01 52 21 11.3 254.1 4.8 56.1 32 1 1 261 00 40 27 00 45 07 --- 01 57 02 10.3 254.7 4.9 56.4 280 F 1 297 00 40 28 00 45 44 J2110-1020 01 57 39 9.8 251.5 4.8 55.6 32 1 1 297 00 45 44 00 47 24 =2107-105 01 59 19 9.5 251.8 4.8 55.8 100 F 1 310 00 45 45 00 47 54 J2110-1020 01 59 49 9.4 251.8 4.8 55.8 28 1 1 310 00 47 54 00 53 54 =2107-105 02 05 50 8.2 252.7 4.9 56.2 360 F 1 356 00 47 55 00 56 54 J2253+1608 02 08 51 43.4 262.9 3.2 62.2 119 1 1 356 00 56 54 01 03 24 =2251+158 02 15 22 42.1 263.9 3.3 62.5 390 F 1 406 00 56 55 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 sh18cm in /afs/mpa/home/overzier/SCHED/catalogs/freq.dat Huang Xinyong 27Sept05 ****** Only 244.98 of 256.00 MHz total bandwidth is within the IFs in the setup file before any FREQ or DOPPLER shifts. Setup group: 9 Station: SHANGHAI 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= 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 this setup were used. Frequency Set: 9 Setup file default. Used pcal sets: 1 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= 689.51 689.51 689.51 689.51 657.51 657.51 657.51 657.51 625.51 625.51 625.51 625.51 593.51 593.51 593.51 593.51 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 The following pulse cal sets were used with this setup: Pulse cal detection set: 1 PCAL = 1MHZ PCALXB1= S1 S3 S5 S7 S9 S11 S13 S15 PCALXB2= S2 S4 S6 S8 S10 S12 S14 S16 PCALFR1= 490 510 490 510 490 510 490 510 PCALFR2= 490 510 490 510 490 510 490 510 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