COVER INFORMATION Station: SHANGHAI (Code Sh ) Experiment: Locating AGN in local analogs of Lyman break galaxies Exp. Code: EO006A 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: J015028 Phase-reference calibrator: J0158+1307 Fringe finder: J0237+2848 Amplitude calibrator: J0204+1514 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 ---------------------------------------------------------------------------------------- --- Wed 4 Jun 2008 Day 156 --- 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 03 00 00 J0158+1307 03 56 31 57.7 242.9 2.0 51.5 0 1 1 0 03 00 00 03 02 00 =0156+128 03 58 31 57.3 243.5 2.0 51.9 120 F 1 15 03 00 01 03 02 40 J015028 03 59 11 55.5 245.9 2.1 53.4 35 1 1 15 03 02 40 03 07 20 --- 04 03 52 54.6 247.1 2.2 54.1 280 F 1 52 03 02 41 03 08 00 J0158+1307 04 04 32 56.1 245.1 2.1 52.9 35 1 1 52 03 08 00 03 09 40 =0156+128 04 06 12 55.8 245.5 2.1 53.2 100 F 1 65 03 08 01 03 10 20 J015028 04 06 52 54.0 247.8 2.3 54.5 35 1 1 65 03 10 20 03 15 00 --- 04 11 33 53.1 249.0 2.3 55.2 280 F 1 101 03 10 21 03 15 40 J0158+1307 04 12 13 54.6 247.0 2.2 54.1 35 1 1 101 03 15 40 03 17 20 =0156+128 04 13 53 54.3 247.5 2.2 54.3 100 F 1 114 03 15 41 03 18 00 J015028 04 14 34 52.5 249.6 2.4 55.5 35 1 1 114 03 18 00 03 22 40 --- 04 19 14 51.5 250.7 2.5 56.1 280 F 1 150 03 18 01 03 23 20 J0158+1307 04 19 54 53.1 248.9 2.3 55.1 35 1 1 150 03 23 20 03 25 00 =0156+128 04 21 35 52.7 249.3 2.4 55.3 100 F 1 163 03 23 21 03 25 40 J015028 04 22 15 50.9 251.3 2.5 56.4 35 1 1 163 03 25 40 03 30 20 --- 04 26 56 50.0 252.3 2.6 56.9 280 F 1 199 03 25 41 03 31 00 J0158+1307 04 27 36 51.5 250.6 2.5 56.0 35 1 1 199 03 31 00 03 32 40 =0156+128 04 29 16 51.2 251.0 2.5 56.2 100 F 1 212 03 31 01 03 33 20 J015028 04 29 56 49.4 252.9 2.7 57.2 35 1 1 212 03 33 20 03 38 00 --- 04 34 37 48.4 253.9 2.7 57.7 280 F 1 248 03 33 21 03 38 40 J0158+1307 04 35 17 50.0 252.2 2.6 56.9 35 1 1 248 03 38 40 03 40 20 =0156+128 04 36 57 49.6 252.6 2.6 57.0 100 F 1 261 03 38 41 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 ---------------------------------------------------------------------------------------- --- Wed 4 Jun 2008 Day 156 --- 03 41 00 J015028 04 37 37 47.8 254.4 2.8 57.9 35 1 1 261 03 41 00 03 45 40 --- 04 42 18 46.8 255.3 2.9 58.3 280 F 1 297 03 41 01 03 46 20 J0158+1307 04 42 58 48.4 253.8 2.7 57.6 35 1 1 297 03 46 20 03 48 00 =0156+128 04 44 39 48.1 254.1 2.8 57.8 100 F 1 310 03 46 21 03 48 40 J015028 04 45 19 46.2 255.9 2.9 58.5 35 1 1 310 03 48 40 03 53 20 --- 04 49 59 45.2 256.7 3.0 58.9 280 F 1 346 03 48 41 03 54 00 J0158+1307 04 50 39 46.8 255.3 2.9 58.3 35 1 1 346 03 54 00 03 55 40 =0156+128 04 52 20 46.5 255.6 2.9 58.4 100 F 1 359 03 54 01 03 56 20 J015028 04 53 00 44.6 257.3 3.0 59.1 35 1 1 359 03 56 20 04 01 00 --- 04 57 41 43.6 258.1 3.1 59.4 280 F 1 395 03 56 21 04 01 40 J0158+1307 04 58 21 45.2 256.7 3.0 58.8 35 1 1 395 04 01 40 04 03 20 =0156+128 05 00 01 44.9 257.0 3.0 59.0 100 F 1 408 04 01 41 04 04 00 J015028 05 00 41 43.0 258.6 3.2 59.6 35 1 1 408 04 04 00 04 08 40 --- 05 05 22 42.0 259.4 3.2 59.8 280 F 1 444 04 04 01 04 09 20 J0158+1307 05 06 02 43.6 258.0 3.1 59.3 35 1 1 444 04 09 20 04 11 00 =0156+128 05 07 42 43.3 258.3 3.1 59.4 100 F 1 457 04 09 21 04 11 40 J015028 05 08 22 41.4 259.9 3.3 60.0 35 1 1 457 04 11 40 04 16 20 --- 05 13 03 40.4 260.6 3.4 60.2 280 F 1 493 04 11 41 04 17 00 J0158+1307 05 13 43 42.0 259.3 3.2 59.8 35 1 1 493 04 17 00 04 18 40 =0156+128 05 15 24 41.6 259.6 3.3 59.9 100 F 1 506 04 17 01 04 19 20 J015028 05 16 04 39.7 261.1 3.4 60.3 35 1 1 506 04 19 20 04 24 00 --- 05 20 44 38.7 261.8 3.5 60.5 280 F 1 542 04 19 21 04 24 40 J0158+1307 05 21 25 40.4 260.6 3.4 60.2 35 1 1 542 04 24 40 04 26 20 =0156+128 05 23 05 40.0 260.8 3.4 60.2 100 F 1 555 04 24 41 04 27 00 J015028 05 23 45 38.1 262.3 3.5 60.6 35 1 1 555 04 27 00 04 31 40 --- 05 28 26 37.1 263.0 3.6 60.8 280 F 1 591 04 27 01 04 32 20 J0158+1307 05 29 06 38.8 261.8 3.5 60.5 35 1 1 591 04 32 20 04 34 00 =0156+128 05 30 46 38.4 262.0 3.5 60.6 100 F 1 604 04 32 21 04 34 40 J015028 05 31 26 36.5 263.4 3.7 60.9 35 1 1 604 04 34 40 04 39 20 --- 05 36 07 35.5 264.1 3.8 61.0 280 F 1 640 04 34 41 Schedule for SHANGHAI (Code Sh ) 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 ---------------------------------------------------------------------------------------- --- Wed 4 Jun 2008 Day 156 --- 04 40 00 J0158+1307 05 36 47 37.1 262.9 3.6 60.8 35 1 1 640 04 40 00 04 41 40 =0156+128 05 38 27 36.8 263.2 3.7 60.8 100 F 1 653 04 40 01 04 42 20 J015028 05 39 07 34.8 264.5 3.8 61.1 35 1 1 653 04 42 20 04 47 00 --- 05 43 48 33.8 265.2 3.9 61.2 280 F 1 689 04 42 21 04 47 40 J0158+1307 05 44 28 35.5 264.1 3.8 61.0 35 1 1 689 04 47 40 04 49 20 =0156+128 05 46 09 35.1 264.3 3.8 61.0 100 F 1 702 04 47 41 04 50 00 J015028 05 46 49 33.2 265.6 3.9 61.3 35 1 1 702 04 50 00 04 54 40 --- 05 51 29 32.2 266.3 4.0 61.4 280 F 1 738 04 50 01 04 55 20 J0158+1307 05 52 10 33.9 265.2 3.9 61.2 35 1 1 738 04 55 20 04 57 00 =0156+128 05 53 50 33.5 265.4 3.9 61.2 100 F 1 751 04 55 21 04 57 40 J015028 05 54 30 31.6 266.7 4.1 61.4 35 1 1 751 04 57 40 05 02 20 --- 05 59 11 30.6 267.3 4.1 61.5 280 F 1 787 04 57 41 05 03 00 J0158+1307 05 59 51 32.2 266.2 4.0 61.3 35 1 1 787 05 03 00 05 04 40 =0156+128 06 01 31 31.9 266.5 4.0 61.4 100 F 1 800 05 03 01 05 05 20 J015028 06 02 11 29.9 267.7 4.2 61.5 35 1 1 800 05 05 20 05 10 00 --- 06 06 52 28.9 268.4 4.3 61.5 280 F 1 836 05 05 21 05 10 40 J0158+1307 06 07 32 30.6 267.3 4.1 61.4 35 1 1 836 05 10 40 05 12 20 =0156+128 06 09 12 30.2 267.5 4.2 61.5 100 F 1 849 05 10 41 05 13 00 J015028 06 09 52 28.3 268.8 4.3 61.6 35 1 1 849 05 13 00 05 17 40 --- 06 14 33 27.3 269.4 4.4 61.6 280 F 1 885 05 13 01 05 18 20 J0158+1307 06 15 13 28.9 268.3 4.3 61.5 35 1 1 885 05 18 20 05 20 00 =0156+128 06 16 54 28.6 268.5 4.3 61.5 100 F 1 898 05 18 21 05 20 40 J015028 06 17 34 26.6 269.8 4.4 61.6 35 1 1 898 05 20 40 05 25 20 --- 06 22 15 25.6 270.4 4.5 61.6 280 F 1 934 05 20 41 05 26 00 J0158+1307 06 22 55 27.3 269.3 4.4 61.6 35 1 1 934 05 26 00 05 27 40 =0156+128 06 24 35 26.9 269.5 4.4 61.6 100 F 1 947 05 26 01 05 28 20 J015028 06 25 15 25.0 270.7 4.6 61.6 35 1 1 947 05 28 20 05 33 00 --- 06 29 56 24.0 271.3 4.7 61.6 280 F 1 983 05 28 21 05 33 40 J0158+1307 06 30 36 25.6 270.3 4.5 61.6 35 1 1 983 05 33 40 05 35 20 =0156+128 06 32 16 25.3 270.5 4.5 61.6 100 F 1 996 05 33 41 Schedule for SHANGHAI (Code Sh ) 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 ---------------------------------------------------------------------------------------- --- Wed 4 Jun 2008 Day 156 --- 05 36 00 J015028 06 32 56 23.3 271.7 4.7 61.5 35 1 1 996 05 36 00 05 40 40 --- 06 37 37 22.3 272.3 4.8 61.5 280 F 1 1032 05 36 01 05 41 20 J0158+1307 06 38 17 24.0 271.3 4.6 61.5 35 1 1 1032 05 41 20 05 43 00 =0156+128 06 39 57 23.6 271.5 4.7 61.5 100 F 1 1045 05 41 21 05 43 40 J015028 06 40 38 21.7 272.7 4.8 61.5 35 1 1 1045 05 43 40 05 48 20 --- 06 45 18 20.7 273.3 4.9 61.4 280 F 1 1081 05 43 41 05 49 00 J0158+1307 06 45 58 22.3 272.3 4.8 61.5 35 1 1 1081 05 49 00 05 50 40 =0156+128 06 47 39 22.0 272.5 4.8 61.5 100 F 1 1094 05 49 01 05 51 20 J015028 06 48 19 20.0 273.6 5.0 61.4 35 1 1 1094 05 51 20 05 56 00 --- 06 53 00 19.0 274.2 5.0 61.3 280 F 1 1130 05 51 21 05 56 40 J0158+1307 06 53 40 20.7 273.2 4.9 61.4 35 1 1 1130 05 56 40 05 58 20 =0156+128 06 55 20 20.3 273.4 4.9 61.4 100 F 1 1143 05 56 41 05 59 00 J015028 06 56 00 18.4 274.6 5.1 61.2 35 1 1 1143 05 59 00 06 03 40 --- 07 00 41 17.4 275.2 5.2 61.2 280 F 1 1179 05 59 01 06 04 20 J0158+1307 07 01 21 19.1 274.2 5.0 61.3 35 1 1 1179 06 04 20 06 06 00 =0156+128 07 03 01 18.7 274.4 5.1 61.3 100 F 1 1192 06 04 21 06 07 30 J0237+2848 07 04 31 33.2 286.2 4.4 69.9 64 1 1 1192 06 07 30 06 15 00 =0234+285 07 12 03 31.7 286.8 4.6 69.3 450 F 1 1250 06 07 31 06 16 30 J0204+1514 07 13 33 18.7 276.9 5.1 61.8 66 1 1 1250 06 16 30 06 24 00 =0202+149 07 21 04 17.1 277.8 5.3 61.6 450 F 1 1308 06 16 31 06 25 40 J0158+1307 07 22 44 14.5 276.8 5.4 60.8 94 1 1 1308 06 25 40 06 27 20 =0156+128 07 24 25 14.1 277.0 5.4 60.8 100 F 1 1321 06 25 41 06 28 00 J015028 07 25 05 12.2 278.2 5.6 60.5 35 1 1 1321 06 28 00 06 32 40 --- 07 29 46 11.2 278.7 5.6 60.4 280 F 1 1357 06 28 01 06 33 20 J0158+1307 07 30 26 12.9 277.8 5.5 60.6 35 1 1 1357 06 33 20 06 35 00 =0156+128 07 32 06 12.5 278.0 5.5 60.6 100 F 1 1370 06 33 21 06 35 40 J015028 07 32 46 10.6 279.1 5.7 60.3 35 1 1 1370 06 35 40 06 40 20 --- 07 37 27 9.6 279.7 5.8 60.1 280 F 1 1406 06 35 41 06 41 00 J0158+1307 07 38 07 11.2 278.7 5.6 60.4 35 1 1 1406 06 41 00 06 42 40 =0156+128 07 39 47 10.9 278.9 5.7 60.3 100 F 1 1419 06 41 01 Schedule for SHANGHAI (Code Sh ) Page 6 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 ---------------------------------------------------------------------------------------- --- Wed 4 Jun 2008 Day 156 --- 06 43 20 J015028 07 40 27 9.0 280.1 5.8 60.0 35 1 1 1419 06 43 20 06 48 00 --- 07 45 08 8.0 280.6 5.9 59.8 280 F 1 1455 06 43 21 06 48 40 J0158+1307 07 45 48 9.6 279.6 5.8 60.1 35 1 1 1455 06 48 40 06 50 20 =0156+128 07 47 28 9.3 279.8 5.8 60.0 100 F 1 1468 06 48 41 06 51 00 J015028 07 48 09 7.4 281.0 6.0 59.7 35 1 1 1468 06 51 00 06 55 40 --- 07 52 49 6.4 281.6 6.0 59.5 280 F 1 1504 06 51 01 06 56 20 J0158+1307 07 53 29 8.0 280.6 5.9 59.8 35 1 1 1504 06 56 20 06 58 00 =0156+128 07 55 10 7.6 280.8 5.9 59.7 100 F 1 1517 06 56 21 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: eo006a.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) * J015028 01 47 47.576311 * 01 50 28.420000 01 50 55.133725 0.00 12 54 07.49997 * 13 08 58.10000 13 11 28.52096 0.00 From catalog imbedded in main SCHED input file. 3.422 scan hours, 175.778 baseline hours above horizon. * J0158+1307 01 56 14.946660 * 01 58 56.273801 01 59 23.037067 0.60 0156+128 12 52 29.70047 * 13 07 02.74128 13 09 30.43668 1.32 /afs/mpa/home/overzier/SCHED/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 1.283 scan hours, 60.250 baseline hours above horizon. * J0204+1514 02 02 07.396229 * 02 04 50.413897 02 05 17.424258 0.31 0202+149 14 59 50.93943 * 15 14 11.04365 15 16 36.23832 0.20 J0204+15 /afs/mpa/home/overzier/SCHED/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.125 scan hours, 6.856 baseline hours above horizon. * J0237+2848 02 34 55.589592 * 02 37 52.405679 02 38 21.491470 0.23 0234+285 28 35 11.40780 * 28 48 08.99005 28 50 18.82438 0.40 J0237+28 /afs/mpa/home/overzier/SCHED/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.125 scan hours, 6.835 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) J015028 43.6 J0158+1307 41.6 J0204+1514 39.6 J0237+2848 30.4 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