COVER INFORMATION Station: SHANGHAI (Code Sh ) Experiment: Dominant heating mechanism in ULIRGs Exp. Code: EP064E Schedule Version: 1.00 Processed by SCHED version: 8.10 Bug fixs and minor enhancements PI: Miguel A. Perez-Torres Address: IAA - CSIC C/ Camino Bajo de Huetor, 50 18008 Granada, Spain Phone: +34-958230644 EMAIL: torres@iaa.es Fax: +34-958814530 Phone during observation: +34-665252538 Observing mode: 1024 Mbps Notes: 6-hr of 1-Gb/s, phase-ref of IRAS 19295-0406 with EVN+MERLIN Second epoch obs-ns at 18cm Schedule for SHANGHAI (Code Sh ) Page 2 Dominant heating mechanism in ULIRGs 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 3 Jun 2009 Day 154 --- 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 21 35 00 3C345 22 29 40 21.7 -55.6 5.8 66.9 0 1 1 0 21 35 00 21 45 00 --- 22 39 42 19.9 -54.8 5.9 65.6 600 F 1 77 21 35 01 21 46 00 3C345 22 40 42 19.8 -54.7 6.0 65.5 58 1 1 77 21 46 00 21 53 00 --- 22 47 43 18.5 -54.1 6.1 64.6 420 F 1 132 21 46 01 21 59 00 J1941-0511 22 53 44 31.7 240.2 3.2 48.3 64 1 1 132 21 59 00 22 00 30 =1939-053 22 55 14 31.4 240.5 3.2 48.5 90 F 1 143 21 59 01 22 00 30 IRAS1929 22 55 14 30.4 243.4 3.4 50.1 -5 1 1 143 No stop 22 04 00 --- 22 58 45 29.8 244.0 3.4 50.5 205 F 1 170 22 00 31 22 04 00 J1941-0511 22 58 45 30.8 241.2 3.3 48.9 -5 1 1 170 No stop 22 05 30 =1939-053 23 00 15 30.5 241.5 3.3 49.1 85 F 1 182 22 04 01 22 05 30 IRAS1929 23 00 15 29.5 244.3 3.5 50.7 -5 1 1 182 No stop 22 09 00 --- 23 03 46 28.8 244.9 3.5 51.0 205 F 1 209 22 05 31 22 09 00 J1941-0511 23 03 46 29.8 242.1 3.4 49.5 -5 1 1 209 No stop 22 10 30 =1939-053 23 05 16 29.5 242.4 3.4 49.6 85 F 1 221 22 09 01 22 10 30 IRAS1929 23 05 16 28.5 245.2 3.5 51.2 -5 1 1 221 No stop 22 14 00 --- 23 08 46 27.8 245.8 3.6 51.5 205 F 1 248 22 10 31 22 15 00 J1941-0511 23 09 47 28.7 243.3 3.5 50.2 55 1 1 248 22 15 00 22 16 30 =1939-053 23 11 17 28.4 243.5 3.5 50.3 90 F 1 259 22 15 01 22 16 30 IRAS1929 23 11 17 27.3 246.2 3.6 51.8 -5 1 1 259 No stop 22 20 00 --- 23 14 47 26.6 246.8 3.7 52.1 205 F 1 286 22 16 31 22 20 00 J1941-0511 23 14 47 27.7 244.2 3.5 50.7 -5 1 1 286 No stop 22 21 30 =1939-053 23 16 18 27.4 244.4 3.6 50.9 85 F 1 298 22 20 01 Schedule for SHANGHAI (Code Sh ) Page 3 Dominant heating mechanism in ULIRGs 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 3 Jun 2009 Day 154 --- 22 21 30 IRAS1929 23 16 18 26.3 247.1 3.7 52.3 -5 1 1 298 No stop 22 25 00 --- 23 19 48 25.6 247.7 3.8 52.6 205 F 1 325 22 21 31 22 25 00 J1941-0511 23 19 48 26.8 245.0 3.6 51.2 -5 1 1 325 No stop 22 26 30 =1939-053 23 21 18 26.5 245.3 3.6 51.4 85 F 1 337 22 25 01 22 26 30 IRAS1929 23 21 18 25.3 247.9 3.8 52.7 -5 1 1 337 No stop 22 30 00 --- 23 24 49 24.6 248.5 3.9 53.0 205 F 1 364 22 26 31 22 31 00 J1941-0511 23 25 49 25.6 246.1 3.7 51.8 56 1 1 364 22 31 00 22 32 30 =1939-053 23 27 19 25.3 246.3 3.8 51.9 90 F 1 375 22 31 01 22 32 30 IRAS1929 23 27 19 24.1 248.9 3.9 53.2 -5 1 1 375 No stop 22 36 00 --- 23 30 50 23.4 249.5 4.0 53.5 205 F 1 403 22 32 31 22 36 00 J1941-0511 23 30 50 24.6 246.9 3.8 52.3 -5 1 1 403 No stop 22 37 30 =1939-053 23 32 20 24.3 247.2 3.8 52.4 85 F 1 414 22 36 01 22 37 30 IRAS1929 23 32 20 23.1 249.8 4.0 53.6 -5 1 1 414 No stop 22 41 00 --- 23 35 51 22.4 250.3 4.0 53.9 205 F 1 441 22 37 31 22 41 00 J1941-0511 23 35 51 23.6 247.8 3.9 52.7 -5 1 1 441 No stop 22 42 30 =1939-053 23 37 21 23.3 248.0 3.9 52.9 85 F 1 453 22 41 01 22 42 30 IRAS1929 23 37 21 22.1 250.6 4.1 54.0 -5 1 1 453 No stop 22 46 00 --- 23 40 52 21.4 251.1 4.1 54.3 205 F 1 480 22 42 31 22 47 00 J1941-0511 23 41 52 22.4 248.7 4.0 53.2 56 1 1 480 22 47 00 22 48 30 =1939-053 23 43 22 22.1 249.0 4.0 53.4 90 F 1 492 22 47 01 22 48 30 IRAS1929 23 43 22 20.9 251.5 4.2 54.5 -5 1 1 492 No stop 22 52 00 --- 23 46 53 20.2 252.0 4.2 54.7 205 F 1 519 22 48 31 22 52 00 J1941-0511 23 46 53 21.4 249.5 4.1 53.7 -5 1 1 519 No stop 22 53 30 =1939-053 23 48 23 21.1 249.8 4.1 53.8 85 F 1 530 22 52 01 22 53 30 IRAS1929 23 48 23 19.9 252.3 4.3 54.8 -4 1 1 530 No stop 22 57 00 --- 23 51 53 19.2 252.8 4.3 55.1 206 F 1 557 22 53 31 22 57 00 J1941-0511 23 51 53 20.4 250.3 4.2 54.1 -4 1 1 557 No stop 22 58 30 =1939-053 23 53 24 20.1 250.6 4.2 54.2 86 F 1 569 22 57 01 22 58 30 IRAS1929 23 53 24 18.9 253.0 4.3 55.2 -4 1 1 569 No stop 23 02 00 --- 23 56 54 18.2 253.6 4.4 55.4 206 F 1 596 22 58 31 Schedule for SHANGHAI (Code Sh ) Page 4 Dominant heating mechanism in ULIRGs 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 3 Jun 2009 Day 154 --- 23 03 00 J1941-0511 23 57 54 19.2 251.3 4.3 54.5 56 1 1 596 23 03 00 23 04 30 =1939-053 23 59 25 18.9 251.5 4.3 54.6 90 F 1 608 23 03 01 23 04 30 IRAS1929 23 59 25 17.6 253.9 4.4 55.6 -4 1 1 608 No stop 23 08 00 --- 00 02 55 16.9 254.4 4.5 55.8 206 F 1 635 23 04 31 23 08 00 J1941-0511 00 02 55 18.2 252.0 4.3 54.9 -4 1 1 635 No stop 23 09 30 =1939-053 00 04 25 17.9 252.2 4.4 55.0 86 F 1 646 23 08 01 23 09 30 IRAS1929 00 04 25 16.6 254.7 4.5 55.9 -4 1 1 646 No stop 23 13 00 --- 00 07 56 15.9 255.2 4.6 56.1 206 F 1 674 23 09 31 23 13 00 J1941-0511 00 07 56 17.1 252.8 4.4 55.2 -4 1 1 674 No stop 23 14 30 =1939-053 00 09 26 16.8 253.0 4.5 55.3 86 F 1 685 23 13 01 23 14 30 IRAS1929 00 09 26 15.6 255.4 4.6 56.2 -4 1 1 685 No stop 23 18 00 --- 00 12 57 14.8 255.9 4.7 56.4 206 F 1 712 23 14 31 23 19 00 J1941-0511 00 13 57 15.9 253.7 4.5 55.6 56 1 1 712 23 19 00 23 20 30 =1939-053 00 15 27 15.6 253.9 4.6 55.7 90 F 1 724 23 19 01 23 20 30 IRAS1929 00 15 27 14.3 256.3 4.7 56.5 -4 1 1 724 No stop 23 24 00 --- 00 18 58 13.6 256.7 4.8 56.7 206 F 1 751 23 20 31 23 24 00 J1941-0511 00 18 58 14.9 254.4 4.6 55.9 -4 1 1 751 No stop 23 25 30 =1939-053 00 20 28 14.6 254.6 4.6 56.0 86 F 1 763 23 24 01 23 25 30 IRAS1929 00 20 28 13.3 257.0 4.8 56.7 -4 1 1 763 No stop 23 29 00 --- 00 23 59 12.5 257.5 4.9 56.9 206 F 1 790 23 25 31 23 29 00 J1941-0511 00 23 59 13.8 255.1 4.7 56.2 -4 1 1 790 No stop 23 30 30 =1939-053 00 25 29 13.5 255.3 4.7 56.3 86 F 1 801 23 29 01 23 30 30 IRAS1929 00 25 29 12.2 257.7 4.9 57.0 -4 1 1 801 No stop 23 34 00 --- 00 28 59 11.5 258.1 4.9 57.1 206 F 1 828 23 30 31 23 35 00 J1941-0511 00 30 00 12.6 256.0 4.8 56.5 56 1 1 828 23 35 00 23 36 30 =1939-053 00 31 30 12.3 256.2 4.8 56.6 90 F 1 840 23 35 01 23 36 30 IRAS1929 00 31 30 11.0 258.5 5.0 57.3 -4 1 1 840 No stop 23 40 00 --- 00 35 00 10.2 259.0 5.0 57.4 206 F 1 867 23 36 31 23 40 00 J1941-0511 00 35 00 11.6 256.7 4.9 56.8 -4 1 1 867 No stop 23 41 30 =1939-053 00 36 31 11.2 256.9 4.9 56.9 86 F 1 879 23 40 01 Schedule for SHANGHAI (Code Sh ) Page 5 Dominant heating mechanism in ULIRGs 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 3 Jun 2009 Day 154 --- 23 41 30 IRAS1929 00 36 31 9.9 259.2 5.1 57.5 -4 1 1 879 No stop 23 45 00 --- 00 40 01 9.2 259.7 5.1 57.6 206 F 1 906 23 41 31 23 45 00 J1941-0511 00 40 01 10.5 257.4 5.0 57.0 -4 1 1 906 No stop 23 46 30 =1939-053 00 41 32 10.2 257.6 5.0 57.1 86 F 1 917 23 45 01 23 46 30 IRAS1929 00 41 32 8.9 259.9 5.1 57.7 -4 1 1 917 No stop 23 50 00 --- 00 45 02 8.1 260.3 5.2 57.8 206 F 1 944 23 46 31 23 51 00 J1941-0511 00 46 02 9.3 258.2 5.1 57.3 56 1 1 944 23 51 00 23 52 30 =1939-053 00 47 33 8.9 258.4 5.1 57.4 90 F 1 956 23 51 01 23 52 30 IRAS1929 00 47 33 7.6 260.7 5.2 57.9 -4 1 1 956 No stop 23 56 00 --- 00 51 03 6.8 261.1 5.3 58.0 206 F 1 983 23 52 31 23 56 00 J1941-0511 00 51 03 8.2 258.9 5.1 57.5 -4 1 1 983 No stop 23 57 30 =1939-053 00 52 33 7.9 259.1 5.2 57.6 86 F 1 995 23 56 01 --- Start: Wed 3 Jun 2009 Day 154 -- Stop: Thu 4 Jun 2009 Day 155 --- 23 57 30 IRAS1929 00 52 33 6.5 261.3 5.3 58.1 -4 1 1 995 No stop 00 01 00 --- 00 56 04 5.8 261.8 5.4 58.2 206 F 1 1022 23 57 31 00 01 00 J1941-0511 00 56 04 7.1 259.5 5.2 57.7 -4 1 1 1022 No stop 00 02 30 =1939-053 00 57 34 6.8 259.7 5.3 57.8 86 F 1 1033 00 01 01 00 02 30 IRAS1929 00 57 34 5.5 262.0 5.4 58.2 -4 1 1 1033 No stop 00 06 00 --- 01 01 05 4.7 262.5 5.5 D 58.3 0 F 1 1061 00 02 31 00 07 00 J1941-0511 01 02 05 5.9 260.3 5.3 57.9 56 1 1 1061 00 07 00 00 08 30 =1939-053 01 03 35 5.6 260.5 5.4 58.0 90 F 1 1072 00 07 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: ep064e.18cm Matches group sh18cm in /Users/torres/home/soft/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: 10 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: 10 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 -- Dominant heating mechanism in ULIRGs 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) * IRAS1929 19 29 44.153581 * 19 32 22.307619 19 32 53.985294 0.00 -04 06 28.85412 *-04 00 01.06801 -03 58 50.39556 0.00 From catalog imbedded in main SCHED input file. 3.608 scan hours, 120.452 baseline hours above horizon. J1331+3030 13 28 49.657764 * 13 31 08.288056 13 31 36.260393 0.36 * 3C286 30 45 58.64058 * 30 30 32.95922 30 27 38.11118 0.47 1328+307 /Users/torres/home/soft/sched/catalogs/sources.vlba J1331+30 VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 0.083 scan hours, 3.000 baseline hours above horizon. J1642+3948 16 41 17.606227 * 16 42 58.809964 16 43 20.240768 0.26 * 3C345 39 54 10.81495 * 39 48 36.99401 39 47 27.70649 0.40 1641+399 /Users/torres/home/soft/sched/catalogs/sources.vlba J1642+39 VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 0.283 scan hours, 9.412 baseline hours above horizon. * J1941-0511 19 39 07.661036 * 19 41 47.008579 19 42 18.885195 0.41 1939-053 -05 18 37.74290 *-05 11 32.38284 -05 10 14.04337 0.87 /Users/torres/home/soft/sched/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 1.575 scan hours, 43.263 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) IRAS1929 136.2 3C286 109.1 3C345 117.8 J1941-0511 134.7 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