COVER INFORMATION Station: SHANGHAI (Code Sh ) Experiment: Dominant heating mechanism in ULIRGs Exp. Code: EP064G 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 Third epoch obs-ns at 6cm 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 ---------------------------------------------------------------------------------------- --- Thu 11 Jun 2009 Day 162 --- Next scan frequencies: 4942.49 4942.49 4942.49 4942.49 4974.49 4974.49 4974.49 4974.49 5006.49 5006.49 5006.49 5006.49 5038.49 5038.49 5038.49 5038.49 Next BBC frequencies: 742.49 742.49 742.49 742.49 774.49 774.49 774.49 774.49 806.49 806.49 806.49 806.49 838.49 838.49 838.49 838.49 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 21 05 00 3C345 22 31 07 21.4 -55.5 5.8 66.7 0 1 1 0 21 05 00 21 15 00 --- 22 41 09 19.7 -54.7 6.0 65.4 600 F 1 77 21 05 01 21 16 00 3C345 22 42 09 19.5 -54.6 6.0 65.3 58 1 1 77 21 16 00 21 23 00 --- 22 49 10 18.3 -54.0 6.1 64.4 420 F 1 132 21 16 01 21 29 00 J1941-0511 22 55 11 31.4 240.5 3.2 48.5 63 1 1 132 21 29 00 21 30 30 =1939-053 22 56 42 31.2 240.8 3.2 48.6 90 F 1 143 21 29 01 21 30 30 IRAS1929 22 56 42 30.2 243.6 3.4 50.3 -5 1 1 143 No stop 21 34 00 --- 23 00 12 29.5 244.3 3.5 50.6 205 F 1 170 21 30 31 21 34 00 J1941-0511 23 00 12 30.5 241.5 3.3 49.1 -5 1 1 170 No stop 21 35 30 =1939-053 23 01 42 30.2 241.8 3.3 49.2 85 F 1 182 21 34 01 21 35 30 IRAS1929 23 01 42 29.2 244.5 3.5 50.8 -5 1 1 182 No stop 21 39 00 --- 23 05 13 28.5 245.2 3.5 51.2 205 F 1 209 21 35 31 21 39 00 J1941-0511 23 05 13 29.6 242.4 3.4 49.6 -5 1 1 209 No stop 21 40 30 =1939-053 23 06 43 29.3 242.7 3.4 49.8 85 F 1 221 21 39 01 21 40 30 IRAS1929 23 06 43 28.2 245.4 3.6 51.3 -5 1 1 221 No stop 21 44 00 --- 23 10 14 27.5 246.1 3.6 51.7 205 F 1 248 21 40 31 21 45 00 J1941-0511 23 11 14 28.4 243.5 3.5 50.3 55 1 1 248 21 45 00 21 46 30 =1939-053 23 12 44 28.1 243.8 3.5 50.5 90 F 1 259 21 45 01 21 46 30 IRAS1929 23 12 44 27.0 246.5 3.7 51.9 -5 1 1 259 No stop 21 50 00 --- 23 16 15 26.3 247.1 3.7 52.2 205 F 1 286 21 46 31 21 50 00 J1941-0511 23 16 15 27.4 244.4 3.6 50.8 -5 1 1 286 No stop 21 51 30 =1939-053 23 17 45 27.2 244.7 3.6 51.0 85 F 1 298 21 50 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 ---------------------------------------------------------------------------------------- --- Thu 11 Jun 2009 Day 162 --- 21 51 30 IRAS1929 23 17 45 26.1 247.3 3.7 52.4 -5 1 1 298 No stop 21 55 00 --- 23 21 16 25.4 247.9 3.8 52.7 205 F 1 325 21 51 31 21 55 00 J1941-0511 23 21 16 26.5 245.3 3.6 51.4 -5 1 1 325 No stop 21 56 30 =1939-053 23 22 46 26.2 245.6 3.7 51.5 85 F 1 337 21 55 01 21 56 30 IRAS1929 23 22 46 25.1 248.2 3.8 52.8 -5 1 1 337 No stop 22 00 00 --- 23 26 16 24.4 248.8 3.9 53.1 205 F 1 364 21 56 31 22 01 00 J1941-0511 23 27 17 25.3 246.3 3.7 51.9 56 1 1 364 22 01 00 22 02 30 =1939-053 23 28 47 25.0 246.6 3.8 52.1 90 F 1 375 22 01 01 22 02 30 IRAS1929 23 28 47 23.9 249.2 3.9 53.4 -5 1 1 375 No stop 22 06 00 --- 23 32 17 23.2 249.7 4.0 53.6 205 F 1 403 22 02 31 22 06 00 J1941-0511 23 32 17 24.3 247.2 3.8 52.4 -5 1 1 403 No stop 22 07 30 =1939-053 23 33 48 24.0 247.4 3.9 52.5 85 F 1 414 22 06 01 22 07 30 IRAS1929 23 33 48 22.9 250.0 4.0 53.8 -5 1 1 414 No stop 22 11 00 --- 23 37 18 22.1 250.5 4.1 54.0 205 F 1 441 22 07 31 22 11 00 J1941-0511 23 37 18 23.3 248.0 3.9 52.9 -5 1 1 441 No stop 22 12 30 =1939-053 23 38 49 23.0 248.2 3.9 53.0 85 F 1 453 22 11 01 22 12 30 IRAS1929 23 38 49 21.8 250.8 4.1 54.1 -5 1 1 453 No stop 22 16 00 --- 23 42 19 21.1 251.3 4.2 54.4 205 F 1 480 22 12 31 22 17 00 J1941-0511 23 43 19 22.1 249.0 4.0 53.4 56 1 1 480 22 17 00 22 18 30 =1939-053 23 44 50 21.8 249.2 4.0 53.5 90 F 1 492 22 17 01 22 18 30 IRAS1929 23 44 50 20.6 251.7 4.2 54.6 -5 1 1 492 No stop 22 22 00 --- 23 48 20 19.9 252.3 4.3 54.8 205 F 1 519 22 18 31 22 22 00 J1941-0511 23 48 20 21.1 249.8 4.1 53.8 -4 1 1 519 No stop 22 23 30 =1939-053 23 49 50 20.8 250.0 4.1 53.9 86 F 1 530 22 22 01 22 23 30 IRAS1929 23 49 50 19.6 252.5 4.3 54.9 -4 1 1 530 No stop 22 27 00 --- 23 53 21 18.9 253.0 4.3 55.2 206 F 1 557 22 23 31 22 27 00 J1941-0511 23 53 21 20.1 250.6 4.2 54.2 -4 1 1 557 No stop 22 28 30 =1939-053 23 54 51 19.8 250.8 4.2 54.3 86 F 1 569 22 27 01 22 28 30 IRAS1929 23 54 51 18.6 253.2 4.4 55.3 -4 1 1 569 No stop 22 32 00 --- 23 58 22 17.9 253.8 4.4 55.5 206 F 1 596 22 28 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 ---------------------------------------------------------------------------------------- --- Thu 11 Jun 2009 Day 162 --- 22 33 00 J1941-0511 23 59 22 18.9 251.5 4.3 54.6 56 1 1 596 22 33 00 22 34 30 =1939-053 00 00 52 18.6 251.7 4.3 54.7 90 F 1 608 22 33 01 22 34 30 IRAS1929 00 00 52 17.3 254.1 4.5 55.7 -4 1 1 608 No stop 22 38 00 --- 00 04 23 16.6 254.7 4.5 55.9 206 F 1 635 22 34 31 22 38 00 J1941-0511 00 04 23 17.9 252.2 4.4 55.0 -4 1 1 635 No stop 22 39 30 =1939-053 00 05 53 17.6 252.5 4.4 55.1 86 F 1 646 22 38 01 22 39 30 IRAS1929 00 05 53 16.3 254.9 4.5 56.0 -4 1 1 646 No stop 22 43 00 --- 00 09 24 15.6 255.4 4.6 56.2 206 F 1 674 22 39 31 22 43 00 J1941-0511 00 09 24 16.8 253.0 4.5 55.3 -4 1 1 674 No stop 22 44 30 =1939-053 00 10 54 16.5 253.2 4.5 55.4 86 F 1 685 22 43 01 22 44 30 IRAS1929 00 10 54 15.3 255.6 4.6 56.2 -4 1 1 685 No stop 22 48 00 --- 00 14 24 14.5 256.1 4.7 56.4 206 F 1 712 22 44 31 22 49 00 J1941-0511 00 15 25 15.6 253.9 4.6 55.7 56 1 1 712 22 49 00 22 50 30 =1939-053 00 16 55 15.3 254.1 4.6 55.8 90 F 1 724 22 49 01 22 50 30 IRAS1929 00 16 55 14.0 256.5 4.7 56.6 -4 1 1 724 No stop 22 54 00 --- 00 20 25 13.3 257.0 4.8 56.7 206 F 1 751 22 50 31 22 54 00 J1941-0511 00 20 25 14.6 254.6 4.6 56.0 -4 1 1 751 No stop 22 55 30 =1939-053 00 21 56 14.3 254.8 4.7 56.1 86 F 1 763 22 54 01 22 55 30 IRAS1929 00 21 56 13.0 257.2 4.8 56.8 -4 1 1 763 No stop 22 59 00 --- 00 25 26 12.2 257.7 4.9 57.0 206 F 1 790 22 55 31 22 59 00 J1941-0511 00 25 26 13.5 255.3 4.7 56.3 -4 1 1 790 No stop 23 00 30 =1939-053 00 26 56 13.2 255.5 4.7 56.4 86 F 1 801 22 59 01 23 00 30 IRAS1929 00 26 56 11.9 257.9 4.9 57.1 -4 1 1 801 No stop 23 04 00 --- 00 30 27 11.2 258.3 5.0 57.2 206 F 1 828 23 00 31 23 05 00 J1941-0511 00 31 27 12.3 256.2 4.8 56.6 56 1 1 828 23 05 00 23 06 30 =1939-053 00 32 57 12.0 256.4 4.8 56.7 90 F 1 840 23 05 01 23 06 30 IRAS1929 00 32 57 10.7 258.7 5.0 57.3 -4 1 1 840 No stop 23 10 00 --- 00 36 28 9.9 259.2 5.1 57.5 206 F 1 867 23 06 31 23 10 00 J1941-0511 00 36 28 11.3 256.9 4.9 56.9 -4 1 1 867 No stop 23 11 30 =1939-053 00 37 58 10.9 257.1 4.9 56.9 86 F 1 879 23 10 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 ---------------------------------------------------------------------------------------- --- Thu 11 Jun 2009 Day 162 --- 23 11 30 IRAS1929 00 37 58 9.6 259.4 5.1 57.5 -4 1 1 879 No stop 23 15 00 --- 00 41 29 8.9 259.9 5.1 57.7 206 F 1 906 23 11 31 23 15 00 J1941-0511 00 41 29 10.2 257.6 5.0 57.1 -4 1 1 906 No stop 23 16 30 =1939-053 00 42 59 9.9 257.8 5.0 57.2 86 F 1 917 23 15 01 23 16 30 IRAS1929 00 42 59 8.6 260.1 5.2 57.7 -4 1 1 917 No stop 23 20 00 --- 00 46 30 7.8 260.5 5.2 57.8 206 F 1 944 23 16 31 23 21 00 J1941-0511 00 47 30 8.9 258.4 5.1 57.4 56 1 1 944 23 21 00 23 22 30 =1939-053 00 49 00 8.6 258.6 5.1 57.4 90 F 1 956 23 21 01 23 22 30 IRAS1929 00 49 00 7.3 260.9 5.3 57.9 -4 1 1 956 No stop 23 26 00 --- 00 52 31 6.5 261.3 5.3 58.1 206 F 1 983 23 22 31 23 26 00 J1941-0511 00 52 31 7.9 259.1 5.2 57.6 -4 1 1 983 No stop 23 27 30 =1939-053 00 54 01 7.6 259.3 5.2 57.6 86 F 1 995 23 26 01 23 27 30 IRAS1929 00 54 01 6.2 261.5 5.4 58.1 -4 1 1 995 No stop 23 31 00 --- 00 57 31 5.5 262.0 5.4 58.2 206 F 1 1022 23 27 31 23 31 00 J1941-0511 00 57 31 6.8 259.7 5.3 57.8 -4 1 1 1022 No stop 23 32 30 =1939-053 00 59 02 6.5 259.9 5.3 57.8 86 F 1 1033 23 31 01 23 32 30 IRAS1929 00 59 02 5.2 262.2 5.4 58.3 -4 1 1 1033 No stop 23 36 00 --- 01 02 32 4.4 262.7 5.5 D 58.4 0 F 1 1061 23 32 31 23 37 00 J1941-0511 01 03 32 5.6 260.5 5.4 58.0 56 1 1 1061 23 37 00 23 38 30 =1939-053 01 05 03 5.3 260.7 5.4 58.1 90 F 1 1072 23 37 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: ep064g.6cm Matches group sh6cm in /Users/torres/home/soft/sched/catalogs/freq.dat Update freq. range AnTao 22Mar08 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= 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 4200.00 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= L L U U L L U U L L U U L L U U 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: 11 Setup file default. Used pcal sets: 1 LO sum= 4942.49 4942.49 4942.49 4942.49 4974.49 4974.49 4974.49 4974.49 5006.49 5006.49 5006.49 5006.49 5038.49 5038.49 5038.49 5038.49 BBC fr= 742.49 742.49 742.49 742.49 774.49 774.49 774.49 774.49 806.49 806.49 806.49 806.49 838.49 838.49 838.49 838.49 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 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 54.199199 0.00 -04 06 28.85412 *-04 00 01.06801 -03 58 49.04229 0.00 From catalog imbedded in main SCHED input file. 3.608 scan hours, 149.983 baseline hours above horizon. J1331+3030 13 28 49.657764 * 13 31 08.288056 13 31 36.198378 0.36 * 3C286 30 45 58.64058 * 30 30 32.95922 30 27 39.18384 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, 3.750 baseline hours above horizon. J1642+3948 16 41 17.606227 * 16 42 58.809964 16 43 20.290165 0.26 * 3C345 39 54 10.81495 * 39 48 36.99401 39 47 30.03792 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, 11.620 baseline hours above horizon. * J1941-0511 19 39 07.661036 * 19 41 47.008579 19 42 19.105386 0.41 1939-053 -05 18 37.74290 *-05 11 32.38284 -05 10 12.70351 0.87 /Users/torres/home/soft/sched/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 1.575 scan hours, 54.618 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 142.9 3C286 103.1 3C345 116.4 J1941-0511 141.6 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