COVER INFORMATION Station: SHANGHAI (Code Sh ) Experiment: Dominant heating mechanism in ULIRGs Exp. Code: EP064M Schedule Version: 1.00 Processed by SCHED version: 8.10 Bug fixs and minor enhancements PI: Miguel A. Perez-Torres Address: IAA - CSIC Glorieta de la Astronomia s/n 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 Fourth 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 27 May 2010 Day 147 --- 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 22 06 00 3C345 22 32 12 21.3 -55.4 5.8 66.6 0 1 1 0 22 06 00 22 20 00 --- 22 46 14 18.8 -54.3 6.0 64.8 840 F 1 108 22 06 01 22 26 00 J1941-0511 22 52 15 32.0 239.9 3.2 48.1 64 1 1 108 22 26 00 22 27 30 =1939-053 22 53 45 31.7 240.2 3.2 48.3 90 F 1 120 22 26 01 22 27 30 IRAS1929 22 53 45 30.7 243.1 3.3 49.9 -5 1 1 120 No stop 22 31 00 --- 22 57 16 30.1 243.7 3.4 50.3 205 F 1 147 22 27 31 22 31 00 J1941-0511 22 57 16 31.1 240.9 3.2 48.7 -5 1 1 147 No stop 22 32 30 =1939-053 22 58 46 30.8 241.2 3.3 48.9 85 F 1 159 22 31 01 22 32 30 IRAS1929 22 58 46 29.8 244.0 3.4 50.5 -5 1 1 159 No stop 22 36 00 --- 23 02 17 29.1 244.6 3.5 50.9 205 F 1 186 22 32 31 22 36 00 J1941-0511 23 02 17 30.1 241.9 3.3 49.3 -5 1 1 186 No stop 22 37 30 =1939-053 23 03 47 29.8 242.1 3.4 49.5 85 F 1 197 22 36 01 22 37 30 IRAS1929 23 03 47 28.8 244.9 3.5 51.0 -5 1 1 197 No stop 22 41 00 --- 23 07 18 28.1 245.5 3.6 51.4 205 F 1 225 22 37 31 22 42 00 J1941-0511 23 08 18 29.0 243.0 3.4 50.0 55 1 1 225 22 42 00 22 43 30 =1939-053 23 09 48 28.7 243.2 3.5 50.2 90 F 1 236 22 42 01 22 43 30 IRAS1929 23 09 48 27.6 246.0 3.6 51.6 -5 1 1 236 No stop 22 47 00 --- 23 13 19 26.9 246.6 3.7 52.0 205 F 1 263 22 43 31 22 47 00 J1941-0511 23 13 19 28.0 243.9 3.5 50.5 -5 1 1 263 No stop 22 48 30 =1939-053 23 14 49 27.7 244.2 3.5 50.7 85 F 1 275 22 47 01 22 48 30 IRAS1929 23 14 49 26.6 246.8 3.7 52.1 -5 1 1 275 No stop 22 52 00 --- 23 18 19 26.0 247.4 3.8 52.4 205 F 1 302 22 48 31 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 27 May 2010 Day 147 --- 22 52 00 J1941-0511 23 18 19 27.1 244.8 3.6 51.1 -5 1 1 302 No stop 22 53 30 =1939-053 23 19 50 26.8 245.0 3.6 51.2 85 F 1 314 22 52 01 22 53 30 IRAS1929 23 19 50 25.7 247.7 3.8 52.6 -5 1 1 314 No stop 22 57 00 --- 23 23 20 25.0 248.3 3.8 52.9 205 F 1 341 22 53 31 22 58 00 J1941-0511 23 24 20 25.9 245.8 3.7 51.7 56 1 1 341 22 58 00 22 59 30 =1939-053 23 25 51 25.6 246.1 3.7 51.8 90 F 1 352 22 58 01 22 59 30 IRAS1929 23 25 51 24.5 248.7 3.9 53.1 -5 1 1 352 No stop 23 03 00 --- 23 29 21 23.8 249.3 3.9 53.4 205 F 1 379 22 59 31 23 03 00 J1941-0511 23 29 21 24.9 246.7 3.8 52.1 -5 1 1 379 No stop 23 04 30 =1939-053 23 30 51 24.6 246.9 3.8 52.3 85 F 1 391 23 03 01 23 04 30 IRAS1929 23 30 51 23.5 249.5 4.0 53.5 -5 1 1 391 No stop 23 08 00 --- 23 34 22 22.7 250.1 4.0 53.8 205 F 1 418 23 04 31 23 08 00 J1941-0511 23 34 22 23.9 247.5 3.9 52.6 -5 1 1 418 No stop 23 09 30 =1939-053 23 35 52 23.6 247.8 3.9 52.7 85 F 1 430 23 08 01 23 09 30 IRAS1929 23 35 52 22.4 250.3 4.0 53.9 -5 1 1 430 No stop 23 13 00 --- 23 39 23 21.7 250.9 4.1 54.2 205 F 1 457 23 09 31 23 14 00 J1941-0511 23 40 23 22.7 248.5 4.0 53.1 56 1 1 457 23 14 00 23 15 30 =1939-053 23 41 53 22.4 248.7 4.0 53.2 90 F 1 468 23 14 01 23 15 30 IRAS1929 23 41 53 21.2 251.3 4.1 54.4 -5 1 1 468 No stop 23 19 00 --- 23 45 24 20.5 251.8 4.2 54.6 205 F 1 495 23 15 31 23 19 00 J1941-0511 23 45 24 21.7 249.3 4.1 53.5 -5 1 1 495 No stop 23 20 30 =1939-053 23 46 54 21.4 249.5 4.1 53.7 85 F 1 507 23 19 01 23 20 30 IRAS1929 23 46 54 20.2 252.0 4.2 54.7 -5 1 1 507 No stop 23 24 00 --- 23 50 25 19.5 252.6 4.3 55.0 205 F 1 534 23 20 31 23 24 00 J1941-0511 23 50 25 20.7 250.1 4.1 53.9 -4 1 1 534 No stop 23 25 30 =1939-053 23 51 55 20.4 250.3 4.2 54.1 86 F 1 546 23 24 01 23 25 30 IRAS1929 23 51 55 19.2 252.8 4.3 55.1 -4 1 1 546 No stop 23 29 00 --- 23 55 25 18.5 253.3 4.4 55.3 206 F 1 573 23 25 31 23 30 00 J1941-0511 23 56 26 19.5 251.0 4.2 54.4 56 1 1 573 23 30 00 23 31 30 =1939-053 23 57 56 19.2 251.3 4.3 54.5 90 F 1 584 23 30 01 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 27 May 2010 Day 147 --- 23 31 30 IRAS1929 23 57 56 18.0 253.7 4.4 55.5 -4 1 1 584 No stop 23 35 00 --- 00 01 26 17.2 254.2 4.5 55.7 206 F 1 612 23 31 31 23 35 00 J1941-0511 00 01 26 18.5 251.8 4.3 54.8 -4 1 1 612 No stop 23 36 30 =1939-053 00 02 57 18.2 252.0 4.3 54.9 86 F 1 623 23 35 01 23 36 30 IRAS1929 00 02 57 16.9 254.4 4.5 55.8 -4 1 1 623 No stop 23 40 00 --- 00 06 27 16.2 255.0 4.6 56.0 206 F 1 650 23 36 31 23 40 00 J1941-0511 00 06 27 17.5 252.5 4.4 55.1 -4 1 1 650 No stop 23 41 30 =1939-053 00 07 58 17.2 252.8 4.4 55.2 86 F 1 662 23 40 01 23 41 30 IRAS1929 00 07 58 15.9 255.2 4.6 56.1 -4 1 1 662 No stop 23 45 00 --- 00 11 28 15.2 255.7 4.6 56.3 206 F 1 689 23 41 31 23 46 00 J1941-0511 00 12 28 16.2 253.4 4.5 55.5 56 1 1 689 23 46 00 23 47 30 =1939-053 00 13 59 15.9 253.7 4.5 55.6 90 F 1 701 23 46 01 23 47 30 IRAS1929 00 13 59 14.6 256.0 4.7 56.4 -4 1 1 701 No stop 23 51 00 --- 00 17 29 13.9 256.5 4.7 56.6 206 F 1 728 23 47 31 23 51 00 J1941-0511 00 17 29 15.2 254.2 4.6 55.8 -4 1 1 728 No stop 23 52 30 =1939-053 00 18 59 14.9 254.4 4.6 55.9 86 F 1 739 23 51 01 23 52 30 IRAS1929 00 18 59 13.6 256.7 4.8 56.7 -4 1 1 739 No stop 23 56 00 --- 00 22 30 12.9 257.2 4.8 56.8 206 F 1 766 23 52 31 23 56 00 J1941-0511 00 22 30 14.2 254.9 4.7 56.1 -4 1 1 766 No stop 23 57 30 =1939-053 00 24 00 13.9 255.1 4.7 56.2 86 F 1 778 23 56 01 --- Start: Thu 27 May 2010 Day 147 -- Stop: Fri 28 May 2010 Day 148 --- 23 57 30 IRAS1929 00 24 00 12.6 257.5 4.9 56.9 -4 1 1 778 No stop 00 01 00 --- 00 27 31 11.8 257.9 4.9 57.1 206 F 1 805 23 57 31 00 02 00 J1941-0511 00 28 31 12.9 255.7 4.8 56.4 56 1 1 805 00 02 00 00 03 30 =1939-053 00 30 01 12.6 256.0 4.8 56.5 90 F 1 817 00 02 01 00 03 30 IRAS1929 00 30 01 11.3 258.3 5.0 57.2 -4 1 1 817 No stop 00 07 00 --- 00 33 32 10.6 258.8 5.0 57.3 206 F 1 844 00 03 31 00 07 00 J1941-0511 00 33 32 11.9 256.4 4.9 56.7 -4 1 1 844 No stop 00 08 30 =1939-053 00 35 02 11.6 256.7 4.9 56.8 86 F 1 855 00 07 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 ---------------------------------------------------------------------------------------- --- Fri 28 May 2010 Day 148 --- 00 08 30 IRAS1929 00 35 02 10.2 259.0 5.0 57.4 -4 1 1 855 No stop 00 12 00 --- 00 38 33 9.5 259.4 5.1 57.5 206 F 1 883 00 08 31 00 12 00 J1941-0511 00 38 33 10.8 257.1 4.9 57.0 -4 1 1 883 No stop 00 13 30 =1939-053 00 40 03 10.5 257.4 5.0 57.0 86 F 1 894 00 12 01 00 13 30 IRAS1929 00 40 03 9.2 259.7 5.1 57.6 -4 1 1 894 No stop 00 17 00 --- 00 43 33 8.4 260.1 5.2 57.7 206 F 1 921 00 13 31 00 18 00 J1941-0511 00 44 34 9.6 258.0 5.0 57.2 56 1 1 921 00 18 00 00 19 30 =1939-053 00 46 04 9.3 258.2 5.1 57.3 90 F 1 933 00 18 01 00 19 30 IRAS1929 00 46 04 7.9 260.5 5.2 57.8 -4 1 1 933 No stop 00 23 00 --- 00 49 34 7.2 260.9 5.3 58.0 206 F 1 960 00 19 31 00 23 00 J1941-0511 00 49 34 8.5 258.7 5.1 57.5 -4 1 1 960 No stop 00 24 30 =1939-053 00 51 05 8.2 258.9 5.1 57.5 86 F 1 972 00 23 01 00 24 30 IRAS1929 00 51 05 6.9 261.1 5.3 58.0 -4 1 1 972 No stop 00 28 00 --- 00 54 35 6.1 261.6 5.4 58.1 206 F 1 999 00 24 31 00 28 00 J1941-0511 00 54 35 7.5 259.3 5.2 57.7 -4 1 1 999 No stop 00 29 30 =1939-053 00 56 05 7.2 259.5 5.2 57.7 86 F 1 1010 00 28 01 00 29 30 IRAS1929 00 56 05 5.8 261.8 5.4 58.2 -4 1 1 1010 No stop 00 33 00 --- 00 59 36 5.1 262.3 5.4 58.3 206 F 1 1037 00 29 31 00 34 00 J1941-0511 01 00 36 6.2 260.1 5.3 57.9 56 1 1 1037 00 34 00 00 35 30 =1939-053 01 02 06 5.9 260.3 5.3 57.9 90 F 1 1049 00 34 01 00 39 00 J1941-0511 01 05 37 5.1 260.8 5.4 58.1 207 1 1 1049 00 39 00 00 40 30 =1939-053 01 07 07 4.8 261.0 5.4 D 58.1 0 F 1 1061 00 39 01 01 22 00 2134+004 01 48 44 23.4 255.9 4.2 56.1 2457 1 1 1061 01 22 00 01 28 00 --- 01 54 45 22.1 256.8 4.3 56.5 360 F 1 1107 01 22 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: ep064m.6cm Matches group sh6cm in /home/cristina/sched_8.1/catalogs/freq.dat Update freq. range AnTao 22Mar08 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= 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: 10 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 57.105382 0.00 -04 06 28.85412 *-04 00 01.06801 -03 58 40.56700 0.00 From catalog imbedded in main SCHED input file. 3.558 scan hours, 118.729 baseline hours above horizon. J1331+3030 13 28 49.657764 * 13 31 08.288056 13 31 39.120637 0.36 * 3C286 30 45 58.64058 * 30 30 32.95922 30 27 18.68335 0.47 1328+307 /home/cristina/sched_8.1/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 22.252446 0.26 * 3C345 39 54 10.81495 * 39 48 36.99401 39 47 21.41304 0.40 1641+399 /home/cristina/sched_8.1/catalogs/sources.vlba J1642+39 VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 0.233 scan hours, 8.028 baseline hours above horizon. * J1941-0511 19 39 07.661036 * 19 41 47.008579 19 42 22.022701 0.41 1939-053 -05 18 37.74290 *-05 11 32.38284 -05 10 03.46571 0.87 /home/cristina/sched_8.1/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 1.550 scan hours, 42.225 baseline hours above horizon. J2136+0041 21 34 05.207389 * 21 36 38.586324 21 37 11.730819 0.30 2134+00 00 28 25.08002 * 00 41 54.21285 00 44 43.82148 0.20 * 2134+004 /home/cristina/sched_8.1/catalogs/sources.vlba J2136+00 VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 0.100 scan hours, 3.901 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 129.9 3C286 114.4 3C345 118.5 J1941-0511 128.2 2134+004 99.5 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