COVER INFORMATION Station: SHANGHAI (Code Sh ) Experiment: Dominant heating mechanism in ULIRGs Exp. Code: EP064P 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 Third 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 ---------------------------------------------------------------------------------------- --- Sat 5 Jun 2010 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 21 36 00 3C345 22 37 36 20.3 -55.0 5.9 65.9 0 1 1 0 21 36 00 21 50 00 --- 22 51 38 17.9 -53.8 6.1 64.0 840 F 1 108 21 36 01 21 56 00 J1941-0511 22 57 39 31.0 241.0 3.3 48.7 63 1 1 108 21 56 00 21 57 30 =1939-053 22 59 09 30.7 241.3 3.3 48.9 90 F 1 120 21 56 01 21 57 30 IRAS1929 22 59 09 29.7 244.1 3.4 50.5 -5 1 1 120 No stop 22 01 00 --- 23 02 40 29.0 244.7 3.5 50.9 205 F 1 147 21 57 31 22 01 00 J1941-0511 23 02 40 30.1 241.9 3.3 49.3 -5 1 1 147 No stop 22 02 30 =1939-053 23 04 10 29.8 242.2 3.4 49.5 85 F 1 159 22 01 01 22 02 30 IRAS1929 23 04 10 28.7 245.0 3.5 51.1 -5 1 1 159 No stop 22 06 00 --- 23 07 41 28.0 245.6 3.6 51.4 205 F 1 186 22 02 31 22 06 00 J1941-0511 23 07 41 29.1 242.9 3.4 49.9 -5 1 1 186 No stop 22 07 30 =1939-053 23 09 11 28.8 243.1 3.4 50.1 85 F 1 197 22 06 01 22 07 30 IRAS1929 23 09 11 27.7 245.9 3.6 51.6 -5 1 1 197 No stop 22 11 00 --- 23 12 42 27.1 246.5 3.7 51.9 205 F 1 225 22 07 31 22 12 00 J1941-0511 23 13 42 28.0 244.0 3.5 50.6 55 1 1 225 22 12 00 22 13 30 =1939-053 23 15 12 27.7 244.2 3.5 50.7 90 F 1 236 22 12 01 22 13 30 IRAS1929 23 15 12 26.6 246.9 3.7 52.1 -5 1 1 236 No stop 22 17 00 --- 23 18 43 25.9 247.5 3.8 52.5 205 F 1 263 22 13 31 22 17 00 J1941-0511 23 18 43 27.0 244.8 3.6 51.1 -5 1 1 263 No stop 22 18 30 =1939-053 23 20 13 26.7 245.1 3.6 51.2 85 F 1 275 22 17 01 22 18 30 IRAS1929 23 20 13 25.6 247.8 3.8 52.6 -5 1 1 275 No stop 22 22 00 --- 23 23 43 24.9 248.3 3.8 52.9 205 F 1 302 22 18 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 ---------------------------------------------------------------------------------------- --- Sat 5 Jun 2010 Day 156 --- 22 22 00 J1941-0511 23 23 43 26.0 245.7 3.7 51.6 -5 1 1 302 No stop 22 23 30 =1939-053 23 25 14 25.7 246.0 3.7 51.7 85 F 1 314 22 22 01 22 23 30 IRAS1929 23 25 14 24.6 248.6 3.9 53.0 -5 1 1 314 No stop 22 27 00 --- 23 28 44 23.9 249.2 3.9 53.3 205 F 1 341 22 23 31 22 28 00 J1941-0511 23 29 44 24.8 246.7 3.8 52.2 56 1 1 341 22 28 00 22 29 30 =1939-053 23 31 15 24.5 247.0 3.8 52.3 90 F 1 352 22 28 01 22 29 30 IRAS1929 23 31 15 23.4 249.6 4.0 53.5 -5 1 1 352 No stop 22 33 00 --- 23 34 45 22.7 250.1 4.0 53.8 205 F 1 379 22 29 31 22 33 00 J1941-0511 23 34 45 23.8 247.6 3.9 52.6 -5 1 1 379 No stop 22 34 30 =1939-053 23 36 16 23.5 247.8 3.9 52.8 85 F 1 391 22 33 01 22 34 30 IRAS1929 23 36 16 22.4 250.4 4.1 53.9 -5 1 1 391 No stop 22 38 00 --- 23 39 46 21.7 250.9 4.1 54.2 205 F 1 418 22 34 31 22 38 00 J1941-0511 23 39 46 22.8 248.4 4.0 53.1 -5 1 1 418 No stop 22 39 30 =1939-053 23 41 16 22.5 248.6 4.0 53.2 85 F 1 430 22 38 01 22 39 30 IRAS1929 23 41 16 21.4 251.2 4.1 54.3 -5 1 1 430 No stop 22 43 00 --- 23 44 47 20.6 251.7 4.2 54.6 205 F 1 457 22 39 31 22 44 00 J1941-0511 23 45 47 21.6 249.4 4.1 53.6 56 1 1 457 22 44 00 22 45 30 =1939-053 23 47 17 21.3 249.6 4.1 53.7 90 F 1 468 22 44 01 22 45 30 IRAS1929 23 47 17 20.1 252.1 4.2 54.8 -4 1 1 468 No stop 22 49 00 --- 23 50 48 19.4 252.6 4.3 55.0 206 F 1 495 22 45 31 22 49 00 J1941-0511 23 50 48 20.6 250.1 4.1 54.0 -4 1 1 495 No stop 22 50 30 =1939-053 23 52 18 20.3 250.4 4.2 54.1 86 F 1 507 22 49 01 22 50 30 IRAS1929 23 52 18 19.1 252.9 4.3 55.1 -4 1 1 507 No stop 22 54 00 --- 23 55 49 18.4 253.4 4.4 55.3 206 F 1 534 22 50 31 22 54 00 J1941-0511 23 55 49 19.6 250.9 4.2 54.3 -4 1 1 534 No stop 22 55 30 =1939-053 23 57 19 19.3 251.2 4.2 54.5 86 F 1 546 22 54 01 22 55 30 IRAS1929 23 57 19 18.1 253.6 4.4 55.4 -4 1 1 546 No stop 22 59 00 --- 00 00 50 17.4 254.1 4.5 55.7 206 F 1 573 22 55 31 23 00 00 J1941-0511 00 01 50 18.4 251.8 4.3 54.8 56 1 1 573 23 00 00 23 01 30 =1939-053 00 03 20 18.1 252.1 4.3 54.9 90 F 1 584 23 00 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 ---------------------------------------------------------------------------------------- --- Sat 5 Jun 2010 Day 156 --- 23 01 30 IRAS1929 00 03 20 16.8 254.5 4.5 55.8 -4 1 1 584 No stop 23 05 00 --- 00 06 51 16.1 255.0 4.6 56.0 206 F 1 612 23 01 31 23 05 00 J1941-0511 00 06 51 17.4 252.6 4.4 55.1 -4 1 1 612 No stop 23 06 30 =1939-053 00 08 21 17.1 252.8 4.4 55.2 86 F 1 623 23 05 01 23 06 30 IRAS1929 00 08 21 15.8 255.2 4.6 56.1 -4 1 1 623 No stop 23 10 00 --- 00 11 51 15.1 255.7 4.6 56.3 206 F 1 650 23 06 31 23 10 00 J1941-0511 00 11 51 16.4 253.3 4.5 55.5 -4 1 1 650 No stop 23 11 30 =1939-053 00 13 22 16.0 253.6 4.5 55.6 86 F 1 662 23 10 01 23 11 30 IRAS1929 00 13 22 14.8 255.9 4.7 56.4 -4 1 1 662 No stop 23 15 00 --- 00 16 52 14.0 256.4 4.7 56.6 206 F 1 689 23 11 31 23 16 00 J1941-0511 00 17 52 15.1 254.2 4.6 55.8 56 1 1 689 23 16 00 23 17 30 =1939-053 00 19 23 14.8 254.4 4.6 55.9 90 F 1 701 23 16 01 23 17 30 IRAS1929 00 19 23 13.5 256.8 4.8 56.7 -4 1 1 701 No stop 23 21 00 --- 00 22 53 12.8 257.3 4.8 56.9 206 F 1 728 23 17 31 23 21 00 J1941-0511 00 22 53 14.1 254.9 4.7 56.1 -4 1 1 728 No stop 23 22 30 =1939-053 00 24 23 13.8 255.2 4.7 56.2 86 F 1 739 23 21 01 23 22 30 IRAS1929 00 24 23 12.5 257.5 4.9 56.9 -4 1 1 739 No stop 23 26 00 --- 00 27 54 11.7 258.0 4.9 57.1 206 F 1 766 23 22 31 23 26 00 J1941-0511 00 27 54 13.0 255.7 4.8 56.4 -4 1 1 766 No stop 23 27 30 =1939-053 00 29 24 12.7 255.9 4.8 56.5 86 F 1 778 23 26 01 23 27 30 IRAS1929 00 29 24 11.4 258.2 4.9 57.2 -4 1 1 778 No stop 23 31 00 --- 00 32 55 10.7 258.7 5.0 57.3 206 F 1 805 23 27 31 23 32 00 J1941-0511 00 33 55 11.8 256.5 4.9 56.7 56 1 1 805 23 32 00 23 33 30 =1939-053 00 35 25 11.5 256.7 4.9 56.8 90 F 1 817 23 32 01 23 33 30 IRAS1929 00 35 25 10.2 259.0 5.0 57.4 -4 1 1 817 No stop 23 37 00 --- 00 38 56 9.4 259.5 5.1 57.6 206 F 1 844 23 33 31 23 37 00 J1941-0511 00 38 56 10.8 257.2 4.9 57.0 -4 1 1 844 No stop 23 38 30 =1939-053 00 40 26 10.4 257.4 5.0 57.0 86 F 1 855 23 37 01 23 38 30 IRAS1929 00 40 26 9.1 259.7 5.1 57.6 -4 1 1 855 No stop 23 42 00 --- 00 43 57 8.4 260.2 5.2 57.8 206 F 1 883 23 38 31 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 ---------------------------------------------------------------------------------------- --- Sat 5 Jun 2010 Day 156 --- 23 42 00 J1941-0511 00 43 57 9.7 257.9 5.0 57.2 -4 1 1 883 No stop 23 43 30 =1939-053 00 45 27 9.4 258.1 5.1 57.3 86 F 1 894 23 42 01 23 43 30 IRAS1929 00 45 27 8.0 260.4 5.2 57.8 -4 1 1 894 No stop 23 47 00 --- 00 48 57 7.3 260.9 5.3 57.9 206 F 1 921 23 43 31 23 48 00 J1941-0511 00 49 58 8.4 258.7 5.1 57.5 56 1 1 921 23 48 00 23 49 30 =1939-053 00 51 28 8.1 258.9 5.2 57.5 90 F 1 933 23 48 01 23 49 30 IRAS1929 00 51 28 6.8 261.2 5.3 58.0 -4 1 1 933 No stop 23 53 00 --- 00 54 58 6.0 261.7 5.4 58.1 206 F 1 960 23 49 31 23 53 00 J1941-0511 00 54 58 7.4 259.4 5.2 57.7 -4 1 1 960 No stop 23 54 30 =1939-053 00 56 29 7.1 259.6 5.2 57.7 86 F 1 972 23 53 01 23 54 30 IRAS1929 00 56 29 5.7 261.8 5.4 58.2 -4 1 1 972 No stop 23 58 00 --- 00 59 59 5.0 262.3 5.5 D 58.3 0 F 1 999 23 54 31 23 58 00 J1941-0511 00 59 59 6.3 260.1 5.3 57.9 -4 1 1 999 No stop 23 59 30 =1939-053 01 01 30 6.0 260.3 5.3 57.9 86 F 1 1010 23 58 01 --- Sun 6 Jun 2010 Day 157 --- 00 04 00 J1941-0511 01 06 00 5.1 260.8 5.4 58.1 266 1 1 1010 00 04 00 00 05 30 =1939-053 01 07 30 4.7 261.0 5.4 D 58.1 0 F 1 1022 00 04 01 00 52 00 2134+004 01 54 08 22.3 256.7 4.3 56.4 2759 1 1 1022 00 52 00 00 58 00 --- 02 00 09 21.0 257.6 4.4 56.7 360 F 1 1068 00 52 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: ep064p.18cm Matches group sh18cm in /home/cristina/sched_8.1/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 -- 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 57.339224 0.00 -04 06 28.85412 *-04 00 01.06801 -03 58 39.31417 0.00 From catalog imbedded in main SCHED input file. 3.558 scan hours, 91.582 baseline hours above horizon. J1331+3030 13 28 49.657764 * 13 31 08.288056 13 31 39.051333 0.36 * 3C286 30 45 58.64058 * 30 30 32.95922 30 27 20.08008 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, 2.333 baseline hours above horizon. J1642+3948 16 41 17.606227 * 16 42 58.809964 16 43 22.325409 0.26 * 3C345 39 54 10.81495 * 39 48 36.99401 39 47 23.89729 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, 6.322 baseline hours above horizon. * J1941-0511 19 39 07.661036 * 19 41 47.008579 19 42 22.263014 0.41 1939-053 -05 18 37.74290 *-05 11 32.38284 -05 10 02.22529 0.87 /home/cristina/sched_8.1/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 1.550 scan hours, 32.241 baseline hours above horizon. J2136+0041 21 34 05.207389 * 21 36 38.586324 21 37 12.012392 0.30 2134+00 00 28 25.08002 * 00 41 54.21285 00 44 45.49850 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, 3.081 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 137.7 3C286 107.8 3C345 117.5 J1941-0511 136.2 2134+004 107.8 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