COVER INFORMATION Station: SHANGHAI (Code Sh ) Experiment: Dominant heating mechanism in ULIRGs Exp. Code: EP064C Schedule Version: 1.00 Processed by SCHED version: 6.05 June 2006 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 07251-0248 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 ---------------------------------------------------------------------------------------- --- Fri 6 Mar 2009 Day 65 --- 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 15 30 00 J0730-0241 10 32 47 35.1 240.5 3.0 48.3 0 1 1 0 15 30 00 15 31 20 =0727-025 10 34 07 34.9 240.8 3.1 48.4 80 F 1 10 15 30 01 15 31 20 IRAS0725 10 34 07 34.2 241.2 3.1 48.7 -3 1 1 10 15 31 20 15 35 00 --- 10 37 47 33.5 241.9 3.2 49.1 217 F 1 39 15 31 21 15 35 00 J0730-0241 10 37 47 34.2 241.5 3.1 48.9 -3 1 1 39 15 35 00 15 36 20 =0727-025 10 39 08 33.9 241.8 3.1 49.1 77 F 1 49 15 35 01 15 36 20 IRAS0725 10 39 08 33.3 242.1 3.2 49.3 -3 1 1 49 15 36 20 15 40 00 --- 10 42 48 32.6 242.9 3.2 49.7 217 F 1 77 15 36 21 15 40 00 J0730-0241 10 42 48 33.2 242.5 3.2 49.5 -3 1 1 77 15 40 00 15 41 20 =0727-025 10 44 08 33.0 242.8 3.2 49.7 77 F 1 88 15 40 01 15 41 20 IRAS0725 10 44 08 32.3 243.1 3.3 49.9 -3 1 1 88 15 41 20 15 45 00 --- 10 47 49 31.6 243.8 3.3 50.3 217 F 1 116 15 41 21 15 46 00 J0730-0241 10 48 49 32.1 243.7 3.3 50.2 57 1 1 116 15 46 00 15 47 20 =0727-025 10 50 09 31.8 243.9 3.3 50.4 80 F 1 126 15 46 01 15 47 20 IRAS0725 10 50 09 31.2 244.2 3.4 50.6 -3 1 1 126 15 47 20 15 51 00 --- 10 53 50 30.4 244.9 3.4 50.9 217 F 1 155 15 47 21 15 51 00 J0730-0241 10 53 50 31.1 244.6 3.4 50.8 -3 1 1 155 15 51 00 15 52 20 =0727-025 10 55 10 30.9 244.9 3.4 50.9 77 F 1 165 15 51 01 15 52 20 IRAS0725 10 55 10 30.2 245.2 3.5 51.1 -3 1 1 165 15 52 20 15 56 00 --- 10 58 51 29.5 245.8 3.5 51.5 217 F 1 194 15 52 21 15 56 00 J0730-0241 10 58 51 30.2 245.5 3.5 51.3 -3 1 1 194 15 56 00 15 57 20 =0727-025 11 00 11 29.9 245.8 3.5 51.4 77 F 1 204 15 56 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 ---------------------------------------------------------------------------------------- --- Fri 6 Mar 2009 Day 65 --- 15 57 20 IRAS0725 11 00 11 29.2 246.1 3.5 51.6 -3 1 1 204 15 57 20 16 01 00 --- 11 03 52 28.5 246.7 3.6 52.0 217 F 1 232 15 57 21 16 02 00 J0730-0241 11 04 52 29.0 246.6 3.6 51.9 57 1 1 232 16 02 00 16 03 20 =0727-025 11 06 12 28.7 246.8 3.6 52.0 80 F 1 243 16 02 01 16 03 20 IRAS0725 11 06 12 28.0 247.1 3.6 52.2 -3 1 1 243 16 03 20 16 07 00 --- 11 09 53 27.3 247.8 3.7 52.5 217 F 1 271 16 03 21 16 07 00 J0730-0241 11 09 53 28.0 247.5 3.6 52.4 -3 1 1 271 16 07 00 16 08 20 =0727-025 11 11 13 27.7 247.7 3.7 52.5 77 F 1 281 16 07 01 16 08 20 IRAS0725 11 11 13 27.0 248.0 3.7 52.6 -3 1 1 281 16 08 20 16 12 00 --- 11 14 53 26.3 248.6 3.8 53.0 217 F 1 310 16 08 21 16 12 00 J0730-0241 11 14 53 27.0 248.3 3.7 52.8 -3 1 1 310 16 12 00 16 13 20 =0727-025 11 16 14 26.7 248.6 3.8 52.9 77 F 1 320 16 12 01 16 13 20 IRAS0725 11 16 14 26.0 248.8 3.8 53.1 -3 1 1 320 16 13 20 16 17 00 --- 11 19 54 25.3 249.4 3.9 53.4 217 F 1 348 16 13 21 16 18 00 J0730-0241 11 20 54 25.8 249.3 3.8 53.3 57 1 1 348 16 18 00 16 19 20 =0727-025 11 22 15 25.5 249.6 3.9 53.4 80 F 1 359 16 18 01 16 19 20 IRAS0725 11 22 15 24.8 249.8 3.9 53.6 -3 1 1 359 16 19 20 16 23 00 --- 11 25 55 24.1 250.4 4.0 53.9 217 F 1 387 16 19 21 16 23 00 J0730-0241 11 25 55 24.8 250.2 3.9 53.7 -3 1 1 387 16 23 00 16 24 20 =0727-025 11 27 15 24.5 250.4 3.9 53.8 77 F 1 397 16 23 01 16 24 20 IRAS0725 11 27 15 23.8 250.6 4.0 54.0 -3 1 1 397 16 24 20 16 28 00 --- 11 30 56 23.1 251.2 4.0 54.3 217 F 1 426 16 24 21 16 28 00 J0730-0241 11 30 56 23.8 251.0 4.0 54.1 -3 1 1 426 16 28 00 16 29 20 =0727-025 11 32 16 23.5 251.2 4.0 54.2 77 F 1 436 16 28 01 16 29 20 IRAS0725 11 32 16 22.8 251.4 4.1 54.4 -3 1 1 436 16 29 20 16 33 00 --- 11 35 57 22.1 252.0 4.1 54.6 217 F 1 464 16 29 21 16 34 00 J0730-0241 11 36 57 22.6 251.9 4.1 54.6 57 1 1 464 16 34 00 16 35 20 =0727-025 11 38 17 22.3 252.1 4.1 54.7 80 F 1 475 16 34 01 16 35 20 IRAS0725 11 38 17 21.6 252.4 4.2 54.8 -3 1 1 475 16 35 20 16 39 00 --- 11 41 58 20.8 252.9 4.2 55.0 217 F 1 503 16 35 21 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 ---------------------------------------------------------------------------------------- --- Fri 6 Mar 2009 Day 65 --- 16 39 00 J0730-0241 11 41 58 21.5 252.7 4.2 54.9 -3 1 1 503 16 39 00 16 40 20 =0727-025 11 43 18 21.3 252.9 4.2 55.0 77 F 1 514 16 39 01 16 40 20 IRAS0725 11 43 18 20.6 253.1 4.3 55.1 -3 1 1 514 16 40 20 16 44 00 --- 11 46 59 19.8 253.7 4.3 55.4 217 F 1 542 16 40 21 16 44 00 J0730-0241 11 46 59 20.5 253.5 4.3 55.3 -3 1 1 542 16 44 00 16 45 20 =0727-025 11 48 19 20.2 253.7 4.3 55.4 77 F 1 552 16 44 01 16 45 20 IRAS0725 11 48 19 19.5 253.9 4.3 55.5 -3 1 1 552 16 45 20 16 49 00 --- 11 52 00 18.8 254.4 4.4 55.7 217 F 1 581 16 45 21 16 50 00 J0730-0241 11 53 00 19.3 254.4 4.4 55.6 57 1 1 581 16 50 00 16 51 20 =0727-025 11 54 20 19.0 254.6 4.4 55.7 80 F 1 591 16 50 01 16 51 20 IRAS0725 11 54 20 18.3 254.8 4.4 55.8 -3 1 1 591 16 51 20 16 55 00 --- 11 58 01 17.5 255.3 4.5 56.0 217 F 1 619 16 51 21 16 55 00 J0730-0241 11 58 01 18.2 255.1 4.5 55.9 -3 1 1 619 16 55 00 16 56 20 =0727-025 11 59 21 18.0 255.3 4.5 56.0 77 F 1 630 16 55 01 16 56 20 IRAS0725 11 59 21 17.3 255.5 4.5 56.1 -3 1 1 630 16 56 20 17 00 00 --- 12 03 01 16.5 256.1 4.6 56.3 217 F 1 658 16 56 21 17 00 00 J0730-0241 12 03 01 17.2 255.8 4.5 56.2 -3 1 1 658 17 00 00 17 01 20 =0727-025 12 04 22 16.9 256.0 4.6 56.3 77 F 1 668 17 00 01 17 01 20 IRAS0725 12 04 22 16.2 256.3 4.6 56.4 -3 1 1 668 17 01 20 17 05 00 --- 12 08 02 15.4 256.8 4.7 56.6 217 F 1 697 17 01 21 17 06 00 J0730-0241 12 09 02 15.9 256.7 4.6 56.5 57 1 1 697 17 06 00 17 07 20 =0727-025 12 10 23 15.7 256.9 4.7 56.6 80 F 1 707 17 06 01 17 07 20 IRAS0725 12 10 23 15.0 257.1 4.7 56.7 -3 1 1 707 17 07 20 17 11 00 --- 12 14 03 14.2 257.6 4.8 56.9 217 F 1 735 17 07 21 17 11 00 J0730-0241 12 14 03 14.9 257.4 4.7 56.8 -3 1 1 735 17 11 00 17 12 20 =0727-025 12 15 23 14.6 257.6 4.7 56.9 77 F 1 746 17 11 01 17 12 20 IRAS0725 12 15 23 13.9 257.8 4.8 56.9 -3 1 1 746 17 12 20 17 16 00 --- 12 19 04 13.1 258.3 4.8 57.1 217 F 1 774 17 12 21 17 16 00 J0730-0241 12 19 04 13.8 258.1 4.8 57.0 -3 1 1 774 17 16 00 17 17 20 =0727-025 12 20 24 13.6 258.3 4.8 57.1 77 F 1 784 17 16 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 6 Mar 2009 Day 65 --- 17 17 20 IRAS0725 12 20 24 12.9 258.5 4.9 57.2 -3 1 1 784 17 17 20 17 21 00 --- 12 24 05 12.1 259.0 4.9 57.3 217 F 1 813 17 17 21 17 22 00 J0730-0241 12 25 05 12.6 259.0 4.9 57.3 57 1 1 813 17 22 00 17 23 20 =0727-025 12 26 25 12.3 259.2 4.9 57.3 80 F 1 823 17 22 01 17 23 20 IRAS0725 12 26 25 11.6 259.3 5.0 57.4 -3 1 1 823 17 23 20 17 27 00 --- 12 30 06 10.8 259.9 5.0 57.6 217 F 1 852 17 23 21 17 27 00 J0730-0241 12 30 06 11.5 259.7 5.0 57.5 -3 1 1 852 17 27 00 17 28 20 =0727-025 12 31 26 11.2 259.8 5.0 57.5 77 F 1 862 17 27 01 17 28 20 IRAS0725 12 31 26 10.5 260.0 5.1 57.6 -3 1 1 862 17 28 20 17 32 00 --- 12 35 07 9.8 260.5 5.1 57.7 217 F 1 890 17 28 21 17 32 00 J0730-0241 12 35 07 10.5 260.3 5.1 57.7 -3 1 1 890 17 32 00 17 33 20 =0727-025 12 36 27 10.2 260.5 5.1 57.7 77 F 1 901 17 32 01 17 33 20 IRAS0725 12 36 27 9.5 260.7 5.1 57.8 -3 1 1 901 17 33 20 17 37 00 --- 12 40 07 8.7 261.2 5.2 57.9 217 F 1 929 17 33 21 17 38 00 J0854+2006 12 41 08 38.5 271.9 3.8 65.7 8 1 1 929 17 38 00 17 43 30 =0851+202 12 46 38 37.3 272.6 3.9 65.6 330 F 1 972 17 38 01 17 43 30 J0730-0241 12 46 38 8.0 261.9 5.3 58.1 -51 1 1 972 17 43 30 17 44 50 =0727-025 12 47 59 7.8 262.1 5.3 58.1 29 F 1 982 17 43 31 17 44 50 IRAS0725 12 47 59 7.0 262.3 5.3 58.2 -3 1 1 982 17 44 50 17 48 30 --- 12 51 39 6.3 262.7 5.4 58.3 217 F 1 1010 17 44 51 17 48 30 J0730-0241 12 51 39 7.0 262.6 5.3 58.2 -3 1 1 1010 17 48 30 17 49 50 =0727-025 12 53 00 6.7 262.7 5.4 58.3 77 F 1 1021 17 48 31 17 49 50 IRAS0725 12 53 00 6.0 262.9 5.4 58.3 -3 1 1 1021 17 49 50 17 53 30 --- 12 56 40 5.2 263.4 5.5 58.4 217 F 1 1049 17 49 51 17 54 30 J0730-0241 12 57 40 5.7 263.4 5.4 58.4 57 1 1 1049 17 54 30 17 55 50 =0727-025 12 59 01 5.4 263.5 5.5 58.4 80 F 1 1059 17 54 31 18 22 50 4C39.25 13 26 05 41.4 296.6 4.0 80.1 1558 1 1 1059 18 22 50 18 28 20 --- 13 31 36 40.4 296.9 4.1 79.4 330 F 1 1102 18 22 51 21 24 30 3C286 16 28 15 52.3 280.8 2.9 77.4 10548 1 1 1102 21 24 30 21 30 00 --- 16 33 46 51.2 281.2 3.0 77.0 330 F 1 1144 21 24 31 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: ep064c.18cm Matches group sh18cm in /usr/local/sched.MacOSX.6.05/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) * IRAS0725 07 25 06.977760 * 07 27 37.613044 07 28 06.889243 0.00 -02 48 45.42650 *-02 54 54.19322 -02 56 08.23741 0.00 From catalog imbedded in main SCHED input file. 3.936 scan hours, 155.388 baseline hours above horizon. * J0730-0241 07 27 54.982196 * 07 30 25.877606 07 30 55.215086 0.28 0727-025 -02 35 04.77199 *-02 41 24.90406 -02 42 41.05965 0.53 /usr/local/sched.MacOSX.6.05/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 1.422 scan hours, 46.149 baseline hours above horizon. * J0854+2006 08 51 57.250618 * 08 54 48.874930 08 55 22.586142 0.21 0851+202 20 17 58.41741 * 20 06 30.64086 20 04 19.63107 0.40 J0854+20 /usr/local/sched.MacOSX.6.05/catalogs/sources.vlba OJ287 VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.092 scan hours, 3.543 baseline hours above horizon. J0927+3902 09 23 55.319213 * 09 27 03.013934 09 27 40.217032 0.26 0923+392 39 15 23.56648 * 39 02 20.85188 38 59 53.81483 0.40 * 4C39.25 /usr/local/sched.MacOSX.6.05/catalogs/sources.vlba J0927+39 VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.092 scan hours, 2.862 baseline hours above horizon. J1331+3030 13 28 49.657756 * 13 31 08.288048 13 31 35.867364 0.37 1328+307 30 45 58.64060 * 30 30 32.95924 30 27 22.90732 0.47 * 3C286 /usr/local/sched.MacOSX.6.05/catalogs/sources.vlba J1331+30 VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.092 scan hours, 0.819 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) IRAS0725 124.1 J0730-0241 124.8 J0854+2006 144.2 4C39.25 139.2 3C286 138.3 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