COVER INFORMATION Station: SHANGHAI (Code Sh ) Experiment: Dominant heating mechanism in ULIRGs Exp. Code: EP064I 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 07251-0248 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 6 Mar 2010 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 31 49 35.3 240.3 3.0 48.1 0 1 1 0 15 30 00 15 31 20 =0727-025 10 33 09 35.1 240.6 3.0 48.3 80 F 1 10 15 30 01 15 31 20 IRAS0725 10 33 09 34.4 241.0 3.1 48.6 -3 1 1 10 No stop 15 35 10 --- 10 37 00 33.7 241.7 3.1 49.0 227 F 1 40 15 31 21 15 35 10 J0730-0241 10 37 00 34.3 241.4 3.1 48.8 -3 1 1 40 No stop 15 36 30 =0727-025 10 38 20 34.1 241.6 3.1 49.0 77 F 1 50 15 35 11 15 36 30 IRAS0725 10 38 20 33.4 242.0 3.2 49.2 -3 1 1 50 No stop 15 40 20 --- 10 42 11 32.7 242.7 3.2 49.6 227 F 1 80 15 36 31 15 40 20 J0730-0241 10 42 11 33.4 242.4 3.2 49.4 -3 1 1 80 No stop 15 41 40 =0727-025 10 43 31 33.1 242.6 3.2 49.6 77 F 1 90 15 40 21 15 41 40 IRAS0725 10 43 31 32.4 243.0 3.3 49.8 -3 1 1 90 No stop 15 45 30 --- 10 47 22 31.7 243.7 3.3 50.2 227 F 1 120 15 41 41 15 46 30 J0730-0241 10 48 22 32.2 243.6 3.3 50.1 57 1 1 120 15 46 30 15 47 50 =0727-025 10 49 42 31.9 243.8 3.3 50.3 80 F 1 130 15 46 31 15 47 50 IRAS0725 10 49 42 31.3 244.1 3.4 50.5 -3 1 1 130 No stop 15 51 40 --- 10 53 33 30.5 244.9 3.4 50.9 227 F 1 160 15 47 51 15 51 40 J0730-0241 10 53 33 31.2 244.5 3.4 50.7 -3 1 1 160 No stop 15 53 00 =0727-025 10 54 53 30.9 244.8 3.4 50.9 77 F 1 170 15 51 41 15 53 00 IRAS0725 10 54 53 30.2 245.1 3.4 51.0 -3 1 1 170 No stop 15 56 50 --- 10 58 44 29.5 245.8 3.5 51.4 227 F 1 200 15 53 01 15 56 50 J0730-0241 10 58 44 30.2 245.5 3.5 51.3 -3 1 1 200 No stop 15 58 10 =0727-025 11 00 04 29.9 245.7 3.5 51.4 77 F 1 210 15 56 51 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 6 Mar 2010 Day 65 --- 15 58 10 IRAS0725 11 00 04 29.2 246.0 3.5 51.6 -3 1 1 210 No stop 16 02 00 --- 11 03 55 28.5 246.7 3.6 52.0 227 F 1 240 15 58 11 16 03 00 J0730-0241 11 04 55 29.0 246.6 3.6 51.9 57 1 1 240 16 03 00 16 04 20 =0727-025 11 06 15 28.7 246.8 3.6 52.0 80 F 1 250 16 03 01 16 04 20 IRAS0725 11 06 15 28.0 247.1 3.6 52.2 -3 1 1 250 No stop 16 08 10 --- 11 10 06 27.3 247.8 3.7 52.5 227 F 1 280 16 04 21 16 08 10 J0730-0241 11 10 06 28.0 247.5 3.7 52.4 -3 1 1 280 No stop 16 09 30 =0727-025 11 11 26 27.7 247.7 3.7 52.5 77 F 1 290 16 08 11 16 09 30 IRAS0725 11 11 26 27.0 248.0 3.7 52.7 -3 1 1 290 No stop 16 13 20 --- 11 15 16 26.2 248.7 3.8 53.0 227 F 1 320 16 09 31 16 13 20 J0730-0241 11 15 16 26.9 248.4 3.7 52.8 -3 1 1 320 No stop 16 14 40 =0727-025 11 16 37 26.7 248.6 3.8 53.0 77 F 1 330 16 13 21 16 14 40 IRAS0725 11 16 37 26.0 248.9 3.8 53.1 -3 1 1 330 No stop 16 18 30 --- 11 20 27 25.2 249.5 3.9 53.4 227 F 1 360 16 14 41 16 19 30 J0730-0241 11 21 27 25.7 249.4 3.8 53.4 57 1 1 360 16 19 30 16 20 50 =0727-025 11 22 48 25.4 249.6 3.9 53.5 80 F 1 370 16 19 31 16 20 50 IRAS0725 11 22 48 24.7 249.9 3.9 53.6 -3 1 1 370 No stop 16 24 40 --- 11 26 38 24.0 250.5 4.0 53.9 227 F 1 400 16 20 51 16 24 40 J0730-0241 11 26 38 24.7 250.3 3.9 53.8 -3 1 1 400 No stop 16 26 00 =0727-025 11 27 58 24.4 250.5 4.0 53.9 77 F 1 410 16 24 41 16 26 00 IRAS0725 11 27 58 23.7 250.7 4.0 54.0 -3 1 1 410 No stop 16 29 50 --- 11 31 49 22.9 251.3 4.1 54.3 227 F 1 440 16 26 01 16 29 50 J0730-0241 11 31 49 23.6 251.1 4.0 54.2 -3 1 1 440 No stop 16 31 10 =0727-025 11 33 09 23.3 251.3 4.0 54.3 77 F 1 450 16 29 51 16 31 10 IRAS0725 11 33 09 22.6 251.6 4.1 54.4 -3 1 1 450 No stop 16 35 00 --- 11 37 00 21.9 252.2 4.1 54.7 227 F 1 480 16 31 11 16 36 00 J0730-0241 11 38 00 22.4 252.1 4.1 54.6 57 1 1 480 16 36 00 16 37 20 =0727-025 11 39 20 22.1 252.3 4.1 54.7 80 F 1 490 16 36 01 16 37 20 IRAS0725 11 39 20 21.4 252.5 4.2 54.9 -3 1 1 490 No stop 16 41 10 --- 11 43 11 20.6 253.1 4.3 55.1 227 F 1 520 16 37 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 ---------------------------------------------------------------------------------------- --- Sat 6 Mar 2010 Day 65 --- 16 41 10 J0730-0241 11 43 11 21.3 252.9 4.2 55.0 -3 1 1 520 No stop 16 42 30 =0727-025 11 44 31 21.0 253.1 4.2 55.1 77 F 1 530 16 41 11 16 42 30 IRAS0725 11 44 31 20.3 253.3 4.3 55.2 -3 1 1 530 No stop 16 46 20 --- 11 48 22 19.5 253.9 4.3 55.5 227 F 1 560 16 42 31 16 46 20 J0730-0241 11 48 22 20.2 253.7 4.3 55.3 -3 1 1 560 No stop 16 47 40 =0727-025 11 49 42 20.0 253.9 4.3 55.4 77 F 1 570 16 46 21 16 47 40 IRAS0725 11 49 42 19.3 254.1 4.4 55.5 -3 1 1 570 No stop 16 51 30 --- 11 53 33 18.5 254.7 4.4 55.8 227 F 1 600 16 47 41 16 52 30 J0730-0241 11 54 33 19.0 254.6 4.4 55.7 57 1 1 600 16 52 30 16 53 50 =0727-025 11 55 53 18.7 254.8 4.4 55.8 80 F 1 610 16 52 31 16 53 50 IRAS0725 11 55 53 18.0 255.0 4.5 55.9 -3 1 1 610 No stop 16 57 40 --- 11 59 44 17.2 255.6 4.5 56.1 227 F 1 640 16 53 51 16 57 40 J0730-0241 11 59 44 17.9 255.4 4.5 56.0 -3 1 1 640 No stop 16 59 00 =0727-025 12 01 04 17.6 255.6 4.5 56.1 77 F 1 650 16 57 41 16 59 00 IRAS0725 12 01 04 16.9 255.8 4.5 56.2 -3 1 1 650 No stop 17 02 50 --- 12 04 55 16.1 256.3 4.6 56.4 227 F 1 680 16 59 01 17 02 50 J0730-0241 12 04 55 16.8 256.1 4.6 56.3 -3 1 1 680 No stop 17 04 10 =0727-025 12 06 15 16.5 256.3 4.6 56.4 77 F 1 690 17 02 51 17 04 10 IRAS0725 12 06 15 15.8 256.5 4.6 56.5 -3 1 1 690 No stop 17 08 00 --- 12 10 05 15.0 257.1 4.7 56.7 227 F 1 720 17 04 11 17 09 00 J0730-0241 12 11 06 15.5 257.0 4.7 56.6 57 1 1 720 17 09 00 17 10 20 =0727-025 12 12 26 15.2 257.2 4.7 56.7 80 F 1 730 17 09 01 17 10 20 IRAS0725 12 12 26 14.5 257.4 4.7 56.8 -3 1 1 730 No stop 17 14 00 --- 12 16 06 13.8 257.9 4.8 57.0 217 F 1 759 17 10 21 17 14 00 J0730-0241 12 16 06 14.5 257.7 4.8 56.9 -3 1 1 759 No stop 17 15 20 =0727-025 12 17 27 14.2 257.9 4.8 56.9 77 F 1 769 17 14 01 17 15 20 IRAS0725 12 17 27 13.5 258.1 4.8 57.0 -3 1 1 769 No stop 17 19 00 --- 12 21 07 12.7 258.6 4.9 57.2 217 F 1 797 17 15 21 17 19 00 J0730-0241 12 21 07 13.4 258.4 4.8 57.1 -3 1 1 797 No stop 17 20 20 =0727-025 12 22 27 13.1 258.6 4.9 57.2 77 F 1 808 17 19 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 ---------------------------------------------------------------------------------------- --- Sat 6 Mar 2010 Day 65 --- 17 20 20 IRAS0725 12 22 27 12.4 258.8 4.9 57.3 -3 1 1 808 No stop 17 24 00 --- 12 26 08 11.7 259.3 5.0 57.4 217 F 1 836 17 20 21 17 25 00 J0730-0241 12 27 08 12.2 259.2 4.9 57.4 57 1 1 836 17 25 00 17 26 20 =0727-025 12 28 28 11.9 259.4 5.0 57.4 80 F 1 846 17 25 01 17 26 20 IRAS0725 12 28 28 11.2 259.6 5.0 57.5 -3 1 1 846 No stop 17 30 00 --- 12 32 09 10.4 260.1 5.1 57.6 217 F 1 875 17 26 21 17 30 00 J0730-0241 12 32 09 11.1 259.9 5.0 57.6 -3 1 1 875 No stop 17 31 20 =0727-025 12 33 29 10.8 260.1 5.0 57.6 77 F 1 885 17 30 01 17 31 20 IRAS0725 12 33 29 10.1 260.3 5.1 57.7 -3 1 1 885 No stop 17 35 00 --- 12 37 10 9.3 260.8 5.1 57.8 217 F 1 913 17 31 21 17 35 00 J0730-0241 12 37 10 10.1 260.6 5.1 57.8 -3 1 1 913 No stop 17 36 20 =0727-025 12 38 30 9.8 260.8 5.1 57.8 77 F 1 924 17 35 01 17 36 20 IRAS0725 12 38 30 9.1 261.0 5.2 57.9 -3 1 1 924 No stop 17 40 00 --- 12 42 11 8.3 261.5 5.2 58.0 217 F 1 952 17 36 21 17 41 00 J0730-0241 12 43 11 8.8 261.4 5.2 58.0 57 1 1 952 17 41 00 17 42 20 =0727-025 12 44 31 8.5 261.6 5.2 58.0 80 F 1 963 17 41 01 17 42 20 IRAS0725 12 44 31 7.8 261.8 5.3 58.1 -3 1 1 963 No stop 17 46 00 --- 12 48 12 7.0 262.3 5.3 58.2 217 F 1 991 17 42 21 17 46 00 J0730-0241 12 48 12 7.7 262.1 5.3 58.1 -3 1 1 991 No stop 17 47 20 =0727-025 12 49 32 7.4 262.3 5.3 58.2 77 F 1 1001 17 46 01 17 47 20 IRAS0725 12 49 32 6.7 262.5 5.4 58.2 -3 1 1 1001 No stop 17 51 00 --- 12 53 12 5.9 262.9 5.4 58.3 217 F 1 1030 17 47 21 17 51 00 J0730-0241 12 53 12 6.7 262.8 5.4 58.3 -3 1 1 1030 No stop 17 52 20 =0727-025 12 54 33 6.4 262.9 5.4 58.3 77 F 1 1040 17 51 01 17 53 20 J0854+2006 12 55 33 35.4 273.6 4.0 65.5 10 1 1 1040 17 53 20 17 58 50 =0851+202 13 01 04 34.2 274.3 4.1 65.4 330 F 1 1083 17 53 21 17 58 50 4C39.25 13 01 04 46.3 295.6 3.6 83.4 -23 1 1 1083 No stop 18 04 20 --- 13 06 35 45.2 295.8 3.6 82.6 307 F 1 1125 17 58 51 21 23 20 3C286 16 26 07 52.8 280.6 2.9 77.5 11923 1 1 1125 21 23 20 21 30 00 --- 16 32 48 51.4 281.1 3.0 77.0 400 F 1 1177 21 23 21 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: ep064i.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) * IRAS0725 07 25 06.977760 * 07 27 37.613044 07 28 10.059878 0.00 -02 48 45.42650 *-02 54 54.19322 -02 56 18.60445 0.00 From catalog imbedded in main SCHED input file. 3.839 scan hours, 135.149 baseline hours above horizon. * J0730-0241 07 27 54.982193 * 07 30 25.877603 07 30 58.390913 0.29 0727-025 -02 35 04.77201 *-02 41 24.90408 -02 42 51.65251 0.55 /home/cristina/sched_8.1/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 1.483 scan hours, 42.025 baseline hours above horizon. * J0854+2006 08 51 57.250618 * 08 54 48.874930 08 55 26.142784 0.21 0851+202 20 17 58.41742 * 20 06 30.64087 20 04 03.10119 0.40 J0854+20 /home/cristina/sched_8.1/catalogs/sources.vlba OJ287 VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 0.092 scan hours, 3.722 baseline hours above horizon. J0927+3902 09 23 55.319214 * 09 27 03.013935 09 27 44.035613 0.26 0923+392 39 15 23.56647 * 39 02 20.85187 38 59 35.54830 0.40 * 4C39.25 /home/cristina/sched_8.1/catalogs/sources.vlba J0927+39 VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 0.092 scan hours, 3.131 baseline hours above horizon. J1331+3030 13 28 49.657764 * 13 31 08.288056 13 31 38.673277 0.36 * 3C286 30 45 58.64058 * 30 30 32.95922 30 27 04.53353 0.47 1328+307 /home/cristina/sched_8.1/catalogs/sources.vlba J1331+30 VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro 0.111 scan hours, 2.530 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 124.3 J0730-0241 125.0 J0854+2006 144.5 4C39.25 139.5 3C286 138.2 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