COVER INFORMATION Station: EB_VLBA (Code Eb ) Experiment: bp116: the HSA for high T_b Exp. Code: BP116 Schedule Version: 1.00 Processed by SCHED version: NRAO internal release of 4 October 2004 PI: Glenn Piner Address: Whittier College Dept. Physics and Astronomy 13406 E. Philadelphia St Whittier CA 90608 Phone: 562-464-4556 EMAIL: gpiner@whittier.edu Fax: 562-464-4514 Phone during observation: 562-464-4556 Observing mode: 256 Mbps Notes: Targets : 1637+574, 1642+690, 0133+476 Calibrators = CSOs: J1545+4751, J1815+6127, J0111+3906 Fringe finders : J1740+5211, J1849+6705, J0154+4743 Schedule for EB_VLBA (Code Eb ) Page 2 bp116: the HSA for high T_b 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. TPStart: Tape motion start time. Frequencies are LO sum (band edge). ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) ---------------------------------------------------------------------------------------- --- Mon 27 Dec 2004 Day 362 --- Next scan frequencies: 4960.49 4968.49 4976.49 4984.49 4992.49 5000.49 5008.49 5016.49 Next BBC frequencies: 860.49 868.49 876.49 884.49 892.49 900.49 908.49 916.49 Next scan bandwidths: 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 17 00 00 J1545+4751 23 53 36 20.2 322.7 8.1 35.0 0 1 1 0 17 00 00 17 04 00 =1543+480 23 57 36 19.8 323.3 8.2 34.5 240 F 1 3200 17 05 10 1637+574 23 58 47 32.1 323.2 7.3 44.8 -1 1 1 3200 17 05 10 17 14 10 --- 00 07 48 31.3 324.3 7.5 43.5 539 F 1 10400 17 15 10 1642+690 00 08 48 39.5 334.4 7.4 49.9 4 1 1 10400 17 15 10 17 24 10 --- 00 17 50 38.9 335.0 7.6 48.3 540 F 1 17600 17 26 10 J1545+4751 00 19 50 17.8 326.6 8.6 31.4 14 1 2 17600 17 26 10 17 29 10 =1543+480 00 22 51 17.5 327.0 8.6 31.0 180 R 1 15200 17 30 20 1637+574 00 24 01 29.8 326.1 7.8 41.0 -1 1 2 15200 17 30 20 17 39 50 --- 00 33 32 29.0 327.3 7.9 39.5 569 R 1 7600 17 40 50 1642+690 00 34 32 37.8 336.4 7.9 45.2 3 1 2 7600 17 40 50 17 50 20 --- 00 44 04 37.2 337.1 8.0 43.4 570 R 1 0 17 51 40 J1740+5211 00 45 24 30.1 317.1 7.1 44.9 -6 1 3 0 17 51 40 17 54 40 =1739+522 00 48 25 29.8 317.5 7.1 44.5 174 F 1 2400 17 55 40 1637+574 00 49 25 27.6 329.2 8.2 37.1 -1 1 3 2400 17 55 40 18 05 10 --- 00 58 56 26.9 330.3 8.3 35.6 569 F 1 10000 18 06 10 1642+690 00 59 57 36.2 338.4 8.3 40.5 1 1 3 10000 18 06 10 18 15 40 --- 01 09 28 35.7 339.3 8.5 38.8 570 F 1 17600 18 17 00 J1740+5211 01 10 48 27.4 320.4 7.5 41.4 -2 1 4 17600 18 17 00 18 20 00 =1739+522 01 13 49 27.1 320.8 7.6 41.0 178 R 1 15200 18 21 10 1637+574 01 14 59 25.7 332.3 8.6 33.1 10 1 4 15200 18 21 10 18 30 40 --- 01 24 31 25.0 333.5 8.8 31.7 570 R 1 7600 18 31 40 1642+690 01 25 31 34.8 340.7 8.7 35.8 -1 1 4 7600 18 31 40 18 41 10 --- 01 35 02 34.3 341.5 8.9 34.1 569 R 1 0 Schedule for EB_VLBA (Code Eb ) Page 3 bp116: the HSA for high T_b 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. TPStart: Tape motion start time. Frequencies are LO sum (band edge). ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) ---------------------------------------------------------------------------------------- --- Mon 27 Dec 2004 Day 362 --- 18 43 10 J1815+6127 01 37 03 34.9 326.9 7.4 46.6 50 1 5 0 18 43 10 18 46 10 =1815+614 01 40 03 34.7 327.2 7.4 46.1 180 F 1 2400 18 47 20 1637+574 01 41 13 23.8 335.7 9.0 29.0 5 1 5 2400 18 47 20 18 56 50 --- 01 50 45 23.2 336.9 9.2 27.5 570 F 1 10000 18 58 00 1642+690 01 51 55 33.5 343.1 9.2 31.0 7 1 5 10000 18 58 00 19 07 30 --- 02 01 27 33.1 343.9 9.3 29.3 570 F 1 17600 19 09 30 J1740+5211 02 03 27 22.5 327.4 8.4 34.0 45 1 6 17600 19 09 30 19 12 30 =1739+522 02 06 28 22.2 327.8 8.4 33.5 180 R 1 15200 19 13 30 1637+574 02 07 28 22.2 339.1 9.5 24.8 0 1 6 15200 19 13 30 19 23 00 --- 02 16 59 21.7 340.4 9.6 23.3 570 R 1 7600 19 24 10 1642+690 02 18 09 32.4 345.5 9.6 26.2 6 1 6 7600 19 24 10 19 33 40 --- 02 27 41 32.0 346.4 9.8 24.5 570 R 1 0 19 34 50 J1849+6705 02 28 51 37.4 333.6 7.7 46.5 6 1 7 0 19 34 50 19 37 50 =1849+670 02 31 52 37.2 333.9 7.7 46.0 180 F 1 2400 19 39 20 1637+574 02 33 22 20.9 342.6 9.9 20.7 3 1 7 2400 19 39 20 19 48 50 --- 02 42 54 20.4 343.9 10.1 19.1 570 F 1 10000 19 50 00 1642+690 02 44 04 31.4 348.0 10.0 21.5 5 1 7 10000 19 50 00 19 59 30 --- 02 53 35 31.1 349.0 10.2 19.8 570 F 1 17600 20 07 30 J1849+6705 03 01 37 35.2 336.5 8.2 40.7 417 1 8 17600 20 07 30 20 10 30 =1849+670 03 04 37 35.0 336.8 8.3 40.1 180 R 1 15200 20 12 30 1637+574 03 06 37 19.5 347.1 10.5 15.2 37 1 8 15200 20 12 30 20 22 00 --- 03 16 09 19.2 348.4 10.6 13.7 570 R 1 7600 20 23 10 1642+690 03 17 19 30.5 351.3 10.6 15.5 3 1 8 7600 20 23 10 20 32 40 --- 03 26 51 30.3 352.3 10.7 13.7 570 R 1 0 20 33 50 J1849+6705 03 28 01 33.6 338.9 8.6 35.9 4 1 9 0 20 33 50 20 36 50 =1849+670 03 31 01 33.4 339.2 8.7 35.4 180 F 1 2400 20 38 50 1637+574 03 33 02 18.7 350.8 10.9 10.9 40 1 9 2400 20 38 50 20 48 20 --- 03 42 33 18.5 352.1 11.1 9.3 570 F 1 10000 20 49 30 1642+690 03 43 43 29.9 354.0 11.0 10.6 3 1 9 10000 20 49 30 20 59 00 --- 03 53 15 29.8 355.0 11.2 8.9 570 F 1 17600 Schedule for EB_VLBA (Code Eb ) Page 4 bp116: the HSA for high T_b 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. TPStart: Tape motion start time. Frequencies are LO sum (band edge). ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Tapes TPStart Stop UT LST EL AZ HA UP ParA Dwell (see above) ---------------------------------------------------------------------------------------- --- Mon 27 Dec 2004 Day 362 --- 21 00 05 J1849+6705 03 54 20 32.2 341.5 9.1 31.3 -1 1 10 17600 21 00 05 21 03 05 =1849+670 03 57 21 32.0 341.8 9.1 30.7 179 R 1 15200 21 04 10 1642+690 03 58 26 29.7 355.5 11.3 8.0 -2 1 10 15200 21 04 10 21 13 40 --- 04 07 57 29.6 356.5 11.4 6.2 568 R 1 7600 21 18 30 0133+476 04 12 48 64.8 279.3 2.6 69.3 33 1 10 7600 21 18 30 21 28 00 --- 04 22 20 63.3 280.6 2.8 68.7 570 R 1 0 21 28 35 J0154+4743 04 22 55 65.9 277.9 2.5 69.5 3 1 11 0 21 28 35 21 32 35 =0151+474 04 26 56 65.3 278.4 2.5 69.3 240 F 1 3200 21 33 10 0133+476 04 27 31 62.5 281.3 2.8 68.4 2 1 11 3200 21 33 10 21 51 10 --- 04 45 34 59.7 283.6 3.1 67.1 1080 F 1 17600 21 51 45 J0154+4743 04 46 09 62.3 281.1 2.8 68.1 3 1 12 17600 21 51 45 21 54 45 =0151+474 04 49 09 61.8 281.5 2.9 67.9 180 R 1 15200 21 55 20 0133+476 04 49 44 59.0 284.2 3.2 66.8 2 1 12 15200 21 55 20 22 14 20 --- 05 08 47 56.1 286.6 3.5 65.3 1140 R 1 0 22 14 55 0133+476 05 09 23 56.0 286.7 3.5 65.3 22 1 13 0 22 14 55 22 33 55 --- 05 28 26 53.1 289.0 3.9 63.7 1140 F 1 15200 22 34 30 J0154+4743 05 29 01 55.7 286.6 3.6 65.0 3 1 13 15200 22 34 30 22 37 30 =0151+474 05 32 01 55.2 287.0 3.6 64.7 180 F 1 17600 22 38 00 0133+476 05 32 31 52.5 289.5 3.9 63.3 -2 1 14 17600 22 38 00 23 00 00 --- 05 54 35 49.2 292.3 4.3 61.3 1318 R 1 0 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: /home/filehost/cwalker/sched/setups/v6cm-256-8-2-L.set Matches group eb_6cm in /home/filehost/cwalker/sched/catalogs/freq.dat 6cm secondary focus. Setup group: 1 Station: EB_VLBA Total bit rate: 256 Format: VLBA1:2 Bits per sample: 2 Sample rate: 16.000 Number of channels: 8 Passes/head pos: 1 Speedup factor: 1.00 Tape speeds: Low density - 266.660 ips, High density - 160.00 ips Time per pass for 17600 ft, High density tapes is: 00:22:00 1st LO= 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 Net SB= U U U U U U U U Pol. = LCP LCP LCP LCP LCP LCP LCP LCP BBC = 1 2 3 4 5 6 7 8 BBC SB= U U U U U U U U IF = C C C C C C C C The following frequency sets based on this setup were used. Frequency Set: 1 Setup file default. Used pcal sets: 1 LO sum= 4960.49 4968.49 4976.49 4984.49 4992.49 5000.49 5008.49 5016.49 BBC fr= 860.49 868.49 876.49 884.49 892.49 900.49 908.49 916.49 Bandwd= 8.000 8.000 8.000 8.000 8.000 8.000 8.000 8.000 The following pulse cal sets were used with this setup: Pulse cal detection set: 1 PCAL = 1MHZ PCALXB1= S1 S3 S5 S7 S1 S3 S5 S7 PCALXB2= S2 S4 S6 S8 S2 S4 S6 S8 PCALFR1= 510 510 510 510 6510 6510 6510 6510 PCALFR2= 510 510 510 510 6510 6510 6510 6510 Track assignments are: track1= 2, 10, 18, 26, 3, 11, 19, 27 barrel=roll_auto SOURCE LIST -- bp116: the HSA for high T_b 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) (B1950) (J2000) (Date) * J0111+3906 01 08 47.254786 * 01 11 37.316982 01 11 53.803708 0108+388 38 50 32.81467 * 39 06 28.10430 39 08 14.74606 J0111+39 /home/filehost/cwalker/sched/catalogs/sources.vlba ICRF - Ext.1 Source - 1998 IERS Annual Report 0.039 scan hours, 1.455 baseline hours above horizon. J0136+4751 01 33 55.103066 * 01 36 58.594811 01 37 16.565244 * 0133+476 47 36 12.85367 * 47 51 29.10006 47 53 14.53825 J0136+47 /home/filehost/cwalker/sched/catalogs/sources.vlba ICRF - Ext.1 Source - 1998 IERS Annual Report 1.458 scan hours, 80.151 baseline hours above horizon. * J0154+4743 01 51 47.798764 * 01 54 56.289875 01 55 14.916082 0151+474 47 28 44.75274 * 47 43 26.53914 47 45 08.64203 /home/filehost/cwalker/sched/catalogs/sources.vlba ICRF - Ext.1 Source - 1998 IERS Annual Report 0.167 scan hours, 9.161 baseline hours above horizon. * J1545+4751 15 43 36.198157 * 15 45 08.529822 15 45 16.168014 1543+480 48 01 13.49950 * 47 51 54.66442 47 50 44.29716 /home/filehost/cwalker/sched/catalogs/sources.vlba VLBA Calib. Survey - ICRF Frame - reduced by GSFC group - Aug 2001 0.117 scan hours, 7.545 baseline hours above horizon. J1638+5720 16 37 17.425178 * 16 38 13.456293 16 38 16.846440 * 1637+574 57 26 15.76147 * 57 20 23.97918 57 19 34.96202 J1638+57 /home/filehost/cwalker/sched/catalogs/sources.vlba ICRF - Ext.1 Source - 1998 IERS Annual Report 1.519 scan hours, 99.035 baseline hours above horizon. J1642+6856 16 42 18.064884 * 16 42 07.848514 16 42 03.834978 * 1642+690 69 02 13.21712 * 68 56 39.75640 68 55 51.84246 J1642+68 /home/filehost/cwalker/sched/catalogs/sources.vlba ICRF - Ext.1 Source - 1998 IERS Annual Report 1.575 scan hours, 103.912 baseline hours above horizon. * J1740+5211 17 39 29.003555 * 17 40 36.977852 17 40 41.379766 1739+522 52 13 10.43856 * 52 11 43.40750 52 11 24.27341 J1740+52 /home/filehost/cwalker/sched/catalogs/sources.vlba ICRF - Ext.1 Source - 1998 IERS Annual Report 0.150 scan hours, 9.875 baseline hours above horizon. * J1815+6127 18 15 05.464518 * 18 15 36.792027 18 15 36.848923 1815+614 61 26 04.51486 * 61 27 11.64786 61 27 09.83114 /home/filehost/cwalker/sched/catalogs/sources.vlba VLBA Calib. Survey - ICRF Frame - reduced by GSFC group - Aug 2001 0.050 scan hours, 3.300 baseline hours above horizon. * J1849+6705 18 49 16.505887 * 18 49 16.072300 18 49 12.207999 1849+670 67 02 07.88019 * 67 05 41.67993 67 05 56.94263 J1849+67 /home/filehost/cwalker/sched/catalogs/sources.vlba ICRF - Ext.1 Source - 1998 IERS Annual Report 0.200 scan hours, 13.173 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) J0111+3906 112.7 0133+476 118.5 J0154+4743 121.5 J1545+4751 80.0 1637+574 83.8 1642+690 94.2 J1740+5211 76.2 J1815+6127 84.8 J1849+6705 90.5 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