COVER INFORMATION Station: URUMQI (Code Ur ) Experiment: Type-2 quasars Exp. Code: EK024B Schedule Version: 1.00 Processed by SCHED version: 6.05 June 2006 PI: Hans-Rainer Kloeckner Address: University of Oxford Keble Road,Oxford OX1 3RH United Kingdom Phone: +44 1865 273435 EMAIL: hrk@astro.ox.ac.uk Fax: +44 1865 273390 Phone during observation: +44 1865 273435 Observing mode: 1 Gbit at 18cm Notes: >>> THANK YOU TO MAKE THIS EXPERIMENT POSSIBLE <<< Schedule for URUMQI (Code Ur ) Page 2 Type-2 quasars 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 10 Mar 2007 Day 69 --- 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: 310.49 310.49 310.49 310.49 342.49 342.49 342.49 342.49 374.49 374.49 374.49 374.49 406.49 406.49 406.49 406.49 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 01 00 00 J1722+5856 17 58 03 73.6 -16.3 0.6 156.7 0 1 1 0 01 00 00 01 05 00 =1721+589 18 03 04 73.3 -18.4 0.7 153.7 300 F 1 39 01 00 04 01 05 00 J1722+6105 18 03 04 71.4 -15.4 0.7 156.6 -9 1 1 39 01 05 00 01 11 00 =1722+611 18 09 05 71.1 -17.4 0.8 153.3 351 F 1 85 01 05 04 01 12 00 J1722+5856 18 10 05 72.9 -21.1 0.8 149.5 51 1 1 85 01 12 00 01 15 00 =1721+589 18 13 05 72.7 -22.3 0.8 147.8 180 F 1 108 01 12 04 01 15 00 AMS08 18 13 05 71.6 -24.0 1.0 144.4 -6 1 1 108 01 15 00 01 23 00 --- 18 21 06 71.0 -26.5 1.1 140.3 474 F 1 170 01 15 04 01 24 00 J1722+5856 18 22 07 72.1 -25.4 1.0 142.9 55 1 1 170 01 24 00 01 27 00 =1721+589 18 25 07 71.8 -26.4 1.0 141.3 180 F 1 194 01 24 04 01 27 00 AMS08 18 25 07 70.7 -27.7 1.2 138.4 -6 1 1 194 01 27 00 01 35 00 --- 18 33 08 70.0 -29.9 1.3 134.6 474 F 1 255 01 27 04 01 36 00 J1722+5856 18 34 09 71.1 -29.2 1.2 136.7 54 1 1 255 01 36 00 01 39 00 =1721+589 18 37 09 70.8 -30.0 1.2 135.3 180 F 1 279 01 36 04 01 39 00 AMS10 18 37 09 69.7 -30.1 1.3 133.8 -6 1 1 279 01 39 00 01 47 00 --- 18 45 10 68.9 -32.1 1.5 130.3 474 F 1 341 01 39 04 01 48 00 J1722+5856 18 46 11 69.9 -32.4 1.4 131.1 55 1 1 341 01 48 00 01 51 00 =1721+589 18 49 11 69.6 -33.1 1.4 129.8 180 F 1 364 01 48 04 01 51 00 AMS10 18 49 11 68.6 -33.0 1.5 128.6 -6 1 1 364 01 51 00 01 59 00 --- 18 57 12 67.7 -34.6 1.7 125.4 474 F 1 426 01 51 04 02 00 00 J1722+5856 18 58 13 68.7 -35.1 1.6 126.0 55 1 1 426 02 00 00 02 03 00 =1721+589 19 01 13 68.4 -35.8 1.6 124.8 180 F 1 449 02 00 04 Schedule for URUMQI (Code Ur ) Page 3 Type-2 quasars 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 10 Mar 2007 Day 69 --- 02 03 00 AMS11 19 01 13 67.5 -35.0 1.7 124.6 -5 1 1 449 02 03 00 02 11 00 --- 19 09 14 66.7 -36.4 1.8 121.5 475 F 1 511 02 03 04 02 12 00 J1722+5856 19 10 15 67.4 -37.4 1.8 121.3 56 1 1 511 02 12 00 02 15 00 =1721+589 19 13 15 67.1 -38.0 1.8 120.2 180 F 1 534 02 12 04 02 15 00 AMS11 19 13 15 66.3 -37.0 1.9 120.1 -5 1 1 534 02 15 00 02 23 00 --- 19 21 16 65.4 -38.2 2.0 117.3 475 F 1 596 02 15 04 02 24 00 J1722+5856 19 22 17 66.1 -39.4 2.0 116.9 56 1 1 596 02 24 00 02 27 00 =1721+589 19 25 17 65.7 -39.8 2.0 115.9 180 F 1 619 02 24 04 02 27 00 AMS18 19 25 17 65.0 -37.7 2.1 117.4 -6 1 1 619 02 27 00 02 35 00 --- 19 33 18 64.1 -38.7 2.2 114.8 474 F 1 681 02 27 04 02 36 00 J1722+5856 19 34 18 64.7 -40.9 2.2 112.9 54 1 1 681 02 36 00 02 39 00 =1721+589 19 37 19 64.3 -41.3 2.2 112.0 180 F 1 704 02 36 04 02 39 00 AMS18 19 37 19 63.7 -39.2 2.3 113.5 -6 1 1 704 02 39 00 02 47 00 --- 19 45 20 62.7 -40.0 2.4 111.0 474 F 1 766 02 39 04 02 48 00 J1722+5856 19 46 20 63.2 -42.2 2.4 109.2 54 1 1 766 02 48 00 02 53 00 =1721+589 19 51 21 62.6 -42.6 2.5 107.7 300 F 1 805 02 48 04 02 53 00 J1722+6105 19 51 21 61.9 -38.3 2.5 111.6 -11 1 1 805 02 53 00 02 59 00 =1722+611 19 57 22 61.2 -38.8 2.6 109.8 349 F 1 852 02 53 04 03 00 00 J1722+5856 19 58 22 61.7 -43.2 2.6 105.7 49 1 1 852 03 00 00 03 03 00 =1721+589 20 01 23 61.4 -43.4 2.6 104.9 180 F 1 875 03 00 04 03 04 00 3C345 20 02 23 53.2 -78.1 3.3 67.6 -11 1 1 875 03 04 00 03 15 00 --- 20 13 25 51.2 -76.8 3.5 66.9 649 F 1 960 03 04 04 03 18 00 J1722+5856 20 16 25 59.5 -44.3 2.9 100.9 113 1 1 960 03 18 00 03 21 00 =1721+589 20 19 26 59.1 -44.4 2.9 100.2 180 F 1 983 03 18 04 03 21 00 AMS08 20 19 26 58.0 -43.6 3.1 99.1 -6 1 1 983 03 21 00 03 29 00 --- 20 27 27 57.0 -43.9 3.2 97.1 474 F 1 1045 03 21 04 03 30 00 J1722+5856 20 28 27 57.9 -44.8 3.1 97.9 55 1 1 1045 03 30 00 03 33 00 =1721+589 20 31 28 57.5 -44.9 3.1 97.2 180 F 1 1068 03 30 04 03 33 00 AMS08 20 31 28 56.4 -44.0 3.3 96.2 -6 1 1 1068 03 33 00 03 41 00 --- 20 39 29 55.4 -44.2 3.4 94.3 474 F 1 1130 03 33 04 Schedule for URUMQI (Code Ur ) Page 4 Type-2 quasars 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 10 Mar 2007 Day 69 --- 03 42 00 J1722+5856 20 40 29 56.4 -45.1 3.3 95.1 55 1 1 1130 03 42 00 03 45 00 =1721+589 20 43 30 56.0 -45.2 3.3 94.4 180 F 1 1153 03 42 04 03 45 00 AMS10 20 43 30 55.1 -44.0 3.5 94.0 -5 1 1 1153 03 45 00 03 53 00 --- 20 51 31 54.1 -44.1 3.6 92.2 475 F 1 1215 03 45 04 03 54 00 J1722+5856 20 52 31 54.8 -45.3 3.5 92.4 56 1 1 1215 03 54 00 03 57 00 =1721+589 20 55 32 54.5 -45.3 3.5 91.7 180 F 1 1239 03 54 04 03 57 00 AMS10 20 55 32 53.6 -44.1 3.7 91.3 -5 1 1 1239 03 57 00 04 05 00 --- 21 03 33 52.6 -44.1 3.8 89.6 475 F 1 1301 03 57 04 04 06 00 J1722+5856 21 04 33 53.3 -45.3 3.7 89.7 56 1 1 1301 04 06 00 04 09 00 =1721+589 21 07 34 52.9 -45.3 3.7 89.1 180 F 1 1324 04 06 04 04 09 00 AMS11 21 07 34 52.4 -44.1 3.8 89.2 -4 1 1 1324 04 09 00 04 17 00 --- 21 15 35 51.4 -44.1 4.0 87.5 476 F 1 1386 04 09 04 04 18 00 J1722+5856 21 16 35 51.7 -45.3 3.9 87.2 56 1 1 1386 04 18 00 04 21 00 =1721+589 21 19 36 51.3 -45.2 3.9 86.6 180 F 1 1409 04 18 04 04 21 00 AMS11 21 19 36 50.8 -44.0 4.0 86.6 -4 1 1 1409 04 21 00 04 29 00 --- 21 27 37 49.8 -43.9 4.2 85.0 476 F 1 1471 04 21 04 04 30 00 J1722+5856 21 28 37 50.2 -45.1 4.1 84.8 56 1 1 1471 04 30 00 04 33 00 =1721+589 21 31 38 49.8 -45.0 4.1 84.2 180 F 1 1494 04 30 04 04 33 00 AMS18 21 31 38 49.7 -43.3 4.2 85.1 -5 1 1 1494 04 33 00 04 41 00 --- 21 39 39 48.7 -43.2 4.3 83.5 475 F 1 1556 04 33 04 04 42 00 J1722+5856 21 40 39 48.6 -44.8 4.3 82.4 55 1 1 1556 04 42 00 04 45 00 =1721+589 21 43 40 48.3 -44.7 4.3 81.8 180 F 1 1579 04 42 04 04 45 00 AMS18 21 43 40 48.2 -43.1 4.4 82.7 -5 1 1 1579 04 45 00 04 53 00 --- 21 51 41 47.2 -42.9 4.5 81.1 475 F 1 1641 04 45 04 04 54 00 J1722+5856 21 52 41 47.1 -44.5 4.5 80.1 55 1 1 1641 04 54 00 04 57 00 =1721+589 21 55 42 46.7 -44.4 4.5 79.5 180 F 1 1664 04 54 04 05 12 00 J2005+7752 22 10 44 53.4 -10.6 2.1 140.7 830 1 1 1664 05 12 00 05 23 00 =2007+777 22 21 46 53.0 -11.3 2.3 137.4 660 F 1 1750 05 12 04 05 25 00 J1722+5856 22 23 46 43.2 -43.2 5.0 74.3 54 1 1 1750 05 25 00 05 28 00 =1721+589 22 26 47 42.8 -43.1 5.1 73.8 180 F 1 1773 05 25 04 Schedule for URUMQI (Code Ur ) Page 5 Type-2 quasars 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 10 Mar 2007 Day 69 --- 05 28 00 J1722+6105 22 26 47 43.4 -40.2 5.1 75.7 -8 1 1 1773 05 28 00 05 33 00 =1722+611 22 31 48 42.8 -40.0 5.2 74.8 292 F 1 1811 05 28 04 05 34 00 J1722+5856 22 32 48 42.1 -42.8 5.2 72.7 52 1 1 1811 05 34 00 05 37 00 =1721+589 22 35 48 41.7 -42.6 5.2 72.2 180 F 1 1835 05 34 04 05 37 00 AMS08 22 35 48 40.9 -41.4 5.4 71.2 -5 1 1 1835 05 37 00 05 45 00 --- 22 43 50 40.0 -41.0 5.5 69.8 475 F 1 1897 05 37 04 05 46 00 J1722+5856 22 44 50 40.6 -42.1 5.4 70.5 56 1 1 1897 05 46 00 05 49 00 =1721+589 22 47 50 40.2 -41.9 5.4 70.0 180 F 1 1920 05 46 04 05 49 00 AMS08 22 47 50 39.5 -40.7 5.6 69.0 -5 1 1 1920 05 49 00 05 57 00 --- 22 55 52 38.5 -40.3 5.7 67.6 475 F 1 1982 05 49 04 05 58 00 J1722+5856 22 56 52 39.2 -41.4 5.6 68.4 56 1 1 1982 05 58 00 06 01 00 =1721+589 22 59 52 38.8 -41.2 5.6 67.9 180 F 1 2005 05 58 04 06 01 00 AMS10 22 59 52 38.3 -40.0 5.7 67.3 -5 1 1 2005 06 01 00 06 09 00 --- 23 07 53 37.4 -39.5 5.9 65.9 475 F 1 2067 06 01 04 06 10 00 J1722+5856 23 08 54 37.7 -40.6 5.8 66.3 56 1 1 2067 06 10 00 06 13 00 =1721+589 23 11 54 37.4 -40.4 5.8 65.8 180 F 1 2090 06 10 04 06 13 00 AMS10 23 11 54 36.9 -39.2 5.9 65.2 -5 1 1 2090 06 13 00 06 21 00 --- 23 19 55 36.0 -38.6 6.1 63.8 475 F 1 2152 06 13 04 06 22 00 J1722+5856 23 20 56 36.3 -39.8 6.0 64.2 56 1 1 2152 06 22 00 06 25 00 =1721+589 23 23 56 36.0 -39.6 6.0 63.7 180 F 1 2175 06 22 04 06 25 00 AMS11 23 23 56 35.8 -38.5 6.1 63.5 -4 1 1 2175 06 25 00 06 33 00 --- 23 31 57 34.9 -37.9 6.2 62.0 476 F 1 2237 06 25 04 06 34 00 J1722+5856 23 32 58 34.9 -39.0 6.2 62.2 56 1 1 2237 06 34 00 06 37 00 =1721+589 23 35 58 34.6 -38.7 6.2 61.6 180 F 1 2261 06 34 04 06 37 00 AMS11 23 35 58 34.5 -37.7 6.3 61.3 -4 1 1 2261 06 37 00 06 45 00 --- 23 43 59 33.6 -37.1 6.4 60.0 476 F 1 2322 06 37 04 06 46 00 J1722+5856 23 45 00 33.6 -38.1 6.4 60.1 56 1 1 2322 06 46 00 06 49 00 =1721+589 23 48 00 33.2 -37.8 6.4 59.6 180 F 1 2346 06 46 04 06 49 00 AMS18 23 48 00 33.6 -36.5 6.5 59.9 -5 1 1 2346 06 49 00 06 57 00 --- 23 56 01 32.7 -35.9 6.6 58.5 475 F 1 2408 06 49 04 Schedule for URUMQI (Code Ur ) Page 6 Type-2 quasars 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 10 Mar 2007 Day 69 --- 06 58 00 J1722+5856 23 57 02 32.2 -37.1 6.6 58.0 56 1 1 2408 06 58 00 07 01 00 =1721+589 00 00 02 31.9 -36.9 6.6 57.5 180 F 1 2431 06 58 04 07 01 00 AMS18 00 00 02 32.3 -35.6 6.7 57.8 -4 1 1 2431 07 01 00 07 09 00 --- 00 08 03 31.5 -35.0 6.8 56.4 476 F 1 2493 07 01 04 07 10 00 J1722+5856 00 09 04 30.9 -36.1 6.8 56.0 56 1 1 2493 07 10 00 07 15 00 =1721+589 00 14 04 30.4 -35.7 6.9 55.1 300 F 1 2531 07 10 04 07 15 00 J1722+6105 00 14 04 31.6 -33.6 6.9 56.2 -6 1 1 2531 07 15 00 07 21 00 =1722+611 00 20 05 31.0 -33.1 7.0 55.1 354 F 1 2578 07 15 04 07 22 00 J1722+5856 00 21 05 29.7 -35.1 7.0 53.9 53 1 1 2578 07 22 00 07 25 00 =1721+589 00 24 06 29.3 -34.8 7.0 53.4 180 F 1 2601 07 22 04 07 25 00 AMS08 00 24 06 28.9 -33.6 7.2 52.3 -5 1 1 2601 07 25 00 07 33 00 --- 00 32 07 28.1 -32.8 7.3 50.9 475 F 1 2663 07 25 04 07 34 00 J1722+5856 00 33 07 28.4 -34.0 7.2 51.9 56 1 1 2663 07 34 00 07 37 00 =1721+589 00 36 08 28.1 -33.7 7.2 51.4 180 F 1 2686 07 34 04 07 37 00 AMS08 00 36 08 27.7 -32.5 7.4 50.2 -5 1 1 2686 07 37 00 07 45 00 --- 00 44 09 26.9 -31.7 7.5 48.8 475 F 1 2748 07 37 04 07 46 00 J1722+5856 00 45 09 27.2 -32.9 7.4 49.8 56 1 1 2748 07 46 00 07 49 00 =1721+589 00 48 10 26.9 -32.6 7.4 49.3 180 F 1 2771 07 46 04 07 49 00 AMS10 00 48 10 26.8 -31.4 7.5 48.5 -4 1 1 2771 07 49 00 07 57 00 --- 00 56 11 26.1 -30.7 7.7 47.1 476 F 1 2833 07 49 04 07 58 00 J1722+5856 00 57 11 26.1 -31.8 7.6 47.7 56 1 1 2833 07 58 00 08 01 00 =1721+589 01 00 12 25.8 -31.5 7.6 47.2 180 F 1 2857 07 58 04 08 01 00 AMS10 01 00 12 25.7 -30.3 7.7 46.4 -4 1 1 2857 08 01 00 08 09 00 --- 01 08 13 25.0 -29.5 7.9 45.0 476 F 1 2919 08 01 04 08 10 00 J1722+5856 01 09 13 24.9 -30.6 7.8 45.7 56 1 1 2919 08 10 00 08 13 00 =1721+589 01 12 14 24.6 -30.3 7.8 45.2 180 F 1 2942 08 10 04 08 13 00 AMS11 01 12 14 24.8 -29.3 7.9 44.7 -4 1 1 2942 08 13 00 08 21 00 --- 01 20 15 24.1 -28.5 8.0 43.3 476 F 1 3004 08 13 04 08 22 00 J1722+5856 01 21 15 23.8 -29.4 8.0 43.6 56 1 1 3004 08 22 00 08 25 00 =1721+589 01 24 16 23.6 -29.1 8.0 43.1 180 F 1 3027 08 22 04 Schedule for URUMQI (Code Ur ) Page 7 Type-2 quasars 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 10 Mar 2007 Day 69 --- 08 25 00 AMS11 01 24 16 23.7 -28.1 8.1 42.6 -4 1 1 3027 08 25 00 08 33 00 --- 01 32 17 23.1 -27.3 8.2 41.1 476 F 1 3089 08 25 04 08 34 00 J1722+5856 01 33 17 22.8 -28.1 8.2 41.5 56 1 1 3089 08 34 00 08 37 00 =1721+589 01 36 18 22.5 -27.8 8.2 41.0 180 F 1 3112 08 34 04 08 37 00 AMS18 01 36 18 23.2 -26.8 8.3 41.0 -4 1 1 3112 08 37 00 08 43 00 --- 01 42 19 22.7 -26.2 8.4 39.9 356 F 1 3159 08 37 04 08 44 00 J1722+5856 01 43 19 21.9 -27.1 8.3 39.8 55 1 1 3159 08 44 00 08 47 00 =1721+589 01 46 19 21.7 -26.7 8.4 39.2 180 F 1 3182 08 44 04 08 47 00 AMS18 01 46 19 22.4 -25.8 8.4 39.2 -4 1 1 3182 08 47 00 08 53 00 --- 01 52 20 21.9 -25.2 8.5 38.1 356 F 1 3228 08 47 04 08 54 00 J1722+5856 01 53 21 21.1 -26.0 8.5 38.0 55 1 1 3228 08 54 00 08 57 00 =1721+589 01 56 21 20.9 -25.7 8.6 37.5 180 F 1 3251 08 54 04 08 57 00 J1722+6105 01 56 21 22.6 -24.2 8.6 38.0 -8 1 1 3251 08 57 00 09 00 00 =1722+611 01 59 22 22.4 -23.9 8.6 37.5 172 F 1 3275 08 57 04 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. Setup file: 1Gbs.18cm Matches group ur18cm in /SOFT/sched/catalogs/freq.dat update L.Xiang 9Feb05 Setup group: 8 Station: URUMQI 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= 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 1300.00 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 = 2 1 2 1 4 3 4 3 6 5 6 5 8 7 8 7 BBC SB= L L U U L L U U L L U U L L U U IF = 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N 2N 1N The following frequency sets based on this setup were used. Frequency Set: 8 Setup file default. No pcal detection. 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= 310.49 310.49 310.49 310.49 342.49 342.49 342.49 342.49 374.49 374.49 374.49 374.49 406.49 406.49 406.49 406.49 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 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 -- Type-2 quasars 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) * AMS08 17 13 47.332999 * 17 14 29.671000 17 14 35.978418 0.00 59 35 52.51054 * 59 32 33.45200 59 31 35.12853 0.00 From catalog imbedded in main SCHED input file. 1.067 scan hours, 35.831 baseline hours above horizon. * AMS10 17 15 38.500916 * 17 16 20.077000 17 16 26.245583 0.00 59 43 37.66447 * 59 40 26.52300 59 39 29.33064 0.00 From catalog imbedded in main SCHED input file. 1.067 scan hours, 34.855 baseline hours above horizon. * AMS11 17 17 39.938299 * 17 18 21.331000 17 18 27.440979 0.00 59 43 29.59671 * 59 40 27.14100 59 39 31.20207 0.00 From catalog imbedded in main SCHED input file. 1.067 scan hours, 34.974 baseline hours above horizon. * AMS18 17 20 06.807738 * 17 20 46.317000 17 20 52.116537 0.00 60 05 21.54246 * 60 02 29.55100 60 01 35.09828 0.00 From catalog imbedded in main SCHED input file. 1.000 scan hours, 31.934 baseline hours above horizon. J1642+3948 16 41 17.606231 * 16 42 58.809968 16 43 13.880305 0.26 1641+399 39 54 10.81494 * 39 48 36.99400 39 47 21.91843 0.40 * 3C345 /SOFT/sched/catalogs/sources.vlba J1642+39 VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.183 scan hours, 6.032 baseline hours above horizon. * J1722+5856 17 21 52.440262 * 17 22 36.726556 17 22 43.187536 0.62 1721+589 58 59 06.49433 * 58 56 22.26071 58 55 29.01306 0.49 /SOFT/sched/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 2.050 scan hours, 70.896 baseline hours above horizon. * J1722+6105 17 22 05.759504 * 17 22 40.059354 17 22 45.074836 0.52 1722+611 61 08 43.42147 * 61 05 59.78736 61 05 06.47173 0.45 /SOFT/sched/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.433 scan hours, 14.008 baseline hours above horizon. * J2005+7752 20 07 20.430185 * 20 05 30.998513 20 05 08.966938 0.96 2007+777 77 43 58.12307 * 77 52 43.24760 77 53 36.08031 0.40 J2005+77 /SOFT/sched/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.183 scan hours, 6.600 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) AMS08 94.4 AMS10 94.2 AMS11 93.9 AMS18 93.6 3C345 99.9 J1722+5856 93.4 J1722+6105 93.4 J2005+7752 86.3 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