COVER INFORMATION Station: URUMQI (Code Ur ) Experiment: Type-2 quasars Exp. Code: EK024C 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 ---------------------------------------------------------------------------------------- --- Sun 11 Mar 2007 Day 70 --- 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 18 01 59 73.4 -18.0 0.7 154.3 0 1 1 0 01 00 00 01 05 00 =1721+589 18 07 00 73.1 -19.9 0.7 151.3 300 F 1 39 01 00 04 01 05 00 J1722+6105 18 07 00 71.2 -16.7 0.7 154.4 -8 1 1 39 01 05 00 01 11 00 =1722+611 18 13 01 70.9 -18.7 0.8 151.2 352 F 1 85 01 05 04 01 12 00 J1722+5856 18 14 01 72.7 -22.6 0.9 147.3 50 1 1 85 01 12 00 01 15 00 =1721+589 18 17 02 72.4 -23.7 0.9 145.6 180 F 1 108 01 12 04 01 15 00 AMS14 18 17 02 72.2 -25.2 1.0 143.4 -5 1 1 108 01 15 00 01 23 00 --- 18 25 03 71.6 -27.8 1.1 139.2 475 F 1 170 01 15 04 01 24 00 J1722+5856 18 26 03 71.7 -26.7 1.1 140.8 56 1 1 170 01 24 00 01 27 00 =1721+589 18 29 04 71.5 -27.7 1.1 139.3 180 F 1 194 01 24 04 01 27 00 AMS14 18 29 04 71.2 -29.0 1.2 137.2 -5 1 1 194 01 27 00 01 35 00 --- 18 37 05 70.5 -31.2 1.3 133.3 475 F 1 255 01 27 04 01 36 00 J1722+5856 18 38 05 70.7 -30.3 1.3 134.8 56 1 1 255 01 36 00 01 39 00 =1721+589 18 41 06 70.4 -31.1 1.3 133.4 180 F 1 279 01 36 04 01 39 00 AMS17 18 41 06 70.3 -31.7 1.3 132.4 -3 1 1 279 01 39 00 01 47 00 --- 18 49 07 69.5 -33.7 1.5 128.9 477 F 1 341 01 39 04 01 48 00 J1722+5856 18 50 07 69.5 -33.3 1.5 129.4 57 1 1 341 01 48 00 01 51 00 =1721+589 18 53 08 69.2 -34.0 1.5 128.1 180 F 1 364 01 48 04 01 51 00 AMS17 18 53 08 69.1 -34.6 1.5 127.2 -3 1 1 364 01 51 00 01 59 00 --- 19 01 09 68.2 -36.3 1.7 123.9 477 F 1 426 01 51 04 02 00 00 J1722+5856 19 02 09 68.3 -35.9 1.7 124.4 57 1 1 426 02 00 00 02 03 00 =1721+589 19 05 10 68.0 -36.5 1.7 123.2 180 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 ---------------------------------------------------------------------------------------- --- Sun 11 Mar 2007 Day 70 --- 02 03 00 AMS13 19 05 10 67.3 -36.4 1.8 122.5 -4 1 1 449 02 03 00 02 11 00 --- 19 13 11 66.5 -37.7 1.9 119.6 476 F 1 511 02 03 04 02 12 00 J1722+5856 19 14 11 67.0 -38.1 1.9 119.8 56 1 1 511 02 12 00 02 15 00 =1721+589 19 17 12 66.6 -38.6 1.9 118.7 180 F 1 534 02 12 04 02 15 00 AMS13 19 17 12 66.0 -38.3 2.0 118.1 -4 1 1 534 02 15 00 02 23 00 --- 19 25 13 65.1 -39.4 2.1 115.4 476 F 1 596 02 15 04 02 24 00 J1722+5856 19 26 13 65.6 -39.9 2.1 115.6 56 1 1 596 02 24 00 02 27 00 =1721+589 19 29 14 65.3 -40.3 2.1 114.6 180 F 1 619 02 24 04 02 27 00 AMS20 19 29 14 64.9 -39.7 2.1 114.8 -3 1 1 619 02 27 00 02 35 00 --- 19 37 15 64.0 -40.7 2.3 112.2 477 F 1 681 02 27 04 02 36 00 J1722+5856 19 38 15 64.2 -41.4 2.3 111.7 57 1 1 681 02 36 00 02 39 00 =1721+589 19 41 16 63.8 -41.7 2.3 110.8 180 F 1 704 02 36 04 02 39 00 AMS20 19 41 16 63.5 -41.1 2.3 110.9 -3 1 1 704 02 39 00 02 47 00 --- 19 49 17 62.5 -41.9 2.5 108.5 477 F 1 766 02 39 04 02 48 00 J1722+5856 19 50 17 62.7 -42.5 2.5 108.1 57 1 1 766 02 48 00 02 53 00 =1721+589 19 55 18 62.1 -43.0 2.5 106.6 300 F 1 805 02 48 04 02 53 00 J1722+6105 19 55 18 61.4 -38.6 2.5 110.4 -11 1 1 805 02 53 00 02 59 00 =1722+611 20 01 19 60.7 -39.1 2.6 108.7 349 F 1 852 02 53 04 03 00 00 J1722+5856 20 02 19 61.2 -43.5 2.7 104.7 49 1 1 852 03 00 00 03 03 00 =1721+589 20 05 19 60.9 -43.7 2.7 103.8 180 F 1 875 03 00 04 03 04 00 3C345 20 06 20 52.5 -77.7 3.4 67.3 -10 1 1 875 03 04 00 03 15 00 --- 20 17 21 50.5 -76.3 3.6 66.6 650 F 1 960 03 04 04 03 18 00 J1722+5856 20 20 22 59.0 -44.5 3.0 99.9 114 1 1 960 03 18 00 03 21 00 =1721+589 20 23 22 58.6 -44.6 3.0 99.2 180 F 1 983 03 18 04 03 21 00 AMS14 20 23 22 58.1 -44.9 3.1 98.1 -4 1 1 983 03 21 00 03 29 00 --- 20 31 24 57.1 -45.1 3.2 96.2 476 F 1 1045 03 21 04 03 30 00 J1722+5856 20 32 24 57.4 -44.9 3.2 97.0 57 1 1 1045 03 30 00 03 33 00 =1721+589 20 35 24 57.0 -45.0 3.2 96.3 180 F 1 1068 03 30 04 03 33 00 AMS14 20 35 24 56.6 -45.2 3.3 95.2 -4 1 1 1068 03 33 00 03 41 00 --- 20 43 26 55.5 -45.4 3.4 93.4 476 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 ---------------------------------------------------------------------------------------- --- Sun 11 Mar 2007 Day 70 --- 03 42 00 J1722+5856 20 44 26 55.9 -45.2 3.4 94.2 57 1 1 1130 03 42 00 03 45 00 =1721+589 20 47 26 55.5 -45.2 3.4 93.5 180 F 1 1153 03 42 04 03 45 00 AMS17 20 47 26 55.3 -45.4 3.4 93.0 -3 1 1 1153 03 45 00 03 53 00 --- 20 55 28 54.2 -45.4 3.6 91.2 477 F 1 1215 03 45 04 03 54 00 J1722+5856 20 56 28 54.3 -45.3 3.6 91.5 58 1 1 1215 03 54 00 03 57 00 =1721+589 20 59 28 53.9 -45.3 3.6 90.8 180 F 1 1239 03 54 04 03 57 00 AMS17 20 59 28 53.7 -45.4 3.6 90.3 -3 1 1 1239 03 57 00 04 05 00 --- 21 07 30 52.7 -45.4 3.8 88.6 477 F 1 1301 03 57 04 04 06 00 J1722+5856 21 08 30 52.8 -45.3 3.8 88.9 58 1 1 1301 04 06 00 04 09 00 =1721+589 21 11 30 52.4 -45.3 3.8 88.3 180 F 1 1324 04 06 04 04 09 00 AMS13 21 11 30 51.9 -44.6 3.9 88.0 -4 1 1 1324 04 09 00 04 17 00 --- 21 19 32 50.9 -44.6 4.0 86.3 476 F 1 1386 04 09 04 04 18 00 J1722+5856 21 20 32 51.2 -45.2 4.0 86.4 57 1 1 1386 04 18 00 04 21 00 =1721+589 21 23 32 50.8 -45.2 4.0 85.8 180 F 1 1409 04 18 04 04 21 00 AMS13 21 23 32 50.4 -44.5 4.1 85.5 -4 1 1 1409 04 21 00 04 29 00 --- 21 31 34 49.4 -44.4 4.2 83.9 476 F 1 1471 04 21 04 04 30 00 J1722+5856 21 32 34 49.7 -45.0 4.2 84.0 57 1 1 1471 04 30 00 04 33 00 =1721+589 21 35 34 49.3 -45.0 4.2 83.4 180 F 1 1494 04 30 04 04 33 00 AMS20 21 35 34 49.1 -44.4 4.2 83.5 -3 1 1 1494 04 33 00 04 41 00 --- 21 43 36 48.1 -44.2 4.4 81.9 477 F 1 1556 04 33 04 04 42 00 J1722+5856 21 44 36 48.1 -44.7 4.4 81.6 57 1 1 1556 04 42 00 04 45 00 =1721+589 21 47 36 47.8 -44.6 4.4 81.1 180 F 1 1579 04 42 04 04 45 00 AMS20 21 47 36 47.6 -44.1 4.4 81.1 -3 1 1 1579 04 45 00 04 53 00 --- 21 55 38 46.6 -43.8 4.6 79.6 477 F 1 1641 04 45 04 04 54 00 J1722+5856 21 56 38 46.6 -44.3 4.6 79.3 57 1 1 1641 04 54 00 04 57 00 =1721+589 21 59 38 46.2 -44.2 4.6 78.8 180 F 1 1664 04 54 04 05 12 00 J2005+7752 22 14 41 53.2 -10.8 2.2 139.5 831 1 1 1664 05 12 00 05 23 00 =2007+777 22 25 42 52.9 -11.5 2.3 136.2 660 F 1 1750 05 12 04 05 25 00 J1722+5856 22 27 43 42.7 -43.0 5.1 73.6 55 1 1 1750 05 25 00 05 28 00 =1721+589 22 30 43 42.3 -42.9 5.1 73.1 180 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 ---------------------------------------------------------------------------------------- --- Sun 11 Mar 2007 Day 70 --- 05 28 00 J1722+6105 22 30 43 42.9 -40.1 5.1 75.0 -8 1 1 1773 05 28 00 05 33 00 =1722+611 22 35 44 42.4 -39.8 5.2 74.0 292 F 1 1811 05 28 04 05 34 00 J1722+5856 22 36 44 41.6 -42.6 5.2 72.0 53 1 1 1811 05 34 00 05 37 00 =1721+589 22 39 45 41.2 -42.4 5.3 71.5 180 F 1 1835 05 34 04 05 37 00 AMS14 22 39 45 40.7 -42.3 5.3 70.7 -4 1 1 1835 05 37 00 05 45 00 --- 22 47 46 39.8 -41.8 5.5 69.3 476 F 1 1897 05 37 04 05 46 00 J1722+5856 22 48 46 40.1 -41.9 5.4 69.8 57 1 1 1897 05 46 00 05 49 00 =1721+589 22 51 47 39.8 -41.7 5.5 69.3 180 F 1 1920 05 46 04 05 49 00 AMS14 22 51 47 39.3 -41.6 5.5 68.6 -4 1 1 1920 05 49 00 05 57 00 --- 22 59 48 38.3 -41.1 5.7 67.2 476 F 1 1982 05 49 04 05 58 00 J1722+5856 23 00 48 38.7 -41.2 5.6 67.7 57 1 1 1982 05 58 00 06 01 00 =1721+589 23 03 49 38.3 -41.0 5.7 67.2 180 F 1 2005 05 58 04 06 01 00 AMS17 23 03 49 38.1 -40.9 5.7 66.8 -3 1 1 2005 06 01 00 06 09 00 --- 23 11 50 37.1 -40.4 5.8 65.4 477 F 1 2067 06 01 04 06 10 00 J1722+5856 23 12 50 37.3 -40.4 5.8 65.6 58 1 1 2067 06 10 00 06 13 00 =1721+589 23 15 51 36.9 -40.2 5.9 65.1 180 F 1 2090 06 10 04 06 13 00 AMS17 23 15 51 36.7 -40.1 5.9 64.7 -3 1 1 2090 06 13 00 06 21 00 --- 23 23 52 35.7 -39.6 6.1 63.4 477 F 1 2152 06 13 04 06 22 00 J1722+5856 23 24 52 35.9 -39.6 6.0 63.6 58 1 1 2152 06 22 00 06 25 00 =1721+589 23 27 53 35.5 -39.3 6.1 63.0 180 F 1 2175 06 22 04 06 25 00 AMS13 23 27 53 35.2 -38.6 6.2 62.6 -3 1 1 2175 06 25 00 06 33 00 --- 23 35 54 34.3 -38.0 6.3 61.2 477 F 1 2237 06 25 04 06 34 00 J1722+5856 23 36 54 34.5 -38.7 6.2 61.5 57 1 1 2237 06 34 00 06 37 00 =1721+589 23 39 55 34.1 -38.5 6.3 61.0 180 F 1 2261 06 34 04 06 37 00 AMS13 23 39 55 33.9 -37.7 6.4 60.5 -3 1 1 2261 06 37 00 06 45 00 --- 23 47 56 33.0 -37.1 6.5 59.1 477 F 1 2322 06 37 04 06 46 00 J1722+5856 23 48 56 33.1 -37.8 6.4 59.4 57 1 1 2322 06 46 00 06 49 00 =1721+589 23 51 57 32.8 -37.5 6.5 58.9 180 F 1 2346 06 46 04 06 49 00 AMS20 23 51 57 32.8 -37.0 6.5 58.8 -3 1 1 2346 06 49 00 06 57 00 --- 23 59 58 31.9 -36.4 6.6 57.4 477 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 ---------------------------------------------------------------------------------------- --- Sun 11 Mar 2007 Day 70 --- 06 58 00 J1722+5856 00 00 58 31.8 -36.8 6.6 57.4 57 1 1 2408 06 58 00 07 01 00 =1721+589 00 03 59 31.5 -36.5 6.7 56.8 180 F 1 2431 06 58 04 07 01 00 AMS20 00 03 59 31.5 -36.1 6.7 56.7 -3 1 1 2431 07 01 00 07 09 00 --- 00 12 00 30.7 -35.4 6.8 55.4 477 F 1 2493 07 01 04 07 10 00 J1722+5856 00 13 00 30.5 -35.8 6.8 55.3 57 1 1 2493 07 10 00 07 15 00 =1721+589 00 18 01 30.0 -35.4 6.9 54.4 300 F 1 2531 07 10 04 07 15 00 J1722+6105 00 18 01 31.2 -33.3 6.9 55.5 -6 1 1 2531 07 15 00 07 21 00 =1722+611 00 24 02 30.6 -32.8 7.0 54.4 354 F 1 2578 07 15 04 07 22 00 J1722+5856 00 25 02 29.3 -34.7 7.0 53.2 53 1 1 2578 07 22 00 07 25 00 =1721+589 00 28 03 28.9 -34.5 7.1 52.7 180 F 1 2601 07 22 04 07 25 00 AMS14 00 28 03 28.5 -34.2 7.2 52.0 -3 1 1 2601 07 25 00 07 33 00 --- 00 36 04 27.7 -33.5 7.3 50.7 477 F 1 2663 07 25 04 07 34 00 J1722+5856 00 37 04 28.0 -33.7 7.2 51.2 57 1 1 2663 07 34 00 07 37 00 =1721+589 00 40 04 27.7 -33.4 7.3 50.7 180 F 1 2686 07 34 04 07 37 00 AMS14 00 40 04 27.3 -33.1 7.4 50.0 -3 1 1 2686 07 37 00 07 45 00 --- 00 48 06 26.5 -32.3 7.5 48.6 477 F 1 2748 07 37 04 07 46 00 J1722+5856 00 49 06 26.8 -32.5 7.4 49.1 57 1 1 2748 07 46 00 07 49 00 =1721+589 00 52 06 26.5 -32.3 7.5 48.6 180 F 1 2771 07 46 04 07 49 00 AMS17 00 52 06 26.3 -32.1 7.5 48.3 -3 1 1 2771 07 49 00 07 57 00 --- 01 00 08 25.6 -31.4 7.7 46.9 477 F 1 2833 07 49 04 07 58 00 J1722+5856 01 01 08 25.7 -31.4 7.6 47.1 58 1 1 2833 07 58 00 08 01 00 =1721+589 01 04 08 25.4 -31.1 7.7 46.5 180 F 1 2857 07 58 04 08 01 00 AMS17 01 04 08 25.2 -31.0 7.7 46.2 -3 1 1 2857 08 01 00 08 09 00 --- 01 12 10 24.4 -30.2 7.9 44.8 477 F 1 2919 08 01 04 08 10 00 J1722+5856 01 13 10 24.6 -30.2 7.8 45.0 58 1 1 2919 08 10 00 08 13 00 =1721+589 01 16 10 24.3 -29.9 7.9 44.5 180 F 1 2942 08 10 04 08 13 00 AMS13 01 16 10 24.2 -29.2 8.0 43.9 -3 1 1 2942 08 13 00 08 21 00 --- 01 24 12 23.5 -28.4 8.1 42.5 477 F 1 3004 08 13 04 08 22 00 J1722+5856 01 25 12 23.5 -29.0 8.0 42.9 57 1 1 3004 08 22 00 08 25 00 =1721+589 01 28 12 23.2 -28.7 8.1 42.4 180 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 ---------------------------------------------------------------------------------------- --- Sun 11 Mar 2007 Day 70 --- 08 25 00 AMS13 01 28 12 23.2 -28.0 8.2 41.8 -3 1 1 3027 08 25 00 08 33 00 --- 01 36 14 22.5 -27.1 8.3 40.4 477 F 1 3089 08 25 04 08 34 00 J1722+5856 01 37 14 22.4 -27.7 8.2 40.8 57 1 1 3089 08 34 00 08 37 00 =1721+589 01 40 14 22.2 -27.4 8.3 40.3 180 F 1 3112 08 34 04 08 37 00 AMS20 01 40 14 22.3 -27.0 8.3 40.1 -3 1 1 3112 08 37 00 08 43 00 --- 01 46 15 21.8 -26.3 8.4 39.1 357 F 1 3159 08 37 04 08 44 00 J1722+5856 01 47 15 21.6 -26.6 8.4 39.1 57 1 1 3159 08 44 00 08 47 00 =1721+589 01 50 16 21.4 -26.3 8.5 38.6 180 F 1 3182 08 44 04 08 47 00 AMS20 01 50 16 21.5 -25.9 8.5 38.4 -3 1 1 3182 08 47 00 08 53 00 --- 01 56 17 21.1 -25.3 8.6 37.3 357 F 1 3228 08 47 04 08 54 00 J1722+5856 01 57 17 20.8 -25.6 8.6 37.3 57 1 1 3228 08 54 00 08 57 00 =1721+589 02 00 18 20.6 -25.2 8.6 36.8 180 F 1 3251 08 54 04 08 57 00 J1722+6105 02 00 18 22.3 -23.8 8.6 37.3 -8 1 1 3251 08 57 00 09 00 00 =1722+611 02 03 18 22.1 -23.5 8.7 36.8 172 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) * AMS13 17 18 01.524102 * 17 18 44.403000 17 18 50.769659 0.00 59 23 01.68907 * 59 20 00.83300 59 19 05.16131 0.00 From catalog imbedded in main SCHED input file. 1.067 scan hours, 35.134 baseline hours above horizon. * AMS14 17 18 00.510454 * 17 18 45.467000 17 18 52.132474 0.00 58 54 23.35754 * 58 51 22.50300 58 50 26.86752 0.00 From catalog imbedded in main SCHED input file. 1.067 scan hours, 35.186 baseline hours above horizon. * AMS20 17 20 16.244303 * 17 20 59.095000 17 21 05.422305 0.00 59 20 41.68858 * 59 17 50.49400 59 16 56.21974 0.00 From catalog imbedded in main SCHED input file. 1.000 scan hours, 32.369 baseline hours above horizon. * AMS17 17 20 00.448488 * 17 20 45.170000 17 20 51.770719 0.00 58 55 13.59647 * 58 52 21.33500 58 51 26.93868 0.00 From catalog imbedded in main SCHED input file. 1.067 scan hours, 35.389 baseline hours above horizon. J1642+3948 16 41 17.606231 * 16 42 58.809968 16 43 13.916489 0.26 1641+399 39 54 10.81494 * 39 48 36.99400 39 47 21.94641 0.40 * 3C345 /SOFT/sched/catalogs/sources.vlba J1642+39 VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.183 scan hours, 6.013 baseline hours above horizon. * J1722+5856 17 21 52.440262 * 17 22 36.726556 17 22 43.235669 0.62 1721+589 58 59 06.49433 * 58 56 22.26071 58 55 29.01987 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 45.125394 0.52 1722+611 61 08 43.42147 * 61 05 59.78736 61 05 06.47932 0.45 /SOFT/sched/catalogs/sources.vlba VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro 0.433 scan hours, 14.013 baseline hours above horizon. * J2005+7752 20 07 20.430185 * 20 05 30.998513 20 05 09.050571 0.96 2007+777 77 43 58.12307 * 77 52 43.24760 77 53 35.90744 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) AMS13 94.0 AMS14 94.0 AMS20 93.7 AMS17 93.7 3C345 100.3 J1722+5856 93.5 J1722+6105 93.5 J2005+7752 86.0 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