COVER INFORMATION Station: KVNYS (Code Ky ) Experiment: RadioAstron polarization imaging Exp. Code: gg083d Schedule Version: 1.20 Processed by SCHED version: 11.40 Release 11.4. March 14, 2015 PI: Jose L. Gomez Address: Instituto de Astrofisica de Andalucia-CSIC Glorieta de la Astronomia E-18008 Granada, Spain Phone: +79165452842 EMAIL: jlgomez@iaa.es, alobanov@mpifr-bonn.mpg.de Fax: Phone during observation: +79165452842 Observing mode: K-band dual-pol Notes: K-band, Radioastron-compatible frequency setup P-CAL is ON Tsys is ON auto-level (AGC) is ON Schedule for KVNYS (Code Ky ) Page 2 RadioAstron polarization imaging UP: D => Below limits; H => Below horizon mask; W => still slewing at end; blank => Up. Early: Seconds between end of slew and start. Dwell: On source seconds. Disk: GBytes recorded to this point. TPStart: Recording start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Disk TPStart Stop UT LST EL AZ HA UP ParA Dwell GBytes SYNC ---------------------------------------------------------------------------------------- --- Thu 8 Feb 2018 Day 39 --- Next scan frequencies: 22236.00 22236.00 22236.00 22236.00 22268.00 22268.00 22268.00 22268.00 Next BBC frequencies: 8986.00 8986.00 8986.00 8986.00 9018.00 9018.00 9018.00 9018.00 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 22 00 00 1226+023 15 43 36 33.2 243.2 3.2 45.1 0 0 21 59 49 22 07 30 --- 15 51 07 31.8 244.8 3.4 45.8 450 30 21 59 50 ---------- K-band VLBI scans. Space segment 01: 1226+023 with EVN ---------- 22 08 00 1226+023 15 51 37 31.7 244.9 3.4 45.9 28 30 22 07 49 22 18 00 --- 16 01 39 29.9 246.9 3.5 46.8 600 69 22 07 50 22 18 30 1226+023 16 02 09 29.8 247.0 3.5 46.9 28 69 22 18 19 22 28 00 --- 16 11 40 28.1 248.8 3.7 47.7 570 106 22 18 20 22 28 30 1226+023 16 12 10 28.0 248.9 3.7 47.7 28 106 22 28 19 22 38 00 --- 16 21 42 26.2 250.7 3.9 48.5 570 143 22 28 20 ---------- KVN observing target during EVN EVPA + FF calibration ---------- 22 38 30 1226+023 16 22 12 26.1 250.8 3.9 48.5 28 143 22 38 19 22 50 30 --- 16 34 14 23.8 253.0 4.1 49.3 720 190 22 38 20 ---------- Block Q-K-bands on target ---------- Next scan frequencies: 43143.25 43143.25 43143.25 43143.25 43175.25 43175.25 43175.25 43175.25 Next BBC frequencies: 9033.25 9033.25 9033.25 9033.25 9065.25 9065.25 9065.25 9065.25 22 51 30 1226+023 16 35 14 23.7 253.1 4.1 49.4 58 190 22 51 19 23 03 30 --- 16 47 16 21.4 255.2 4.3 50.1 720 237 22 51 20 ---------- K-band target ---------- Next scan frequencies: 22236.00 22236.00 22236.00 22236.00 22268.00 22268.00 22268.00 22268.00 Next BBC frequencies: 8986.00 8986.00 8986.00 8986.00 9018.00 9018.00 9018.00 9018.00 23 04 30 1226+023 16 48 16 21.2 255.4 4.3 50.1 58 237 23 04 19 23 14 30 --- 16 58 18 19.2 257.1 4.5 50.6 600 276 23 04 20 ---------- K-band target ---------- 23 14 30 1226+023 16 58 18 19.2 257.1 4.5 50.6 -2 276 No stop 23 24 30 --- 17 08 19 17.3 258.8 4.6 51.1 598 315 23 14 31 ---------- K-band target ---------- 23 24 30 1226+023 17 08 19 17.3 258.8 4.6 51.1 -2 315 No stop 23 34 30 --- 17 18 21 15.3 260.4 4.8 51.4 598 353 23 24 31 Schedule for KVNYS (Code Ky ) Page 3 RadioAstron polarization imaging UP: D => Below limits; H => Below horizon mask; W => still slewing at end; blank => Up. Early: Seconds between end of slew and start. Dwell: On source seconds. Disk: GBytes recorded to this point. TPStart: Recording start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Disk TPStart Stop UT LST EL AZ HA UP ParA Dwell GBytes SYNC ---------------------------------------------------------------------------------------- --- Thu 8 Feb 2018 Day 39 --- ---------- K-band target ---------- 23 34 30 1226+023 17 18 21 15.3 260.4 4.8 51.4 -2 353 No stop 23 44 30 --- 17 28 23 13.4 262.0 5.0 51.8 598 391 23 34 31 23 46 30 1226+023 17 30 23 13.0 262.3 5.0 51.8 118 391 23 46 19 23 54 30 --- 17 38 24 11.4 263.6 5.1 52.0 480 423 23 46 20 --- Start: Thu 8 Feb 2018 Day 39 -- Stop: Fri 9 Feb 2018 Day 40 --- 23 55 00 1226+023 17 38 54 11.3 263.7 5.1 52.0 28 423 23 54 49 00 14 30 --- 17 58 28 7.4 266.7 5.5 52.4 1170 499 23 54 50 ---------- KVN + VLA observing calibrator ---------- 13 30 30 0923+392 07 16 38 64.3 436.6 -2.2 -82.6 47738 499 13 30 19 13 35 30 --- 07 21 39 65.2 436.9 -2.1 -83.2 300 519 13 30 20 Next scan frequencies: 43143.25 43143.25 43143.25 43143.25 43175.25 43175.25 43175.25 43175.25 Next BBC frequencies: 9033.25 9033.25 9033.25 9033.25 9065.25 9065.25 9065.25 9065.25 13 36 30 0923+392 07 22 39 65.4 437.0 -2.1 -83.3 58 519 13 36 19 13 43 30 --- 07 29 41 66.8 437.3 -2.0 -84.0 420 546 13 36 20 Next scan frequencies: 22236.00 22236.00 22236.00 22236.00 22268.00 22268.00 22268.00 22268.00 Next BBC frequencies: 8986.00 8986.00 8986.00 8986.00 9018.00 9018.00 9018.00 9018.00 13 44 30 0923+392 07 30 41 67.0 437.4 -2.0 -84.2 58 546 13 44 19 13 49 30 --- 07 35 42 68.0 437.6 -1.9 -84.7 300 566 13 44 20 ---------- VLA back ---------- 13 54 30 1226+023 07 40 42 15.1 99.4 -4.8 -51.5 182 566 13 54 19 13 55 30 --- 07 41 43 15.3 99.6 -4.8 -51.5 60 571 13 54 20 13 55 40 1226+023 07 41 53 15.4 99.6 -4.8 -51.4 8 571 No stop 14 04 30 --- 07 50 44 17.1 101.0 -4.7 -51.1 530 605 13 55 31 14 05 00 1226+023 07 51 14 17.2 101.1 -4.6 -51.1 28 605 14 04 49 14 06 00 --- 07 52 14 17.4 101.3 -4.6 -51.1 60 610 14 04 50 14 06 10 1226+023 07 52 24 17.4 101.3 -4.6 -51.0 8 610 No stop 14 14 00 --- 08 00 16 18.9 102.6 -4.5 -50.7 470 641 14 06 01 14 14 30 1226+023 08 00 46 19.0 102.7 -4.5 -50.7 28 641 14 14 19 14 15 30 --- 08 01 46 19.2 102.9 -4.5 -50.6 60 645 14 14 20 Schedule for KVNYS (Code Ky ) Page 4 RadioAstron polarization imaging UP: D => Below limits; H => Below horizon mask; W => still slewing at end; blank => Up. Early: Seconds between end of slew and start. Dwell: On source seconds. Disk: GBytes recorded to this point. TPStart: Recording start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Disk TPStart Stop UT LST EL AZ HA UP ParA Dwell GBytes SYNC ---------------------------------------------------------------------------------------- --- Fri 9 Feb 2018 Day 40 --- 14 15 40 1226+023 08 01 56 19.3 102.9 -4.5 -50.6 8 645 No stop 14 23 30 --- 08 09 47 20.8 104.2 -4.3 -50.2 470 676 14 15 31 ---------- Q-band block on target ---------- Next scan frequencies: 43143.25 43143.25 43143.25 43143.25 43175.25 43175.25 43175.25 43175.25 Next BBC frequencies: 9033.25 9033.25 9033.25 9033.25 9065.25 9065.25 9065.25 9065.25 14 25 00 1226+023 08 11 17 21.1 104.5 -4.3 -50.2 88 676 14 24 49 14 35 00 --- 08 21 19 23.0 106.2 -4.1 -49.6 600 715 14 24 50 ---------- All back to K-band ---------- Next scan frequencies: 22236.00 22236.00 22236.00 22236.00 22268.00 22268.00 22268.00 22268.00 Next BBC frequencies: 8986.00 8986.00 8986.00 8986.00 9018.00 9018.00 9018.00 9018.00 14 35 30 1226+023 08 21 49 23.1 106.3 -4.1 -49.6 28 715 14 35 19 14 36 30 --- 08 22 49 23.3 106.5 -4.1 -49.5 60 720 14 35 20 14 36 40 1226+023 08 22 59 23.3 106.5 -4.1 -49.5 8 720 No stop 14 45 00 --- 08 31 21 24.9 108.0 -4.0 -49.0 500 752 14 36 31 14 45 30 1226+023 08 31 51 25.0 108.1 -4.0 -48.9 28 752 14 45 19 14 46 30 --- 08 32 51 25.2 108.3 -4.0 -48.9 60 757 14 45 20 14 46 40 1226+023 08 33 01 25.2 108.3 -4.0 -48.8 8 757 No stop 14 53 30 --- 08 39 52 26.5 109.6 -3.8 -48.4 410 784 14 46 31 ---------- KVN observing calibrator ---------- Next scan frequencies: 43143.25 43143.25 43143.25 43143.25 43175.25 43175.25 43175.25 43175.25 Next BBC frequencies: 9033.25 9033.25 9033.25 9033.25 9065.25 9065.25 9065.25 9065.25 14 55 00 0923+392 08 41 22 80.7 77.8 -0.8 -95.0 69 784 14 54 49 15 00 00 --- 08 46 23 81.7 77.2 -0.7 -96.4 300 804 14 54 50 Next scan frequencies: 22236.00 22236.00 22236.00 22236.00 22268.00 22268.00 22268.00 22268.00 Next BBC frequencies: 8986.00 8986.00 8986.00 8986.00 9018.00 9018.00 9018.00 9018.00 15 01 00 0923+392 08 47 23 81.9 77.0 -0.7 -96.7 58 804 15 00 49 15 06 00 --- 08 52 24 82.8 76.0 -0.6 -98.4 300 824 15 00 50 ---------- LBA + KVN on source ---------- 15 06 30 1226+023 08 52 54 28.9 112.1 -3.6 -47.3 9 824 15 06 19 15 07 30 --- 08 53 54 29.1 112.2 -3.6 -47.2 60 828 15 06 20 15 07 40 1226+023 08 54 04 29.1 112.3 -3.6 -47.2 8 828 No stop 15 16 30 --- 09 02 56 30.7 114.0 -3.5 -46.4 530 863 15 07 31 Schedule for KVNYS (Code Ky ) Page 5 RadioAstron polarization imaging UP: D => Below limits; H => Below horizon mask; W => still slewing at end; blank => Up. Early: Seconds between end of slew and start. Dwell: On source seconds. Disk: GBytes recorded to this point. TPStart: Recording start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Disk TPStart Stop UT LST EL AZ HA UP ParA Dwell GBytes SYNC ---------------------------------------------------------------------------------------- --- Fri 9 Feb 2018 Day 40 --- 15 17 00 1226+023 09 03 26 30.8 114.1 -3.4 -46.4 28 863 15 16 49 15 18 00 --- 09 04 26 31.0 114.3 -3.4 -46.3 60 867 15 16 50 15 18 10 1226+023 09 04 36 31.0 114.4 -3.4 -46.3 8 867 No stop 15 24 30 --- 09 10 57 32.2 115.7 -3.3 -45.6 380 892 15 18 01 ---------- K-band VLBI scans. Space segment 06: 1226+023 with LBA+VLA27+KVN+T6+Ur ---------- 15 25 00 1226+023 09 11 27 32.3 115.8 -3.3 -45.6 28 892 15 24 49 15 26 00 --- 09 12 27 32.4 116.0 -3.3 -45.5 60 897 15 24 50 15 26 10 1226+023 09 12 37 32.5 116.0 -3.3 -45.5 8 897 No stop 15 35 00 --- 09 21 29 34.0 117.9 -3.1 -44.5 530 932 15 26 01 15 35 30 1226+023 09 21 59 34.1 118.0 -3.1 -44.5 28 932 15 35 19 15 36 30 --- 09 22 59 34.3 118.2 -3.1 -44.3 60 936 15 35 20 15 36 40 1226+023 09 23 09 34.3 118.2 -3.1 -44.3 8 936 No stop 15 45 00 --- 09 31 31 35.8 120.1 -3.0 -43.3 500 969 15 36 31 15 45 30 1226+023 09 32 01 35.9 120.2 -3.0 -43.3 28 969 15 45 19 15 46 30 --- 09 33 01 36.0 120.4 -3.0 -43.2 60 973 15 45 20 15 46 40 1226+023 09 33 11 36.1 120.4 -2.9 -43.1 8 973 No stop 15 55 00 --- 09 41 32 37.5 122.4 -2.8 -42.1 500 1006 15 46 31 15 55 30 1226+023 09 42 02 37.6 122.5 -2.8 -42.0 28 1006 15 55 19 15 56 30 --- 09 43 02 37.7 122.7 -2.8 -41.9 60 1011 15 55 20 15 56 40 1226+023 09 43 12 37.7 122.8 -2.8 -41.8 8 1011 No stop 16 05 00 --- 09 51 34 39.1 124.8 -2.6 -40.7 500 1043 15 56 31 Next scan frequencies: 43143.25 43143.25 43143.25 43143.25 43175.25 43175.25 43175.25 43175.25 Next BBC frequencies: 9033.25 9033.25 9033.25 9033.25 9065.25 9065.25 9065.25 9065.25 16 06 00 1226+023 09 52 34 39.3 125.0 -2.6 -40.5 58 1043 16 05 49 16 15 30 --- 10 02 06 40.8 127.4 -2.5 -39.1 570 1081 16 05 50 ---------- KVN observing calibrator ---------- 16 16 30 0923+392 10 03 06 83.0 284.2 0.6 98.8 4 1081 16 16 19 16 21 30 --- 10 08 07 82.0 283.1 0.7 97.0 300 1101 16 16 20 Schedule for KVNYS (Code Ky ) Page 6 RadioAstron polarization imaging UP: D => Below limits; H => Below horizon mask; W => still slewing at end; blank => Up. Early: Seconds between end of slew and start. Dwell: On source seconds. Disk: GBytes recorded to this point. TPStart: Recording start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Disk TPStart Stop UT LST EL AZ HA UP ParA Dwell GBytes SYNC ---------------------------------------------------------------------------------------- --- Fri 9 Feb 2018 Day 40 --- Next scan frequencies: 22236.00 22236.00 22236.00 22236.00 22268.00 22268.00 22268.00 22268.00 Next BBC frequencies: 8986.00 8986.00 8986.00 8986.00 9018.00 9018.00 9018.00 9018.00 16 22 30 0923+392 10 09 07 81.9 283.0 0.7 96.6 58 1101 16 22 19 16 27 30 --- 10 14 08 80.9 282.3 0.8 95.2 300 1120 16 22 20 ---------- All back to target ---------- 16 29 10 1226+023 10 15 48 42.9 131.0 -2.2 -36.8 46 1120 16 28 59 16 30 10 --- 10 16 48 43.1 131.3 -2.2 -36.6 60 1125 16 29 00 16 30 20 1226+023 10 16 58 43.1 131.3 -2.2 -36.5 8 1125 No stop 16 39 10 --- 10 25 49 44.4 133.8 -2.1 -34.9 530 1160 16 30 11 16 39 40 1226+023 10 26 20 44.5 134.0 -2.1 -34.8 28 1160 16 39 29 16 40 40 --- 10 27 20 44.6 134.3 -2.0 -34.6 60 1164 16 39 30 16 40 50 1226+023 10 27 30 44.6 134.3 -2.0 -34.6 8 1164 No stop 16 49 10 --- 10 35 51 45.8 136.8 -1.9 -32.9 500 1197 16 40 41 16 49 40 1226+023 10 36 21 45.8 136.9 -1.9 -32.8 28 1197 16 49 29 16 50 40 --- 10 37 21 46.0 137.2 -1.9 -32.6 60 1201 16 49 30 16 50 50 1226+023 10 37 31 46.0 137.3 -1.9 -32.5 8 1201 No stop 16 57 30 --- 10 44 12 46.9 139.3 -1.8 -31.1 400 1228 16 50 41 ---------- rest on target ---------- 16 58 00 1226+023 10 44 43 47.0 139.5 -1.8 -31.0 28 1228 16 57 49 17 08 00 --- 10 54 44 48.2 142.7 -1.6 -28.7 600 1267 16 57 50 ---------- All back to target ---------- 17 08 30 1226+023 10 55 14 48.3 142.9 -1.6 -28.6 28 1267 17 08 19 17 09 30 --- 10 56 14 48.4 143.2 -1.6 -28.4 60 1271 17 08 20 17 09 40 1226+023 10 56 24 48.4 143.3 -1.6 -28.3 8 1271 No stop 17 18 30 --- 11 05 16 49.4 146.3 -1.4 -26.1 530 1306 17 09 31 17 19 00 1226+023 11 05 46 49.5 146.4 -1.4 -26.0 28 1306 17 18 49 17 20 00 --- 11 06 46 49.6 146.8 -1.4 -25.7 60 1311 17 18 50 17 20 10 1226+023 11 06 56 49.6 146.8 -1.4 -25.7 8 1311 No stop 17 28 30 --- 11 15 18 50.5 149.8 -1.2 -23.5 500 1343 17 20 01 Schedule for KVNYS (Code Ky ) Page 7 RadioAstron polarization imaging UP: D => Below limits; H => Below horizon mask; W => still slewing at end; blank => Up. Early: Seconds between end of slew and start. Dwell: On source seconds. Disk: GBytes recorded to this point. TPStart: Recording start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Disk TPStart Stop UT LST EL AZ HA UP ParA Dwell GBytes SYNC ---------------------------------------------------------------------------------------- --- Fri 9 Feb 2018 Day 40 --- 17 29 00 1226+023 11 15 48 50.5 150.0 -1.2 -23.4 28 1343 17 28 49 17 30 00 --- 11 16 48 50.6 150.3 -1.2 -23.1 60 1348 17 28 50 17 30 10 1226+023 11 16 58 50.6 150.4 -1.2 -23.1 8 1348 No stop 17 38 30 --- 11 25 19 51.4 153.5 -1.1 -20.7 500 1381 17 30 01 Next scan frequencies: 43143.25 43143.25 43143.25 43143.25 43175.25 43175.25 43175.25 43175.25 Next BBC frequencies: 9033.25 9033.25 9033.25 9033.25 9065.25 9065.25 9065.25 9065.25 17 39 00 1226+023 11 25 49 51.5 153.7 -1.1 -20.6 28 1381 17 38 49 17 49 00 --- 11 35 51 52.3 157.5 -0.9 -17.7 600 1420 17 38 50 ---------- KVN observing calibrator ---------- 17 50 00 0923+392 11 36 51 64.8 283.2 2.1 82.9 14 1420 17 49 49 17 55 00 --- 11 41 52 63.9 283.5 2.2 82.4 300 1440 17 49 50 Next scan frequencies: 22236.00 22236.00 22236.00 22236.00 22268.00 22268.00 22268.00 22268.00 Next BBC frequencies: 8986.00 8986.00 8986.00 8986.00 9018.00 9018.00 9018.00 9018.00 17 56 00 0923+392 11 42 52 63.7 283.5 2.2 82.3 58 1440 17 55 49 18 01 00 --- 11 47 53 62.7 283.8 2.3 81.8 300 1460 17 55 50 ---------- All back to target ---------- 18 01 00 1226+023 11 47 53 53.1 162.3 -0.7 -14.0 -44 1460 No stop 18 02 00 --- 11 48 53 53.2 162.7 -0.7 -13.7 16 1463 18 01 01 18 02 10 1226+023 11 49 03 53.2 162.8 -0.7 -13.6 8 1463 No stop 18 11 00 --- 11 57 55 53.6 166.4 -0.5 -10.8 530 1498 18 02 01 18 11 00 1226+023 11 57 55 53.6 166.4 -0.5 -10.8 -2 1498 No stop 18 12 00 --- 11 58 55 53.7 166.8 -0.5 -10.4 58 1502 18 11 01 18 12 10 1226+023 11 59 05 53.7 166.9 -0.5 -10.4 8 1502 No stop 18 19 10 --- 12 06 06 54.0 169.8 -0.4 -8.1 420 1529 18 12 01 ---------- K-band VLBI scans. Space segment 07: 1226+023 with LBA+KVN+T6+Ur ---------- 18 20 00 1226+023 12 06 56 54.0 170.1 -0.4 -7.8 48 1529 18 19 49 18 21 00 --- 12 07 56 54.0 170.6 -0.4 -7.5 60 1534 18 19 50 18 21 10 1226+023 12 08 06 54.0 170.6 -0.4 -7.4 8 1534 No stop 18 30 00 --- 12 16 58 54.3 174.4 -0.2 -4.4 530 1569 18 21 01 18 30 30 1226+023 12 17 28 54.3 174.6 -0.2 -4.3 28 1569 18 30 19 18 31 30 --- 12 18 28 54.3 175.0 -0.2 -3.9 60 1573 18 30 20 Schedule for KVNYS (Code Ky ) Page 8 RadioAstron polarization imaging UP: D => Below limits; H => Below horizon mask; W => still slewing at end; blank => Up. Early: Seconds between end of slew and start. Dwell: On source seconds. Disk: GBytes recorded to this point. TPStart: Recording start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Disk TPStart Stop UT LST EL AZ HA UP ParA Dwell GBytes SYNC ---------------------------------------------------------------------------------------- --- Fri 9 Feb 2018 Day 40 --- 18 31 40 1226+023 12 18 38 54.3 175.1 -0.2 -3.9 8 1573 No stop 18 40 00 --- 12 26 59 54.4 178.7 -0.1 -1.0 500 1606 18 31 31 18 40 30 1226+023 12 27 29 54.4 178.9 -0.0 -0.9 28 1606 18 40 19 18 41 30 --- 12 28 30 54.4 179.3 -0.0 -0.5 60 1610 18 40 20 18 41 40 1226+023 12 28 40 54.4 179.4 -0.0 -0.5 8 1610 No stop 18 50 00 --- 12 37 01 54.4 183.0 0.1 2.4 500 1643 18 41 31 18 50 30 1226+023 12 37 31 54.3 183.2 0.1 2.5 28 1643 18 50 19 18 51 30 --- 12 38 31 54.3 183.6 0.1 2.9 60 1648 18 50 20 18 51 40 1226+023 12 38 41 54.3 183.7 0.1 2.9 8 1648 No stop 19 00 00 --- 12 47 03 54.2 187.3 0.3 5.8 500 1680 18 51 31 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: ra1cm2.set --- WARNING --- This group does not match an entry in the frequency catalog. This might be ok because the catalog is not complete. But be very careful to be sure that the setup is correct. Setup group: 26 Station: KVNYS Total bit rate: 512 Format: MARK5B Bits per sample: 2 Sample rate: 32.000 Number of channels: 8 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 13250.00 13250.00 13250.00 13250.00 13250.00 13250.00 13250.00 13250.00 Net SB= L L U U L L U U IF SB = U U U U U U U U Pol. = RCP LCP RCP LCP RCP LCP RCP LCP BBC = 2 1 2 1 2 1 2 1 BBC SB= L L U U L L U U IF = D C D C D C D C The following frequency sets based on these setups were used. Frequency Set: 9 Setup file default. Used with PCAL = 1MHz LO sum= 22236.00 22236.00 22236.00 22236.00 22268.00 22268.00 22268.00 22268.00 BBC fr= 8986.00 8986.00 8986.00 8986.00 9018.00 9018.00 9018.00 9018.00 Bandwd= 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 Matching frequency sets: 9 10 11 Track assignments are: track1= 2, 4, 6, 8, 10, 12, 14, 16 barrel=roll_off ======== Setup file: ra7mm2.set --- WARNING --- This group does not match an entry in the frequency catalog. This might be ok because the catalog is not complete. But be very careful to be sure that the setup is correct. Setup group: 57 Station: KVNYS Total bit rate: 512 Format: MARK5B Bits per sample: 2 Sample rate: 32.000 Number of channels: 8 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 34110.00 34110.00 34110.00 34110.00 34110.00 34110.00 34110.00 34110.00 Net SB= U U L L U U L L IF SB = U U U U U U U U Pol. = RCP LCP RCP LCP RCP LCP RCP LCP BBC = 2 1 2 1 2 1 2 1 BBC SB= U U L L U U L L IF = D C D C D C D C The following frequency sets based on these setups were used. Frequency Set: 16 Setup file default. Used with PCAL = 1MHz LO sum= 43143.25 43143.25 43143.25 43143.25 43175.25 43175.25 43175.25 43175.25 BBC fr= 9033.25 9033.25 9033.25 9033.25 9065.25 9065.25 9065.25 9065.25 Bandwd= 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 Matching frequency sets: 16 17 18 Track assignments are: track1= 2, 4, 6, 8, 10, 12, 14, 16 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) * FAKERA 11 57 21.769299 * 12 00 00.000000 12 01 00.483936 0.00 85 16 41.77889 * 85 00 00.00000 84 53 47.52470 0.00 From catalog imbedded in main SCHED input file. fake circumpolar target for a TS to look at 1328+307 13 28 49.657778 * 13 31 08.288070 13 31 58.208451 0.00 J1331+3030 30 45 58.64060 * 30 30 32.95924 30 24 50.67595 0.00 * 3C286 ./gg083d_sources.radioastron WSRT calibrator, not for 92cm, rfc_2013d Petrov, 2013, unpublished 542 observati * 0727-115 07 27 58.097813 * 07 30 19.112473 07 31 10.802612 0.00 J0730-1141 -11 34 52.58107 *-11 41 12.60063 -11 43 44.55700 0.00 ./gg083d_sources.radioastron AGN, rfc_2013d Petrov, 2013, unpublished 155894 observations, RA-AO3-04, RA-AO2- * 0923+392 09 23 55.319218 * 09 27 03.013939 09 28 11.366254 0.00 J0927+3902 39 15 23.56637 * 39 02 20.85177 38 57 28.85387 0.00 4C39.25 ./gg083d_sources.radioastron AGN, rfc_2013d Petrov, 2013, unpublished 245863 observations, RA-AO3-04, RA-AO3- * 1226+023 12 26 33.245835 * 12 29 06.699731 12 30 02.412902 0.00 J1229+0203 02 19 43.30547 * 02 03 08.59797 01 57 07.17814 0.00 3C273B ./gg083d_sources.radioastron 3C273 AGN, rfc_2013d Petrov, 2013, unpublished 32011 observations, RA-AO3-04, RA-AO3-0 1253-055 12 53 35.831289 * 12 56 11.166557 12 57 07.519618 0.00 J1256-0547 -05 31 07.99603 *-05 47 21.52489 -05 53 12.02711 0.00 * 3C279 ./gg083d_sources.radioastron AGN, rfc_2013d Petrov, 2013, unpublished 7924 observations, RA-AO3-04, RA-AO3-05 SOURCE SCAN SUMMARY FOR SOURCES LISTED ABOVE Scan hours are for recording scans only. Baseline hours are only counted for scans above horizon at both ends. Source Setup file Frequency sets Observing hours (duplicates not shown) Scan Baseline FAKERA ra1cm2.set 14 5.283 0.000 3C286 ra1cm2.set 53 0.500 0.000 ra2cm2.set 54 0.500 0.000 ra7mm2.set 52 0.500 0.000 0727-115 ra1cm2.set 56 57 58 59 60 1.686 16.383 0923+392 ra1cm2.set 1 2 3 4 5 6 7 9 12 13 29 47 + 1.583 49.745 ra2cm2.set 38 54 0.667 20.333 ra7mm2.set 15 16 19 20 52 1.483 32.239 1226+023 ra1cm2.set 1 2 3 4 5 6 7 9 12 13 29 47 + 20.494 1018.787 ra2cm2.set 38 51 54 0.883 38.200 ra7mm2.set 15 16 19 20 52 1.642 47.821 3C279 ra1cm2.set 56 57 58 59 60 0.164 1.590 EFFECT OF SOLAR CORONA 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) FAKERA 108.7 3C286 123.0 0727-115 140.1 0923+392 155.6 1226+023 134.3 3C279 125.2 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