COVER INFORMATION Station: HART (Code Hh ) Experiment: Are g-ray blazars associated with neutrinos? The case of IC 200109A Exp. Code: rg011 Schedule Version: 2.00 Processed by SCHED version: 11.50 Development version 11.5. Started Apr. 2 PI: M. Giroletti Address: INAF/IRA Bologna, 40129 Italy Phone: +39-051-639-9394 EMAIL: marcello.giroletti@inaf.it Fax: +39-051-639-9431 Phone during observation: +39-347-906-6221 Observing mode: 6cm Notes: Schedule for HART (Code Hh ) Page 2 Are g-ray blazars associated with neutrinos? The case of IC 200109A 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 ---------------------------------------------------------------------------------------- --- Sat 29 Feb 2020 Day 60 --- Next scan frequencies: 4830.49 4830.49 4830.49 4830.49 4894.49 4894.49 4894.49 4894.49 4958.49 4958.49 4958.49 4958.49 5022.49 5022.49 5022.49 5022.49 Next BBC frequencies: 230.49 230.49 230.49 230.49 294.49 294.49 294.49 294.49 358.49 358.49 358.49 358.49 422.49 422.49 422.49 422.49 Next scan bandwidths: 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 18 36 30 1100+122 07 03 24 20.4 64.9 -4.0 0.0 0 0 18 36 30 18 42 30 --- 07 09 25 21.6 64.0 -3.9 0.0 360 93 18 36 31 18 43 10 SOURCEB1 07 10 05 19.1 65.2 -4.1 0.0 7 93 18 43 10 18 44 40 --- 07 11 35 19.4 65.0 -4.1 0.0 90 116 18 43 11 18 45 20 1100+122 07 12 15 22.2 63.6 -3.9 0.0 7 116 18 45 20 18 49 20 --- 07 16 16 23.0 63.0 -3.8 0.0 240 178 18 45 21 18 50 00 SOURCEB2 07 16 56 20.5 64.2 -4.0 0.0 7 178 18 50 00 18 51 30 --- 07 18 26 20.8 64.0 -4.0 0.0 90 201 18 50 01 18 52 10 1100+122 07 19 06 23.5 62.6 -3.8 0.0 7 201 18 52 10 18 56 10 --- 07 23 07 24.3 61.9 -3.7 0.0 240 263 18 52 11 18 56 50 SOURCEC 07 23 47 26.6 62.2 -3.6 0.0 10 263 18 56 50 18 58 20 --- 07 25 17 26.9 61.9 -3.5 0.0 90 286 18 56 51 18 59 00 1100+122 07 25 58 24.9 61.5 -3.6 0.0 11 286 18 59 00 19 03 00 --- 07 29 58 25.7 60.9 -3.6 0.0 240 348 18 59 01 19 03 40 SOURCEB1 07 30 38 23.3 62.1 -3.8 0.0 7 348 19 03 40 19 05 10 --- 07 32 09 23.6 61.9 -3.7 0.0 90 371 19 03 41 19 05 50 1100+122 07 32 49 26.2 60.4 -3.5 0.0 7 371 19 05 50 19 09 50 --- 07 36 49 27.0 59.7 -3.5 0.0 240 433 19 05 51 19 10 30 SOURCEB2 07 37 29 24.6 61.0 -3.6 0.0 7 433 19 10 30 19 12 00 --- 07 39 00 24.9 60.8 -3.6 0.0 90 456 19 10 31 19 12 40 1100+122 07 39 40 27.6 59.3 -3.4 0.0 7 456 19 12 40 19 16 40 --- 07 43 41 28.4 58.6 -3.3 0.0 240 518 19 12 41 19 17 20 SOURCEC 07 44 21 30.6 58.7 -3.2 0.0 10 518 19 17 20 19 18 50 --- 07 45 51 30.9 58.4 -3.2 0.0 90 541 19 17 21 19 19 30 1100+122 07 46 31 28.9 58.1 -3.3 0.0 11 541 19 19 30 19 23 30 --- 07 50 32 29.7 57.4 -3.2 0.0 240 603 19 19 31 Schedule for HART (Code Hh ) Page 3 Are g-ray blazars associated with neutrinos? The case of IC 200109A 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 ---------------------------------------------------------------------------------------- --- Sat 29 Feb 2020 Day 60 --- 19 24 10 SOURCEB1 07 51 12 27.3 58.8 -3.4 0.0 7 603 19 24 10 19 25 40 --- 07 52 42 27.6 58.6 -3.4 0.0 90 626 19 24 11 19 26 20 1100+122 07 53 22 30.2 56.9 -3.2 0.0 7 626 19 26 20 19 30 20 --- 07 57 23 30.9 56.1 -3.1 0.0 240 688 19 26 21 19 31 00 SOURCEB2 07 58 03 28.6 57.6 -3.3 0.0 7 688 19 31 00 19 32 30 --- 07 59 33 28.9 57.4 -3.3 0.0 90 711 19 31 01 19 33 10 1100+122 08 00 13 31.5 55.6 -3.1 0.0 7 711 19 33 10 19 37 10 --- 08 04 14 32.2 54.8 -3.0 0.0 240 773 19 33 11 19 37 50 SOURCEC 08 04 54 34.5 54.8 -2.9 0.0 10 773 19 37 50 19 39 20 --- 08 06 24 34.7 54.5 -2.9 0.0 90 796 19 37 51 19 40 00 1100+122 08 07 04 32.7 54.3 -3.0 0.0 11 796 19 40 00 19 44 00 --- 08 11 05 33.5 53.5 -2.9 0.0 240 858 19 40 01 19 45 40 1156+295 08 12 45 12.5 48.6 -3.8 0.0 38 858 19 45 40 19 48 40 --- 08 15 46 13.0 48.2 -3.7 0.0 180 904 19 45 41 19 50 20 1100+122 08 17 26 34.6 52.2 -2.8 0.0 38 904 19 50 20 19 56 20 --- 08 23 27 35.7 51.0 -2.7 0.0 360 997 19 50 21 19 57 05 SOURCEB1 08 24 12 33.4 52.8 -2.9 0.0 12 997 19 57 05 19 58 35 --- 08 25 42 33.7 52.5 -2.8 0.0 90 1020 19 57 06 19 59 20 1100+122 08 26 28 36.2 50.3 -2.6 0.0 12 1020 19 59 20 20 03 20 --- 08 30 28 36.9 49.5 -2.6 0.0 240 1082 19 59 21 20 04 05 SOURCEB2 08 31 13 34.7 51.3 -2.7 0.0 12 1082 20 04 05 20 05 35 --- 08 32 44 34.9 51.0 -2.7 0.0 90 1105 20 04 06 20 06 20 1100+122 08 33 29 37.4 48.8 -2.5 0.0 12 1105 20 06 20 20 10 20 --- 08 37 29 38.1 47.9 -2.4 0.0 240 1167 20 06 21 20 11 00 SOURCEC 08 38 09 40.3 47.6 -2.3 0.0 10 1167 20 11 00 20 12 30 --- 08 39 40 40.5 47.2 -2.3 0.0 90 1190 20 11 01 20 13 10 1100+122 08 40 20 38.5 47.3 -2.4 0.0 11 1190 20 13 10 20 17 10 --- 08 44 20 39.2 46.3 -2.3 0.0 240 1252 20 13 11 20 17 55 SOURCEB1 08 45 06 37.1 48.4 -2.5 0.0 12 1252 20 17 55 20 19 25 --- 08 46 36 37.3 48.0 -2.5 0.0 90 1275 20 17 56 Schedule for HART (Code Hh ) Page 4 Are g-ray blazars associated with neutrinos? The case of IC 200109A 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 ---------------------------------------------------------------------------------------- --- Sat 29 Feb 2020 Day 60 --- 20 20 10 1100+122 08 47 21 39.7 45.6 -2.3 0.0 12 1275 20 20 10 20 24 10 --- 08 51 22 40.3 44.6 -2.2 0.0 240 1337 20 20 11 20 24 55 SOURCEB2 08 52 07 38.2 46.8 -2.4 0.0 12 1337 20 24 55 20 26 25 --- 08 53 37 38.5 46.4 -2.4 0.0 90 1360 20 24 56 20 27 10 1100+122 08 54 22 40.8 43.9 -2.2 0.0 12 1360 20 27 10 20 31 10 --- 08 58 23 41.4 42.9 -2.1 0.0 240 1422 20 27 11 20 31 50 SOURCEC 08 59 03 43.6 42.3 -2.0 0.0 10 1422 20 31 50 20 33 20 --- 09 00 33 43.8 41.9 -2.0 0.0 90 1445 20 31 51 20 34 00 1100+122 09 01 13 41.8 42.2 -2.0 0.0 11 1445 20 34 00 20 38 00 --- 09 05 14 42.4 41.1 -2.0 0.0 240 1507 20 34 01 20 38 45 SOURCEB1 09 05 59 40.4 43.5 -2.2 0.0 12 1507 20 38 45 20 40 15 --- 09 07 29 40.7 43.1 -2.1 0.0 90 1530 20 38 46 20 41 00 1100+122 09 08 14 42.9 40.3 -1.9 0.0 12 1530 20 41 00 20 45 00 --- 09 12 15 43.5 39.2 -1.9 0.0 240 1592 20 41 01 20 45 45 SOURCEB2 09 13 00 41.5 41.7 -2.0 0.0 12 1592 20 45 45 20 47 15 --- 09 14 30 41.7 41.3 -2.0 0.0 90 1615 20 45 46 20 48 00 1100+122 09 15 16 43.9 38.4 -1.8 0.0 12 1615 20 48 00 20 52 00 --- 09 19 16 44.4 37.3 -1.7 0.0 240 1677 20 48 01 20 52 40 SOURCEC 09 19 56 46.6 36.4 -1.6 0.0 10 1677 20 52 40 20 54 10 --- 09 21 27 46.8 35.9 -1.6 0.0 90 1700 20 52 41 20 54 50 1100+122 09 22 07 44.8 36.4 -1.7 0.0 11 1700 20 54 50 20 58 50 --- 09 26 07 45.3 35.3 -1.6 0.0 240 1762 20 54 51 21 00 35 1156+295 09 27 53 23.9 36.2 -2.5 0.0 43 1762 21 00 35 21 03 35 --- 09 30 53 24.3 35.6 -2.5 0.0 180 1809 21 00 36 21 13 10 1100+122 09 40 30 47.1 30.9 -1.4 0.0 513 1809 21 13 10 21 19 10 --- 09 46 31 47.8 28.9 -1.3 0.0 360 1901 21 13 11 21 19 55 SOURCEB1 09 47 16 46.1 32.0 -1.5 0.0 12 1901 21 19 55 21 21 25 --- 09 48 46 46.3 31.6 -1.4 0.0 90 1925 21 19 56 21 22 10 1100+122 09 49 31 48.1 28.0 -1.2 0.0 12 1925 21 22 10 21 26 10 --- 09 53 32 48.5 26.6 -1.2 0.0 240 1986 21 22 11 Schedule for HART (Code Hh ) Page 5 Are g-ray blazars associated with neutrinos? The case of IC 200109A 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 ---------------------------------------------------------------------------------------- --- Sat 29 Feb 2020 Day 60 --- 21 26 55 SOURCEB2 09 54 17 46.9 29.8 -1.4 0.0 12 1986 21 26 55 21 28 25 --- 09 55 47 47.1 29.3 -1.3 0.0 90 2010 21 26 56 21 29 10 1100+122 09 56 32 48.8 25.6 -1.1 0.0 12 2010 21 29 10 21 33 10 --- 10 00 33 49.2 24.2 -1.1 0.0 240 2071 21 29 11 21 33 50 SOURCEC 10 01 13 51.2 22.6 -0.9 0.0 10 2071 21 33 50 21 35 20 --- 10 02 43 51.3 22.0 -0.9 0.0 90 2095 21 33 51 21 36 00 1100+122 10 03 23 49.5 23.2 -1.0 0.0 11 2095 21 36 00 21 40 00 --- 10 07 24 49.8 21.8 -0.9 0.0 240 2156 21 36 01 21 40 45 SOURCEB1 10 08 09 48.4 25.3 -1.1 0.0 12 2156 21 40 45 21 42 15 --- 10 09 39 48.5 24.8 -1.1 0.0 90 2180 21 40 46 21 43 00 1100+122 10 10 25 50.0 20.7 -0.9 0.0 12 2180 21 43 00 21 47 00 --- 10 14 25 50.4 19.3 -0.8 0.0 240 2241 21 43 01 21 47 45 SOURCEB2 10 15 10 49.0 22.8 -1.0 0.0 12 2241 21 47 45 21 49 15 --- 10 16 41 49.2 22.3 -1.0 0.0 90 2265 21 47 46 21 50 00 1100+122 10 17 26 50.6 18.2 -0.8 0.0 12 2265 21 50 00 21 54 00 --- 10 21 26 50.8 16.7 -0.7 0.0 240 2326 21 50 01 21 54 40 SOURCEC 10 22 06 52.7 14.6 -0.6 0.0 10 2326 21 54 40 21 56 10 --- 10 23 37 52.8 14.0 -0.6 0.0 90 2350 21 54 41 21 56 50 1100+122 10 24 17 51.0 15.6 -0.7 0.0 11 2350 21 56 50 22 00 50 --- 10 28 17 51.3 14.1 -0.6 0.0 240 2411 21 56 51 22 01 35 SOURCEB1 10 29 03 50.1 17.9 -0.8 0.0 12 2411 22 01 35 22 03 05 --- 10 30 33 50.2 17.4 -0.8 0.0 90 2435 22 01 36 22 03 50 1100+122 10 31 18 51.4 12.9 -0.5 0.0 12 2435 22 03 50 22 07 50 --- 10 35 19 51.6 11.4 -0.5 0.0 240 2497 22 03 51 22 08 35 SOURCEB2 10 36 04 50.6 15.3 -0.7 0.0 12 2497 22 08 35 22 10 05 --- 10 37 34 50.7 14.7 -0.6 0.0 90 2520 22 08 36 22 10 50 1100+122 10 38 19 51.7 10.2 -0.4 0.0 12 2520 22 10 50 22 14 50 --- 10 42 20 51.9 8.7 -0.4 0.0 240 2582 22 10 51 22 15 30 SOURCEC 10 43 00 53.5 6.2 -0.2 0.0 10 2582 22 15 30 22 17 00 --- 10 44 30 53.6 5.5 -0.2 0.0 90 2605 22 15 31 Schedule for HART (Code Hh ) Page 6 Are g-ray blazars associated with neutrinos? The case of IC 200109A 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 ---------------------------------------------------------------------------------------- --- Sat 29 Feb 2020 Day 60 --- 22 17 40 1100+122 10 45 10 52.0 7.5 -0.3 0.0 11 2605 22 17 40 22 21 40 --- 10 49 11 52.1 6.0 -0.2 0.0 240 2667 22 17 41 22 23 40 1156+295 10 51 11 32.5 18.0 -1.2 0.0 58 2667 22 23 40 22 26 40 --- 10 54 12 32.7 17.2 -1.1 0.0 180 2713 22 23 41 22 28 30 1100+122 10 56 02 52.2 3.2 -0.1 0.0 48 2713 22 28 30 22 36 30 --- 11 04 03 52.2 0.0 -0.0 0.0 480 2837 22 28 31 22 36 35 1100+122 11 04 08 52.2 360.0 0.0 0.0 -16 2837 No stop 22 38 35 --- 11 06 09 52.2 359.2 0.0 0.0 104 2869 22 36 31 22 39 20 SOURCEB1 11 06 54 51.7 3.5 -0.1 0.0 12 2869 22 39 20 22 40 50 --- 11 08 24 51.7 2.9 -0.1 0.0 90 2892 22 39 21 22 41 35 1100+122 11 09 09 52.2 358.0 0.1 0.0 12 2892 22 41 35 22 45 35 --- 11 13 10 52.2 356.4 0.2 0.0 240 2954 22 41 36 22 46 20 SOURCEB2 11 13 55 51.8 0.6 -0.0 0.0 12 2954 22 46 20 22 47 50 --- 11 15 25 51.8 0.1 -0.0 0.0 90 2977 22 46 21 22 48 35 1100+122 11 16 10 52.1 355.2 0.2 0.0 12 2977 22 48 35 22 52 35 --- 11 20 11 52.0 353.6 0.3 0.0 240 3039 22 48 36 22 53 15 SOURCEC 11 20 51 53.3 350.5 0.4 0.0 10 3039 22 53 15 22 54 45 --- 11 22 21 53.2 349.9 0.4 0.0 90 3062 22 53 16 22 55 25 1100+122 11 23 01 52.0 352.5 0.3 0.0 11 3062 22 55 25 22 59 25 --- 11 27 02 51.8 350.9 0.4 0.0 240 3124 22 55 26 23 00 10 SOURCEB1 11 27 47 51.7 355.2 0.2 0.0 12 3124 23 00 10 23 01 40 --- 11 29 17 51.6 354.6 0.2 0.0 90 3147 23 00 11 23 02 25 1100+122 11 30 03 51.7 349.7 0.4 0.0 12 3147 23 02 25 23 06 25 --- 11 34 03 51.6 348.2 0.5 0.0 240 3209 23 02 26 23 07 10 SOURCEB2 11 34 48 51.5 352.4 0.3 0.0 12 3209 23 07 10 23 08 40 --- 11 36 19 51.4 351.9 0.3 0.0 90 3232 23 07 11 23 09 25 1100+122 11 37 04 51.4 347.0 0.5 0.0 12 3232 23 09 25 23 13 25 --- 11 41 04 51.2 345.5 0.6 0.0 240 3294 23 09 26 23 14 05 SOURCEC 11 41 45 52.2 342.2 0.7 0.0 10 3294 23 14 05 23 15 35 --- 11 43 15 52.1 341.7 0.8 0.0 90 3317 23 14 06 Schedule for HART (Code Hh ) Page 7 Are g-ray blazars associated with neutrinos? The case of IC 200109A 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 ---------------------------------------------------------------------------------------- --- Sat 29 Feb 2020 Day 60 --- 23 16 15 1100+122 11 43 55 51.0 344.4 0.7 0.0 11 3317 23 16 15 23 20 15 --- 11 47 56 50.8 342.9 0.7 0.0 240 3379 23 16 16 23 21 00 SOURCEB1 11 48 41 50.9 347.1 0.6 0.0 12 3379 23 21 00 23 22 30 --- 11 50 11 50.9 346.6 0.6 0.0 90 3402 23 21 01 23 23 15 1100+122 11 50 56 50.6 341.8 0.8 0.0 12 3402 23 23 15 23 27 15 --- 11 54 57 50.3 340.3 0.8 0.0 240 3464 23 23 16 23 28 00 SOURCEB2 11 55 42 50.5 344.5 0.7 0.0 12 3464 23 28 00 23 29 30 --- 11 57 12 50.4 343.9 0.7 0.0 90 3487 23 28 01 23 30 15 1100+122 11 57 57 50.0 339.2 0.9 0.0 12 3487 23 30 15 23 34 15 --- 12 01 58 49.7 337.8 1.0 0.0 240 3549 23 30 16 23 34 55 SOURCEC 12 02 38 50.4 334.5 1.1 0.0 10 3549 23 34 55 23 36 25 --- 12 04 08 50.3 334.0 1.1 0.0 90 3572 23 34 56 23 37 05 1100+122 12 04 48 49.5 336.8 1.0 0.0 11 3572 23 37 05 23 41 05 --- 12 08 49 49.1 335.4 1.1 0.0 240 3634 23 37 06 23 43 05 1156+295 12 10 49 34.9 357.3 0.2 0.0 58 3634 23 43 05 23 46 05 --- 12 13 50 34.9 356.5 0.2 0.0 180 3680 23 43 06 23 48 05 1100+122 12 15 50 48.4 333.0 1.2 0.0 58 3680 23 48 05 23 54 05 --- 12 21 51 47.8 331.0 1.3 0.0 360 3773 23 48 06 23 54 50 SOURCEB1 12 22 36 48.4 334.9 1.1 0.0 12 3773 23 54 50 23 56 20 --- 12 24 06 48.3 334.4 1.1 0.0 90 3796 23 54 51 --- Start: Sat 29 Feb 2020 Day 60 -- Stop: Sun 1 Mar 2020 Day 61 --- 23 57 05 1100+122 12 24 52 47.4 330.0 1.3 0.0 12 3796 23 57 05 00 01 05 --- 12 28 52 47.0 328.8 1.4 0.0 240 3858 23 57 06 00 01 50 SOURCEB2 12 29 37 47.7 332.5 1.2 0.0 12 3858 00 01 50 00 03 20 --- 12 31 08 47.6 332.0 1.3 0.0 90 3881 00 01 51 00 04 05 1100+122 12 31 53 46.6 327.8 1.5 0.0 12 3881 00 04 05 00 08 05 --- 12 35 53 46.1 326.6 1.5 0.0 240 3943 00 04 06 00 08 45 SOURCEC 12 36 33 46.5 323.4 1.6 0.0 10 3943 00 08 45 00 10 15 --- 12 38 04 46.3 322.9 1.7 0.0 90 3966 00 08 46 Schedule for HART (Code Hh ) Page 8 Are g-ray blazars associated with neutrinos? The case of IC 200109A 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 ---------------------------------------------------------------------------------------- --- Sun 1 Mar 2020 Day 61 --- 00 10 55 1100+122 12 38 44 45.8 325.7 1.6 0.0 11 3966 00 10 55 00 14 55 --- 12 42 45 45.3 324.5 1.6 0.0 240 4028 00 10 56 00 15 40 SOURCEB1 12 43 30 46.2 328.2 1.5 0.0 12 4028 00 15 40 00 17 10 --- 12 45 00 46.0 327.7 1.5 0.0 90 4051 00 15 41 00 17 55 1100+122 12 45 45 44.9 323.7 1.7 0.0 12 4051 00 17 55 00 21 55 --- 12 49 46 44.3 322.5 1.8 0.0 240 4113 00 17 56 00 22 40 SOURCEB2 12 50 31 45.3 326.0 1.6 0.0 12 4113 00 22 40 00 24 10 --- 12 52 01 45.1 325.6 1.6 0.0 90 4136 00 22 41 00 24 55 1100+122 12 52 46 43.9 321.7 1.8 0.0 12 4136 00 24 55 00 28 55 --- 12 56 47 43.3 320.6 1.9 0.0 240 4198 00 24 56 00 29 35 SOURCEC 12 57 27 43.5 317.5 2.0 0.0 10 4198 00 29 35 00 31 05 --- 12 58 57 43.3 317.1 2.0 0.0 90 4221 00 29 36 00 31 45 1100+122 12 59 37 42.9 319.8 1.9 0.0 11 4221 00 31 45 00 35 45 --- 13 03 38 42.3 318.7 2.0 0.0 240 4283 00 31 46 00 36 30 SOURCEB1 13 04 23 43.5 322.0 1.8 0.0 12 4283 00 36 30 00 38 00 --- 13 05 53 43.3 321.6 1.8 0.0 90 4306 00 36 31 00 38 45 1100+122 13 06 38 41.9 317.9 2.0 0.0 12 4306 00 38 45 00 42 45 --- 13 10 39 41.3 316.9 2.1 0.0 240 4368 00 38 46 00 43 30 SOURCEB2 13 11 24 42.5 320.1 1.9 0.0 12 4368 00 43 30 00 45 00 --- 13 12 54 42.3 319.7 2.0 0.0 90 4391 00 43 31 00 45 45 1100+122 13 13 40 40.8 316.2 2.2 0.0 12 4391 00 45 45 00 49 45 --- 13 17 40 40.2 315.2 2.2 0.0 240 4453 00 45 46 00 50 25 SOURCEC 13 18 20 40.2 312.2 2.3 0.0 10 4453 00 50 25 00 51 55 --- 13 19 51 39.9 311.9 2.4 0.0 90 4476 00 50 26 00 52 35 1100+122 13 20 31 39.7 314.5 2.3 0.0 11 4476 00 52 35 00 56 35 --- 13 24 31 39.1 313.5 2.3 0.0 240 4538 00 52 36 00 58 20 1156+295 13 26 17 31.3 338.1 1.4 0.0 43 4538 00 58 20 01 01 20 --- 13 29 17 31.0 337.4 1.5 0.0 180 4585 00 58 21 01 04 20 OQ208 13 32 18 35.1 9.6 -0.6 0.0 90 4585 01 04 20 01 07 20 --- 13 35 18 35.2 8.8 -0.5 0.0 180 4631 01 04 21 Schedule for HART (Code Hh ) Page 9 Are g-ray blazars associated with neutrinos? The case of IC 200109A 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 ---------------------------------------------------------------------------------------- --- Sun 1 Mar 2020 Day 61 --- 01 11 10 1100+122 13 39 09 36.6 310.2 2.6 0.0 110 4631 01 11 10 01 17 10 --- 13 45 10 35.6 308.9 2.7 0.0 360 4724 01 11 11 01 17 55 SOURCEB1 13 45 55 37.1 311.7 2.5 0.0 12 4724 01 17 55 01 19 25 --- 13 47 25 36.9 311.4 2.5 0.0 90 4747 01 17 56 01 20 10 1100+122 13 48 10 35.1 308.3 2.7 0.0 12 4747 01 20 10 01 24 10 --- 13 52 11 34.4 307.5 2.8 0.0 240 4809 01 20 11 01 24 55 SOURCEB2 13 52 56 35.9 310.1 2.6 0.0 12 4809 01 24 55 01 26 25 --- 13 54 26 35.6 309.8 2.6 0.0 90 4832 01 24 56 01 27 10 1100+122 13 55 11 33.8 306.9 2.9 0.0 12 4832 01 27 10 01 31 10 --- 13 59 12 33.1 306.1 2.9 0.0 240 4894 01 27 11 01 31 50 SOURCEC 13 59 52 32.8 303.4 3.0 0.0 10 4894 01 31 50 01 33 20 --- 14 01 22 32.5 303.2 3.1 0.0 90 4917 01 31 51 01 34 00 1100+122 14 02 02 32.6 305.5 3.0 0.0 11 4917 01 34 00 01 38 00 --- 14 06 03 31.8 304.8 3.0 0.0 240 4979 01 34 01 01 38 45 SOURCEB1 14 06 48 33.5 307.3 2.9 0.0 12 4979 01 38 45 01 40 15 --- 14 08 19 33.2 307.0 2.9 0.0 90 5002 01 38 46 01 41 00 1100+122 14 09 04 31.3 304.2 3.1 0.0 12 5002 01 41 00 01 45 00 --- 14 13 04 30.5 303.5 3.1 0.0 240 5064 01 41 01 01 45 45 SOURCEB2 14 13 49 32.2 305.9 3.0 0.0 12 5064 01 45 45 01 47 15 --- 14 15 20 31.9 305.6 3.0 0.0 90 5087 01 45 46 01 48 00 1100+122 14 16 05 30.0 302.9 3.2 0.0 12 5087 01 48 00 01 52 00 --- 14 20 05 29.2 302.2 3.3 0.0 240 5149 01 48 01 01 52 40 SOURCEC 14 20 46 28.8 299.7 3.4 0.0 10 5149 01 52 40 01 54 10 --- 14 22 16 28.5 299.4 3.4 0.0 90 5172 01 52 41 01 54 50 1100+122 14 22 56 28.7 301.7 3.3 0.0 11 5172 01 54 50 01 58 50 --- 14 26 57 27.9 301.0 3.4 0.0 240 5234 01 54 51 01 59 35 SOURCEB1 14 27 42 29.6 303.3 3.2 0.0 12 5234 01 59 35 02 01 05 --- 14 29 12 29.4 303.1 3.2 0.0 90 5257 01 59 36 02 01 50 1100+122 14 29 57 27.3 300.5 3.4 0.0 12 5257 02 01 50 02 05 50 --- 14 33 58 26.5 299.8 3.5 0.0 240 5319 02 01 51 Schedule for HART (Code Hh ) Page 10 Are g-ray blazars associated with neutrinos? The case of IC 200109A 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 ---------------------------------------------------------------------------------------- --- Sun 1 Mar 2020 Day 61 --- 02 06 35 SOURCEB2 14 34 43 28.3 302.1 3.3 0.0 12 5319 02 06 35 02 08 05 --- 14 36 13 28.0 301.8 3.3 0.0 90 5342 02 06 36 02 08 50 1100+122 14 36 58 25.9 299.4 3.5 0.0 12 5342 02 08 50 02 12 50 --- 14 40 59 25.2 298.7 3.6 0.0 240 5404 02 08 51 02 13 30 SOURCEC 14 41 39 24.6 296.3 3.7 0.0 10 5404 02 13 30 02 15 00 --- 14 43 09 24.3 296.1 3.8 0.0 90 5427 02 13 31 02 15 40 1100+122 14 43 49 24.6 298.3 3.7 0.0 11 5427 02 15 40 02 19 40 --- 14 47 50 23.8 297.6 3.7 0.0 240 5489 02 15 41 02 21 25 1156+295 14 49 35 21.7 320.8 2.8 0.0 43 5489 02 21 25 02 24 25 --- 14 52 36 21.2 320.3 2.9 0.0 180 5535 02 21 26 02 25 55 1100+122 14 54 06 22.5 296.7 3.8 0.0 28 5535 02 25 55 02 33 55 --- 15 02 07 20.9 295.5 4.0 0.0 480 5659 02 25 56 02 34 00 1100+122 15 02 12 20.9 295.5 4.0 0.0 -16 5659 No stop 02 36 00 --- 15 04 13 20.5 295.2 4.0 0.0 104 5691 02 33 56 02 36 40 SOURCEB1 15 04 53 22.4 297.2 3.8 0.0 7 5691 02 36 40 02 38 10 --- 15 06 23 22.1 297.0 3.8 0.0 90 5714 02 36 41 02 38 50 1100+122 15 07 03 19.9 294.8 4.0 0.0 7 5714 02 38 50 02 42 50 --- 15 11 04 19.1 294.2 4.1 0.0 240 5776 02 38 51 02 43 30 SOURCEB2 15 11 44 21.0 296.2 3.9 0.0 7 5776 02 43 30 02 45 00 --- 15 13 14 20.7 296.0 4.0 0.0 90 5799 02 43 31 02 45 40 1100+122 15 13 54 18.5 293.8 4.2 0.0 7 5799 02 45 40 02 49 40 --- 15 17 55 17.7 293.2 4.2 0.0 240 5861 02 45 41 02 50 20 SOURCEC 15 18 35 17.0 291.0 4.3 0.0 10 5861 02 50 20 02 51 50 --- 15 20 05 16.7 290.8 4.4 0.0 90 5884 02 50 21 02 52 30 1100+122 15 20 45 17.1 292.9 4.3 0.0 11 5884 02 52 30 02 56 30 --- 15 24 46 16.3 292.3 4.3 0.0 240 5946 02 52 31 02 57 10 SOURCEB1 15 25 26 18.3 294.2 4.2 0.0 7 5946 02 57 10 02 58 40 --- 15 26 56 17.9 294.0 4.2 0.0 90 5969 02 57 11 02 59 20 1100+122 15 27 37 15.7 291.9 4.4 0.0 7 5969 02 59 20 03 03 20 --- 15 31 37 14.8 291.4 4.5 0.0 240 6031 02 59 21 Schedule for HART (Code Hh ) Page 11 Are g-ray blazars associated with neutrinos? The case of IC 200109A 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 ---------------------------------------------------------------------------------------- --- Sun 1 Mar 2020 Day 61 --- 03 04 00 SOURCEB2 15 32 17 16.8 293.3 4.3 0.0 7 6031 03 04 00 03 05 30 --- 15 33 48 16.5 293.1 4.3 0.0 90 6055 03 04 01 03 06 10 1100+122 15 34 28 14.2 291.0 4.5 0.0 7 6055 03 06 10 03 10 10 --- 15 38 28 13.4 290.5 4.6 0.0 240 6116 03 06 11 03 10 50 SOURCEC 15 39 08 12.7 288.3 4.7 0.0 10 6116 03 10 50 03 12 20 --- 15 40 39 12.3 288.2 4.7 0.0 90 6140 03 10 51 03 13 00 1100+122 15 41 19 12.8 290.2 4.6 0.0 11 6140 03 13 00 03 17 00 --- 15 45 19 11.9 289.6 4.7 0.0 240 6201 03 13 01 03 17 40 SOURCEB1 15 46 00 14.0 291.5 4.5 0.0 7 6201 03 17 40 03 19 10 --- 15 47 30 13.7 291.3 4.5 0.0 90 6225 03 17 41 03 19 50 1100+122 15 48 10 11.3 289.3 4.7 0.0 7 6225 03 19 50 03 23 50 --- 15 52 11 10.5 288.8 4.8 0.0 240 6286 03 19 51 03 24 30 SOURCEB2 15 52 51 12.5 290.6 4.6 0.0 7 6286 03 24 30 03 26 00 --- 15 54 21 12.2 290.4 4.6 0.0 90 6310 03 24 31 03 26 40 1100+122 15 55 01 9.9 288.5 4.8 0.0 7 6310 03 26 40 03 30 40 --- 15 59 02 9.0 288.0 4.9 0.0 240 6371 03 26 41 03 31 20 SOURCEC 15 59 42 8.2 285.8 5.0 0.0 10 6371 03 31 20 03 32 50 --- 16 01 12 7.9 285.7 5.1 D 0.0 0 6395 03 31 21 03 33 30 1100+122 16 01 52 8.4 287.6 5.0 0.0 11 6395 03 33 30 03 37 30 --- 16 05 53 7.6 287.2 5.0 D 0.0 0 6456 03 33 31 03 39 25 1156+295 16 07 48 9.1 308.8 4.1 H 0.0 53 6456 03 39 25 03 42 25 --- 16 10 49 8.6 308.4 4.2 H 0.0 0 6503 03 39 26 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess120.C2048 Matching groups in /home/guest/rmc/SCHED/sched11.5/catalogs/freq_RDBE.dat: hh6cm Values confirmed by E-mail Jonathan Quick 20140219 (CR) ****** Only 256.00 of 512.00 MHz total bandwidth is within the IFs in the setup file before any FREQ or DOPPLER shifts. Setup group: 7 Station: HART Total bit rate: 2048 Format: VDIF Bits per sample: 2 Sample rate: 64.000 Number of channels: 16 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 4600.00 Net SB= L L U U L L U U L L U U L L U U IF SB = U U U U U U U U U U U U U U U U Pol. = RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP BBC = 1 9 1 9 2 10 2 10 3 11 3 11 4 12 4 12 BBC SB= L L U U L L U U L L U U L L U U IF = A1 C1 A1 C1 A1 C1 A1 C1 A1 C1 A1 C1 A1 C1 A1 C1 The following frequency sets based on these setups were used. Frequency Set: 13 Setup file default. Used with PCAL = off LO sum= 4830.49 4830.49 4830.49 4830.49 4894.49 4894.49 4894.49 4894.49 4958.49 4958.49 4958.49 4958.49 5022.49 5022.49 5022.49 5022.49 BBC fr= 230.49 230.49 230.49 230.49 294.49 294.49 294.49 294.49 358.49 358.49 358.49 358.49 422.49 422.49 422.49 422.49 Bandwd= 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 Matching frequency sets: 13 Track assignments are: track1= 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) * SOURCEB1 11 12 00.228909 * 11 14 37.003840 11 15 40.405868 0.00 12 43 34.48321 * 12 27 13.17350 12 20 34.91362 0.00 From catalog imbedded in main SCHED input file. from VLASS JMFIT * SOURCEB2 11 11 52.947675 * 11 14 29.733790 11 15 33.140353 0.00 12 44 24.66534 * 12 28 03.46310 12 21 25.24568 0.00 From catalog imbedded in main SCHED input file. from VLASS JMFIT * SOURCEC 10 54 10.544300 * 10 56 47.786000 10 57 51.382445 0.00 10 46 30.80319 * 10 30 28.20000 10 23 57.43613 0.00 From catalog imbedded in main SCHED input file. TXS 1054+107; from SDSS through NED * 1100+122 11 00 26.171569 * 11 03 03.529837 11 04 07.170151 0.04 J1103+1158 12 14 26.46477 * 11 58 16.62448 11 51 42.95561 0.08 /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 493 observations. * 1156+295 11 56 57.786211 * 11 59 31.833912 12 00 34.165666 0.00 J1159+2914 29 31 25.73880 * 29 14 43.82690 29 07 56.09691 0.00 J1159+29 /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 78215 observations. * OQ208 14 04 45.615156 * 14 07 00.394415 14 07 54.664800 0.24 J1407+2827 28 41 29.23515 * 28 27 14.69019 28 21 23.08750 0.35 1404+286 /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc J1407+28 GSFC 2016a X/S astro solution, 68278 observations. 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 SOURCEB1 sess120.C2048 1 2 3 4 5 6 7 11 12 13 0.650 36.195 SOURCEB2 sess120.C2048 1 2 3 4 5 6 7 11 12 13 0.650 36.498 SOURCEC sess120.C2048 1 2 3 4 5 6 7 11 12 13 0.650 34.623 1100+122 sess120.C2048 1 2 3 4 5 6 7 11 12 13 6.236 336.667 1156+295 sess120.C2048 1 2 3 4 5 6 7 11 12 13 0.762 33.628 OQ208 sess120.C2048 1 2 3 4 5 6 7 11 12 13 0.412 13.411 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) SOURCEB1 171.9 SOURCEB2 171.9 SOURCEC 176.4 1100+122 174.3 1156+295 152.6 OQ208 128.8 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