COVER INFORMATION Station: PICKMERE (Code Pi ) Experiment: Characterizing OCRs in dwarf galaxies Exp. Code: ev026f Schedule Version: 2.00 Processed by SCHED version: 11.60 Release 11.6; April 2020 PI: Dany Vohl Address: Anton Pannekoek Institute for Astronomy, University of Amsterdam 1098 XH Amsterdam Amsterdam The Netherlands Phone: +31 6 1887 9982 EMAIL: d.vohl@uva.nl Fax: Phone during observation: +31 6 1887 9982 Observing mode: vlbi Notes: # Please, make sure PHASE CAL is OFF # COVER LETTER: This observation is to observe ILT J121407.57+423829.2 first identified in the LoTSS DR2 data as potential analogue to persistent radio sources associated to some fast radio bursts. With the observation, we wish to constrain it s source size, and evalute if the radio emission is due to star formation processes or not. Schedule for PICKMERE (Code Pi ) Page 2 Characterizing OCRs in dwarf galaxies 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 ---------------------------------------------------------------------------------------- --- Tue 28 May 2024 Day 149 --- ---------- Fringe-finder ---------- Next scan frequencies: 1626.49 1626.49 Next BBC frequencies: 645.51 645.51 Next scan bandwidths: 64.00 64.00 14 00 00 J1159+2914 06 16 38 25.2 74.5 -5.7 -41.2 0 0 14 00 00 14 02 00 =1156+295 06 18 38 25.5 74.8 -5.7 -41.3 120 8 14 00 01 14 02 10 J1159+2914 06 18 48 25.5 74.8 -5.7 -41.3 7 8 14 02 10 14 06 10 =1156+295 06 22 49 26.1 75.6 -5.6 -41.5 240 23 14 02 11 ---------- test pulsar ---------- 14 07 10 B1237+25_D 06 23 49 17.2 71.4 -6.3 -38.6 10 23 14 07 10 14 10 10 --- 06 26 50 17.6 72.0 -6.2 -38.8 180 35 14 07 11 ---------- Going to ILTJ1214 ---------- 14 12 10 J1209+4119 06 28 50 34.3 65.2 -5.7 -46.2 47 35 14 12 10 14 13 40 =1206+416 06 30 20 34.5 65.5 -5.7 -46.3 90 41 14 12 11 14 13 40 ILTJ1214 06 30 20 34.8 63.6 -5.8 -46.6 -23 41 No stop 14 18 40 --- 06 35 21 35.5 64.4 -5.7 -47.0 277 60 14 13 41 14 19 20 J1209+4119 06 36 01 35.3 66.4 -5.6 -46.7 16 60 14 19 20 14 20 40 =1206+416 06 37 21 35.5 66.6 -5.6 -46.8 80 65 14 19 21 14 20 40 ILTJ1214 06 37 21 35.7 64.7 -5.6 -47.1 -24 65 No stop 14 25 40 --- 06 42 22 36.4 65.4 -5.5 -47.5 276 84 14 20 41 14 26 20 J1209+4119 06 43 02 36.3 67.5 -5.5 -47.2 16 84 14 26 20 14 27 40 =1206+416 06 44 22 36.4 67.7 -5.4 -47.3 80 90 14 26 21 14 27 40 ILTJ1214 06 44 22 36.7 65.8 -5.5 -47.7 -24 90 No stop 14 32 40 --- 06 49 23 37.4 66.5 -5.4 -48.1 276 109 14 27 41 14 33 20 J1209+4119 06 50 03 37.2 68.6 -5.3 -47.7 15 109 14 33 20 14 34 40 =1206+416 06 51 24 37.4 68.8 -5.3 -47.8 80 114 14 33 21 14 34 40 J1214+3309 06 51 24 31.0 75.1 -5.4 -43.6 -42 114 No stop 14 37 40 =1211+334 06 54 24 31.5 75.6 -5.3 -43.7 138 126 14 34 41 14 38 20 J1209+4119 06 55 04 37.9 69.4 -5.3 -48.0 -2 126 14 38 20 14 39 40 =1206+416 06 56 24 38.1 69.6 -5.2 -48.1 78 131 14 38 21 Schedule for PICKMERE (Code Pi ) Page 3 Characterizing OCRs in dwarf galaxies 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 ---------------------------------------------------------------------------------------- --- Tue 28 May 2024 Day 149 --- 14 39 40 ILTJ1214 06 56 24 38.3 67.6 -5.3 -48.6 -24 131 No stop 14 44 40 --- 07 01 25 39.0 68.4 -5.2 -48.9 276 150 14 39 41 14 45 20 J1209+4119 07 02 05 38.9 70.5 -5.1 -48.5 15 150 14 45 20 14 46 40 =1206+416 07 03 26 39.1 70.7 -5.1 -48.6 80 155 14 45 21 14 46 40 ILTJ1214 07 03 26 39.3 68.7 -5.2 -49.1 -24 155 No stop 14 51 40 --- 07 08 26 40.0 69.5 -5.1 -49.4 276 175 14 46 41 14 52 20 J1209+4119 07 09 07 39.9 71.7 -5.0 -48.9 15 175 14 52 20 14 53 40 =1206+416 07 10 27 40.1 71.9 -5.0 -49.0 80 180 14 52 21 14 53 40 ILTJ1214 07 10 27 40.3 69.8 -5.1 -49.6 -24 180 No stop 14 58 40 --- 07 15 28 41.0 70.6 -5.0 -49.9 276 199 14 53 41 14 59 20 J1209+4119 07 16 08 40.9 72.8 -4.9 -49.4 15 199 14 59 20 15 00 40 =1206+416 07 17 28 41.1 73.0 -4.9 -49.4 80 204 14 59 21 15 00 40 ILTJ1214 07 17 28 41.3 70.9 -5.0 -50.0 -25 204 No stop 15 05 40 --- 07 22 29 42.0 71.7 -4.9 -50.3 275 224 15 00 41 15 06 20 J1209+4119 07 23 09 41.9 73.9 -4.8 -49.8 15 224 15 06 20 15 07 40 =1206+416 07 24 29 42.1 74.1 -4.8 -49.8 80 229 15 06 21 15 07 40 J1214+3309 07 24 29 35.9 81.1 -4.8 -44.8 -44 229 No stop 15 10 40 =1211+334 07 27 30 36.3 81.6 -4.8 -44.9 136 240 15 07 41 15 11 20 J1209+4119 07 28 10 42.6 74.8 -4.7 -50.0 -3 240 15 11 20 15 12 40 =1206+416 07 29 30 42.8 75.0 -4.7 -50.1 77 245 15 11 21 15 12 40 ILTJ1214 07 29 30 43.0 72.8 -4.8 -50.8 -25 245 No stop 15 17 40 --- 07 34 31 43.7 73.6 -4.7 -51.1 275 265 15 12 41 15 18 20 J1209+4119 07 35 11 43.6 75.9 -4.6 -50.4 14 265 15 18 20 15 19 40 =1206+416 07 36 31 43.8 76.1 -4.6 -50.5 80 270 15 18 21 ---------- Fringe-finder ---------- 15 21 00 J1159+2914 07 37 51 37.2 89.8 -4.4 -43.2 16 270 15 21 00 15 26 00 =1156+295 07 42 52 38.0 90.8 -4.3 -43.2 300 289 15 21 01 ---------- Going to ILTJ1214 ---------- 15 27 20 J1209+4119 07 44 12 45.0 77.4 -4.4 -50.8 17 289 15 27 20 15 28 50 =1206+416 07 45 43 45.2 77.7 -4.4 -50.9 90 295 15 27 21 Schedule for PICKMERE (Code Pi ) Page 4 Characterizing OCRs in dwarf galaxies 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 ---------------------------------------------------------------------------------------- --- Tue 28 May 2024 Day 149 --- 15 28 50 ILTJ1214 07 45 43 45.3 75.4 -4.5 -51.7 -25 295 No stop 15 33 50 --- 07 50 43 46.0 76.2 -4.4 -52.0 275 314 15 28 51 15 34 30 J1209+4119 07 51 23 46.0 78.6 -4.3 -51.2 14 314 15 34 30 15 35 50 =1206+416 07 52 44 46.2 78.9 -4.3 -51.2 80 319 15 34 31 15 35 50 ILTJ1214 07 52 44 46.3 76.6 -4.4 -52.1 -26 319 No stop 15 40 50 --- 07 57 44 47.1 77.4 -4.3 -52.3 274 339 15 35 51 15 41 30 J1209+4119 07 58 25 47.0 79.8 -4.2 -51.4 14 339 15 41 30 15 42 50 =1206+416 07 59 45 47.2 80.1 -4.2 -51.5 80 344 15 41 31 15 42 50 ILTJ1214 07 59 45 47.4 77.7 -4.3 -52.4 -26 344 No stop 15 47 50 --- 08 04 46 48.1 78.6 -4.2 -52.6 274 363 15 42 51 15 48 30 J1209+4119 08 05 26 48.1 81.0 -4.1 -51.7 13 363 15 48 30 15 49 50 =1206+416 08 06 46 48.3 81.3 -4.1 -51.7 80 368 15 48 31 15 49 50 J1214+3309 08 06 46 42.2 89.1 -4.1 -45.5 -47 368 No stop 15 52 50 =1211+334 08 09 46 42.6 89.7 -4.1 -45.5 133 380 15 49 51 15 53 30 J1209+4119 08 10 27 48.8 81.9 -4.0 -51.9 -6 380 15 53 30 15 54 50 =1206+416 08 11 47 49.0 82.2 -4.0 -51.9 74 385 15 53 31 15 54 50 ILTJ1214 08 11 47 49.1 79.7 -4.1 -52.9 -26 385 No stop 15 59 50 --- 08 16 48 49.9 80.6 -4.0 -53.1 274 404 15 54 51 16 00 30 J1209+4119 08 17 28 49.9 83.2 -3.9 -52.1 13 404 16 00 30 16 01 50 =1206+416 08 18 48 50.1 83.4 -3.9 -52.1 80 410 16 00 31 16 01 50 ILTJ1214 08 18 48 50.1 80.9 -3.9 -53.2 -26 410 No stop 16 06 50 --- 08 23 49 50.9 81.8 -3.9 -53.4 274 429 16 01 51 16 07 30 J1209+4119 08 24 29 50.9 84.4 -3.8 -52.3 13 429 16 07 30 16 08 50 =1206+416 08 25 49 51.1 84.7 -3.7 -52.3 80 434 16 07 31 16 08 50 ILTJ1214 08 25 49 51.2 82.2 -3.8 -53.5 -27 434 No stop 16 13 50 --- 08 30 50 51.9 83.1 -3.7 -53.6 273 453 16 08 51 16 14 30 J1209+4119 08 31 30 51.9 85.7 -3.7 -52.4 12 453 16 14 30 16 15 50 =1206+416 08 32 50 52.1 86.0 -3.6 -52.4 80 459 16 14 31 16 15 50 ILTJ1214 08 32 50 52.2 83.4 -3.7 -53.7 -27 459 No stop 16 20 50 --- 08 37 51 53.0 84.3 -3.6 -53.8 273 478 16 15 51 Schedule for PICKMERE (Code Pi ) Page 5 Characterizing OCRs in dwarf galaxies 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 ---------------------------------------------------------------------------------------- --- Tue 28 May 2024 Day 149 --- 16 21 30 J1209+4119 08 38 31 53.0 87.1 -3.5 -52.5 12 478 16 21 30 16 22 50 =1206+416 08 39 51 53.2 87.3 -3.5 -52.5 80 483 16 21 31 16 22 50 J1214+3309 08 39 51 47.1 95.9 -3.6 -45.2 -49 483 No stop 16 25 50 =1211+334 08 42 52 47.5 96.6 -3.5 -45.1 131 495 16 22 51 16 26 30 J1209+4119 08 43 32 53.7 88.0 -3.5 -52.6 -9 495 16 26 30 16 27 50 =1206+416 08 44 52 53.9 88.3 -3.4 -52.6 71 500 16 26 31 16 27 50 ILTJ1214 08 44 52 54.0 85.6 -3.5 -54.0 -28 500 No stop 16 32 50 --- 08 49 53 54.8 86.5 -3.4 -54.0 272 519 16 27 51 16 33 30 J1209+4119 08 50 33 54.8 89.4 -3.3 -52.6 11 519 16 33 30 16 34 50 =1206+416 08 51 53 55.0 89.7 -3.3 -52.6 80 524 16 33 31 16 34 50 ILTJ1214 08 51 53 55.1 86.9 -3.4 -54.1 -28 524 No stop 16 39 50 --- 08 56 54 55.8 87.9 -3.3 -54.1 272 544 16 34 51 16 40 30 J1209+4119 08 57 34 55.8 90.8 -3.2 -52.6 11 544 16 40 30 16 41 50 =1206+416 08 58 55 56.0 91.1 -3.2 -52.6 80 549 16 40 31 16 41 50 ILTJ1214 08 58 55 56.1 88.2 -3.3 -54.1 -28 549 No stop 16 46 50 --- 09 03 55 56.9 89.2 -3.2 -54.2 272 568 16 41 51 16 47 30 J1209+4119 09 04 35 56.9 92.2 -3.1 -52.5 11 568 16 47 30 16 48 50 =1206+416 09 05 56 57.1 92.5 -3.1 -52.5 80 573 16 47 31 16 48 50 ILTJ1214 09 05 56 57.2 89.6 -3.2 -54.2 -29 573 No stop 16 53 50 --- 09 10 56 57.9 90.6 -3.1 -54.2 271 593 16 48 51 16 54 30 J1209+4119 09 11 37 57.9 93.7 -3.0 -52.4 10 593 16 54 30 16 55 50 =1206+416 09 12 57 58.1 94.0 -3.0 -52.4 80 598 16 54 31 16 55 50 J1214+3309 09 12 57 52.0 103.6 -3.0 -43.9 -52 598 No stop 16 58 50 =1211+334 09 15 57 52.4 104.3 -3.0 -43.7 128 609 16 55 51 16 59 30 J1209+4119 09 16 37 58.7 94.8 -2.9 -52.3 -11 609 16 59 30 17 00 50 =1206+416 09 17 58 58.9 95.1 -2.9 -52.3 69 614 16 59 31 17 00 50 ILTJ1214 09 17 58 59.0 92.1 -3.0 -54.1 -29 614 No stop 17 05 50 --- 09 22 58 59.7 93.1 -2.9 -54.1 271 634 17 00 51 17 06 30 J1209+4119 09 23 39 59.7 96.4 -2.8 -52.1 10 634 17 06 30 17 07 50 =1206+416 09 24 59 59.9 96.7 -2.8 -52.1 80 639 17 06 31 Schedule for PICKMERE (Code Pi ) Page 6 Characterizing OCRs in dwarf galaxies 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 ---------------------------------------------------------------------------------------- --- Tue 28 May 2024 Day 149 --- 17 07 50 ILTJ1214 09 24 59 60.0 93.6 -2.8 -54.0 -30 639 No stop 17 12 50 --- 09 30 00 60.8 94.7 -2.8 -53.9 270 658 17 07 51 17 13 30 J1209+4119 09 30 40 60.8 98.1 -2.7 -51.9 9 658 17 13 30 17 14 50 =1206+416 09 32 00 61.0 98.4 -2.6 -51.8 80 663 17 13 31 17 14 50 ILTJ1214 09 32 00 61.1 95.1 -2.7 -53.9 -30 663 No stop 17 19 50 --- 09 37 01 61.8 96.3 -2.6 -53.7 270 683 17 14 51 17 20 30 J1209+4119 09 37 41 61.8 99.8 -2.5 -51.5 9 683 17 20 30 17 21 50 =1206+416 09 39 01 62.0 100.1 -2.5 -51.5 80 688 17 20 31 17 21 50 ILTJ1214 09 39 01 62.1 96.7 -2.6 -53.6 -31 688 No stop 17 26 50 --- 09 44 02 62.8 97.9 -2.5 -53.4 269 707 17 21 51 17 27 30 J1209+4119 09 44 42 62.8 101.5 -2.4 -51.1 8 707 17 27 30 17 28 50 =1206+416 09 46 02 63.0 101.9 -2.4 -51.0 80 712 17 27 31 17 28 50 J1214+3309 09 46 02 56.7 112.3 -2.5 -41.3 -55 712 No stop 17 31 50 =1211+334 09 49 03 57.1 113.2 -2.4 -40.9 125 724 17 28 51 17 32 30 J1209+4119 09 49 43 63.6 102.9 -2.3 -50.8 -14 724 17 32 30 17 33 50 =1206+416 09 51 03 63.8 103.2 -2.3 -50.7 66 729 17 32 31 17 33 50 ILTJ1214 09 51 03 63.9 99.6 -2.4 -53.1 -31 729 No stop 17 38 50 --- 09 56 04 64.6 100.9 -2.3 -52.8 269 748 17 33 51 17 39 30 J1209+4119 09 56 44 64.6 104.8 -2.2 -50.2 7 748 17 39 30 17 40 50 =1206+416 09 58 04 64.8 105.2 -2.2 -50.1 80 754 17 39 31 17 40 50 ILTJ1214 09 58 04 64.9 101.4 -2.3 -52.6 -32 754 No stop 17 45 50 --- 10 03 05 65.6 102.8 -2.2 -52.3 268 773 17 40 51 17 46 30 J1209+4119 10 03 45 65.6 106.8 -2.1 -49.5 7 773 17 46 30 17 47 50 =1206+416 10 05 05 65.8 107.2 -2.1 -49.4 80 778 17 46 31 17 47 50 ILTJ1214 10 05 05 65.9 103.3 -2.2 -52.1 -32 778 No stop 17 52 50 --- 10 10 06 66.7 104.8 -2.1 -51.6 268 797 17 47 51 17 53 30 J1209+4119 10 10 46 66.6 108.9 -2.0 -48.7 6 797 17 53 30 17 54 50 =1206+416 10 12 07 66.8 109.3 -2.0 -48.6 80 803 17 53 31 17 54 50 ILTJ1214 10 12 07 66.9 105.3 -2.1 -51.4 -33 803 No stop 17 59 50 --- 10 17 07 67.7 106.8 -2.0 -50.9 267 822 17 54 51 Schedule for PICKMERE (Code Pi ) Page 7 Characterizing OCRs in dwarf galaxies 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 ---------------------------------------------------------------------------------------- --- Tue 28 May 2024 Day 149 --- 18 00 30 J1209+4119 10 17 47 67.6 111.2 -1.9 -47.8 5 822 18 00 30 18 01 50 =1206+416 10 19 08 67.8 111.6 -1.9 -47.6 80 827 18 00 31 18 01 50 J1214+3309 10 19 08 61.1 122.7 -1.9 -36.9 -57 827 No stop 18 04 50 =1211+334 10 22 08 61.4 123.8 -1.9 -36.3 123 839 18 01 51 18 05 30 J1209+4119 10 22 48 68.3 112.9 -1.8 -47.0 -15 839 18 05 30 18 06 50 =1206+416 10 24 08 68.5 113.3 -1.8 -46.8 65 844 18 05 31 18 06 50 ILTJ1214 10 24 08 68.7 109.1 -1.9 -50.0 -34 844 No stop 18 11 50 --- 10 29 09 69.4 110.7 -1.8 -49.3 266 863 18 06 51 18 12 30 J1209+4119 10 29 49 69.2 115.4 -1.7 -45.9 4 863 18 12 30 18 13 50 =1206+416 10 31 10 69.4 115.9 -1.7 -45.6 80 868 18 12 31 18 13 50 ILTJ1214 10 31 10 69.6 111.4 -1.7 -49.0 -35 868 No stop 18 18 50 --- 10 36 10 70.3 113.2 -1.7 -48.2 265 888 18 13 51 18 19 30 J1209+4119 10 36 51 70.2 118.1 -1.6 -44.5 3 888 18 19 30 18 20 50 =1206+416 10 38 11 70.3 118.6 -1.5 -44.2 80 893 18 19 31 18 20 50 ILTJ1214 10 38 11 70.6 113.9 -1.6 -47.8 -35 893 No stop 18 25 50 --- 10 43 12 71.3 115.9 -1.5 -46.9 265 912 18 20 51 18 26 30 J1209+4119 10 43 52 71.1 121.0 -1.4 -42.9 2 912 18 26 30 18 27 50 =1206+416 10 45 12 71.2 121.5 -1.4 -42.6 80 917 18 26 31 18 27 50 ILTJ1214 10 45 12 71.6 116.7 -1.5 -46.4 -36 917 No stop 18 32 50 --- 10 50 13 72.2 118.7 -1.4 -45.3 264 937 18 27 51 18 33 30 J1209+4119 10 50 53 72.0 124.0 -1.3 -41.2 2 937 18 33 30 18 34 50 =1206+416 10 52 13 72.1 124.7 -1.3 -40.8 80 942 18 33 31 18 34 50 J1214+3309 10 52 13 64.9 135.5 -1.4 -30.0 -56 942 No stop 18 37 50 =1211+334 10 55 14 65.2 136.8 -1.3 -29.2 124 953 18 34 51 18 38 30 J1209+4119 10 55 54 72.6 126.4 -1.2 -39.7 -14 953 18 38 30 18 39 50 =1206+416 10 57 14 72.7 127.1 -1.2 -39.3 66 958 18 38 31 18 39 50 ILTJ1214 10 57 14 73.1 121.8 -1.3 -43.5 -37 958 No stop 18 44 50 --- 11 02 15 73.8 124.2 -1.2 -42.1 263 978 18 39 51 18 45 30 J1209+4119 11 02 55 73.4 129.9 -1.1 -37.5 0 978 18 45 30 18 46 50 =1206+416 11 04 15 73.6 130.6 -1.1 -37.1 80 983 18 45 31 Schedule for PICKMERE (Code Pi ) Page 8 Characterizing OCRs in dwarf galaxies 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 ---------------------------------------------------------------------------------------- --- Tue 28 May 2024 Day 149 --- 18 46 50 ILTJ1214 11 04 15 74.0 125.2 -1.2 -41.5 -38 983 No stop 18 51 50 --- 11 09 16 74.6 127.8 -1.1 -39.8 262 1002 18 46 51 18 52 30 J1209+4119 11 09 56 74.2 133.7 -1.0 -35.0 0 1002 18 52 30 18 53 50 =1206+416 11 11 16 74.3 134.5 -1.0 -34.5 80 1007 18 52 31 ---------- Fringe-finder ---------- 18 55 00 J1159+2914 11 12 26 64.3 155.1 -0.8 -16.7 -15 1007 18 55 00 19 00 00 =1156+295 11 17 27 64.6 157.5 -0.7 -15.2 285 1027 18 55 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess224.L1024 --- 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: 13 Station: PICKMERE Total bit rate: 512 Format: VDIF Bits per sample: 2 Sample rate:128.000 Number of channels: 2 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 2272.00 2272.00 Net SB= U U IF SB = L L Pol. = RCP LCP BBC = 1 9 BBC SB= L L IF = A1 B1 The following frequency sets based on these setups were used. Frequency Set: 10 Setup file default. Used with PCAL = off LO sum= 1626.49 1626.49 BBC fr= 645.51 645.51 Bandwd= 64.00 64.00 Matching frequency sets: 10 11 12 13 14 Track assignments are: track1= 1, 2 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) * ILTJ1214 12 11 37.280056 * 12 14 07.570000 12 15 21.707455 0.00 42 55 09.49919 * 42 38 29.20000 42 30 32.22412 0.00 From catalog imbedded in main SCHED input file. * B1237+25_D 12 37 11.843793 * 12 39 40.400000 12 40 53.567676 0.00 25 10 17.10031 * 24 53 49.20000 24 45 52.16493 0.00 From catalog imbedded in main SCHED input file. 1156+295 11 56 57.786211 * 11 59 31.833912 12 00 47.466951 0.00 * J1159+2914 29 31 25.73880 * 29 14 43.82690 29 06 42.77135 0.00 J1159+29 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 78215 observations. 1206+416 12 06 51.117947 * 12 09 22.788006 12 10 37.529148 0.17 * J1209+4119 41 36 22.62761 * 41 19 41.37011 41 11 43.78026 0.16 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 150 observations. 1211+334 12 11 32.805725 * 12 14 04.115761 12 15 18.573025 0.10 * J1214+3309 33 26 25.95140 * 33 09 45.59508 33 01 45.93285 0.13 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 144 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 ILTJ1214 sess224.L1024 1 2 3 4 5 6 7 8 9 10 2.750 220.837 B1237+25_D sess224.L1024 1 3 4 5 6 7 8 9 10 0.050 3.877 J1159+2914 sess224.L1024 1 2 3 4 5 6 7 8 9 10 0.267 23.537 J1209+4119 sess224.L1024 1 2 3 4 5 6 7 8 9 10 0.961 77.882 J1214+3309 sess224.L1024 1 2 3 4 5 6 7 8 9 10 0.400 24.710 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) ILTJ1214 94.0 B1237+25_D 108.7 J1159+2914 98.8 J1209+4119 94.1 J1214+3309 99.3 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