COVER INFORMATION Station: PICKMERE (Code Pi ) Experiment: Characterizing OCRs in dwarf galaxies Exp. Code: ev026a Schedule Version: 3.00 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 J075257.15+401026.3 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 its 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 ---------------------------------------------------------------------------------------- --- Fri 1 Mar 2024 Day 61 --- ---------- test pulsar ---------- Next scan frequencies: 1626.49 1626.49 Next BBC frequencies: 645.51 645.51 Next scan bandwidths: 64.00 64.00 16 00 00 B0540+23_D 02 30 01 43.0 109.8 -3.2 -37.8 0 0 16 00 00 16 03 00 --- 02 33 01 43.4 110.5 -3.2 -37.6 180 12 16 00 01 ---------- Fringe-finder ---------- 16 04 40 J0555+3948 02 34 42 53.6 90.8 -3.4 -51.1 18 12 16 04 40 16 08 40 =0552+398 02 38 42 54.2 91.6 -3.3 -51.1 240 27 16 04 41 ---------- Going to ILTJ0752 region ---------- 16 10 40 J0743+3941 02 40 43 38.5 72.7 -5.1 -47.8 40 27 16 10 40 16 12 10 =0739+398 02 42 13 38.7 73.0 -5.0 -47.9 90 33 16 10 41 16 12 10 ILTJ0752 02 42 13 37.6 70.9 -5.2 -47.6 -24 33 No stop 16 17 10 --- 02 47 14 38.4 71.7 -5.1 -47.9 276 52 16 12 11 16 17 50 J0743+3941 02 47 54 39.5 73.9 -4.9 -48.2 15 52 16 17 50 16 19 10 =0739+398 02 49 14 39.7 74.1 -4.9 -48.3 80 57 16 17 51 16 19 10 ILTJ0752 02 49 14 38.6 72.1 -5.1 -48.0 -24 57 No stop 16 24 10 --- 02 54 15 39.4 72.9 -5.0 -48.3 276 77 16 19 11 16 24 50 J0743+3941 02 54 55 40.5 75.1 -4.8 -48.6 15 77 16 24 50 16 26 10 =0739+398 02 56 15 40.7 75.3 -4.8 -48.7 80 82 16 24 51 16 26 10 ILTJ0752 02 56 15 39.6 73.2 -5.0 -48.5 -25 82 No stop 16 31 10 --- 03 01 16 40.4 74.1 -4.9 -48.7 275 101 16 26 11 16 31 50 J0743+3941 03 01 56 41.6 76.3 -4.7 -48.9 15 101 16 31 50 16 33 10 =0739+398 03 03 16 41.8 76.5 -4.7 -49.0 80 106 16 31 51 16 33 10 J0754+3910 03 03 16 39.8 75.1 -4.9 -48.1 -24 106 No stop 16 36 10 =0751+393 03 06 17 40.2 75.6 -4.8 -48.3 156 118 16 33 11 16 36 50 J0743+3941 03 06 57 42.3 77.1 -4.6 -49.2 15 118 16 36 50 16 38 10 =0739+398 03 08 17 42.5 77.4 -4.6 -49.2 80 123 16 36 51 16 38 10 ILTJ0752 03 08 17 41.4 75.2 -4.8 -49.1 -25 123 No stop 16 43 10 --- 03 13 18 42.1 76.1 -4.7 -49.3 275 142 16 38 11 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 ---------------------------------------------------------------------------------------- --- Fri 1 Mar 2024 Day 61 --- 16 43 50 J0743+3941 03 13 58 43.3 78.3 -4.5 -49.5 14 142 16 43 50 16 45 10 =0739+398 03 15 18 43.5 78.6 -4.5 -49.5 80 147 16 43 51 16 45 10 ILTJ0752 03 15 18 42.4 76.4 -4.7 -49.4 -25 147 No stop 16 50 10 --- 03 20 19 43.1 77.2 -4.6 -49.7 275 167 16 45 11 16 50 50 J0743+3941 03 20 59 44.3 79.5 -4.4 -49.8 14 167 16 50 50 16 52 10 =0739+398 03 22 19 44.5 79.8 -4.4 -49.8 80 172 16 50 51 16 52 10 ILTJ0752 03 22 19 43.4 77.6 -4.5 -49.8 -25 172 No stop 16 57 10 --- 03 27 20 44.1 78.4 -4.5 -50.0 275 191 16 52 11 16 57 50 J0743+3941 03 28 00 45.4 80.8 -4.3 -50.0 14 191 16 57 50 16 59 10 =0739+398 03 29 20 45.6 81.0 -4.3 -50.1 80 196 16 57 51 16 59 10 ILTJ0752 03 29 20 44.4 78.8 -4.4 -50.1 -25 196 No stop 17 04 10 --- 03 34 21 45.2 79.6 -4.3 -50.3 275 216 16 59 11 17 04 50 J0743+3941 03 35 01 46.4 82.0 -4.2 -50.2 14 216 17 04 50 17 06 10 =0739+398 03 36 22 46.6 82.3 -4.1 -50.3 80 221 17 04 51 17 06 10 J0754+3910 03 36 22 44.6 80.8 -4.3 -49.5 -24 221 No stop 17 09 10 =0751+393 03 39 22 45.0 81.3 -4.3 -49.6 156 233 17 06 11 17 09 50 J0743+3941 03 40 02 47.2 82.9 -4.1 -50.4 15 233 17 09 50 17 11 10 =0739+398 03 41 22 47.4 83.2 -4.1 -50.4 80 238 17 09 51 17 11 10 ILTJ0752 03 41 22 46.2 80.9 -4.2 -50.5 -26 238 No stop 17 16 10 --- 03 46 23 46.9 81.8 -4.1 -50.7 274 257 17 11 11 17 16 50 J0743+3941 03 47 03 48.2 84.2 -4.0 -50.6 14 257 17 16 50 17 18 10 =0739+398 03 48 24 48.4 84.4 -3.9 -50.6 80 262 17 16 51 ---------- Fringe-finder ---------- 17 19 50 J0555+3948 03 50 04 64.6 109.2 -2.1 -47.3 3 262 17 19 50 17 23 50 =0552+398 03 54 05 65.2 110.4 -2.1 -46.8 240 278 17 19 51 ---------- Going to ILTJ0752 region ---------- 17 25 50 J0743+3941 03 56 05 49.5 85.9 -3.8 -50.7 23 278 17 25 50 17 27 20 =0739+398 03 57 35 49.8 86.2 -3.8 -50.8 90 283 17 25 51 17 27 20 ILTJ0752 03 57 35 48.6 83.8 -4.0 -51.0 -26 283 No stop 17 32 20 --- 04 02 36 49.4 84.7 -3.9 -51.1 274 303 17 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 ---------------------------------------------------------------------------------------- --- Fri 1 Mar 2024 Day 61 --- 17 33 00 J0743+3941 04 03 16 50.6 87.2 -3.7 -50.8 13 303 17 33 00 17 34 20 =0739+398 04 04 36 50.8 87.5 -3.7 -50.8 80 308 17 33 01 17 34 20 ILTJ0752 04 04 36 49.7 85.1 -3.8 -51.1 -26 308 No stop 17 39 20 --- 04 09 37 50.4 86.0 -3.7 -51.2 274 327 17 34 21 17 40 00 J0743+3941 04 10 17 51.7 88.6 -3.6 -50.9 13 327 17 40 00 17 41 20 =0739+398 04 11 37 51.9 88.9 -3.6 -50.9 80 332 17 40 01 17 41 20 ILTJ0752 04 11 37 50.7 86.4 -3.7 -51.3 -26 332 No stop 17 46 20 --- 04 16 38 51.4 87.3 -3.6 -51.3 274 352 17 41 21 17 47 00 J0743+3941 04 17 18 52.7 90.0 -3.5 -50.9 12 352 17 47 00 17 48 20 =0739+398 04 18 39 52.9 90.2 -3.4 -50.9 80 357 17 47 01 17 48 20 J0754+3910 04 18 39 50.9 88.6 -3.6 -50.4 -24 357 No stop 17 51 20 =0751+393 04 21 39 51.3 89.2 -3.6 -50.4 156 368 17 48 21 17 52 00 J0743+3941 04 22 19 53.5 91.0 -3.4 -50.9 15 368 17 52 00 17 53 20 =0739+398 04 23 39 53.7 91.3 -3.4 -50.9 80 374 17 52 01 17 53 20 ILTJ0752 04 23 39 52.5 88.7 -3.5 -51.4 -27 374 No stop 17 58 20 --- 04 28 40 53.2 89.7 -3.4 -51.4 273 393 17 53 21 17 59 00 J0743+3941 04 29 20 54.5 92.4 -3.3 -50.9 12 393 17 59 00 18 00 20 =0739+398 04 30 41 54.7 92.7 -3.2 -50.8 80 398 17 59 01 18 00 20 ILTJ0752 04 30 41 53.5 90.1 -3.4 -51.4 -27 398 No stop 18 05 20 --- 04 35 41 54.3 91.1 -3.3 -51.4 273 417 18 00 21 18 06 00 J0743+3941 04 36 21 55.6 93.9 -3.1 -50.8 12 417 18 06 00 18 07 20 =0739+398 04 37 42 55.8 94.2 -3.1 -50.7 80 423 18 06 01 18 07 20 ILTJ0752 04 37 42 54.6 91.5 -3.3 -51.4 -28 423 No stop 18 12 20 --- 04 42 43 55.3 92.5 -3.2 -51.3 272 442 18 07 21 18 13 00 J0743+3941 04 43 23 56.6 95.5 -3.0 -50.6 11 442 18 13 00 18 14 20 =0739+398 04 44 43 56.8 95.8 -3.0 -50.6 80 447 18 13 01 18 14 20 ILTJ0752 04 44 43 55.6 93.0 -3.2 -51.3 -28 447 No stop 18 19 20 --- 04 49 44 56.4 94.0 -3.1 -51.2 272 466 18 14 21 18 20 00 J0743+3941 04 50 24 57.6 97.1 -2.9 -50.4 11 466 18 20 00 18 21 20 =0739+398 04 51 44 57.8 97.4 -2.9 -50.3 80 471 18 20 01 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 ---------------------------------------------------------------------------------------- --- Fri 1 Mar 2024 Day 61 --- 18 21 20 J0754+3910 04 51 44 55.8 95.5 -3.1 -50.1 -24 471 No stop 18 24 20 =0751+393 04 54 44 56.3 96.2 -3.0 -50.0 156 483 18 21 21 18 25 00 J0743+3941 04 55 25 58.4 98.2 -2.8 -50.2 15 483 18 25 00 18 26 20 =0739+398 04 56 45 58.6 98.5 -2.8 -50.1 80 488 18 25 01 18 26 20 ILTJ0752 04 56 45 57.4 95.6 -3.0 -51.1 -29 488 No stop 18 31 20 --- 05 01 46 58.2 96.7 -2.9 -50.9 271 508 18 26 21 18 32 00 J0743+3941 05 02 26 59.4 99.9 -2.7 -49.9 10 508 18 32 00 18 33 20 =0739+398 05 03 46 59.6 100.2 -2.7 -49.8 80 513 18 32 01 18 33 20 ILTJ0752 05 03 46 58.5 97.2 -2.8 -50.9 -29 513 No stop 18 38 20 --- 05 08 47 59.2 98.4 -2.8 -50.7 271 532 18 33 21 18 39 00 J0743+3941 05 09 27 60.5 101.6 -2.6 -49.5 10 532 18 39 00 18 40 20 =0739+398 05 10 47 60.6 102.0 -2.6 -49.4 80 537 18 39 01 18 40 20 ILTJ0752 05 10 47 59.5 98.8 -2.7 -50.6 -30 537 No stop 18 45 20 --- 05 15 48 60.3 100.0 -2.6 -50.3 270 556 18 40 21 18 46 00 J0743+3941 05 16 28 61.5 103.5 -2.5 -49.0 9 556 18 46 00 18 47 20 =0739+398 05 17 48 61.7 103.8 -2.5 -48.9 80 562 18 46 01 18 47 20 ILTJ0752 05 17 48 60.5 100.5 -2.6 -50.2 -30 562 No stop 18 52 20 --- 05 22 49 61.3 101.8 -2.5 -49.9 270 581 18 47 21 18 53 00 J0743+3941 05 23 29 62.5 105.4 -2.4 -48.5 8 581 18 53 00 18 54 20 =0739+398 05 24 49 62.7 105.7 -2.3 -48.3 80 586 18 53 01 18 54 20 J0754+3910 05 24 49 60.7 103.5 -2.5 -48.5 -25 586 No stop 18 57 20 =0751+393 05 27 50 61.1 104.2 -2.5 -48.3 155 598 18 54 21 18 58 00 J0743+3941 05 28 30 63.2 106.8 -2.3 -48.0 13 598 18 58 00 18 59 20 =0739+398 05 29 50 63.4 107.1 -2.2 -47.9 80 603 18 58 01 18 59 20 ILTJ0752 05 29 50 62.3 103.6 -2.4 -49.4 -31 603 No stop 19 04 20 --- 05 34 51 63.0 105.0 -2.3 -49.0 269 622 18 59 21 19 05 00 J0743+3941 05 35 31 64.2 108.8 -2.2 -47.3 7 622 19 05 00 19 06 20 =0739+398 05 36 51 64.4 109.2 -2.1 -47.1 80 627 19 05 01 19 06 20 ILTJ0752 05 36 51 63.3 105.6 -2.3 -48.8 -32 627 No stop 19 11 20 --- 05 41 52 64.0 107.0 -2.2 -48.4 268 647 19 06 21 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 ---------------------------------------------------------------------------------------- --- Fri 1 Mar 2024 Day 61 --- 19 12 00 J0743+3941 05 42 32 65.2 111.0 -2.0 -46.4 7 647 19 12 00 19 13 20 =0739+398 05 43 53 65.4 111.4 -2.0 -46.3 80 652 19 12 01 19 13 20 ILTJ0752 05 43 53 64.3 107.6 -2.2 -48.2 -32 652 No stop 19 18 20 --- 05 48 53 65.0 109.1 -2.1 -47.6 268 671 19 13 21 19 19 00 J0743+3941 05 49 33 66.2 113.3 -1.9 -45.5 6 671 19 19 00 19 20 20 =0739+398 05 50 54 66.4 113.7 -1.9 -45.3 80 676 19 19 01 19 20 20 ILTJ0752 05 50 54 65.3 109.7 -2.1 -47.4 -33 676 No stop 19 25 20 --- 05 55 54 66.0 111.3 -2.0 -46.7 267 696 19 20 21 19 26 00 J0743+3941 05 56 35 67.1 115.7 -1.8 -44.4 5 696 19 26 00 19 27 20 =0739+398 05 57 55 67.3 116.2 -1.8 -44.2 80 701 19 26 01 19 27 20 J0754+3910 05 57 55 65.4 113.1 -2.0 -45.1 -29 701 No stop 19 30 20 =0751+393 06 00 55 65.8 114.1 -1.9 -44.7 151 712 19 27 21 19 31 00 J0743+3941 06 01 35 67.8 117.5 -1.7 -43.5 9 712 19 31 00 19 32 20 =0739+398 06 02 56 68.0 118.0 -1.7 -43.3 80 718 19 31 01 19 32 20 ILTJ0752 06 02 56 67.0 113.6 -1.9 -45.7 -34 718 No stop 19 37 20 --- 06 07 56 67.7 115.4 -1.8 -44.9 266 737 19 32 21 19 38 00 J0743+3941 06 08 37 68.7 120.2 -1.6 -42.2 3 737 19 38 00 19 39 20 =0739+398 06 09 57 68.9 120.7 -1.6 -41.9 80 742 19 38 01 19 39 20 ILTJ0752 06 09 57 67.9 116.1 -1.7 -44.6 -35 742 No stop 19 44 20 --- 06 14 58 68.6 117.9 -1.7 -43.7 265 761 19 39 21 19 45 00 J0743+3941 06 15 38 69.6 123.0 -1.5 -40.6 3 761 19 45 00 19 46 20 =0739+398 06 16 58 69.8 123.6 -1.5 -40.3 80 766 19 45 01 19 46 20 ILTJ0752 06 16 58 68.9 118.7 -1.6 -43.3 -36 766 No stop 19 51 20 --- 06 21 59 69.5 120.7 -1.5 -42.2 264 786 19 46 21 19 52 00 J0743+3941 06 22 39 70.5 126.1 -1.4 -38.9 1 786 19 52 00 19 53 20 =0739+398 06 23 59 70.6 126.7 -1.3 -38.5 80 791 19 52 01 19 53 20 ILTJ0752 06 23 59 69.8 121.5 -1.5 -41.8 -37 791 No stop 19 58 20 --- 06 29 00 70.4 123.6 -1.4 -40.6 263 810 19 53 21 19 59 00 J0743+3941 06 29 40 71.3 129.3 -1.3 -36.9 0 810 19 59 00 20 00 20 =0739+398 06 31 00 71.5 130.0 -1.2 -36.5 80 815 19 59 01 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 ---------------------------------------------------------------------------------------- --- Fri 1 Mar 2024 Day 61 --- 20 00 20 J0754+3910 06 31 00 69.7 125.7 -1.4 -38.8 -34 815 No stop 20 03 20 =0751+393 06 34 01 70.1 127.0 -1.4 -38.0 146 827 20 00 21 20 04 00 J0743+3941 06 34 41 71.9 131.8 -1.2 -35.4 4 827 20 04 00 20 05 20 =0739+398 06 36 01 72.0 132.5 -1.1 -34.9 80 832 20 04 01 20 05 20 ILTJ0752 06 36 01 71.3 126.8 -1.3 -38.8 -39 832 No stop 20 10 20 --- 06 41 02 71.9 129.2 -1.2 -37.3 261 851 20 05 21 20 11 00 J0743+3941 06 41 42 72.6 135.5 -1.1 -33.0 -2 851 20 11 00 20 12 20 =0739+398 06 43 02 72.8 136.2 -1.0 -32.5 78 857 20 11 01 20 12 20 ILTJ0752 06 43 02 72.1 130.2 -1.2 -36.7 -40 857 No stop 20 17 20 --- 06 48 03 72.7 132.7 -1.1 -35.0 260 876 20 12 21 20 18 00 J0743+3941 06 48 43 73.3 139.4 -0.9 -30.4 -3 876 20 18 00 20 19 20 =0739+398 06 50 03 73.5 140.2 -0.9 -29.8 77 881 20 18 01 20 19 20 ILTJ0752 06 50 03 72.9 133.8 -1.1 -34.4 -41 881 No stop 20 24 20 --- 06 55 04 73.4 136.5 -1.0 -32.5 259 900 20 19 21 20 25 00 J0743+3941 06 55 44 74.0 143.6 -0.8 -27.4 -4 900 20 25 00 20 26 20 =0739+398 06 57 05 74.1 144.4 -0.8 -26.8 76 906 20 25 01 20 26 20 ILTJ0752 06 57 05 73.6 137.7 -1.0 -31.7 -42 906 No stop 20 31 20 --- 07 02 05 74.1 140.7 -0.9 -29.7 258 925 20 26 21 20 32 00 J0743+3941 07 02 45 74.6 148.1 -0.7 -24.2 -5 925 20 32 00 20 33 20 =0739+398 07 04 06 74.7 149.0 -0.7 -23.6 75 930 20 32 01 20 33 20 J0754+3910 07 04 06 73.3 142.6 -0.9 -27.9 -41 930 No stop 20 36 20 =0751+393 07 07 06 73.5 144.4 -0.8 -26.7 139 942 20 33 21 20 37 00 J0743+3941 07 07 46 75.0 151.5 -0.6 -21.8 -4 942 20 37 00 20 38 20 =0739+398 07 09 06 75.1 152.4 -0.6 -21.1 76 947 20 37 01 20 38 20 ILTJ0752 07 09 06 74.7 145.1 -0.8 -26.6 -43 947 No stop 20 43 20 --- 07 14 07 75.1 148.4 -0.7 -24.2 257 966 20 38 21 20 44 00 J0743+3941 07 14 47 75.4 156.4 -0.5 -18.1 -7 966 20 44 00 20 45 20 =0739+398 07 16 08 75.5 157.4 -0.5 -17.3 73 971 20 44 01 20 45 20 ILTJ0752 07 16 08 75.3 149.8 -0.6 -23.2 -44 971 No stop 20 49 20 --- 07 20 08 75.6 152.6 -0.6 -21.1 196 987 20 45 21 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 ---------------------------------------------------------------------------------------- --- Fri 1 Mar 2024 Day 61 --- 20 50 00 J0743+3941 07 20 48 75.7 160.9 -0.4 -14.7 -8 987 20 50 00 20 51 00 =0739+398 07 21 49 75.8 161.7 -0.4 -14.1 52 991 20 50 01 ---------- eMERLIN amplitude calibrator ---------- 20 56 00 3C286 07 26 49 23.2 69.7 -6.1 -40.5 1 991 20 56 00 21 00 00 --- 07 30 50 23.7 70.4 -6.0 -40.8 240 1006 20 56 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess124.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: 15 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: 12 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: 12 13 14 15 16 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) * ILTJ0752 07 49 33.412353 * 07 52 57.153200 07 54 36.548346 0.00 40 18 13.89419 * 40 10 26.38587 40 06 46.70064 0.00 From catalog imbedded in main SCHED input file. * B0540+23_D 05 40 06.938912 * 05 43 09.600000 05 44 37.961073 0.00 23 27 44.80457 * 23 29 05.00000 23 29 48.17973 0.00 From catalog imbedded in main SCHED input file. 0552+398 05 52 01.407168 * 05 55 30.805611 05 57 12.208822 0.00 * J0555+3948 39 48 21.94581 * 39 48 49.16496 39 49 11.53323 0.00 DA193 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc J0555+39 GSFC 2016a X/S astro solution, 415688 observations. 0739+398 07 39 45.940018 * 07 43 09.886529 07 44 49.321045 0.14 * J0743+3941 39 48 40.02304 * 39 41 30.78073 39 38 09.86367 0.16 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 151 observations. 0751+393 07 51 15.248476 * 07 54 37.069183 07 56 15.529668 1.86 * J0754+3910 39 18 41.79503 * 39 10 47.79774 39 07 04.69953 2.17 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 15 observations. * 3C286 13 28 49.657769 * 13 31 08.288061 13 32 16.347471 0.17 J1331+3030 30 45 58.64066 * 30 30 32.95930 30 22 51.59404 0.16 1328+307 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc J1331+30 GSFC 2016a X/S astro solution, 269 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 ILTJ0752 sess124.L1024 1 2 3 4 5 6 7 8 9 10 11 12 2.733 285.041 B0540+23_D sess124.L1024 1 2 3 4 5 6 7 8 9 10 11 12 0.050 6.000 J0555+3948 sess124.L1024 1 2 3 4 5 6 7 8 9 10 11 12 0.133 15.800 J0743+3941 sess124.L1024 1 2 3 4 5 6 7 8 9 10 11 12 0.956 105.302 J0754+3910 sess124.L1024 2 3 4 5 6 7 8 9 10 11 12 0.400 33.754 3C286 sess124.L1024 1 2 3 4 5 6 7 8 9 11 12 0.067 6.496 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) ILTJ0752 128.5 B0540+23_D 104.8 J0555+3948 107.0 J0743+3941 127.0 J0754+3910 129.2 3C286 136.0 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