COVER INFORMATION Station: WSTRBORK (Code Wb ) Experiment: Characterizing OCRs in dwarf galaxies Exp. Code: ev026g 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 ILTJ231715.38+184339.0 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 WSTRBORK (Code Wb ) 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 ---------------------------------------------------------------------------------------- --- Wed 29 May 2024 Day 150 --- ---------- test pulsar ---------- Next scan frequencies: 1626.49 1626.49 1626.49 1626.49 1690.49 1690.49 1690.49 1690.49 Next BBC frequencies: 379.49 379.49 379.49 379.49 443.49 443.49 443.49 443.49 Next scan bandwidths: 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 02 00 00 B2319+60_D 18 54 46 54.1 50.6 -4.5 0.0 0 0 02 00 00 02 01 30 --- 18 56 16 54.3 50.7 -4.4 0.0 90 12 02 00 01 ---------- test pulsar ---------- 02 01 30 B2319+60_D 18 56 16 54.3 50.7 -4.4 0.0 -10 12 No stop 02 04 30 --- 18 59 16 54.6 50.9 -4.4 0.0 170 35 02 01 31 ---------- Fringe-finder ---------- 02 08 10 J2253+1608 19 02 57 32.0 106.2 -3.9 0.0 59 35 02 08 10 02 12 20 =3C454.3 19 07 08 32.6 107.1 -3.8 0.0 250 67 02 08 11 ---------- Going to ILTJ2317 ---------- 02 13 20 J2320+1829 19 08 08 30.7 99.7 -4.2 0.0 25 67 02 13 20 02 15 20 =2318+182 19 10 08 31.0 100.1 -4.2 0.0 120 82 02 13 21 02 15 20 ILTJ2317 19 10 08 31.7 100.7 -4.1 0.0 -16 82 No stop 02 20 20 --- 19 15 09 32.4 101.8 -4.1 0.0 284 121 02 15 21 02 20 50 J2320+1829 19 15 39 31.8 101.3 -4.1 0.0 14 121 02 20 50 02 22 10 =2318+182 19 16 59 32.0 101.6 -4.1 0.0 80 131 02 20 51 02 22 10 ILTJ2317 19 16 59 32.7 102.2 -4.0 0.0 -16 131 No stop 02 27 10 --- 19 22 00 33.4 103.3 -3.9 0.0 284 170 02 22 11 02 27 40 J2320+1829 19 22 30 32.8 102.8 -4.0 0.0 14 170 02 27 40 02 29 00 =2318+182 19 23 50 33.0 103.1 -4.0 0.0 80 180 02 27 41 02 29 00 ILTJ2317 19 23 50 33.7 103.8 -3.9 0.0 -16 180 No stop 02 34 00 --- 19 28 51 34.4 104.9 -3.8 0.0 284 219 02 29 01 02 34 30 J2320+1829 19 29 21 33.8 104.4 -3.9 0.0 14 219 02 34 30 02 35 50 =2318+182 19 30 42 34.0 104.7 -3.9 0.0 80 229 02 34 31 02 35 50 J2236+2828 19 30 42 48.2 106.7 -3.1 0.0 -51 229 No stop 02 39 20 =2234+282 19 34 12 48.7 107.6 -3.1 0.0 159 256 02 35 51 Schedule for WSTRBORK (Code Wb ) 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 ---------------------------------------------------------------------------------------- --- Wed 29 May 2024 Day 150 --- 02 40 30 J2320+1829 19 35 22 34.7 105.7 -3.8 0.0 20 256 02 40 30 02 41 50 =2318+182 19 36 43 34.9 106.0 -3.8 0.0 80 267 02 40 31 02 41 50 ILTJ2317 19 36 43 35.6 106.7 -3.7 0.0 -16 267 No stop 02 46 50 --- 19 41 43 36.3 107.8 -3.6 0.0 284 305 02 41 51 02 47 20 J2320+1829 19 42 13 35.7 107.3 -3.7 0.0 14 305 02 47 20 02 48 40 =2318+182 19 43 34 35.9 107.6 -3.6 0.0 80 316 02 47 21 02 48 40 ILTJ2317 19 43 34 36.5 108.3 -3.6 0.0 -16 316 No stop 02 53 40 --- 19 48 34 37.3 109.4 -3.5 0.0 284 354 02 48 41 02 54 10 J2320+1829 19 49 05 36.6 108.9 -3.5 0.0 14 354 02 54 10 02 55 30 =2318+182 19 50 25 36.8 109.2 -3.5 0.0 80 365 02 54 11 02 55 30 ILTJ2317 19 50 25 37.5 109.9 -3.5 0.0 -16 365 No stop 03 00 30 --- 19 55 26 38.2 111.1 -3.4 0.0 284 403 02 55 31 03 01 00 J2320+1829 19 55 56 37.6 110.5 -3.4 0.0 14 403 03 01 00 03 02 20 =2318+182 19 57 16 37.8 110.9 -3.4 0.0 80 414 03 01 01 03 02 20 ILTJ2317 19 57 16 38.5 111.5 -3.4 0.0 -16 414 No stop 03 07 20 --- 20 02 17 39.2 112.8 -3.3 0.0 284 452 03 02 21 03 07 50 J2320+1829 20 02 47 38.6 112.2 -3.3 0.0 14 452 03 07 50 03 09 10 =2318+182 20 04 07 38.8 112.5 -3.3 0.0 80 462 03 07 51 03 09 10 J2236+2828 20 04 07 52.9 115.6 -2.6 0.0 -51 462 No stop 03 12 40 =2234+282 20 07 38 53.3 116.6 -2.5 0.0 159 490 03 09 11 03 13 50 J2320+1829 20 08 48 39.4 113.7 -3.2 0.0 20 490 03 13 50 03 15 10 =2318+182 20 10 08 39.6 114.0 -3.2 0.0 80 500 03 13 51 03 15 10 ILTJ2317 20 10 08 40.3 114.7 -3.1 0.0 -16 500 No stop 03 20 10 --- 20 15 09 41.0 116.0 -3.1 0.0 284 538 03 15 11 03 20 40 J2320+1829 20 15 39 40.4 115.4 -3.1 0.0 14 538 03 20 40 03 22 00 =2318+182 20 16 59 40.5 115.8 -3.1 0.0 80 549 03 20 41 ---------- Fringe-finder ---------- 03 23 00 J2253+1608 20 17 59 42.2 124.9 -2.6 0.0 24 549 03 23 00 03 27 00 =3C454.3 20 22 00 42.7 126.0 -2.6 0.0 240 580 03 23 01 Schedule for WSTRBORK (Code Wb ) 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 ---------------------------------------------------------------------------------------- --- Wed 29 May 2024 Day 150 --- ---------- Going to ILTJ2317 ---------- 03 28 00 J2320+1829 20 23 00 41.3 117.3 -3.0 0.0 25 580 03 28 00 03 30 00 =2318+182 20 25 00 41.6 117.8 -2.9 0.0 120 595 03 28 01 03 30 00 ILTJ2317 20 25 00 42.3 118.6 -2.9 0.0 -16 595 No stop 03 35 00 --- 20 30 01 42.9 119.9 -2.8 0.0 284 634 03 30 01 03 35 30 J2320+1829 20 30 31 42.3 119.3 -2.9 0.0 14 634 03 35 30 03 36 50 =2318+182 20 31 52 42.5 119.6 -2.8 0.0 80 644 03 35 31 03 36 50 ILTJ2317 20 31 52 43.2 120.4 -2.8 0.0 -16 644 No stop 03 41 50 --- 20 36 52 43.8 121.8 -2.7 0.0 284 683 03 36 51 03 42 20 J2320+1829 20 37 22 43.2 121.1 -2.7 0.0 14 683 03 42 20 03 43 40 =2318+182 20 38 43 43.4 121.5 -2.7 0.0 80 693 03 42 21 03 43 40 ILTJ2317 20 38 43 44.1 122.3 -2.7 0.0 -16 693 No stop 03 48 40 --- 20 43 43 44.7 123.7 -2.6 0.0 284 732 03 43 41 03 49 10 J2320+1829 20 44 14 44.1 123.0 -2.6 0.0 14 732 03 49 10 03 50 30 =2318+182 20 45 34 44.3 123.4 -2.6 0.0 80 742 03 49 11 03 50 30 J2236+2828 20 45 34 58.1 128.7 -1.9 0.0 -51 742 No stop 03 54 00 =2234+282 20 49 04 58.6 129.9 -1.8 0.0 159 769 03 50 31 03 55 10 J2320+1829 20 50 15 44.9 124.7 -2.5 0.0 20 769 03 55 10 03 56 30 =2318+182 20 51 35 45.0 125.1 -2.5 0.0 80 779 03 55 11 03 56 30 ILTJ2317 20 51 35 45.7 125.9 -2.4 0.0 -16 779 No stop 04 01 30 --- 20 56 36 46.3 127.4 -2.4 0.0 284 818 03 56 31 04 02 00 J2320+1829 20 57 06 45.7 126.7 -2.4 0.0 14 818 04 02 00 04 03 20 =2318+182 20 58 26 45.9 127.1 -2.4 0.0 80 828 04 02 01 04 03 20 ILTJ2317 20 58 26 46.5 128.0 -2.3 0.0 -16 828 No stop 04 08 20 --- 21 03 27 47.1 129.5 -2.3 0.0 284 867 04 03 21 04 08 50 J2320+1829 21 03 57 46.5 128.7 -2.3 0.0 14 867 04 08 50 04 10 10 =2318+182 21 05 17 46.7 129.1 -2.3 0.0 80 877 04 08 51 04 10 10 ILTJ2317 21 05 17 47.3 130.0 -2.2 0.0 -16 877 No stop 04 15 10 --- 21 10 18 47.9 131.6 -2.1 0.0 284 916 04 10 11 Schedule for WSTRBORK (Code Wb ) 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 ---------------------------------------------------------------------------------------- --- Wed 29 May 2024 Day 150 --- 04 15 40 J2320+1829 21 10 48 47.3 130.8 -2.2 0.0 14 916 04 15 40 04 17 00 =2318+182 21 12 08 47.5 131.2 -2.2 0.0 80 926 04 15 41 04 17 00 ILTJ2317 21 12 08 48.1 132.1 -2.1 0.0 -16 926 No stop 04 22 00 --- 21 17 09 48.6 133.7 -2.0 0.0 284 965 04 17 01 04 22 30 J2320+1829 21 17 39 48.1 132.9 -2.1 0.0 14 965 04 22 30 04 23 50 =2318+182 21 18 59 48.2 133.3 -2.1 0.0 80 975 04 22 31 04 23 50 J2236+2828 21 18 59 61.7 141.5 -1.3 0.0 -51 975 No stop 04 27 20 =2234+282 21 22 30 62.0 143.0 -1.3 0.0 159 1002 04 23 51 04 28 30 J2320+1829 21 23 40 48.7 134.8 -2.0 0.0 20 1002 04 28 30 04 29 50 =2318+182 21 25 00 48.9 135.3 -1.9 0.0 80 1013 04 28 31 04 29 50 ILTJ2317 21 25 00 49.5 136.2 -1.9 0.0 -16 1013 No stop 04 34 50 --- 21 30 01 50.0 137.9 -1.8 0.0 284 1051 04 29 51 04 35 20 J2320+1829 21 30 31 49.5 137.0 -1.9 0.0 14 1051 04 35 20 04 36 40 =2318+182 21 31 51 49.6 137.5 -1.8 0.0 80 1061 04 35 21 04 36 40 ILTJ2317 21 31 51 50.2 138.5 -1.8 0.0 -16 1061 No stop 04 41 40 --- 21 36 52 50.7 140.2 -1.7 0.0 284 1100 04 36 41 04 42 10 J2320+1829 21 37 22 50.1 139.3 -1.7 0.0 14 1100 04 42 10 04 43 30 =2318+182 21 38 42 50.3 139.8 -1.7 0.0 80 1110 04 42 11 04 43 30 ILTJ2317 21 38 42 50.8 140.8 -1.7 0.0 -16 1110 No stop 04 48 30 --- 21 43 43 51.3 142.6 -1.6 0.0 284 1149 04 43 31 04 49 00 J2320+1829 21 44 13 50.8 141.7 -1.6 0.0 14 1149 04 49 00 04 50 20 =2318+182 21 45 34 50.9 142.1 -1.6 0.0 80 1159 04 49 01 04 50 20 ILTJ2317 21 45 34 51.5 143.2 -1.5 0.0 -16 1159 No stop 04 55 20 --- 21 50 34 51.9 145.0 -1.5 0.0 284 1198 04 50 21 04 55 50 J2320+1829 21 51 05 51.4 144.0 -1.5 0.0 14 1198 04 55 50 04 57 10 =2318+182 21 52 25 51.5 144.5 -1.5 0.0 80 1208 04 55 51 04 57 10 J2236+2828 21 52 25 64.3 156.7 -0.8 0.0 -51 1208 No stop 05 00 40 =2234+282 21 55 55 64.5 158.4 -0.7 0.0 159 1235 04 57 11 05 01 50 J2320+1829 21 57 06 51.9 146.2 -1.4 0.0 20 1235 05 01 50 05 03 10 =2318+182 21 58 26 52.1 146.7 -1.4 0.0 80 1246 05 01 51 Schedule for WSTRBORK (Code Wb ) 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 ---------------------------------------------------------------------------------------- --- Wed 29 May 2024 Day 150 --- 05 03 10 ILTJ2317 21 58 26 52.6 147.8 -1.3 0.0 -16 1246 No stop 05 08 10 --- 22 03 27 53.0 149.7 -1.3 0.0 284 1284 05 03 11 05 08 40 J2320+1829 22 03 57 52.5 148.7 -1.3 0.0 14 1284 05 08 40 05 10 00 =2318+182 22 05 17 52.6 149.2 -1.3 0.0 80 1295 05 08 41 05 10 00 ILTJ2317 22 05 17 53.1 150.4 -1.2 0.0 -16 1295 No stop 05 15 00 --- 22 10 18 53.5 152.2 -1.1 0.0 284 1333 05 10 01 05 15 30 J2320+1829 22 10 48 53.0 151.2 -1.2 0.0 14 1333 05 15 30 05 16 50 =2318+182 22 12 08 53.1 151.7 -1.2 0.0 80 1344 05 15 31 05 16 50 ILTJ2317 22 12 08 53.6 152.9 -1.1 0.0 -16 1344 No stop 05 21 50 --- 22 17 09 53.9 154.9 -1.0 0.0 284 1382 05 16 51 05 22 20 J2320+1829 22 17 39 53.5 153.8 -1.1 0.0 14 1382 05 22 20 05 23 40 =2318+182 22 18 59 53.6 154.3 -1.1 0.0 80 1393 05 22 21 05 23 40 ILTJ2317 22 18 59 54.0 155.6 -1.0 0.0 -16 1393 No stop 05 28 40 --- 22 24 00 54.3 157.5 -0.9 0.0 284 1431 05 23 41 05 29 10 J2320+1829 22 24 30 53.9 156.5 -1.0 0.0 14 1431 05 29 10 05 30 30 =2318+182 22 25 50 54.0 157.0 -0.9 0.0 80 1441 05 29 11 05 30 30 J2236+2828 22 25 50 65.6 173.8 -0.2 0.0 -51 1441 No stop 05 34 00 =2234+282 22 29 21 65.6 175.7 -0.1 0.0 159 1469 05 30 31 05 35 10 J2320+1829 22 30 31 54.3 158.8 -0.9 0.0 20 1469 05 35 10 05 36 30 =2318+182 22 31 51 54.3 159.3 -0.8 0.0 80 1479 05 35 11 05 36 30 ILTJ2317 22 31 51 54.8 160.7 -0.8 0.0 -16 1479 No stop 05 41 30 --- 22 36 52 55.0 162.7 -0.7 0.0 284 1517 05 36 31 05 42 00 J2320+1829 22 37 22 54.6 161.5 -0.7 0.0 14 1517 05 42 00 05 43 20 =2318+182 22 38 42 54.7 162.1 -0.7 0.0 80 1528 05 42 01 05 43 20 ILTJ2317 22 38 42 55.1 163.4 -0.7 0.0 -16 1528 No stop 05 48 20 --- 22 43 43 55.3 165.5 -0.6 0.0 284 1566 05 43 21 05 48 50 J2320+1829 22 44 13 54.9 164.3 -0.6 0.0 14 1566 05 48 50 05 50 10 =2318+182 22 45 33 55.0 164.8 -0.6 0.0 80 1577 05 48 51 05 50 10 ILTJ2317 22 45 33 55.3 166.2 -0.5 0.0 -16 1577 No stop 05 55 10 --- 22 50 34 55.5 168.3 -0.5 0.0 284 1615 05 50 11 Schedule for WSTRBORK (Code Wb ) 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 ---------------------------------------------------------------------------------------- --- Wed 29 May 2024 Day 150 --- 05 55 40 J2320+1829 22 51 04 55.2 167.1 -0.5 0.0 14 1615 05 55 40 05 57 00 =2318+182 22 52 25 55.2 167.7 -0.5 0.0 80 1626 05 55 41 05 57 00 ILTJ2317 22 52 25 55.6 169.1 -0.4 0.0 -16 1626 No stop 06 02 00 --- 22 57 25 55.7 171.1 -0.4 0.0 284 1664 05 57 01 06 02 30 J2320+1829 22 57 55 55.4 169.9 -0.4 0.0 14 1664 06 02 30 06 03 50 =2318+182 22 59 16 55.4 170.5 -0.4 0.0 80 1675 06 02 31 06 03 50 J2236+2828 22 59 16 65.4 191.5 0.4 0.0 -51 1675 No stop 06 07 20 =2234+282 23 02 46 65.2 193.3 0.4 0.0 159 1702 06 03 51 06 08 30 J2320+1829 23 03 56 55.5 172.4 -0.3 0.0 20 1702 06 08 30 06 09 50 =2318+182 23 05 17 55.6 173.0 -0.3 0.0 80 1712 06 08 31 06 09 50 ILTJ2317 23 05 17 55.8 174.4 -0.2 0.0 -16 1712 No stop 06 14 50 --- 23 10 17 55.9 176.6 -0.1 0.0 284 1751 06 09 51 06 15 20 J2320+1829 23 10 48 55.6 175.3 -0.2 0.0 14 1751 06 15 20 06 16 40 =2318+182 23 12 08 55.7 175.9 -0.2 0.0 80 1761 06 15 21 06 16 40 ILTJ2317 23 12 08 55.9 177.3 -0.1 0.0 -16 1761 No stop 06 21 40 --- 23 17 09 55.9 179.4 -0.0 0.0 284 1800 06 16 41 06 22 10 J2320+1829 23 17 39 55.7 178.2 -0.1 0.0 14 1800 06 22 10 06 23 30 =2318+182 23 18 59 55.7 178.7 -0.1 0.0 80 1810 06 22 11 06 23 30 ILTJ2317 23 18 59 55.9 180.2 0.0 0.0 -16 1810 No stop 06 28 30 --- 23 24 00 55.9 182.3 0.1 0.0 284 1849 06 23 31 06 29 00 J2320+1829 23 24 30 55.7 181.1 0.0 0.0 14 1849 06 29 00 06 30 20 =2318+182 23 25 50 55.7 181.6 0.1 0.0 80 1859 06 29 01 06 30 20 ILTJ2317 23 25 50 55.9 183.1 0.1 0.0 -16 1859 No stop 06 35 20 --- 23 30 51 55.9 185.2 0.2 0.0 284 1898 06 30 21 06 35 50 J2320+1829 23 31 21 55.7 183.9 0.2 0.0 14 1898 06 35 50 06 37 10 =2318+182 23 32 41 55.6 184.5 0.2 0.0 80 1908 06 35 51 06 37 10 J2236+2828 23 32 41 63.6 208.1 0.9 0.0 -51 1908 No stop 06 40 40 =2234+282 23 36 12 63.4 209.8 1.0 0.0 159 1935 06 37 11 06 41 50 J2320+1829 23 37 22 55.6 186.5 0.3 0.0 20 1935 06 41 50 06 43 10 =2318+182 23 38 42 55.6 187.0 0.3 0.0 80 1945 06 41 51 Schedule for WSTRBORK (Code Wb ) 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 ---------------------------------------------------------------------------------------- --- Wed 29 May 2024 Day 150 --- 06 43 10 ILTJ2317 23 38 42 55.7 188.5 0.3 0.0 -16 1945 No stop 06 48 10 --- 23 43 43 55.6 190.6 0.4 0.0 284 1984 06 43 11 06 48 40 J2320+1829 23 44 13 55.4 189.3 0.4 0.0 14 1984 06 48 40 06 50 00 =2318+182 23 45 33 55.4 189.9 0.4 0.0 80 1994 06 48 41 06 50 00 ILTJ2317 23 45 33 55.5 191.4 0.5 0.0 -16 1994 No stop 06 53 20 --- 23 48 54 55.4 192.8 0.5 0.0 184 2020 06 50 01 06 54 00 J2320+1829 23 49 34 55.3 191.5 0.5 0.0 24 2020 06 54 00 06 55 00 =2318+182 23 50 34 55.3 191.9 0.5 0.0 60 2028 06 54 01 ---------- Fringe-finder ---------- 06 56 00 J2253+1608 23 51 34 51.7 202.2 0.9 0.0 24 2028 06 56 00 07 00 00 =3C454.3 23 55 35 51.5 203.7 1.0 0.0 240 2059 06 56 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: 2 Station: WSTRBORK Total bit rate: 1024 Format: VDIF Bits per sample: 2 Sample rate: 64.000 Number of channels: 8 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 1247.00 1247.00 1247.00 1247.00 1247.00 1247.00 1247.00 1247.00 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 = 1 9 1 9 2 10 2 10 BBC SB= L L U U L L U U IF = A1 B1 A1 B1 A1 B1 A1 B1 The following frequency sets based on these setups were used. Frequency Set: 2 Setup file default. Used with PCAL = off LO sum= 1626.49 1626.49 1626.49 1626.49 1690.49 1690.49 1690.49 1690.49 BBC fr= 379.49 379.49 379.49 379.49 443.49 443.49 443.49 443.49 Bandwd= 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 Matching frequency sets: 2 Track assignments are: track1= 1, 2, 3, 4, 5, 6, 7, 8 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) * ILTJ2317 23 14 45.892345 * 23 17 15.380000 23 18 27.698821 0.00 18 27 15.44487 * 18 43 39.10000 18 51 27.48916 0.00 From catalog imbedded in main SCHED input file. * B2319+60_D 23 19 41.329180 * 23 21 55.200000 23 22 59.103077 0.00 60 08 03.45038 * 60 24 30.70000 60 32 11.63925 0.00 From catalog imbedded in main SCHED input file. 2234+282 22 34 01.728802 * 22 36 22.470847 22 37 30.696616 0.34 * J2236+2828 28 13 23.21045 * 28 28 57.41317 28 36 17.90081 0.31 J2236+28 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 91001 observations. 3C454.3 22 51 29.519739 * 22 53 57.747939 22 55 09.602203 0.65 * J2253+1608 15 52 54.34808 * 16 08 53.56091 16 16 30.32517 0.73 2251+158 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc J2253+16 GSFC 2016a X/S astro solution, 41272 observations. 2318+182 23 18 16.895310 * 23 20 46.775967 23 21 59.268461 0.13 * J2320+1829 18 12 59.29947 * 18 29 25.77527 18 37 15.69772 0.18 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 136 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 ILTJ2317 sess224.L1024 1 2 3 4 5 6 7 8 13 14 2.722 230.361 B2319+60_D sess224.L1024 1 2 3 4 5 6 7 8 0.075 4.831 J2236+2828 sess224.L1024 1 2 3 4 5 6 7 8 13 0.467 24.791 J2253+1608 sess224.L1024 1 2 3 4 5 6 7 8 13 14 0.203 18.433 J2320+1829 sess224.L1024 1 2 3 4 5 6 7 8 13 14 0.972 82.780 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) ILTJ2317 71.5 B2319+60_D 64.3 J2236+2828 77.5 J2253+1608 77.5 J2320+1829 70.7 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