COVER INFORMATION Station: KVNUS (Code Ku ) Experiment: Unravelling the Nature of the Jets Magnetic Field within PKS 1510-089 Exp. Code: GM079 Schedule Version: 7.00 Processed by SCHED version: 11.60 Release 11.6; April 2020 PI: Nicholas Roy MacDonald Address: Max Planck Institute for Radio Astronomy Auf dem Hugel 69 Bonn Germany Phone: +49228525424 EMAIL: nmacdona@mpifr-bonn.mpg.de Fax: Phone during observation: +492257301155 Observing mode: Notes: PHASECAL should be ON Schedule for KVNUS (Code Ku ) Page 2 Unravelling the Nature of the Jets Magnetic Field within PKS 1510-089 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 16 Mar 2022 Day 75 --- ---------- POINTING ---------- Next scan frequencies: 43072.00 43072.00 43136.00 43136.00 43200.00 43200.00 43264.00 43264.00 43072.00 43072.00 43136.00 43136.00 43200.00 43200.00 43264.00 43264.00 Next BBC frequencies: 8962.00 8962.00 9026.00 9026.00 9090.00 9090.00 9154.00 9154.00 8962.00 8962.00 9026.00 9026.00 9090.00 9090.00 9154.00 9154.00 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 15 00 00 1510-089 11 13 44 17.9 115.9 -4.0 -47.8 0 0 15 00 00 15 07 00 --- 11 20 45 19.2 117.2 -3.9 -47.2 420 108 15 00 01 15 07 45 1510-089 11 21 30 19.3 117.3 -3.9 -47.1 43 108 15 07 45 15 14 45 --- 11 28 32 20.6 118.6 -3.8 -46.4 420 216 15 07 46 15 15 30 1510-089 11 29 17 20.7 118.7 -3.7 -46.3 43 216 15 15 30 15 22 30 --- 11 36 18 22.0 120.0 -3.6 -45.5 420 325 15 15 31 ---------- POINTING ---------- 15 29 10 3C279 11 42 59 45.0 153.4 -1.2 -21.5 386 325 15 29 10 15 35 50 --- 11 49 40 45.6 155.6 -1.1 -19.8 400 428 15 29 11 ---------- POINTING ---------- 15 42 30 1510-089 11 56 21 25.4 123.9 -3.3 -43.2 386 428 15 42 30 15 49 30 --- 12 03 22 26.6 125.3 -3.2 -42.3 420 536 15 42 31 15 50 15 1510-089 12 04 07 26.7 125.4 -3.2 -42.2 43 536 15 50 15 15 57 15 --- 12 11 09 27.9 126.9 -3.0 -41.2 420 644 15 50 16 15 58 00 1510-089 12 11 54 28.0 127.0 -3.0 -41.1 43 644 15 58 00 16 05 00 --- 12 18 55 29.2 128.5 -2.9 -40.1 420 752 15 58 01 ---------- POINTING ---------- 16 11 40 3C279 12 25 36 47.9 168.2 -0.5 -9.6 384 752 16 11 40 16 18 20 --- 12 32 17 48.1 170.6 -0.4 -7.6 400 855 16 11 41 ---------- POINTING ---------- 16 25 00 1510-089 12 38 58 32.2 133.0 -2.6 -37.0 384 855 16 25 00 16 32 00 --- 12 45 59 33.3 134.7 -2.5 -35.9 420 964 16 25 01 16 32 45 1510-089 12 46 44 33.4 134.9 -2.5 -35.7 43 964 16 32 45 16 39 45 --- 12 53 45 34.4 136.6 -2.3 -34.5 420 1072 16 32 46 Schedule for KVNUS (Code Ku ) Page 3 Unravelling the Nature of the Jets Magnetic Field within PKS 1510-089 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 16 Mar 2022 Day 75 --- 16 40 30 1510-089 12 54 31 34.5 136.8 -2.3 -34.4 43 1072 16 40 30 16 47 30 --- 13 01 32 35.4 138.5 -2.2 -33.1 420 1180 16 40 31 ---------- POINTING ---------- 16 54 10 3C279 13 08 13 48.5 184.1 0.2 3.3 382 1180 16 54 10 17 00 50 --- 13 14 54 48.3 186.6 0.3 5.4 400 1283 16 54 11 ---------- POINTING ---------- 17 07 30 1510-089 13 21 35 38.0 143.8 -1.9 -29.1 382 1283 17 07 30 17 14 30 --- 13 28 36 38.8 145.8 -1.8 -27.6 420 1391 17 07 31 17 15 15 1510-089 13 29 21 38.9 146.0 -1.7 -27.5 43 1391 17 15 15 17 22 15 --- 13 36 22 39.7 148.0 -1.6 -25.9 420 1499 17 15 16 17 23 00 1510-089 13 37 08 39.8 148.2 -1.6 -25.7 43 1499 17 23 00 17 30 00 --- 13 44 09 40.5 150.2 -1.5 -24.1 420 1608 17 23 01 ---------- POINTING ---------- 17 36 40 3C279 13 50 50 46.7 199.6 0.9 15.9 381 1608 17 36 40 17 43 20 --- 13 57 31 46.2 201.9 1.0 17.8 400 1711 17 36 41 ---------- POINTING ---------- 17 50 00 1510-089 14 04 12 42.3 156.4 -1.2 -19.3 381 1711 17 50 00 17 57 00 --- 14 11 13 42.9 158.6 -1.0 -17.5 420 1819 17 50 01 17 57 45 1510-089 14 11 58 42.9 158.9 -1.0 -17.3 43 1819 17 57 45 18 04 45 --- 14 18 59 43.4 161.1 -0.9 -15.5 420 1927 17 57 46 18 05 30 1510-089 14 19 45 43.5 161.4 -0.9 -15.3 43 1927 18 05 30 18 12 30 --- 14 26 46 43.9 163.7 -0.8 -13.4 420 2035 18 05 31 ---------- POINTING ---------- 18 19 10 3C279 14 33 27 42.8 213.5 1.6 26.8 381 2035 18 19 10 18 25 50 --- 14 40 08 42.0 215.5 1.7 28.4 400 2138 18 19 11 ---------- POINTING ---------- 18 32 30 1510-089 14 46 49 44.8 170.5 -0.5 -7.8 381 2138 18 32 30 18 39 30 --- 14 53 50 45.0 172.9 -0.3 -5.8 420 2247 18 32 31 Schedule for KVNUS (Code Ku ) Page 4 Unravelling the Nature of the Jets Magnetic Field within PKS 1510-089 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 16 Mar 2022 Day 75 --- 18 40 15 1510-089 14 54 35 45.0 173.2 -0.3 -5.6 43 2247 18 40 15 18 47 15 --- 15 01 36 45.2 175.6 -0.2 -3.6 420 2355 18 40 16 18 48 00 1510-089 15 02 22 45.2 175.9 -0.2 -3.4 43 2355 18 48 00 18 55 00 --- 15 09 23 45.3 178.4 -0.1 -1.3 420 2463 18 48 01 ---------- POINTING ---------- 19 01 40 3C279 15 16 04 37.3 225.3 2.3 35.6 382 2463 19 01 40 19 08 20 --- 15 22 45 36.3 227.0 2.4 36.8 400 2566 19 01 41 ---------- POINTING ---------- 19 15 00 1510-089 15 29 26 45.1 185.4 0.3 4.4 382 2566 19 15 00 19 22 00 --- 15 36 27 45.0 187.8 0.4 6.4 420 2674 19 15 01 19 22 45 1510-089 15 37 12 44.9 188.1 0.4 6.7 43 2674 19 22 45 19 29 45 --- 15 44 13 44.7 190.5 0.5 8.6 420 2782 19 22 46 19 30 30 1510-089 15 44 59 44.7 190.8 0.5 8.9 43 2782 19 30 30 19 37 30 --- 15 52 00 44.4 193.2 0.6 10.8 420 2891 19 30 31 ---------- POINTING ---------- 19 44 10 3C279 15 58 41 30.6 235.3 3.0 42.2 383 2891 19 44 10 19 50 50 --- 16 05 22 29.5 236.7 3.1 43.1 400 2994 19 44 11 ---------- POINTING ---------- 19 57 30 1510-089 16 12 03 43.2 199.8 1.0 16.2 384 2994 19 57 30 20 04 30 --- 16 19 04 42.7 202.1 1.1 18.1 420 3102 19 57 31 20 05 15 1510-089 16 19 49 42.7 202.3 1.1 18.3 43 3102 20 05 15 20 12 15 --- 16 26 50 42.1 204.5 1.2 20.0 420 3210 20 05 16 20 13 00 1510-089 16 27 36 42.0 204.8 1.2 20.2 43 3210 20 13 00 20 20 00 --- 16 34 37 41.4 206.9 1.3 21.9 420 3318 20 13 01 ---------- POINTING ---------- 20 26 40 3C279 16 41 18 23.1 243.7 3.7 47.2 385 3318 20 26 40 20 33 20 --- 16 47 59 21.9 244.9 3.8 47.8 400 3421 20 26 41 Schedule for KVNUS (Code Ku ) Page 5 Unravelling the Nature of the Jets Magnetic Field within PKS 1510-089 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 16 Mar 2022 Day 75 --- ---------- POINTING ---------- 20 40 00 1510-089 16 54 40 39.4 212.9 1.7 26.6 386 3421 20 40 00 20 47 00 --- 17 01 41 38.6 214.9 1.8 28.1 420 3530 20 40 01 20 47 45 1510-089 17 02 26 38.5 215.1 1.8 28.3 43 3530 20 47 45 20 54 45 --- 17 09 27 37.6 217.0 1.9 29.7 420 3638 20 47 46 20 55 30 1510-089 17 10 12 37.5 217.2 1.9 29.9 43 3638 20 55 30 21 02 30 --- 17 17 14 36.7 219.1 2.1 31.3 420 3746 20 55 31 ---------- POINTING ---------- 21 09 10 3C279 17 23 55 15.1 251.1 4.4 50.7 387 3746 21 09 10 21 15 50 --- 17 30 36 13.8 252.2 4.6 51.1 400 3849 21 09 11 ---------- POINTING ---------- 21 22 30 1510-089 17 37 17 34.0 224.1 2.4 35.0 387 3849 21 22 30 21 29 30 --- 17 44 18 32.9 225.8 2.5 36.2 420 3957 21 22 31 21 30 15 1510-089 17 45 03 32.8 226.0 2.5 36.4 43 3957 21 30 15 21 37 15 --- 17 52 04 31.8 227.6 2.6 37.5 420 4066 21 30 16 21 38 00 1510-089 17 52 49 31.7 227.8 2.6 37.6 43 4066 21 38 00 21 45 00 --- 17 59 51 30.6 229.4 2.8 38.7 420 4174 21 38 01 ---------- POINTING ---------- 21 51 40 3C279 18 06 32 6.8 257.7 5.2 53.1 388 4174 21 51 40 21 58 20 --- 18 13 13 5.5 258.7 5.3 H 53.3 0 4277 21 51 41 ---------- POINTING ---------- 22 05 00 1510-089 18 19 54 27.4 233.7 3.1 41.6 388 4277 22 05 00 22 12 00 --- 18 26 55 26.3 235.2 3.2 42.6 420 4385 22 05 01 22 12 45 1510-089 18 27 40 26.1 235.3 3.2 42.7 43 4385 22 12 45 22 19 45 --- 18 34 41 24.9 236.7 3.3 43.6 420 4493 22 12 46 22 20 30 1510-089 18 35 26 24.8 236.9 3.4 43.6 43 4493 22 20 30 22 27 30 --- 18 42 28 23.6 238.2 3.5 44.5 420 4601 22 20 31 Schedule for KVNUS (Code Ku ) Page 6 Unravelling the Nature of the Jets Magnetic Field within PKS 1510-089 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 16 Mar 2022 Day 75 --- ---------- POINTING ---------- 22 34 10 1156+295 18 49 09 7.7 300.5 6.8 53.4 376 4601 22 34 10 22 40 50 --- 18 55 50 6.5 301.4 6.9 52.7 400 4704 22 34 11 ---------- POINTING ---------- 22 47 30 1510-089 19 02 31 20.1 242.0 3.8 46.7 376 4704 22 47 30 22 54 30 --- 19 09 32 18.8 243.2 3.9 47.4 420 4813 22 47 31 22 55 15 1510-089 19 10 17 18.7 243.4 3.9 47.4 43 4813 22 55 15 23 02 15 --- 19 17 18 17.4 244.6 4.1 48.1 420 4921 22 55 16 23 03 00 1510-089 19 18 03 17.3 244.7 4.1 48.2 43 4921 23 03 00 23 10 00 --- 19 25 05 16.0 245.9 4.2 48.8 420 5029 23 03 01 23 24 05 1510-089 19 39 12 13.3 248.2 4.4 50.0 843 5029 23 24 05 23 29 30 --- 19 44 38 12.3 249.1 4.5 50.4 325 5113 23 24 06 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess122.Q2048glob --- 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: 19 Station: KVNUS Total bit rate: 2048 Format: VDIF Bits per sample: 2 Sample rate: 64.000 Number of channels: 16 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 34110.00 34110.00 34110.00 34110.00 34110.00 34110.00 34110.00 34110.00 34110.00 34110.00 34110.00 34110.00 34110.00 34110.00 34110.00 34110.00 Net SB= L U L U L U L U L U L U L U L U IF SB = U U U U U U U U U U U U U U U U Pol. = LCP LCP LCP LCP LCP LCP LCP LCP RCP RCP RCP RCP RCP RCP RCP RCP BBC = 2 2 2 2 2 2 2 2 4 4 4 4 4 4 4 4 BBC SB= L U L U L U L U L U L U L U L U IF = A A A A A A A A B B B B B B B B The following frequency sets based on these setups were used. Frequency Set: 1 Setup file default. Used with PCAL = 1MHz LO sum= 43072.00 43072.00 43136.00 43136.00 43200.00 43200.00 43264.00 43264.00 43072.00 43072.00 43136.00 43136.00 43200.00 43200.00 43264.00 43264.00 BBC fr= 8962.00 8962.00 9026.00 9026.00 9090.00 9090.00 9154.00 9154.00 8962.00 8962.00 9026.00 9026.00 9090.00 9090.00 9154.00 9154.00 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: 1 2 3 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) J1159+2914 11 56 57.786211 * 11 59 31.833912 12 00 40.929516 0.11 * 1156+295 29 31 25.73868 * 29 14 43.82678 29 07 16.19518 0.10 J1159+29 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.vlba.2012jul rfc_2012b Petrov, 2012, unpublished 64535 observations J1256-0547 12 53 35.831299 * 12 56 11.166567 12 57 20.504851 0.69 * 3C279 -05 31 07.99595 *-05 47 21.52481 -05 54 36.62774 0.92 1253-055 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.vlba.2012jul J1256-05 GSFC 2011B astro solution 7402 Observations J1512-0905 15 10 08.900178 * 15 12 50.532926 15 14 02.216367 0.10 * 1510-089 -08 54 47.61966 *-09 05 59.82981 -09 11 01.93761 0.10 J1512-09 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.vlba.2012jul rfc_2012b Petrov, 2012, unpublished 6238 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 1156+295 sess122.Q2048glob 1 4 5 6 7 8 9 10 0.417 12.331 3C279 sess122.Q2048glob 1 4 5 6 7 8 9 10 2.711 46.869 1510-089 sess122.Q2048glob 1 4 5 6 7 8 9 10 12.621 279.808 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) 1156+295 152.1 3C279 161.0 1510-089 127.4 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