COVER INFORMATION Station: IRBENE16 (Code Ib ) Experiment: Spatially resolved near-infrared and EVN observations of two blazars Exp. Code: eh042a Schedule Version: 2.00 Processed by SCHED version: 11.60 Release 11.6; April 2020 PI: Hovatta Address: Finnish Centre for Astronomy with ESO Vesilinnantie 5 University of Turku Finland Phone: +358504916007 EMAIL: talvikki.hovatta@utu.fi Fax: Phone during observation: +358504916007 Observing mode: vlbi Notes: # Please, make sure PHASE CAL is OFF # COVER LETTER: Schedule for IRBENE16 (Code Ib ) Page 2 Spatially resolved near-infrared and EVN observations of two blazars 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 26 May 2023 Day 146 --- 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: 730.49 730.49 730.49 730.49 794.49 794.49 794.49 794.49 858.49 858.49 858.49 858.49 922.49 922.49 922.49 922.49 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 21 30 00 1901+319 15 14 10 43.8-262.0 -3.8 -38.8 0 0 21 30 00 21 35 00 --- 15 19 11 44.5-260.8 -3.7 -38.7 300 77 21 30 01 21 37 00 1749+096 15 21 11 34.0-226.9 -2.5 -23.4 100 77 21 37 00 21 42 00 --- 15 26 12 34.5-225.5 -2.4 -22.8 300 155 21 37 01 21 43 00 1811+062 15 27 12 29.3-229.5 -2.8 -24.2 54 155 21 43 00 21 46 00 --- 15 30 12 29.6-228.7 -2.7 -23.9 180 201 21 43 01 21 46 30 1811+062 15 30 42 29.6-228.6 -2.7 -23.9 27 201 21 46 30 22 01 00 --- 15 45 15 31.1-224.8 -2.5 -22.3 870 425 21 46 31 22 01 30 1811+062 15 45 45 31.1-224.6 -2.5 -22.3 27 425 22 01 30 22 16 00 --- 16 00 17 32.4-220.7 -2.2 -20.6 870 649 22 01 31 22 16 30 1811+062 16 00 47 32.5-220.5 -2.2 -20.5 27 649 22 16 30 22 31 00 --- 16 15 20 33.7-216.5 -2.0 -18.7 870 873 22 16 31 22 33 00 1901+319 16 17 20 52.0-246.0 -2.8 -35.3 102 873 22 33 00 22 38 00 --- 16 22 21 52.6-244.6 -2.7 -34.9 300 951 22 33 01 22 40 00 1749+096 16 24 21 39.2-208.5 -1.5 -15.1 99 951 22 40 00 22 45 00 --- 16 29 22 39.5-207.0 -1.4 -14.3 300 1028 22 40 01 22 46 00 1811+062 16 30 22 34.8-212.2 -1.7 -16.7 54 1028 22 46 00 22 49 00 --- 16 33 23 35.0-211.3 -1.7 -16.3 180 1074 22 46 01 22 49 30 1811+062 16 33 53 35.1-211.1 -1.7 -16.2 27 1074 22 49 30 23 04 00 --- 16 48 25 36.0-206.9 -1.4 -14.1 870 1298 22 49 31 23 04 30 1811+062 16 48 55 36.0-206.7 -1.4 -14.0 27 1298 23 04 30 23 19 00 --- 17 03 28 36.9-202.3 -1.2 -11.8 870 1523 23 04 31 23 19 30 1811+062 17 03 58 36.9-202.2 -1.2 -11.8 27 1523 23 19 30 23 34 00 --- 17 18 30 37.5-197.7 -0.9 -9.5 870 1747 23 19 31 23 36 15 1901+319 17 20 45 59.0-225.7 -1.7 -26.9 118 1747 23 36 15 23 41 15 --- 17 25 46 59.5-223.8 -1.6 -26.0 300 1824 23 36 16 Schedule for IRBENE16 (Code Ib ) Page 3 Spatially resolved near-infrared and EVN observations of two blazars 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 26 May 2023 Day 146 --- 23 43 45 1749+096 17 28 17 41.9-188.1 -0.4 -4.4 129 1824 23 43 45 23 48 45 --- 17 33 18 41.9-186.4 -0.3 -3.5 300 1901 23 43 46 23 50 45 1811+062 17 35 18 38.1-192.5 -0.7 -6.7 114 1901 23 50 45 23 58 45 --- 17 43 19 38.3-190.0 -0.5 -5.4 480 2025 23 50 46 --- Sat 27 May 2023 Day 147 --- 00 02 15 2201+171 17 46 50 28.4-257.8 -4.3 -33.4 173 2025 00 02 15 00 10 15 --- 17 54 51 29.4-256.0 -4.2 -33.1 480 2149 00 02 16 00 12 15 1811+062 17 56 51 38.6-185.7 -0.3 -3.1 82 2149 00 12 15 00 20 15 --- 18 04 53 38.7-183.1 -0.2 -1.7 480 2272 00 12 16 00 23 45 2201+171 18 08 23 31.2-252.9 -3.9 -32.5 172 2272 00 23 45 00 31 45 --- 18 16 25 32.2-251.0 -3.8 -32.1 480 2396 00 23 46 00 33 45 1811+062 18 18 25 38.7-178.8 0.1 0.6 81 2396 00 33 45 00 41 45 --- 18 26 26 38.7-176.3 0.2 2.0 480 2520 00 33 46 00 45 15 2201+171 18 29 57 33.9-247.7 -3.6 -31.4 171 2520 00 45 15 00 53 15 --- 18 37 58 34.9-245.7 -3.4 -30.8 480 2643 00 45 16 00 55 15 2131-021 18 39 58 21.1-227.9 -2.9 -23.5 108 2643 00 55 15 01 00 15 --- 18 44 59 21.6-226.7 -2.8 -23.0 300 2721 00 55 16 01 03 15 1749+096 18 48 00 40.9-161.8 0.9 9.8 145 2721 01 03 15 01 08 15 --- 18 53 01 40.7-160.2 1.0 10.6 300 2798 01 03 16 01 09 15 1811+062 18 54 01 38.1-167.5 0.7 6.7 53 2798 01 09 15 01 17 15 --- 19 02 02 37.9-165.0 0.8 8.0 480 2922 01 09 16 01 20 55 2201+171 19 05 43 38.2-238.6 -3.0 -28.7 180 2922 01 20 55 01 28 55 --- 19 13 44 39.1-236.4 -2.8 -27.9 480 3045 01 20 56 01 31 55 1811+062 19 16 44 37.3-160.5 1.0 10.4 139 3045 01 31 55 01 39 55 --- 19 24 46 36.9-158.0 1.2 11.6 480 3169 01 31 56 01 42 55 2201+171 19 27 46 40.6-232.5 -2.6 -26.5 139 3169 01 42 55 01 50 55 --- 19 35 48 41.4-230.2 -2.5 -25.6 480 3293 01 42 56 01 52 25 2131-021 19 37 18 26.1-213.3 -2.0 -17.1 79 3293 01 52 25 01 57 25 --- 19 42 19 26.5-211.9 -1.9 -16.5 300 3370 01 52 26 Schedule for IRBENE16 (Code Ib ) Page 4 Spatially resolved near-infrared and EVN observations of two blazars 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 27 May 2023 Day 147 --- 02 00 25 1749+096 19 45 19 37.4-144.1 1.9 18.6 143 3370 02 00 25 02 05 25 --- 19 50 20 37.0-142.7 2.0 19.3 300 3447 02 00 26 02 07 25 1811+062 19 52 20 35.3-149.8 1.6 15.8 113 3447 02 07 25 02 15 25 --- 20 00 22 34.7-147.5 1.8 16.9 480 3571 02 07 26 02 18 55 2201+171 20 03 52 44.1-221.9 -2.0 -22.1 169 3571 02 18 55 02 26 55 --- 20 11 53 44.8-219.4 -1.9 -20.9 480 3695 02 18 56 02 28 55 1811+062 20 13 54 33.7-143.6 2.0 18.7 79 3695 02 28 55 02 36 55 --- 20 21 55 33.0-141.3 2.1 19.7 480 3818 02 28 56 02 40 25 2201+171 20 25 26 45.9-215.1 -1.7 -18.9 170 3818 02 40 25 02 48 25 --- 20 33 27 46.5-212.5 -1.5 -17.6 480 3942 02 40 26 02 50 25 1811+062 20 35 27 31.9-137.6 2.3 21.3 80 3942 02 50 25 02 58 25 --- 20 43 29 31.1-135.4 2.5 22.3 480 4066 02 50 26 03 01 55 2201+171 20 46 59 47.5-207.9 -1.3 -15.3 170 4066 03 01 55 03 09 55 --- 20 55 01 47.9-205.2 -1.2 -13.8 480 4189 03 01 56 03 11 25 2131-021 20 56 31 30.1-191.2 -0.6 -6.0 78 4189 03 11 25 03 16 25 --- 21 01 32 30.3-189.8 -0.6 -5.2 300 4266 03 11 26 03 19 25 1749+096 21 04 32 29.7-122.5 3.2 27.3 144 4266 03 19 25 03 24 25 --- 21 09 33 29.1-121.3 3.3 27.7 300 4344 03 19 26 03 26 25 1811+062 21 11 33 28.3-128.1 2.9 25.1 113 4344 03 26 25 03 34 25 --- 21 19 35 27.5-126.0 3.1 25.9 480 4467 03 26 26 03 37 55 2201+171 21 23 05 49.2-195.2 -0.7 -8.5 172 4467 03 37 55 03 45 55 --- 21 31 06 49.5-192.3 -0.6 -6.9 480 4591 03 37 56 03 47 55 1811+062 21 33 07 26.0-122.7 3.3 27.0 82 4591 03 47 55 03 55 55 --- 21 41 08 25.0-120.7 3.4 27.6 480 4715 03 47 56 03 59 25 2201+171 21 44 39 49.8-187.4 -0.3 -4.1 173 4715 03 59 25 04 07 25 --- 21 52 40 49.9-184.4 -0.2 -2.5 480 4838 03 59 26 04 09 25 1811+062 21 54 40 23.5-117.4 3.7 28.6 84 4838 04 09 25 04 17 25 --- 22 02 42 22.5-115.5 3.8 29.1 480 4962 04 09 26 04 20 55 2201+171 22 06 12 50.0-179.4 0.0 0.3 175 4962 04 20 55 04 28 55 --- 22 14 14 49.9-176.4 0.2 2.0 480 5086 04 20 56 Schedule for IRBENE16 (Code Ib ) Page 5 Spatially resolved near-infrared and EVN observations of two blazars 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 27 May 2023 Day 147 --- 04 30 55 2131-021 22 16 14 30.1-168.2 0.7 6.3 107 5086 04 30 55 04 35 55 --- 22 21 15 29.9-166.7 0.8 7.1 300 5163 04 30 56 04 37 55 1811+062 22 23 15 20.0-110.8 4.1 30.3 89 5163 04 37 55 04 45 55 --- 22 31 16 18.9-109.0 4.3 30.7 480 5287 04 37 56 04 49 25 2201+171 22 34 47 49.6-168.8 0.5 6.2 177 5287 04 49 25 04 57 25 --- 22 42 48 49.4-165.9 0.6 7.9 480 5410 04 49 26 04 59 25 1811+062 22 44 49 17.2-105.9 4.5 31.3 87 5410 04 59 25 05 07 25 --- 22 52 50 16.2-104.2 4.6 31.6 480 5534 04 59 26 05 10 55 2201+171 22 56 20 48.8-161.1 0.9 10.5 178 5534 05 10 55 05 18 55 --- 23 04 22 48.5-158.2 1.0 12.0 480 5658 05 10 56 05 21 55 1811+062 23 07 22 14.3-101.0 4.9 32.0 149 5658 05 21 55 05 29 55 --- 23 15 24 13.2 -99.2 5.0 32.2 480 5781 05 21 56 05 33 35 2201+171 23 19 04 47.6-153.1 1.2 14.7 189 5781 05 33 35 05 41 35 --- 23 27 05 47.1-150.4 1.4 16.1 480 5905 05 33 36 05 44 35 1811+062 23 30 06 11.3 -96.1 5.3 32.5 150 5905 05 44 35 05 52 35 --- 23 38 07 10.2 -94.4 5.4 32.6 480 6029 05 44 36 05 55 35 2201+171 23 41 08 46.1-145.7 1.6 18.5 151 6029 05 55 35 06 03 35 --- 23 49 09 45.5-143.2 1.7 19.7 480 6152 05 55 36 06 05 35 2131-021 23 51 09 24.7-142.1 2.3 19.3 107 6152 06 05 35 06 10 35 --- 23 56 10 24.3-140.8 2.3 19.8 300 6230 06 05 36 06 12 35 2201+171 23 58 11 44.8-140.3 1.9 21.1 107 6230 06 12 35 06 15 35 --- 00 01 11 44.5-139.4 1.9 21.5 180 6276 06 12 36 06 16 05 2201+171 00 01 41 44.5-139.2 2.0 21.6 27 6276 06 16 05 06 30 35 --- 00 16 14 43.1-134.8 2.2 23.5 870 6500 06 16 06 06 31 05 2201+171 00 16 44 43.1-134.6 2.2 23.6 27 6500 06 31 05 06 45 35 --- 00 31 16 41.6-130.3 2.4 25.4 870 6724 06 31 06 06 46 05 2201+171 00 31 46 41.6-130.2 2.5 25.4 27 6724 06 46 05 07 00 35 --- 00 46 18 40.1-126.1 2.7 27.0 870 6949 06 46 06 07 02 35 2131-021 00 48 19 19.3-127.8 3.2 25.1 107 6949 07 02 35 07 07 35 --- 00 53 20 18.8-126.6 3.3 25.5 300 7026 07 02 36 Schedule for IRBENE16 (Code Ib ) Page 6 Spatially resolved near-infrared and EVN observations of two blazars 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 27 May 2023 Day 147 --- 07 09 35 2201+171 00 55 20 39.1-123.6 2.8 27.9 107 7026 07 09 35 07 12 35 --- 00 58 20 38.7-122.8 2.9 28.2 180 7072 07 09 36 07 13 05 2201+171 00 58 50 38.7-122.7 2.9 28.3 27 7072 07 13 05 07 27 35 --- 01 13 23 37.0-118.8 3.1 29.5 870 7296 07 13 06 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess223.C2048 --- 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: 9 Station: IRBENE16 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= 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 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: 12 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= 730.49 730.49 730.49 730.49 794.49 794.49 794.49 794.49 858.49 858.49 858.49 858.49 922.49 922.49 922.49 922.49 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: 12 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) * 1749+096 17 49 10.387930 * 17 51 32.818574 17 52 40.161310 0.00 J1751+0939 09 39 42.82586 * 09 39 00.72841 09 38 32.71210 0.00 J1751+09 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 192391 observations. * 1811+062 18 11 06.934749 * 18 13 33.411594 18 14 42.554849 0.11 J1813+0615 06 14 48.08455 * 06 15 42.03418 06 15 58.90887 0.18 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 112 observations. 3C395 19 01 02.310064 * 19 02 55.938900 19 03 49.774383 0.02 J1902+3159 31 55 13.94285 * 31 59 41.70165 32 01 31.95169 0.02 * 1901+319 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc J1902+31 GSFC 2016a X/S astro solution, 2536 observations. * 2131-021 21 31 35.130682 * 21 34 10.309593 21 35 22.557730 0.01 J2134-0153 -02 06 39.92005 *-01 53 17.23894 -01 47 09.65909 0.01 J2134-01 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 7810 observations. * 2201+171 22 01 03.345094 * 22 03 26.893679 22 04 33.508589 0.05 J2203+1725 17 11 15.54383 * 17 25 48.24774 17 32 22.17060 0.09 J2203+17 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 284 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 1749+096 sess223.C2048 1 2 3 4 5 6 7 8 9 10 11 12 0.500 26.053 1811+062 sess223.C2048 1 2 3 4 5 6 7 8 9 10 11 12 3.550 184.494 1901+319 sess223.C2048 1 2 3 4 5 6 7 8 9 10 11 12 0.250 16.500 2131-021 sess223.C2048 1 2 3 4 5 6 7 8 9 10 11 12 0.500 26.833 2201+171 sess223.C2048 1 2 3 4 5 6 7 8 9 10 11 12 3.067 166.258 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) 1749+096 140.9 1811+062 139.7 1901+319 113.1 2131-021 99.8 2201+171 86.0 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