COVER INFORMATION Station: WSTRBORK (Code Wb ) Experiment: A second active nucleus in Cygnus A? Exp. Code: EB060C Schedule Version: 2.00 Processed by SCHED version: 11.40 Release 11.4. March 14, 2015 PI: Uwe Bach Address: Max-Planck-Institut fuer Radioastronomie Auf dem Huegel 69 53121 Bonn Germany Phone: 0049-2257-301-168 EMAIL: ubach@mpifr-bonn.mpg.de Fax: 0049-2257-301-106 Phone during observation: 0049-2257-301-155 Observing mode: Notes: Use 2013+370 as fring tracer and BL Lac as 2nd calibrators COVER LETTER: This is the schedule for epoch B of EB060 at 6cm. It involves 15 antennas Jb2, Ef, Wb, Mc, Nt, On85, T6, Ur, Tr, Ys, Sv, Zc, Bd, Hh, and Ir and runs at a standard 1 Gbps continuum mode. There are two gaps to allow some pointings at Effelsberg. Fringe finders are 2013+370 and BL Lac. Schedule for WSTRBORK (Code Wb ) Page 2 A second active nucleus in Cygnus A? 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 9 Jun 2017 Day 160 --- Next scan frequencies: 4958.49 4958.49 4958.49 4958.49 5022.49 5022.49 5022.49 5022.49 Next BBC frequencies: 371.49 371.49 371.49 371.49 435.49 435.49 435.49 435.49 Next scan bandwidths: 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 22 00 00 CYG-A 15 40 13 45.6 78.6 -4.3 0.0 0 0 22 00 00 22 10 00 --- 15 50 14 47.1 80.3 -4.2 0.0 600 77 22 00 01 22 10 30 CYG-A 15 50 45 47.1 80.4 -4.2 0.0 19 77 22 10 30 22 20 30 --- 16 00 46 48.6 82.1 -4.0 0.0 600 154 22 10 31 22 21 30 2013+370 16 01 46 44.1 83.4 -4.2 0.0 34 154 22 21 30 22 26 30 --- 16 06 47 44.9 84.3 -4.2 0.0 300 192 22 21 31 22 27 30 CYG-A 16 07 47 49.7 83.4 -3.9 0.0 33 192 22 27 30 22 37 30 --- 16 17 49 51.2 85.2 -3.7 0.0 600 269 22 27 31 22 38 00 CYG-A 16 18 19 51.3 85.3 -3.7 0.0 19 269 22 38 00 22 48 00 --- 16 28 21 52.8 87.2 -3.5 0.0 600 346 22 38 01 22 48 30 CYG-A 16 28 51 52.8 87.3 -3.5 0.0 19 346 22 48 30 22 58 30 --- 16 38 52 54.4 89.2 -3.4 0.0 600 423 22 48 31 22 59 00 CYG-A 16 39 22 54.4 89.3 -3.3 0.0 19 423 22 59 00 23 09 00 --- 16 49 24 55.9 91.3 -3.2 0.0 600 500 22 59 01 23 09 30 CYG-A 16 49 54 56.0 91.4 -3.2 0.0 19 500 23 09 30 23 19 30 --- 16 59 56 57.5 93.5 -3.0 0.0 600 577 23 09 31 23 20 00 CYG-A 17 00 26 57.6 93.6 -3.0 0.0 19 577 23 20 00 23 30 00 --- 17 10 28 59.1 95.8 -2.8 0.0 600 654 23 20 01 23 30 30 CYG-A 17 10 58 59.2 95.9 -2.8 0.0 19 654 23 30 30 23 40 30 --- 17 20 59 60.7 98.3 -2.7 0.0 600 731 23 30 31 23 41 00 CYG-A 17 21 29 60.8 98.4 -2.6 0.0 19 731 23 41 00 23 51 00 --- 17 31 31 62.3 100.9 -2.5 0.0 600 808 23 41 01 23 53 00 BLLAC 17 33 31 45.1 75.2 -4.5 0.0 6 808 23 53 00 23 58 00 --- 17 38 32 45.8 76.0 -4.4 0.0 300 846 23 53 01 --- Sat 10 Jun 2017 Day 161 --- 00 00 00 CYG-A 17 40 33 63.6 103.2 -2.3 0.0 3 846 00 00 00 00 10 00 --- 17 50 34 65.0 106.0 -2.2 0.0 600 923 00 00 01 Schedule for WSTRBORK (Code Wb ) Page 3 A second active nucleus in Cygnus A? 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 10 Jun 2017 Day 161 --- 00 10 30 CYG-A 17 51 04 65.1 106.1 -2.2 0.0 19 923 00 10 30 00 20 30 --- 18 01 06 66.6 109.2 -2.0 0.0 600 1000 00 10 31 00 21 00 CYG-A 18 01 36 66.6 109.3 -2.0 0.0 19 1000 00 21 00 00 31 00 --- 18 11 38 68.0 112.6 -1.8 0.0 600 1077 00 21 01 00 31 30 CYG-A 18 12 08 68.1 112.8 -1.8 0.0 19 1077 00 31 30 00 41 30 --- 18 22 09 69.5 116.4 -1.6 0.0 600 1154 00 31 31 00 42 00 CYG-A 18 22 39 69.6 116.6 -1.6 0.0 19 1154 00 42 00 00 52 00 --- 18 32 41 70.9 120.6 -1.5 0.0 600 1231 00 42 01 00 52 30 CYG-A 18 33 11 70.9 120.8 -1.4 0.0 19 1231 00 52 30 01 02 30 --- 18 43 13 72.2 125.3 -1.3 0.0 600 1308 00 52 31 01 03 00 CYG-A 18 43 43 72.3 125.5 -1.3 0.0 19 1308 01 03 00 01 13 00 --- 18 53 44 73.5 130.6 -1.1 0.0 600 1385 01 03 01 01 13 30 CYG-A 18 54 15 73.5 130.8 -1.1 0.0 19 1385 01 13 30 01 23 30 --- 19 04 16 74.6 136.5 -0.9 0.0 600 1462 01 13 31 ---------- 6-min gap for pointing ---------- 01 29 30 2013+370 19 10 17 70.6 137.3 -1.1 0.0 334 1462 01 29 30 01 34 30 --- 19 15 18 71.1 139.9 -1.0 0.0 300 1500 01 29 31 01 35 30 CYG-A 19 16 18 75.8 144.2 -0.7 0.0 33 1500 01 35 30 01 45 30 --- 19 26 20 76.6 151.4 -0.6 0.0 600 1577 01 35 31 01 46 00 CYG-A 19 26 50 76.6 151.8 -0.6 0.0 19 1577 01 46 00 01 56 00 --- 19 36 52 77.2 159.7 -0.4 0.0 600 1654 01 46 01 01 56 30 CYG-A 19 37 22 77.3 160.1 -0.4 0.0 19 1654 01 56 30 02 06 30 --- 19 47 23 77.7 168.7 -0.2 0.0 600 1731 01 56 31 02 07 00 CYG-A 19 47 53 77.7 169.1 -0.2 0.0 19 1731 02 07 00 02 17 00 --- 19 57 55 77.9 178.0 -0.0 0.0 600 1808 02 07 01 02 17 30 CYG-A 19 58 25 77.9 178.5 -0.0 0.0 19 1808 02 17 30 02 27 30 --- 20 08 27 77.8 187.5 0.1 0.0 600 1885 02 17 31 02 28 00 CYG-A 20 08 57 77.8 187.9 0.1 0.0 19 1885 02 28 00 02 38 00 --- 20 18 58 77.5 196.7 0.3 0.0 600 1962 02 28 01 Schedule for WSTRBORK (Code Wb ) Page 4 A second active nucleus in Cygnus A? 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 10 Jun 2017 Day 161 --- 02 38 30 CYG-A 20 19 29 77.4 197.1 0.3 0.0 19 1962 02 38 30 02 48 30 --- 20 29 30 76.9 205.3 0.5 0.0 600 2038 02 38 31 02 50 00 2013+370 20 31 00 74.1 190.9 0.2 0.0 64 2038 02 50 00 02 55 00 --- 20 36 01 73.9 194.4 0.3 0.0 300 2077 02 50 01 02 56 30 CYG-A 20 37 32 76.3 211.3 0.6 0.0 63 2077 02 56 30 03 06 30 --- 20 47 33 75.4 218.3 0.8 0.0 600 2154 02 56 31 03 07 00 CYG-A 20 48 03 75.4 218.6 0.8 0.0 19 2154 03 07 00 03 17 00 --- 20 58 05 74.4 224.8 1.0 0.0 600 2231 03 07 01 03 17 30 CYG-A 20 58 35 74.3 225.1 1.0 0.0 19 2231 03 17 30 03 27 30 --- 21 08 37 73.2 230.6 1.1 0.0 600 2308 03 17 31 03 28 00 CYG-A 21 09 07 73.2 230.8 1.2 0.0 19 2308 03 28 00 03 38 00 --- 21 19 08 71.9 235.7 1.3 0.0 600 2385 03 28 01 03 38 30 CYG-A 21 19 38 71.9 235.9 1.3 0.0 19 2385 03 38 30 03 48 30 --- 21 29 40 70.6 240.3 1.5 0.0 600 2462 03 38 31 03 49 00 CYG-A 21 30 10 70.5 240.5 1.5 0.0 19 2462 03 49 00 03 59 00 --- 21 40 12 69.2 244.4 1.7 0.0 600 2538 03 49 01 03 59 30 CYG-A 21 40 42 69.1 244.6 1.7 0.0 19 2538 03 59 30 04 09 30 --- 21 50 43 67.7 248.1 1.8 0.0 600 2615 03 59 31 ---------- 6-min gap for pointing ---------- 04 18 30 BLLAC 21 59 45 79.4 176.3 -0.1 0.0 426 2615 04 18 30 04 23 30 --- 22 04 46 79.4 181.3 0.0 0.0 300 2654 04 18 31 04 28 40 CYG-A 22 09 57 65.0 254.1 2.2 0.0 193 2654 04 28 40 04 38 40 --- 22 19 58 63.5 256.9 2.3 0.0 600 2731 04 28 41 04 39 10 CYG-A 22 20 28 63.5 257.0 2.3 0.0 19 2731 04 39 10 04 48 50 --- 22 30 10 62.0 259.5 2.5 0.0 580 2805 04 39 11 04 49 20 CYG-A 22 30 40 62.0 259.7 2.5 0.0 19 2805 04 49 20 04 59 00 --- 22 40 22 60.5 262.0 2.7 0.0 580 2879 04 49 21 04 59 30 CYG-A 22 40 52 60.4 262.1 2.7 0.0 19 2879 04 59 30 05 09 10 --- 22 50 33 59.0 264.4 2.8 0.0 580 2954 04 59 31 Schedule for WSTRBORK (Code Wb ) Page 5 A second active nucleus in Cygnus A? 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 10 Jun 2017 Day 161 --- 05 09 40 CYG-A 22 51 03 58.9 264.5 2.8 0.0 19 2954 05 09 40 05 19 20 --- 23 00 45 57.5 266.6 3.0 0.0 580 3028 05 09 41 05 19 50 CYG-A 23 01 15 57.4 266.7 3.0 0.0 19 3028 05 19 50 05 29 30 --- 23 10 57 55.9 268.7 3.2 0.0 580 3103 05 19 51 05 30 00 CYG-A 23 11 27 55.8 268.8 3.2 0.0 19 3103 05 30 00 05 39 40 --- 23 21 08 54.4 270.8 3.4 0.0 580 3177 05 30 01 05 40 10 CYG-A 23 21 38 54.3 270.9 3.4 0.0 19 3177 05 40 10 05 49 50 --- 23 31 20 52.9 272.7 3.5 0.0 580 3251 05 40 11 05 50 20 CYG-A 23 31 50 52.8 272.8 3.5 0.0 19 3251 05 50 20 06 00 00 --- 23 41 32 51.3 274.6 3.7 0.0 580 3326 05 50 21 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess217.C1024 --- 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: 14 Station: WSTRBORK Total bit rate: 1024 Format: MARK5B 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= 4587.00 4587.00 4587.00 4587.00 4587.00 4587.00 4587.00 4587.00 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 5 1 5 3 7 3 7 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= 4958.49 4958.49 4958.49 4958.49 5022.49 5022.49 5022.49 5022.49 BBC fr= 371.49 371.49 371.49 371.49 435.49 435.49 435.49 435.49 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= 10, 14, 2, 6, 12, 16, 4, 8 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) CYGNUS-A 19 57 44.440804 * 19 59 28.356482 20 00 05.762364 0.80 J1959+4044 40 35 46.36249 * 40 44 02.09630 40 46 52.22193 0.53 * CYG-A /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc.2015feb J1959+40 GSFC 2015a astro solution, unpublished 27 observations. 1957+405 1957+404 * 2013+370 20 13 37.014511 * 20 15 28.729797 20 16 08.681654 0.13 J2015+3710 37 01 44.45895 * 37 10 59.51482 37 14 09.76368 0.18 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc.2015feb GSFC 2015a astro solution, unpublished 131 observations. VR422201 22 00 39.362505 * 22 02 43.291372 22 03 27.100969 0.00 J2202+4216 42 02 08.59077 * 42 16 39.97990 42 21 31.67676 0.00 * BLLAC /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc.2015feb 2200+420 GSFC 2015a astro solution, unpublished 51226 observations. J2202+42 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 CYG-A sess217.C1024 1 2 3 4 5 6 7 8 9 10 11 14 6.789 591.086 2013+370 sess217.C1024 1 2 3 4 5 6 7 8 9 10 11 14 0.250 25.083 BLLAC sess217.C1024 1 2 3 4 5 6 7 8 9 10 11 14 0.167 16.333 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) CYG-A 105.4 2013+370 106.1 BLLAC 86.7 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