COVER INFORMATION Station: YEBES40M (Code Ys ) Experiment: The core of the radio galaxy 3C 411 Exp. Code: EP104B Schedule Version: 1.00 Processed by SCHED version: 11.40 Release 11.4. March 14, 2015 PI: Krisztina Perger Address: Eotvos University Pazmany P setany 1/A H-1117 Budapest Hungary Phone: +36 20 9959334 EMAIL: pergertina@gmail.com Fax: Phone during observation: +36 20 9959334 Observing mode: 6 cm 1 Gb/s Notes: Schedule for YEBES40M (Code Ys ) Page 2 The core of the radio galaxy 3C 411 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 ---------------------------------------------------------------------------------------- --- Mon 12 Jun 2017 Day 163 --- Next scan frequencies: 4942.49 4942.49 4942.49 4942.49 4974.49 4974.49 4974.49 4974.49 5006.49 5006.49 5006.49 5006.49 5038.49 5038.49 5038.49 5038.49 Next BBC frequencies: 784.49 784.49 784.49 784.49 816.49 816.49 816.49 816.49 848.49 848.49 848.49 848.49 880.49 880.49 880.49 880.49 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 22 00 00 J2022+1001 15 13 19 16.1 90.4 -5.2 -50.5 0 0 22 00 00 22 14 00 =2019+098 15 27 21 18.7 92.7 -4.9 -50.5 840 108 22 00 01 22 14 30 J2022+1001 15 27 51 18.8 92.8 -4.9 -50.5 15 108 22 14 30 22 29 00 =2019+098 15 42 24 21.6 95.2 -4.7 -50.3 870 220 22 14 31 22 29 30 J2022+1001 15 42 54 21.7 95.3 -4.7 -50.2 15 220 22 29 30 22 44 00 =2019+098 15 57 26 24.4 97.8 -4.4 -49.9 870 332 22 29 31 22 45 30 J2123+0535 15 58 57 10.2 91.2 -5.4 -49.8 61 332 22 45 30 22 55 30 =2121+053 16 08 58 12.1 92.9 -5.3 -49.7 600 410 22 45 31 22 57 00 J2022+1001 16 10 28 26.9 100.1 -4.2 -49.5 60 410 22 57 00 23 11 00 =2019+098 16 24 31 29.5 102.6 -4.0 -48.9 840 518 22 57 01 23 11 30 J2022+1001 16 25 01 29.6 102.7 -4.0 -48.9 15 518 23 11 30 23 25 30 =2019+098 16 39 03 32.2 105.4 -3.7 -48.1 840 626 23 11 31 23 26 00 J2022+1001 16 39 33 32.3 105.5 -3.7 -48.1 15 626 23 26 00 23 40 00 =2019+098 16 53 36 34.8 108.3 -3.5 -47.1 840 734 23 26 01 23 40 30 J2022+1001 16 54 06 34.9 108.4 -3.5 -47.1 15 734 23 40 30 23 54 30 =2019+098 17 08 08 37.4 111.3 -3.2 -46.0 840 842 23 40 31 23 55 30 J2031+1219 17 09 08 37.4 107.4 -3.4 -48.0 41 842 23 55 30 23 59 59 =2029+121 17 13 39 38.2 108.3 -3.3 -47.6 269 877 23 55 31 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: 10 Station: YEBES40M Total bit rate: 1024 Format: VDIF Bits per sample: 2 Sample rate: 32.000 Number of channels: 16 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 4158.00 4158.00 4158.00 4158.00 4158.00 4158.00 4158.00 4158.00 4158.00 4158.00 4158.00 4158.00 4158.00 4158.00 4158.00 4158.00 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 3 11 3 11 5 13 5 13 7 15 7 15 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 B1 D1 B1 D1 B1 D1 B1 D1 The following frequency sets based on these setups were used. Frequency Set: 10 Setup file default. Used with PCAL = off LO sum= 4942.49 4942.49 4942.49 4942.49 4974.49 4974.49 4974.49 4974.49 5006.49 5006.49 5006.49 5006.49 5038.49 5038.49 5038.49 5038.49 BBC fr= 784.49 784.49 784.49 784.49 816.49 816.49 816.49 816.49 848.49 848.49 848.49 848.49 880.49 880.49 880.49 880.49 Bandwd= 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 Matching frequency sets: 10 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) 2019+098 20 19 44.215720 * 20 22 08.439532 20 22 59.227519 0.58 * J2022+1001 09 51 33.15230 * 10 01 11.31421 10 04 36.10493 1.08 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.rfc rfc_2015a Petrov, 2015, unpublished. 36 observations 2029+121 20 29 32.681262 * 20 31 54.994269 20 32 45.111160 0.10 * J2031+1219 12 09 28.75309 * 12 19 41.34025 12 23 17.04135 0.10 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.rfc rfc_2015a Petrov, 2015, unpublished. 3457 observations 2121+053 21 21 14.801998 * 21 23 44.517405 21 24 36.890660 0.10 * J2123+0535 05 22 27.44223 * 05 35 22.09303 05 39 53.45105 0.10 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.rfc rfc_2015a Petrov, 2015, unpublished. 53555 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 J2022+1001 sess217.C1024 1 2 3 4 5 6 7 8 9 10 11 14 1.650 173.250 J2031+1219 sess217.C1024 1 2 3 4 5 6 7 8 9 10 11 14 0.075 7.846 J2123+0535 sess217.C1024 1 2 3 4 5 6 7 8 9 10 11 14 0.167 17.500 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) J2022+1001 125.4 J2031+1219 122.1 J2123+0535 115.0 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