COVER INFORMATION Station: YEBES40M (Code Ys ) Experiment: Network Monitoring Experiment Exp. Code: N21K1 Schedule Version: 1.00 Processed by SCHED version: 11.60 Release 11.6; April 2020 PI: Olga Bayandina Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31-521-596508 EMAIL: bayandina@jive.eu Fax: Phone during observation: +31-521-596508 Observing mode: Notes: 1.3 cm (K-band) ftp fringe test for session 1/2021 (2048 Mbps, L+R, 2-bit sampling, 16 x 32 MHz filters) Please send the disk pack by express to JIVE, NO PCAL Please DO NOT use the phase cal signal. COVER LETTER: This is the schedule for the 1.3 cm K-band fringe test on March 8, 2021 involving 21 telescopes: Jb2 Ef Mc On60 T6 Ur Tr Ys Hh Sv Zc Bd Sr Mh Kt Ky Ku Cm Da Kn Pi With 4 sec integration time The FTP-NME uses a standard setup at 2048 Mbps: The schedule consists of long integrations on strong calibrators: Ftp-fringe tests are scheduled every 20 min throughout the experiment: 12:18:00 scan02 J0205+3212 12:38:00 scan04 J0205+3212 12:58:00 scan06 J0205+3212 13:18:00 scan08 J0530+1331 13:38:00 scan10 J0530+1331 13:58:00 scan12 J0530+1331 14:18:00 scan14 J0530+1331 14:38:00 scan16 J0530+1331 14:58:00 scan18 J0530+1331 Clear skies! Olga Bayandina Mattermost: coms.evlbi.org Schedule for YEBES40M (Code Ys ) Page 2 Network Monitoring Experiment 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 8 Mar 2021 Day 67 --- Next scan frequencies: 22139.49 22139.49 22139.49 22139.49 22203.49 22203.49 22203.49 22203.49 22267.49 22267.49 22267.49 22267.49 22331.49 22331.49 22331.49 22331.49 Next BBC frequencies: 659.49 659.49 659.49 659.49 723.49 723.49 723.49 723.49 787.49 787.49 787.49 787.49 851.49 851.49 851.49 851.49 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 12 00 00 J0205+3212 22 53 19 50.8 86.3 -3.2 -63.8 0 0 12 00 00 12 05 00 =0202+319 22 58 19 51.8 87.1 -3.1 -63.9 300 77 12 00 01 12 07 00 J0205+3212 23 00 20 52.1 87.4 -3.1 -64.0 105 77 12 07 00 12 20 00 =0202+319 23 13 22 54.6 89.4 -2.9 -64.1 780 278 12 07 01 12 22 45 J0205+3212 23 16 07 55.1 89.8 -2.8 -64.1 150 278 12 22 45 12 25 00 =0202+319 23 18 23 55.6 90.2 -2.8 -64.1 135 313 12 22 46 12 27 00 J0205+3212 23 20 23 56.0 90.5 -2.8 -64.1 105 313 12 27 00 12 40 00 =0202+319 23 33 25 58.4 92.8 -2.5 -63.9 780 514 12 27 01 12 42 45 J0205+3212 23 36 11 59.0 93.3 -2.5 -63.9 150 514 12 42 45 12 45 00 =0202+319 23 38 26 59.4 93.7 -2.5 -63.8 135 549 12 42 46 12 47 00 J0205+3212 23 40 26 59.8 94.0 -2.4 -63.8 105 549 12 47 00 13 00 00 =0202+319 23 53 28 62.2 96.6 -2.2 -63.3 780 750 12 47 01 13 07 00 J0530+1331 00 00 30 14.1 84.1 -5.5 D -51.1 358 750 13 07 00 13 20 00 =0528+134 00 13 32 16.6 86.1 -5.3 -51.3 0 951 13 07 01 13 22 05 J0530+1331 00 15 37 17.0 86.5 -5.3 -51.3 110 951 13 22 05 13 25 00 =0528+134 00 18 33 17.5 86.9 -5.2 -51.3 175 996 13 22 06 13 27 00 J0530+1331 00 20 33 17.9 87.3 -5.2 -51.4 105 996 13 27 00 13 40 00 =0528+134 00 33 35 20.4 89.3 -5.0 -51.4 780 1197 13 27 01 13 42 00 J0530+1331 00 35 35 20.7 89.7 -4.9 -51.4 105 1197 13 42 00 13 45 00 =0528+134 00 38 36 21.3 90.2 -4.9 -51.4 180 1243 13 42 01 13 47 00 J0530+1331 00 40 36 21.7 90.5 -4.9 -51.4 105 1243 13 47 00 14 00 00 =0528+134 00 53 38 24.2 92.6 -4.6 -51.4 780 1444 13 47 01 14 03 00 J0530+1331 00 56 39 24.7 93.1 -4.6 -51.3 165 1444 14 03 00 14 05 00 =0528+134 00 58 39 25.1 93.5 -4.6 -51.3 120 1475 14 03 01 14 07 00 J0530+1331 01 00 39 25.5 93.8 -4.5 -51.3 105 1475 14 07 00 14 20 00 =0528+134 01 13 42 28.0 96.0 -4.3 -51.0 780 1676 14 07 01 Schedule for YEBES40M (Code Ys ) Page 3 Network Monitoring Experiment 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 8 Mar 2021 Day 67 --- 14 22 00 J0530+1331 01 15 42 28.4 96.4 -4.3 -51.0 105 1676 14 22 00 14 25 00 =0528+134 01 18 42 28.9 96.9 -4.2 -50.9 180 1722 14 22 01 14 27 00 J0530+1331 01 20 43 29.3 97.3 -4.2 -50.9 105 1722 14 27 00 14 40 00 =0528+134 01 33 45 31.8 99.6 -4.0 -50.4 780 1923 14 27 01 14 42 00 J0530+1331 01 35 45 32.1 100.0 -3.9 -50.4 105 1923 14 42 00 14 45 00 =0528+134 01 38 46 32.7 100.5 -3.9 -50.2 180 1970 14 42 01 14 47 00 J0530+1331 01 40 46 33.1 100.9 -3.9 -50.2 105 1970 14 47 00 15 00 00 =0528+134 01 53 48 35.5 103.4 -3.6 -49.5 780 2171 14 47 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess121.K2048 --- 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: 11 Station: YEBES40M 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= 21480.00 21480.00 21480.00 21480.00 21480.00 21480.00 21480.00 21480.00 21480.00 21480.00 21480.00 21480.00 21480.00 21480.00 21480.00 21480.00 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 = A4 C4 A4 C4 A4 C4 A4 C4 A4 C4 A4 C4 A4 C4 A4 C4 The following frequency sets based on these setups were used. Frequency Set: 8 Setup file default. Used with PCAL = off LO sum= 22139.49 22139.49 22139.49 22139.49 22203.49 22203.49 22203.49 22203.49 22267.49 22267.49 22267.49 22267.49 22331.49 22331.49 22331.49 22331.49 BBC fr= 659.49 659.49 659.49 659.49 723.49 723.49 723.49 723.49 787.49 787.49 787.49 787.49 851.49 851.49 851.49 851.49 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: 8 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) 0202+319 02 02 09.652800 * 02 05 04.925362 02 06 17.118726 0.00 * J0205+3212 31 58 10.39522 * 32 12 30.09544 32 18 28.98170 0.00 J0205+32 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 49141 observations. 0528+134 05 28 06.759216 * 05 30 56.416746 05 32 07.404212 0.21 * J0530+1331 13 29 42.28882 * 13 31 55.14948 13 32 46.42756 0.24 J0530+13 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 138236 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 J0205+3212 sess121.K2048 1 2 3 4 5 6 7 8 10 13 15 18 0.808 169.750 J0530+1331 sess121.K2048 1 2 3 4 5 6 7 8 10 13 15 18 1.582 323.451 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) J0205+3212 54.7 J0530+1331 94.9 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