COVER INFORMATION Station: CAMBG32M (Code Cm ) Experiment: Network Monitoring Experiment Exp. Code: N20K1 Schedule Version: 2.00 Processed by SCHED version: 11.50 Development version 11.5. Started Apr. 2 PI: Dhanya G.Nair Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31-521-596508 EMAIL: nair@jive.eu Fax: Phone during observation: +31-521-596508 Observing mode: Notes: 1.3 cm (K-band) ftp fringe test for session 1/2020 (1024 Mbps, L+R, 2-bit sampling, 16 x 16 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 2nd March 2020 involving 20 telescopes: Jb2 Ef 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 1024 Mbps: The schedule consists of long integrations on strong calibrators: Ftp-fringe tests are scheduled every 20 min throughout the experiment: 10:18:00 J0205+3212 10:38:00 J0205+3212 10:58:00 J0205+3212 11:18:00 J0238+1636 11:38:00 J0238+1636 11:58:00 0234+285 12:18:00 0234+285 12:38:00 0234+285 12:58:00 0234+285 Clear skies! Dhanya G.Nair Skype account: jive.support.scientist Mattermost: coms.evlbi.org Schedule for CAMBG32M (Code Cm ) 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 2 Mar 2020 Day 62 --- Next scan frequencies: 22203.49 22203.49 Next BBC frequencies: 820.51 820.51 Next scan bandwidths: 64.00 64.00 10 00 00 J0205+3212 20 42 47 30.3 435.1 -5.4 -44.5 0 0 10 00 00 10 05 00 =0202+319 20 47 47 31.0 436.0 -5.3 -44.8 300 19 10 00 01 10 07 00 J0205+3212 20 49 48 31.3 436.3 -5.3 -44.8 116 19 10 07 00 10 20 00 =0202+319 21 02 50 33.3 438.6 -5.1 -45.4 780 70 10 07 01 10 22 45 J0205+3212 21 05 35 33.7 439.1 -5.0 -45.5 161 70 10 22 45 10 25 00 =0202+319 21 07 51 34.0 439.5 -5.0 -45.5 135 78 10 22 46 10 27 00 J0205+3212 21 09 51 34.3 439.9 -4.9 -45.6 116 78 10 27 00 10 40 00 =0202+319 21 22 53 36.3 442.3 -4.7 -46.0 780 128 10 27 01 10 42 45 J0205+3212 21 25 39 36.7 442.8 -4.7 -46.0 161 128 10 42 45 10 45 00 =0202+319 21 27 54 37.1 443.2 -4.6 -46.1 135 137 10 42 46 10 47 00 J0205+3212 21 29 54 37.4 443.5 -4.6 -46.1 116 137 10 47 00 11 00 00 =0202+319 21 42 56 39.4 446.0 -4.4 -46.4 780 187 10 47 01 11 02 00 J0205+3212 21 44 57 39.7 446.3 -4.4 -46.4 116 187 11 02 00 11 05 00 =0202+319 21 47 57 40.1 446.9 -4.3 -46.4 180 199 11 02 01 11 07 00 J0238+1636 21 49 58 23.8 453.3 -4.8 -39.7 54 199 11 07 00 11 20 00 =0235+164 22 03 00 25.8 455.9 -4.6 -39.6 780 249 11 07 01 11 22 05 J0238+1636 22 05 05 26.1 456.3 -4.6 -39.5 121 249 11 22 05 11 25 00 =0235+164 22 08 01 26.6 456.9 -4.5 -39.5 175 261 11 22 06 11 27 00 J0238+1636 22 10 01 26.9 457.3 -4.5 -39.4 116 261 11 27 00 11 40 00 =0235+164 22 23 03 28.9 460.1 -4.3 -39.1 780 311 11 27 01 11 42 00 J0238+1636 22 25 03 29.2 460.5 -4.2 -39.0 116 311 11 42 00 11 45 00 =0235+164 22 28 04 29.6 461.2 -4.2 -38.9 180 322 11 42 01 11 47 00 0234+285 22 30 04 39.2 451.9 -4.1 -44.4 75 322 11 47 00 12 00 00 --- 22 43 06 41.2 454.6 -3.9 -44.3 780 373 11 47 01 12 02 00 0234+285 22 45 07 41.5 455.0 -3.9 -44.3 116 373 12 02 00 12 05 00 --- 22 48 07 41.9 455.6 -3.8 -44.2 180 384 12 02 01 12 07 00 0234+285 22 50 07 42.2 456.0 -3.8 -44.2 116 384 12 07 00 12 20 00 --- 23 03 10 44.2 458.9 -3.6 -43.8 780 434 12 07 01 Schedule for CAMBG32M (Code Cm ) 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 2 Mar 2020 Day 62 --- 12 22 00 0234+285 23 05 10 44.5 459.3 -3.6 -43.7 116 434 12 22 00 12 25 00 --- 23 08 10 45.0 460.0 -3.5 -43.6 180 446 12 22 01 12 27 00 0234+285 23 10 11 45.3 460.4 -3.5 -43.5 116 446 12 27 00 12 40 00 --- 23 23 13 47.2 463.4 -3.3 -42.9 780 496 12 27 01 12 42 00 0234+285 23 25 13 47.5 463.9 -3.2 -42.8 116 496 12 42 00 12 45 00 --- 23 28 14 48.0 464.6 -3.2 -42.7 180 508 12 42 01 12 47 00 0234+285 23 30 14 48.3 465.1 -3.1 -42.6 116 508 12 47 00 13 00 00 --- 23 43 16 50.2 468.4 -2.9 -41.7 780 558 12 47 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess120.K1024 --- 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: 17 Station: CAMBG32M Total bit rate: 512 Format: VDIF Bits per sample: 2 Sample rate:128.000 Number of channels: 2 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 23024.00 23024.00 Net SB= U U IF SB = L L Pol. = RCP LCP BBC = 1 9 BBC SB= L L IF = A1 B1 The following frequency sets based on these setups were used. Frequency Set: 17 Setup file default. Used with PCAL = off LO sum= 22203.49 22203.49 BBC fr= 820.51 820.51 Bandwd= 64.00 64.00 Matching frequency sets: 17 18 19 20 Track assignments are: track1= 1, 2 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 13.714633 0.00 * J0205+3212 31 58 10.39522 * 32 12 30.09544 32 18 10.65415 0.00 J0205+32 /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 49141 observations. * 0234+285 02 34 55.589590 * 02 37 52.405677 02 39 01.986830 0.00 J0237+2848 28 35 11.40773 * 28 48 08.98999 28 53 16.22933 0.00 J0237+28 /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 58420 observations. 0235+164 02 35 52.630214 * 02 38 38.930106 02 39 44.342468 0.12 * J0238+1636 16 24 04.01612 * 16 36 59.27454 16 42 01.81891 0.16 J0238+16 /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 64441 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 sess120.K1024 1 2 3 4 5 6 7 8 9 12 13 14 + 0.858 163.083 0234+285 sess120.K1024 1 2 3 4 5 6 7 8 9 12 13 14 + 1.017 193.167 J0238+1636 sess120.K1024 1 2 3 4 5 6 7 8 9 12 13 14 + 0.532 98.126 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 60.1 0234+285 64.7 J0238+1636 60.4 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