COVER INFORMATION Station: ONSALA85 (Code O8 ) Experiment: Network Monitoring Experiment Exp. Code: N17M1 Schedule Version: 1.00 Processed by SCHED version: 11.40 Release 11.4. March 14, 2015 PI: Jay Blanchard Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31-521-596508 EMAIL: blanchard@jive.eu Fax: Phone during observation: +31-521-596508 Observing mode: Notes: 5cm (M-band) ftp fringe test for session 2/2017 (128 Mbps, L+R, 2-bit sampling, 16 x 2 MHz filters) Please send the disk pack by express to JIVE COVER LETTER: This is the schedule for the 6cm M band test on 05 June 2017 involving 9 telescopes: Jb2, Wb1, Ef, Mc, Nt, O8, Tr, Ys, Ir The FTP-NME uses a standard setup with 128 Mbps. The schedule consists of: - long integrations on strong calibrators: for ftp-fringe tests; Ftp-fringe tests are scheduled every half hour throughout the experiment: 12:28:00 J0319+4130 12:58:00 J0319+4130 13:28:00 J0319+4130 13:58:00 J0319+4130 14:28:00 J1927+7358 14:58:00 J1927+7358 Clear skies! Jay Skype account: jive.support.scientist Schedule for ONSALA85 (Code O8 ) 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 5 Jun 2017 Day 156 --- Next scan frequencies: 6661.49 6661.49 6661.49 6661.49 6665.49 6665.49 6665.49 6665.49 6669.49 6669.49 6669.49 6669.49 6673.49 6673.49 6673.49 6673.49 Next BBC frequencies: 411.49 411.49 411.49 411.49 415.49 415.49 415.49 415.49 419.49 419.49 419.49 419.49 423.49 423.49 423.49 423.49 Next scan bandwidths: 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 12 00 00 J0319+4130 05 44 06 62.4 250.7 2.4 0.0 0 0 12 00 00 12 15 00 =3C84 05 59 08 60.4 254.9 2.6 0.0 900 14 12 00 01 12 17 00 J0319+4130 06 01 09 60.2 255.5 2.7 0.0 114 14 12 17 00 12 30 00 =3C84 06 14 11 58.5 258.9 2.9 0.0 780 27 12 17 01 12 32 00 J0319+4130 06 16 11 58.2 259.4 2.9 0.0 114 27 12 32 00 12 45 00 =3C84 06 29 13 56.5 262.5 3.1 0.0 780 40 12 32 01 12 47 00 J0319+4130 06 31 13 56.2 263.0 3.2 0.0 114 40 12 47 00 13 00 00 =3C84 06 44 16 54.4 266.0 3.4 0.0 780 52 12 47 01 13 02 00 J0319+4130 06 46 16 54.2 266.5 3.4 0.0 114 52 13 02 00 13 15 00 =3C84 06 59 18 52.4 269.3 3.6 0.0 780 65 13 02 01 13 17 00 J0319+4130 07 01 18 52.2 269.7 3.7 0.0 114 65 13 17 00 13 30 00 =3C84 07 14 21 50.4 272.4 3.9 0.0 780 77 13 17 01 13 32 00 J0319+4130 07 16 21 50.1 272.8 3.9 0.0 114 77 13 32 00 13 45 00 =3C84 07 29 23 48.4 275.4 4.1 0.0 780 90 13 32 01 13 47 00 J0319+4130 07 31 23 48.1 275.8 4.2 0.0 114 90 13 47 00 14 00 00 =3C84 07 44 25 46.4 278.3 4.4 0.0 780 102 13 47 01 14 02 00 J0319+4130 07 46 26 46.1 278.7 4.4 0.0 114 102 14 02 00 14 15 00 =3C84 07 59 28 44.4 281.1 4.6 0.0 780 115 14 02 01 14 17 00 J1927+7358 08 01 28 41.5 3.1-11.4 0.0 -701 115 14 17 00 14 30 00 =1928+738 08 14 30 41.6 4.3-11.2 0.0 79 128 14 17 01 14 32 00 J1927+7358 08 16 31 41.7 4.5-11.2 0.0 114 128 14 32 00 14 45 00 =1928+738 08 29 33 41.8 5.7-11.0 0.0 780 140 14 32 01 14 47 00 J1927+7358 08 31 33 41.8 5.9-10.9 0.0 114 140 14 47 00 15 00 00 =1928+738 08 44 35 42.0 7.0-10.7 0.0 780 153 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: sess217.M128nme --- 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: 8 Station: ONSALA85 Total bit rate: 128 Format: VDIF Bits per sample: 2 Sample rate: 4.000 Number of channels: 16 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 6250.00 6250.00 6250.00 6250.00 6250.00 6250.00 6250.00 6250.00 6250.00 6250.00 6250.00 6250.00 6250.00 6250.00 6250.00 6250.00 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: 6 Setup file default. Used with PCAL = off LO sum= 6661.49 6661.49 6661.49 6661.49 6665.49 6665.49 6665.49 6665.49 6669.49 6669.49 6669.49 6669.49 6673.49 6673.49 6673.49 6673.49 BBC fr= 411.49 411.49 411.49 411.49 415.49 415.49 415.49 415.49 419.49 419.49 419.49 419.49 423.49 423.49 423.49 423.49 Bandwd= 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 Matching frequency sets: 6 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) 3C84 03 16 29.567263 * 03 19 48.160094 03 20 55.475822 1.30 * J0319+4130 41 19 51.91701 * 41 30 42.10413 41 34 09.87766 2.69 0316+413 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc J0319+41 GSFC 2015a astro solution, unpublished 10208 observations. 1928+738 19 28 49.350209 * 19 27 48.495162 19 27 31.710388 0.04 * J1927+7358 73 51 44.92746 * 73 58 01.56990 74 00 06.15074 0.01 J1927+73 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc GSFC 2015a astro solution, unpublished 4075 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 J0319+4130 sess217.M128nme 1 2 3 4 5 6 7 8 9 10 1.983 154.700 J1927+7358 sess217.M128nme 1 3 4 5 6 7 8 9 10 14 0.650 39.750 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) J0319+4130 27.4 J1927+7358 80.3 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