COVER INFORMATION Station: METSAHOV (Code Mh ) Experiment: Network Monitoring Experiment Exp. Code: F17Q1 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: 7mm (Q-band) ftp fringe test for session 1/2017 (1024 Mbps, L+R, 2-bit sampling, 16 MHz filters) Please send the disk pack by express to JIVE COVER LETTER: This is the schedule for the 7mm Q band test on 10 March 2017 involving 8 telescopes: Ef Nt O6 Ys Mh Kt Ky Ku The FTP-NME uses a standard setup with 1024 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: 12:10:00 - J1642+6856 12:34:00 - J2005+7752 12:58:00 - J2005+7752 Clear skies! Jay Skype account: jive.support.scientist Schedule for METSAHOV (Code Mh ) 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 ---------------------------------------------------------------------------------------- --- Fri 10 Mar 2017 Day 69 --- Next scan frequencies: 43138.49 43138.49 43138.49 43138.49 43170.49 43170.49 43170.49 43170.49 43202.49 43202.49 43202.49 43202.49 43234.49 43234.49 43234.49 43234.49 Next BBC frequencies: 738.49 738.49 738.49 738.49 770.49 770.49 770.49 770.49 802.49 802.49 802.49 802.49 834.49 834.49 834.49 834.49 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 12 00 00 J1642+6856 00 50 59 45.6 -25.8 8.1 36.9 0 0 12 00 00 12 12 00 =1642+690 01 03 01 45.0 -24.5 8.3 35.0 720 92 12 00 01 12 14 00 J1642+6856 01 05 02 44.9 -24.3 8.4 34.7 118 92 12 14 00 12 24 00 =1642+690 01 15 03 44.4 -23.3 8.5 33.1 600 169 12 14 01 12 26 00 J2005+7752 01 17 04 60.5 -24.5 5.2 80.5 98 169 12 26 00 12 36 00 =2007+777 01 27 05 60.0 -24.4 5.4 78.2 600 246 12 26 01 12 38 00 J2005+7752 01 29 06 59.9 -24.3 5.4 77.8 118 246 12 38 00 12 48 00 =2007+777 01 39 07 59.4 -24.1 5.6 75.6 600 323 12 38 01 12 50 00 J2005+7752 01 41 08 59.3 -24.0 5.6 75.1 118 323 12 50 00 13 00 00 =2007+777 01 51 09 58.8 -23.7 5.8 72.9 600 400 12 50 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess117.Q1024 --- 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: METSAHOV Total bit rate: 1024 Format: MARK5B 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= 42400.00 42400.00 42400.00 42400.00 42400.00 42400.00 42400.00 42400.00 42400.00 42400.00 42400.00 42400.00 42400.00 42400.00 42400.00 42400.00 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 B1 A1 B1 A1 B1 A1 B1 A1 B1 A1 B1 A1 B1 A1 B1 The following frequency sets based on these setups were used. Frequency Set: 5 Setup file default. Used with PCAL = 1MHz LO sum= 43138.49 43138.49 43138.49 43138.49 43170.49 43170.49 43170.49 43170.49 43202.49 43202.49 43202.49 43202.49 43234.49 43234.49 43234.49 43234.49 BBC fr= 738.49 738.49 738.49 738.49 770.49 770.49 770.49 770.49 802.49 802.49 802.49 802.49 834.49 834.49 834.49 834.49 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: 5 Track assignments are: track1= 18, 26, 2, 10, 20, 28, 4, 12, 22, 30, 6, 14, 24, 32, 8, 16 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) 1642+690 16 42 18.064885 * 16 42 07.848515 16 42 04.568059 0.01 * J1642+6856 69 02 13.21714 * 68 56 39.75642 68 54 32.66785 0.01 J1642+68 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc GSFC 2015a astro solution, unpublished 16092 observations. 2007+777 20 07 20.430197 * 20 05 30.998526 20 04 49.737230 0.03 * J2005+7752 77 43 58.12302 * 77 52 43.24755 77 55 31.97778 0.01 J2005+77 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc GSFC 2015a astro solution, unpublished 15597 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 J1642+6856 sess117.Q1024 1 2 3 4 5 6 0.367 10.267 J2005+7752 sess117.Q1024 1 2 3 4 5 6 0.500 14.000 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) J1642+6856 97.4 J2005+7752 86.1 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