COVER INFORMATION Station: TIANMA65 (Code T6 ) Experiment: OH EGOs PtII Exp. Code: EB063A Schedule Version: 1.00 Processed by SCHED version: 11.40 Release 11.4. March 14, 2015 PI: Ross Burns Address: JIVE Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31-521-596508 EMAIL: burns@jive.eu Fax: Phone during observation: +31-521-596508 Observing mode: Notes: COVER LETTER: OH maser polarisation at L-band. Targets are Extended Green Objects (EGOs) Schedule for TIANMA65 (Code T6 ) Page 2 OH EGOs PtII 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 ---------------------------------------------------------------------------------------- --- Wed 1 Nov 2017 Day 305 --- ---------- R-L phase difference ---------- Next scan frequencies: 1662.02 1662.02 Next BBC frequencies: 607.98 607.98 Next scan bandwidths: 8.00 8.00 11 30 00 J2202+4216 22 18 20 78.3 -13.7 0.2 164.1 0 0 11 30 00 11 34 00 =VR422201 22 22 21 78.1 -17.2 0.3 160.0 240 2 11 30 01 ---------- Fringe Finder ---------- 11 34 00 J1800+3848 22 22 21 37.0 -62.5 4.4 77.1 -168 2 No stop 11 41 30 =1758+388 22 29 52 35.6 -62.1 4.5 76.2 282 6 11 34 01 ---------- Tsys ---------- 11 41 45 J1800+3848 22 30 07 35.5 -62.0 4.5 76.1 13 6 11 41 45 11 42 00 =1758+388 22 30 22 35.5 -62.0 4.5 76.1 15 6 11 41 46 11 50 15 G034.40+0.23 22 38 38 29.4 252.2 3.7 54.7 -136 6 11 50 15 12 02 00 --- 22 50 25 26.9 254.1 3.9 55.5 569 11 11 50 16 12 02 15 G034.40+0.23 22 50 40 26.9 254.2 3.9 55.5 13 11 12 02 15 12 14 00 --- 23 02 27 24.5 256.0 4.1 56.2 705 17 12 02 16 12 14 15 G034.40+0.23 23 02 42 24.4 256.0 4.1 56.2 13 17 12 14 15 12 26 00 --- 23 14 29 22.0 257.8 4.3 56.9 705 23 12 14 16 12 26 15 G034.40+0.23 23 14 44 21.9 257.8 4.3 56.9 13 23 12 26 15 12 38 00 --- 23 26 31 19.4 259.6 4.5 57.4 705 28 12 26 16 ---------- Pol Cal ---------- 12 38 15 J2202+4216 23 26 46 69.9 310.0 1.4 117.4 -187 28 12 38 15 12 46 00 =VR422201 23 34 32 68.7 308.2 1.5 114.4 278 32 12 38 16 12 46 15 G034.40+0.23 23 34 47 17.7 260.7 4.7 57.7 -194 32 12 46 15 12 58 00 --- 23 46 34 15.2 262.4 4.9 58.1 511 38 12 46 16 12 58 15 G034.40+0.23 23 46 49 15.1 262.4 4.9 58.1 13 38 12 58 15 13 10 00 --- 23 58 36 12.6 264.0 5.1 58.4 705 43 12 58 16 13 10 15 G034.40+0.23 23 58 51 12.6 264.0 5.1 58.4 13 43 13 10 15 13 22 00 --- 00 10 38 10.1 265.6 5.3 58.7 705 49 13 10 16 Schedule for TIANMA65 (Code T6 ) Page 3 OH EGOs PtII 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 ---------------------------------------------------------------------------------------- --- Wed 1 Nov 2017 Day 305 --- 13 22 15 G034.40+0.23 00 10 53 10.0 265.6 5.3 58.7 13 49 13 22 15 13 34 00 --- 00 22 40 7.5 267.2 5.5 58.8 705 55 13 22 16 ---------- Pol Cal ---------- 13 34 15 J2202+4216 00 22 55 60.1 302.0 2.3 100.6 -195 55 13 34 15 13 42 00 =VR422201 00 30 42 58.7 301.5 2.5 98.9 270 58 13 34 16 ---------- Pol Cal ---------- 14 30 15 J2202+4216 01 19 05 49.8 300.4 3.3 89.8 2893 58 14 30 15 14 38 00 =VR422201 01 26 51 48.4 300.4 3.4 88.5 465 62 14 30 16 ---------- Pol Cal ---------- 15 26 15 J2202+4216 02 15 14 39.5 301.5 4.2 81.1 2893 62 15 26 15 15 34 00 =VR422201 02 23 00 38.1 301.8 4.3 80.0 465 66 15 26 16 ---------- Pol Cal ---------- 16 22 15 J2202+4216 03 11 23 29.4 304.3 5.1 73.2 2893 66 16 22 15 16 30 00 =VR422201 03 19 09 28.0 304.8 5.3 72.1 465 69 16 22 16 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess317.L64 --- 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: 13 Station: TIANMA65 Total bit rate: 64 Format: MARK5B Bits per sample: 2 Sample rate: 16.000 Number of channels: 2 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 2270.00 2270.00 Net SB= U U IF SB = L L Pol. = RCP LCP BBC = 1 9 BBC SB= L L IF = A2 C1 The following frequency sets based on these setups were used. Frequency Set: 6 Based on FREQ, BW, and/or DOPPLER in schedule. Used with PCAL = off LO sum= 1662.02 1662.02 BBC fr= 607.98 607.98 Bandwd= 8.00 8.00 Matching frequency sets: 6 Track assignments are: track1= 2, 4 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) * G034.40+0.23 18 50 45.714204 * 18 53 17.920000 18 54 10.770830 0.00 01 21 39.89169 * 01 25 25.48000 01 27 00.76894 0.00 From catalog imbedded in main SCHED input file. Doppler based on LSR frame and radio definition. Velocities: 57.00 57.00 * OQ208 14 04 45.615156 * 14 07 00.394414 14 07 46.069478 0.24 J1407+2827 28 41 29.23518 * 28 27 14.69022 28 22 22.87907 0.34 1404+286 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc J1407+28 GSFC 2015a astro solution, unpublished 67871 observations. Doppler based on other sources. 1758+388 17 58 44.703952 * 18 00 24.765362 18 00 58.799731 0.01 * J1800+3848 38 48 32.47350 * 38 48 30.69749 38 48 52.69580 0.01 J1800+38 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc GSFC 2015a astro solution, unpublished 4173 observations. Doppler based on other sources. VR422201 22 00 39.362505 * 22 02 43.291372 22 03 27.827879 0.00 * J2202+4216 42 02 08.59077 * 42 16 39.97990 42 22 08.03182 0.00 BLLAC /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc 2200+420 GSFC 2015a astro solution, unpublished 51226 observations. J2202+42 Doppler based on other sources. 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 G034.40+0.2sess317.L64 1 3 4 5 6 7 8 11 12 13 3.917 239.310 OQ208 sess317.L64 1 3 4 5 7 8 11 12 13 0.129 3.567 J1800+3848 sess317.L64 1 3 4 5 6 7 8 11 12 13 0.129 6.541 J2202+4216 sess317.L64 1 3 4 5 6 7 8 11 12 13 0.712 28.094 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) G034.40+0.23 67.8 OQ208 43.3 J1800+3848 73.0 J2202+4216 117.4 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