COVER INFORMATION Station: TORUN (Code Tr ) Experiment: RadioAstron AGN polarization imaging Exp. Code: gg081j Schedule Version: 1.00 Processed by SCHED version: 11.40 Release 11.4. March 14, 2015 PI: Jose L. Gomez Address: Instituto de Astrofisica de Andalucia-CSIC Glorieta de la Astronomia E-18008 Granada, Spain Phone: +79165452842 EMAIL: jlgomez@iaa.es, alobanov@mpifr-bonn.mpg.de Fax: Phone during observation: +79165452842 Observing mode: K-band,Q-band, dual-pol Notes: K-band, Radioastron-compatible frequency setup P-CAL is ON Tsys is ON auto-level (AGC) is ON Schedule for TORUN (Code Tr ) Page 2 RadioAstron AGN polarization imaging 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 ---------------------------------------------------------------------------------------- --- Thu 9 Mar 2017 Day 68 --- ---------- K-band VLBI scans. Space segment 01: 0851+202 with EVN +RA ---------- Next scan frequencies: 22236.00 22236.00 22236.00 22236.00 22268.00 22268.00 22268.00 22268.00 Next BBC frequencies: 736.00 736.00 736.00 736.00 768.00 768.00 768.00 768.00 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 23 00 00 0851+202 11 25 32 46.2 235.6 2.5 31.8 0 0 23 00 00 23 10 00 --- 11 35 34 45.0 238.5 2.7 33.0 600 38 23 00 01 23 10 30 0851+202 11 36 04 44.9 238.6 2.7 33.1 24 38 23 10 30 23 20 00 --- 11 45 36 43.7 241.2 2.8 34.1 570 75 23 10 31 23 20 30 0851+202 11 46 06 43.6 241.3 2.8 34.1 24 75 23 20 30 23 30 00 --- 11 55 37 42.3 243.9 3.0 35.0 570 112 23 20 31 23 30 30 0851+202 11 56 07 42.2 244.0 3.0 35.1 24 112 23 30 30 23 40 00 --- 12 05 39 41.0 246.4 3.2 35.9 570 148 23 30 31 23 40 30 0851+202 12 06 09 40.9 246.5 3.2 35.9 24 148 23 40 30 23 50 00 --- 12 15 41 39.6 248.9 3.3 36.6 570 185 23 40 31 23 50 30 0851+202 12 16 11 39.5 249.0 3.3 36.6 24 185 23 50 30 23 59 59 --- 12 25 42 38.1 251.3 3.5 37.3 569 221 23 50 31 --- Fri 10 Mar 2017 Day 69 --- 00 00 30 0851+202 12 26 12 38.1 251.4 3.5 37.3 24 221 00 00 30 00 10 00 --- 12 35 44 36.7 253.7 3.7 37.8 570 258 00 00 31 00 10 30 0851+202 12 36 14 36.6 253.8 3.7 37.9 24 258 00 10 30 00 20 00 --- 12 45 46 35.3 256.0 3.8 38.3 570 294 00 10 31 00 20 30 0851+202 12 46 16 35.2 256.1 3.8 38.3 24 294 00 20 30 00 30 00 --- 12 55 47 33.8 258.2 4.0 38.7 570 331 00 20 31 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: ra1cm2.set --- 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: 14 Station: TORUN Total bit rate: 512 Format: MARK5B Bits per sample: 2 Sample rate: 32.000 Number of channels: 8 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 21500.00 21500.00 21500.00 21500.00 21500.00 21500.00 21500.00 21500.00 Net SB= U U L L U U L L IF SB = U U U U U U U U Pol. = RCP LCP RCP LCP RCP LCP RCP LCP BBC = 1 5 1 5 3 7 3 7 BBC SB= U U L L U U L L IF = A1 B1 A1 B1 A1 B1 A1 B1 The following frequency sets based on these setups were used. Frequency Set: 6 Setup file default. Used with PCAL = 1MHz LO sum= 22236.00 22236.00 22236.00 22236.00 22268.00 22268.00 22268.00 22268.00 BBC fr= 736.00 736.00 736.00 736.00 768.00 768.00 768.00 768.00 Bandwd= 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 Matching frequency sets: 6 Track assignments are: track1= 2, 6, 10, 14, 4, 8, 12, 16 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) * FAKERA 11 57 21.769299 * 12 00 00.000000 12 01 00.078159 0.00 85 16 41.77889 * 85 00 00.00000 84 54 13.66473 0.00 From catalog imbedded in main SCHED input file. fake circumpolar target for a TS to look at * 0851+202 08 51 57.250618 * 08 54 48.874930 08 55 48.272298 0.00 J0854+2006 20 17 58.41733 * 20 06 30.64078 20 02 24.65225 0.00 OJ287 ./gg081j_sources.radioastron AGN, rfc_2013d Petrov, 2013, unpublished 213710 observations, RA-AO3-04, RA-AO3- 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 FAKERA ra1cm2.set 14 1.433 0.000 0851+202 ra1cm2.set 1 2 3 4 5 6 7 8 9 10 11 1.433 111.778 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) FAKERA 99.1 0851+202 141.1 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