COVER INFORMATION Station: SHANGHAI (Code Sh ) Experiment: The Relativistic Jet of the Peculiar TeV Source IC 310; Exp. Code: EE009C Schedule Version: 1.00 Processed by SCHED version: 10.20 Release of about July 12, 2012 PI: D. Eisenacher Address: Institut fuer Theoretische Physik und Astronomie Universitaet Wuerzburg, Am Hubland D-97074 Wuerzburg Germany Phone: +49 931 31 83335 EMAIL: eduardo.ros@uv.es Fax: +34 96 3543084 Phone during observation: +34 679 517 813 Observing mode: EVN Continuum Dual Pol, 3.6cm, 512 Mbps Notes: Contact name for PI - observing contact: Eduardo Ros Univ. Valencia (obsphone, email & fax) Schedule for SHANGHAI (Code Sh ) Page 2 The Relativistic Jet of the Peculiar TeV Source IC 310; 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 1 Nov 2012 Day 306 --- Next scan frequencies: 8391.49 8391.49 8391.49 8391.49 8407.49 8407.49 8407.49 8407.49 8423.49 8423.49 8423.49 8423.49 8439.49 8439.49 8439.49 8439.49 Next BBC frequencies: 708.51 708.51 708.51 708.51 692.51 692.51 692.51 692.51 676.51 676.51 676.51 676.51 660.51 660.51 660.51 660.51 Next scan bandwidths: 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 21 30 00 3C84 08 21 04 30.5 -57.1 5.0 73.8 0 0 21 30 00 21 35 00 --- 08 26 04 29.6 -56.7 5.1 73.1 300 19 21 30 01 21 35 40 J0316+4119 08 26 45 28.9 -56.7 5.2 72.5 35 19 21 35 40 21 43 40 =0313+411 08 34 46 27.4 -56.2 5.3 71.4 480 50 21 35 41 21 43 55 J0316+4119 08 35 01 27.4 -56.2 5.3 71.4 13 50 21 43 55 21 52 10 =0313+411 08 43 17 25.9 -55.6 5.4 70.3 495 82 21 43 56 21 52 25 J0316+4119 08 43 32 25.9 -55.6 5.4 70.3 13 82 21 52 25 22 00 40 =0313+411 08 51 49 24.4 -55.0 5.6 69.2 495 114 21 52 26 22 00 55 J0316+4119 08 52 04 24.4 -55.0 5.6 69.1 13 114 22 00 55 22 09 10 =0313+411 09 00 20 22.9 -54.3 5.7 68.0 495 146 22 00 56 22 09 25 J0316+4119 09 00 35 22.9 -54.3 5.7 68.0 13 146 22 09 25 22 17 40 =0313+411 09 08 52 21.5 -53.7 5.9 66.8 495 178 22 09 26 22 17 55 J0316+4119 09 09 07 21.4 -53.7 5.9 66.8 13 178 22 17 55 22 26 10 =0313+411 09 17 23 20.0 -53.0 6.0 65.7 495 210 22 17 56 22 26 50 3C84 09 18 03 20.5 -53.0 6.0 66.1 35 210 22 26 50 22 33 50 --- 09 25 04 19.3 -52.4 6.1 65.1 420 237 22 26 51 22 34 30 J0316+4119 09 25 44 18.6 -52.3 6.1 64.5 35 237 22 34 30 22 42 30 =0313+411 09 33 46 17.2 -51.6 6.3 63.4 480 268 22 34 31 22 42 45 J0316+4119 09 34 01 17.2 -51.6 6.3 63.4 13 268 22 42 45 22 51 00 =0313+411 09 42 17 15.8 -50.8 6.4 62.2 495 300 22 42 46 22 51 15 J0316+4119 09 42 32 15.8 -50.8 6.4 62.2 13 300 22 51 15 22 59 30 =0313+411 09 50 48 14.4 -50.1 6.6 61.0 495 332 22 51 16 22 59 45 J0316+4119 09 51 03 14.4 -50.0 6.6 61.0 13 332 22 59 45 23 08 00 =0313+411 09 59 20 13.0 -49.2 6.7 59.8 495 364 22 59 46 23 08 15 J0316+4119 09 59 35 13.0 -49.2 6.7 59.8 13 364 23 08 15 23 16 30 =0313+411 10 07 51 11.6 -48.4 6.8 58.6 495 396 23 08 16 Schedule for SHANGHAI (Code Sh ) Page 3 The Relativistic Jet of the Peculiar TeV Source IC 310; 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 1 Nov 2012 Day 306 --- 23 16 45 J0316+4119 10 08 06 11.6 -48.4 6.8 58.5 13 396 23 16 45 23 25 00 =0313+411 10 16 23 10.3 -47.5 7.0 57.3 495 428 23 16 46 23 25 40 3C84 10 17 03 10.8 -47.6 6.9 57.7 35 428 23 25 40 23 31 40 --- 10 23 04 9.8 -47.0 7.0 56.8 360 451 23 25 41 23 32 20 J0316+4119 10 23 44 9.1 -46.8 7.1 56.2 35 451 23 32 20 23 40 20 =0313+411 10 31 45 7.9 -45.9 7.2 55.0 480 482 23 32 21 23 40 35 J0316+4119 10 32 00 7.8 -45.9 7.2 55.0 13 482 23 40 35 23 48 50 =0313+411 10 40 16 6.6 -45.0 7.4 53.8 495 514 23 40 36 23 49 05 J0316+4119 10 40 32 6.5 -44.9 7.4 53.7 13 514 23 49 05 23 57 20 =0313+411 10 48 48 5.3 -44.0 7.5 52.4 495 546 23 49 06 --- Start: Thu 1 Nov 2012 Day 306 -- Stop: Fri 2 Nov 2012 Day 307 --- 23 57 35 J0316+4119 10 49 03 5.3 -44.0 7.5 52.4 13 546 23 57 35 00 05 50 =0313+411 10 57 19 4.0 -43.0 7.7 D 51.1 0 578 23 57 36 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess312.X512 Matching groups in /homes/vlbsoft/sched10.2/catalogs/freq.dat: shxd From An Tao 18May2006. Dummy dual pol - only RCP available Setup group: 7 Station: SHANGHAI Total bit rate: 512 Format: MARK5B Bits per sample: 2 Sample rate: 16.000 Number of channels: 16 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 9100.00 9100.00 9100.00 9100.00 9100.00 9100.00 9100.00 9100.00 9100.00 9100.00 9100.00 9100.00 9100.00 9100.00 9100.00 9100.00 Net SB= L L U U L L U U L L U U L L U U Pol. = RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP BBC = 1 2 1 2 3 4 3 4 5 6 5 6 7 8 7 8 BBC SB= U U L L U U L L U U L L U U L L IF = A C A C A C A C A C A C A C A C The following frequency sets based on these setups were used. Frequency Set: 10 Setup file default. Used pcal sets: 1 LO sum= 8391.49 8391.49 8391.49 8391.49 8407.49 8407.49 8407.49 8407.49 8423.49 8423.49 8423.49 8423.49 8439.49 8439.49 8439.49 8439.49 BBC fr= 708.51 708.51 708.51 708.51 692.51 692.51 692.51 692.51 676.51 676.51 676.51 676.51 660.51 660.51 660.51 660.51 Bandwd= 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 8.00 Matching frequency sets: 10 The following pulse cal sets were used with this setup: Pulse cal detection set: 1 PCAL = 1MHZ PCALXB1= S1 S3 S5 S7 S9 S11 S13 S15 PCALXB2= S2 S4 S6 S8 S10 S12 S14 S16 PCALFR1= 490 510 490 510 490 510 490 510 PCALFR2= 490 510 490 510 490 510 490 510 Track assignments are: track1= 2, 4, 6, 8, 10, 12, 14, 16, 18, 20, 22, 24, 26, 28, 30, 32 barrel=roll_off SOURCES USED IN RECORDING SCANS -- The Relativistic Jet of the Peculiar TeV Source IC 310; Catalog positions marked with *. Precession of date coordinates is based on stop time of first scan. Names used in schedule marked with *. Short names used in VLA and SNAP files marked with +. Observation date used in B1950/J2000 coordinate conversion (PRECDATE): 1979.900 No adjustments are made for rates (DRA, DDEC). Scan hours are for recording scans only. Baseline hours are only counted for scans above horizon at both ends. Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) 0313+411 03 13 25.195761 * 03 16 42.978246 03 17 36.846536 0.19 * J0316+4119 41 08 29.24375 * 41 19 29.61595 41 22 20.28354 0.20 /homes/vlbsoft/sched10.2/catalogs/sources.vlba rfc_2012b Petrov, 2012, unpublished 90 observations 2.463 scan and 131.946 baseline hours in setup: sess312.X512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 9 10 12 J0319+4130 03 16 29.567260 * 03 19 48.160090 03 20 42.240804 1.30 0316+413 41 19 51.91699 * 41 30 42.10412 41 33 29.83898 2.72 * 3C84 /homes/vlbsoft/sched10.2/catalogs/sources.vlba J0319+41 GSFC 2011A astro solution 9957 Observations 0.408 scan and 20.458 baseline hours in setup: sess312.X512 Frequency sets (dups not shown): 1 2 3 4 5 6 7 9 10 12 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) J0316+4119 151.5 3C84 151.1 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