COVER INFORMATION Station: YEBES40M (Code Ys ) Experiment: 6.7GHz CH3OH maser polarization towards massive protostars. II. Exp. Code: ES072B Schedule Version: 1.00 Processed by SCHED version: 10.20 Release of about July 12, 2012 PI: G. Surcis Address: Joint Institute for VLBI in Europe Postbus 2 7990 AA Dwingeloo The Netherlands Phone: +31 (0)521-596508 EMAIL: surcis@jive.nl Fax: +31 (0)521-596539 Phone during observation: +31 (0)521-596508 Observing mode: Polarization observations of 4 sources at 6.7 GHz (32 Mb/s Notes: phase-cal OFF source = G25.65+1.05 Schedule for YEBES40M (Code Ys ) Page 2 6.7GHz CH3OH maser polarization towards massive protostars. II. 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 31 May 2013 Day 151 --- Next scan frequencies: 6667.25 6667.25 6667.25 6667.25 Next BBC frequencies: 757.25 757.25 757.25 757.25 Next scan bandwidths: 2.00 2.00 2.00 2.00 22 30 00 J2202+4216 14 55 58 16.0 47.4 -7.1 -49.2 0 0 22 30 00 22 40 00 =BLLAC 15 06 00 17.4 48.6 -7.0 -50.5 600 2 22 30 01 22 44 05 J1827-0405 15 10 05 26.4 122.0 -3.3 -40.3 157 2 22 44 05 22 47 05 =1825-041 15 13 06 26.9 122.6 -3.3 -39.9 180 3 22 44 06 22 47 40 G25.65+1.05 15 13 41 24.5 122.7 -3.4 -40.0 17 3 22 47 40 22 57 40 --- 15 23 42 26.1 124.8 -3.2 -38.9 600 6 22 47 41 22 58 15 J1827-0405 15 24 18 28.7 125.1 -3.1 -38.6 17 6 22 58 15 23 01 15 =1825-041 15 27 18 29.1 125.7 -3.0 -38.2 180 6 22 58 16 23 01 50 G25.65+1.05 15 27 53 26.7 125.7 -3.1 -38.3 17 6 23 01 50 23 11 50 --- 15 37 55 28.3 128.0 -3.0 -37.1 600 9 23 01 51 23 12 25 J1827-0405 15 38 30 30.8 128.3 -2.8 -36.7 17 9 23 12 25 23 15 25 =1825-041 15 41 30 31.3 129.0 -2.8 -36.3 180 9 23 12 26 23 16 00 G25.65+1.05 15 42 06 28.9 128.9 -2.9 -36.5 18 9 23 16 00 23 26 00 --- 15 52 07 30.3 131.2 -2.7 -35.1 600 12 23 16 01 23 30 10 J2202+4216 15 56 18 24.9 54.5 -6.1 -56.9 158 12 23 30 10 23 39 10 =BLLAC 16 05 19 26.3 55.5 -6.0 -58.0 540 14 23 30 11 23 43 35 J1827-0405 16 09 45 35.3 136.0 -2.3 -32.0 170 14 23 43 35 23 46 35 =1825-041 16 12 46 35.6 136.7 -2.3 -31.5 180 15 23 43 36 23 47 05 G25.65+1.05 16 13 16 33.2 136.4 -2.4 -31.8 13 15 23 47 05 23 57 05 --- 16 23 17 34.5 139.0 -2.2 -30.1 600 17 23 47 06 --- Start: Fri 31 May 2013 Day 151 -- Stop: Sat 1 Jun 2013 Day 152 --- 23 57 35 J1827-0405 16 23 47 37.0 139.7 -2.1 -29.5 13 17 23 57 35 00 00 35 =1825-041 16 26 48 37.4 140.5 -2.0 -29.0 180 18 23 57 36 00 01 05 G25.65+1.05 16 27 18 35.0 140.0 -2.1 -29.4 13 18 00 01 05 00 11 05 --- 16 37 20 36.2 142.7 -2.0 -27.6 600 20 00 01 06 00 11 35 J1827-0405 16 37 50 38.7 143.6 -1.8 -26.9 13 20 00 11 35 00 14 35 =1825-041 16 40 50 39.0 144.5 -1.8 -26.3 180 21 00 11 36 Schedule for YEBES40M (Code Ys ) Page 3 6.7GHz CH3OH maser polarization towards massive protostars. II. 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 ---------------------------------------------------------------------------------------- --- Sat 1 Jun 2013 Day 152 --- 00 15 05 G25.65+1.05 16 41 20 36.7 143.8 -1.9 -26.8 13 21 00 15 05 00 25 05 --- 16 51 22 37.7 146.6 -1.7 -24.9 600 23 00 15 06 00 25 35 J1827-0405 16 51 52 40.2 147.7 -1.6 -24.0 13 23 00 25 35 00 28 35 =1825-041 16 54 52 40.5 148.6 -1.6 -23.4 180 24 00 25 36 00 29 05 G25.65+1.05 16 55 23 38.2 147.8 -1.7 -24.0 13 24 00 29 05 00 39 05 --- 17 05 24 39.1 150.7 -1.5 -22.0 600 27 00 29 06 00 43 37 J2202+4216 17 09 57 36.8 62.1 -4.9 -65.4 168 27 00 43 37 00 52 37 =BLLAC 17 18 58 38.3 63.0 -4.7 -66.4 540 29 00 43 38 00 57 27 J1827-0405 17 23 49 43.0 157.7 -1.1 -16.8 181 29 00 57 27 01 00 27 =1825-041 17 26 50 43.2 158.7 -1.0 -16.1 180 30 00 57 28 01 00 57 G25.65+1.05 17 27 20 41.0 157.4 -1.1 -17.1 13 30 01 00 57 01 09 57 --- 17 36 21 41.6 160.3 -1.0 -14.9 540 32 01 00 58 01 10 27 J1827-0405 17 36 51 43.8 162.0 -0.9 -13.6 13 32 01 10 27 01 13 27 =1825-041 17 39 52 44.0 163.0 -0.8 -12.9 180 32 01 10 28 01 13 57 G25.65+1.05 17 40 22 41.8 161.6 -0.9 -14.0 13 32 01 13 57 01 22 57 --- 17 49 23 42.3 164.5 -0.8 -11.8 540 35 01 13 58 01 23 27 J1827-0405 17 49 53 44.5 166.4 -0.6 -10.3 13 35 01 23 27 01 26 27 =1825-041 17 52 54 44.7 167.5 -0.6 -9.5 180 35 01 23 28 01 26 57 G25.65+1.05 17 53 24 42.5 165.9 -0.7 -10.8 13 35 01 26 57 01 35 57 --- 18 02 25 42.9 168.9 -0.5 -8.5 540 37 01 26 58 01 36 27 J1827-0405 18 02 56 45.0 171.0 -0.4 -6.9 13 37 01 36 27 01 39 27 =1825-041 18 05 56 45.1 172.0 -0.4 -6.1 180 38 01 36 28 01 39 57 G25.65+1.05 18 06 26 43.0 170.2 -0.5 -7.5 13 38 01 39 57 01 48 57 --- 18 15 28 43.3 173.3 -0.3 -5.1 540 40 01 39 58 01 53 53 J2202+4216 18 20 24 48.9 68.4 -3.7 -73.0 176 40 01 53 53 02 02 53 =BLLAC 18 29 26 50.5 69.2 -3.6 -74.0 540 43 01 53 54 02 08 08 J1827-0405 18 34 42 45.4 182.2 0.1 1.7 188 43 02 08 08 02 11 08 =1825-041 18 37 42 45.3 183.3 0.2 2.5 180 43 02 08 09 02 11 40 G25.65+1.05 18 38 14 43.5 181.1 0.1 0.8 15 43 02 11 40 02 21 40 --- 18 48 16 43.4 184.5 0.2 3.4 600 46 02 11 41 Schedule for YEBES40M (Code Ys ) Page 4 6.7GHz CH3OH maser polarization towards massive protostars. II. 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 ---------------------------------------------------------------------------------------- --- Sat 1 Jun 2013 Day 152 --- 02 22 12 J1827-0405 18 48 48 45.1 187.2 0.3 5.5 14 46 02 22 12 02 25 12 =1825-041 18 51 49 45.1 188.2 0.4 6.3 180 46 02 22 13 02 25 44 G25.65+1.05 18 52 21 43.3 185.9 0.3 4.5 14 46 02 25 44 02 35 44 --- 19 02 22 43.1 189.3 0.5 7.1 600 49 02 25 45 02 36 16 J1827-0405 19 02 54 44.7 192.1 0.6 9.2 14 49 02 36 16 02 39 16 =1825-041 19 05 55 44.6 193.2 0.6 10.0 180 50 02 36 17 02 39 48 G25.65+1.05 19 06 27 42.9 190.7 0.5 8.1 14 50 02 39 48 02 49 48 --- 19 16 29 42.5 194.0 0.7 10.7 600 52 02 39 49 02 55 00 J2202+4216 19 21 41 59.9 73.0 -2.7 -79.6 176 52 02 55 00 03 04 00 =BLLAC 19 30 43 61.6 73.6 -2.5 -80.6 540 54 02 55 01 03 09 30 J1827-0405 19 36 14 42.8 203.3 1.1 17.6 186 54 03 09 30 03 12 30 =1825-041 19 39 14 42.5 204.3 1.2 18.3 180 55 03 09 31 03 13 02 G25.65+1.05 19 39 46 41.2 201.6 1.1 16.3 14 55 03 13 02 03 23 02 --- 19 49 48 40.4 204.7 1.2 18.6 600 57 03 13 03 03 23 34 J1827-0405 19 50 20 41.6 207.8 1.4 20.8 14 57 03 23 34 03 26 34 =1825-041 19 53 21 41.3 208.7 1.4 21.5 180 58 03 23 35 03 27 06 G25.65+1.05 19 53 53 40.1 206.0 1.3 19.6 14 58 03 27 06 03 37 06 --- 20 03 54 39.2 209.0 1.5 21.8 600 60 03 27 07 03 37 38 J1827-0405 20 04 26 40.3 212.1 1.6 23.9 14 60 03 37 38 03 40 38 =1825-041 20 07 27 40.0 213.0 1.6 24.5 180 61 03 37 39 03 41 10 G25.65+1.05 20 07 59 38.8 210.2 1.5 22.6 14 61 03 41 10 03 51 10 --- 20 18 01 37.8 213.1 1.7 24.7 600 64 03 41 11 03 56 20 J2202+4216 20 23 12 71.2 76.2 -1.7 -87.1 158 64 03 56 20 04 05 20 =BLLAC 20 32 13 72.9 76.4 -1.5 -88.4 540 66 03 56 21 04 08 20 J2136+0041 20 35 14 47.8 156.5 -1.0 -17.6 86 66 04 08 20 04 16 20 =2134+00 20 43 15 48.4 159.4 -0.9 -15.5 480 68 04 08 21 04 19 30 J1827-0405 20 46 25 35.4 223.8 2.3 31.8 111 68 04 19 30 04 22 30 =1825-041 20 49 26 35.0 224.6 2.3 32.4 180 68 04 19 31 04 23 02 G25.65+1.05 20 49 58 34.1 221.8 2.2 30.6 14 68 04 23 02 04 33 02 --- 21 00 00 32.8 224.4 2.4 32.3 600 71 04 23 03 Schedule for YEBES40M (Code Ys ) Page 5 6.7GHz CH3OH maser polarization towards massive protostars. II. 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 ---------------------------------------------------------------------------------------- --- Sat 1 Jun 2013 Day 152 --- 04 33 34 J1827-0405 21 00 32 33.4 227.4 2.5 34.1 14 71 04 33 34 04 36 34 =1825-041 21 03 32 33.0 228.1 2.6 34.6 180 72 04 33 35 04 37 06 G25.65+1.05 21 04 04 32.3 225.4 2.5 33.0 14 72 04 37 06 04 47 06 --- 21 14 06 30.9 227.8 2.6 34.5 600 74 04 37 07 04 47 38 J1827-0405 21 14 38 31.4 230.8 2.8 36.2 14 74 04 47 38 04 50 38 =1825-041 21 17 38 31.0 231.5 2.8 36.6 180 75 04 47 39 04 51 10 G25.65+1.05 21 18 11 30.3 228.8 2.7 35.1 14 75 04 51 10 05 01 10 --- 21 28 12 28.9 231.1 2.9 36.5 600 77 04 51 11 05 01 42 J1827-0405 21 28 44 29.3 234.1 3.0 38.1 14 77 05 01 42 05 04 42 =1825-041 21 31 45 28.8 234.7 3.1 38.5 180 78 05 01 43 05 05 14 G25.65+1.05 21 32 17 28.3 232.0 3.0 37.1 14 78 05 05 14 05 15 14 --- 21 42 19 26.7 234.3 3.1 38.3 600 80 05 05 15 05 19 59 J2202+4216 21 47 04 86.5 57.8 -0.3 -119.5 96 80 05 19 59 05 29 59 =BLLAC 21 57 06 87.8 32.1 -0.1 -146.9 600 83 05 20 00 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess213.M32 Matching groups in /aps3/sched10.2/catalogs/freq.dat: ys40_5cm RF and LO values by de Vicente (FEB09), BBC 500-1000MHz Setup group: 6 Station: YEBES40M Total bit rate: 32 Format: MARK5B Bits per sample: 2 Sample rate: 4.000 Number of channels: 4 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 5910.00 5910.00 5910.00 5910.00 Net SB= U U U U Pol. = RCP LCP RCP LCP BBC = 1 2 3 4 BBC SB= U U U U IF = A C A C The following frequency sets based on these setups were used. Frequency Set: 7 Based on FREQ, BW, and/or DOPPLER in schedule. Used pcal sets: 1 LO sum= 6667.25 6667.25 6667.25 6667.25 BBC fr= 757.25 757.25 757.25 757.25 Bandwd= 2.00 2.00 2.00 2.00 Matching frequency sets: 7 The following pulse cal sets were used with this setup: Pulse cal detection set: 1 PCAL = OFF PCALXB1= S1 S2 S3 S4 OFF OFF OFF OFF PCALXB2= M1 M2 M3 M4 OFF OFF OFF OFF PCALFR1= 0 0 0 0 0 0 0 0 PCALFR2= 0 0 0 0 0 0 0 0 Track assignments are: track1= 2, 4, 6, 8 barrel=roll_off SOURCES USED IN RECORDING SCANS -- 6.7GHz CH3OH maser polarization towards massive protostars. II. 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) * G25.65+1.05 18 31 40.145161 * 18 34 20.900000 18 35 05.956119 0.00 -06 02 05.96283 *-05 59 42.10000 -05 58 55.86133 0.00 From catalog imbedded in main SCHED input file. Doppler based on LSR frame and radio definition. Velocities: 41.60 41.60 41.60 41.60 3.433 scan and 96.132 baseline hours in setup: sess213.M32 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 * J1827-0405 18 25 06.481697 * 18 27 45.040495 18 28 29.516577 2.15 1825-041 -04 07 39.91460 *-04 05 44.57832 -04 05 06.46651 1.99 /aps3/sched10.2/catalogs/sources.vlba GSFC 2011A astro solution 22 Observations Doppler based on other sources. 1.050 scan and 29.398 baseline hours in setup: sess213.M32 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 * J2136+0041 21 34 05.207371 * 21 36 38.586306 21 37 20.829296 0.74 2134+00 00 28 25.08000 * 00 41 54.21282 00 45 37.21822 1.25 2134+004 /aps3/sched10.2/catalogs/sources.vlba J2136+00 GSFC 2011A astro solution 26937 Observations Doppler based on other sources. 0.133 scan and 3.518 baseline hours in setup: sess213.M32 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 * J2202+4216 22 00 39.362504 * 22 02 43.291371 22 03 17.855554 0.14 BLLAC 42 02 08.59073 * 42 16 39.97987 42 20 26.72580 0.10 2200+420 /aps3/sched10.2/catalogs/sources.vlba J2202+42 rfc_2012b Petrov, 2012, unpublished 59418 observations VR422201 Doppler based on other sources. 1.083 scan and 29.165 baseline hours in setup: sess213.M32 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 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) G25.65+1.05 147.2 J1827-0405 147.5 J2136+0041 103.4 J2202+4216 81.2 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