COVER INFORMATION Station: TORUN (Code Tr ) Experiment: How do O-type forming stars accrete their mass? Exp. Code: EG073B Schedule Version: 2.00 Processed by SCHED version: 11.40 Release 11.4. March 14, 2015 PI: Ciriaco Goddi Address: Radboud Astronomy Department Heyendaalseweg 135, 6525 AJ Nijmegen Netherlands Phone: +31 243652845 EMAIL: goddi@astro.ru.nl Fax: Phone during observation: +31 243652845 Observing mode: Polarimetric observations in phase-reference of 1 maser so Notes: There are two sources ~1arcmin apart in the sky. We observe at an intermediate position. At correlation, we require two passes at each source position. This is a multi-epoch experiment. This is the second epoch; next in 2yr Phase-cal OFF Schedule for TORUN (Code Tr ) Page 2 How do O-type forming stars accrete their mass? 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 23 Oct 2015 Day 296 --- Next scan frequencies: 6664.12 6664.12 6664.12 6664.12 6668.12 6668.12 6668.12 6668.12 6672.12 6672.12 6672.12 6672.12 6676.12 6676.12 6676.12 6676.12 Next BBC frequencies: 764.12 764.12 764.12 764.12 768.12 768.12 768.12 768.12 772.12 772.12 772.12 772.12 776.12 776.12 776.12 776.12 Next scan bandwidths: 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 13 30 00 J2202+4216 16 50 51 39.1 68.6 -5.2 -49.2 0 0 13 30 00 13 38 00 =VR422201 16 58 53 40.2 69.9 -5.1 -49.7 480 8 13 30 01 13 47 30 J1331+3030 17 08 24 45.1 261.9 3.6 43.6 172 8 13 47 30 13 58 30 =3C286 17 19 26 43.5 264.3 3.8 43.9 660 18 13 47 31 14 08 00 W51 17 28 58 45.2 138.4 -1.9 -24.3 300 18 14 08 00 14 15 00 --- 17 35 59 45.9 140.7 -1.8 -23.2 420 25 14 08 01 14 15 40 J1930+1532 17 36 39 46.2 138.0 -1.9 -24.7 20 25 14 15 40 14 17 40 =1928+154 17 38 39 46.4 138.6 -1.9 -24.3 120 27 14 15 41 14 17 40 W51 17 38 39 46.2 141.5 -1.8 -22.7 -20 27 No stop 14 19 40 --- 17 40 40 46.3 142.2 -1.7 -22.4 100 29 14 17 41 14 19 40 J1930+1532 17 40 40 46.6 139.3 -1.8 -24.0 -20 29 No stop 14 21 40 =1928+154 17 42 40 46.8 139.9 -1.8 -23.7 100 31 14 19 41 14 21 40 W51 17 42 40 46.5 142.8 -1.7 -22.0 -20 31 No stop 14 23 40 --- 17 44 40 46.7 143.5 -1.7 -21.7 100 33 14 21 41 14 23 40 J1930+1532 17 44 40 47.0 140.6 -1.8 -23.3 -20 33 No stop 14 25 40 =1928+154 17 46 41 47.2 141.2 -1.7 -23.0 100 35 14 23 41 14 26 20 W51 17 47 21 47.0 144.4 -1.6 -21.2 19 35 14 26 20 14 28 20 --- 17 49 21 47.1 145.0 -1.6 -20.8 120 37 14 26 21 14 29 00 J1930+1532 17 50 01 47.5 142.3 -1.7 -22.4 20 37 14 29 00 14 31 00 =1928+154 17 52 01 47.7 143.0 -1.7 -22.1 120 38 14 29 01 14 31 00 W51 17 52 01 47.4 145.9 -1.5 -20.3 -21 38 No stop 14 33 00 --- 17 54 02 47.5 146.6 -1.5 -20.0 99 40 14 31 01 14 33 00 J1930+1532 17 54 02 47.9 143.6 -1.6 -21.7 -20 40 No stop 14 35 00 =1928+154 17 56 02 48.0 144.3 -1.6 -21.3 100 42 14 33 01 14 35 00 W51 17 56 02 47.7 147.3 -1.5 -19.6 -21 42 No stop 14 37 00 --- 17 58 02 47.8 147.9 -1.4 -19.2 99 44 14 35 01 Schedule for TORUN (Code Tr ) Page 3 How do O-type forming stars accrete their mass? 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 23 Oct 2015 Day 296 --- 14 37 00 J1930+1532 17 58 02 48.2 145.0 -1.6 -21.0 -20 44 No stop 14 39 00 =1928+154 18 00 03 48.4 145.7 -1.5 -20.6 100 46 14 37 01 14 39 40 W51 18 00 43 48.1 148.9 -1.4 -18.7 19 46 14 39 40 14 41 40 --- 18 02 43 48.2 149.5 -1.4 -18.3 120 48 14 39 41 14 42 20 J1930+1532 18 03 23 48.7 146.8 -1.5 -20.0 20 48 14 42 20 14 44 20 =1928+154 18 05 24 48.8 147.5 -1.4 -19.6 120 50 14 42 21 14 44 20 W51 18 05 24 48.4 150.5 -1.3 -17.8 -21 50 No stop 14 46 20 --- 18 07 24 48.6 151.2 -1.3 -17.4 99 52 14 44 21 14 46 20 J1930+1532 18 07 24 49.0 148.2 -1.4 -19.2 -20 52 No stop 14 48 20 =1928+154 18 09 24 49.1 148.9 -1.4 -18.8 100 54 14 46 21 14 48 20 W51 18 09 24 48.7 151.9 -1.3 -17.0 -21 54 No stop 14 50 20 --- 18 11 25 48.8 152.6 -1.2 -16.6 99 56 14 48 21 14 50 20 J1930+1532 18 11 25 49.3 149.6 -1.3 -18.4 -20 56 No stop 14 52 20 =1928+154 18 13 25 49.5 150.3 -1.3 -18.0 100 58 14 50 21 14 53 00 W51 18 14 05 49.0 153.5 -1.2 -16.1 19 58 14 53 00 14 55 00 --- 18 16 05 49.2 154.2 -1.1 -15.6 120 60 14 53 01 14 55 40 J1930+1532 18 16 45 49.7 151.5 -1.2 -17.3 20 60 14 55 40 14 57 40 =1928+154 18 18 46 49.8 152.2 -1.2 -16.9 120 62 14 55 41 15 00 51 J2202+4216 18 21 57 52.3 83.5 -3.7 -53.9 38 62 15 00 51 15 08 51 =VR422201 18 29 58 53.5 85.0 -3.6 -54.1 480 69 15 00 52 15 12 18 W51 18 33 26 50.2 160.5 -0.8 -11.9 42 69 15 12 18 15 16 18 --- 18 37 27 50.4 162.0 -0.8 -11.0 240 73 15 12 19 15 16 58 J1930+1532 18 38 07 51.0 159.3 -0.9 -12.8 20 73 15 16 58 15 18 58 =1928+154 18 40 07 51.1 160.0 -0.9 -12.3 120 75 15 16 59 15 18 58 W51 18 40 07 50.5 163.0 -0.7 -10.4 -21 75 No stop 15 20 58 --- 18 42 08 50.6 163.8 -0.7 -10.0 99 77 15 18 59 15 20 58 J1930+1532 18 42 08 51.2 160.8 -0.8 -11.9 -20 77 No stop 15 22 58 =1928+154 18 44 08 51.3 161.5 -0.8 -11.4 100 79 15 20 59 15 22 58 W51 18 44 08 50.6 164.5 -0.7 -9.5 -21 79 No stop 15 24 58 --- 18 46 08 50.7 165.3 -0.6 -9.1 99 81 15 22 59 Schedule for TORUN (Code Tr ) Page 4 How do O-type forming stars accrete their mass? 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 23 Oct 2015 Day 296 --- 15 24 58 J1930+1532 18 46 08 51.4 162.3 -0.8 -10.9 -20 81 No stop 15 26 58 =1928+154 18 48 09 51.5 163.0 -0.7 -10.5 100 83 15 24 59 15 27 38 W51 18 48 49 50.8 166.3 -0.6 -8.5 19 83 15 27 38 15 29 38 --- 18 50 49 50.9 167.0 -0.6 -8.0 120 85 15 27 39 15 30 18 J1930+1532 18 51 29 51.7 164.3 -0.7 -9.7 20 85 15 30 18 15 32 18 =1928+154 18 53 30 51.7 165.1 -0.6 -9.2 120 87 15 30 19 15 32 18 W51 18 53 30 51.0 168.1 -0.5 -7.4 -21 87 No stop 15 34 18 --- 18 55 30 51.0 168.8 -0.5 -6.9 99 88 15 32 19 15 34 18 J1930+1532 18 55 30 51.8 165.9 -0.6 -8.8 -20 88 No stop 15 36 18 =1928+154 18 57 30 51.9 166.6 -0.6 -8.3 100 90 15 34 19 15 36 18 W51 18 57 30 51.1 169.6 -0.4 -6.4 -21 90 No stop 15 38 18 --- 18 59 31 51.1 170.4 -0.4 -6.0 99 92 15 36 19 15 38 18 J1930+1532 18 59 31 52.0 167.4 -0.5 -7.8 -20 92 No stop 15 40 18 =1928+154 19 01 31 52.0 168.2 -0.5 -7.3 100 94 15 38 19 15 40 58 W51 19 02 11 51.2 171.4 -0.4 -5.3 19 94 15 40 58 15 42 58 --- 19 04 11 51.2 172.2 -0.3 -4.9 120 96 15 40 59 15 43 38 J1930+1532 19 04 51 52.1 169.5 -0.4 -6.5 20 96 15 43 38 15 45 38 =1928+154 19 06 52 52.2 170.3 -0.4 -6.1 120 98 15 43 39 15 45 38 W51 19 06 52 51.3 173.2 -0.3 -4.2 -21 98 No stop 15 47 38 --- 19 08 52 51.3 174.0 -0.3 -3.7 99 100 15 45 39 15 47 38 J1930+1532 19 08 52 52.2 171.0 -0.4 -5.6 -20 100 No stop 15 49 38 =1928+154 19 10 52 52.3 171.8 -0.3 -5.1 100 102 15 47 39 15 49 38 W51 19 10 52 51.4 174.7 -0.2 -3.3 -21 102 No stop 15 51 38 --- 19 12 53 51.4 175.5 -0.2 -2.8 99 104 15 49 39 15 51 38 J1930+1532 19 12 53 52.3 172.6 -0.3 -4.6 -20 104 No stop 15 53 38 =1928+154 19 14 53 52.3 173.4 -0.3 -4.1 100 106 15 51 39 15 54 18 W51 19 15 33 51.4 176.6 -0.1 -2.1 20 106 15 54 18 15 56 18 --- 19 17 33 51.4 177.3 -0.1 -1.7 120 108 15 54 19 15 56 58 J1930+1532 19 18 14 52.4 174.7 -0.2 -3.3 20 108 15 56 58 15 58 58 =1928+154 19 20 14 52.4 175.5 -0.2 -2.8 120 110 15 56 59 Schedule for TORUN (Code Tr ) Page 5 How do O-type forming stars accrete their mass? 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 23 Oct 2015 Day 296 --- 16 02 35 J2202+4216 19 23 51 61.6 95.9 -2.7 -53.9 42 110 16 02 35 16 10 35 =VR422201 19 31 53 62.7 97.8 -2.5 -53.6 480 117 16 02 36 16 14 33 W51 19 35 51 51.4 184.4 0.2 2.7 50 117 16 14 33 16 18 33 --- 19 39 52 51.3 186.0 0.3 3.7 240 121 16 14 34 16 19 13 J1930+1532 19 40 32 52.4 183.5 0.1 2.2 21 121 16 19 13 16 21 13 =1928+154 19 42 32 52.4 184.3 0.2 2.7 120 123 16 19 14 16 21 13 W51 19 42 32 51.3 187.0 0.3 4.3 -20 123 No stop 16 23 13 --- 19 44 32 51.3 187.8 0.3 4.8 100 125 16 21 14 16 23 13 J1930+1532 19 44 32 52.4 185.1 0.2 3.2 -19 125 No stop 16 25 13 =1928+154 19 46 33 52.4 185.9 0.2 3.7 101 127 16 23 14 16 25 13 W51 19 46 33 51.2 188.6 0.4 5.3 -20 127 No stop 16 27 13 --- 19 48 33 51.2 189.3 0.4 5.8 100 129 16 25 14 16 27 13 J1930+1532 19 48 33 52.3 186.7 0.3 4.2 -19 129 No stop 16 29 13 =1928+154 19 50 33 52.3 187.5 0.3 4.7 101 131 16 27 14 16 29 53 W51 19 51 14 51.1 190.4 0.4 6.4 20 131 16 29 53 16 31 53 --- 19 53 14 51.0 191.1 0.5 6.9 120 133 16 29 54 16 32 33 J1930+1532 19 53 54 52.2 188.8 0.4 5.5 21 133 16 32 33 16 34 33 =1928+154 19 55 54 52.2 189.6 0.4 6.0 120 135 16 32 34 16 34 33 W51 19 55 54 51.0 192.1 0.5 7.5 -20 135 No stop 16 36 33 --- 19 57 55 50.9 192.9 0.6 8.0 100 137 16 34 34 16 36 33 J1930+1532 19 57 55 52.1 190.4 0.4 6.4 -19 137 No stop 16 38 33 =1928+154 19 59 55 52.1 191.1 0.5 6.9 101 138 16 36 34 16 38 33 W51 19 59 55 50.8 193.7 0.6 8.4 -19 138 No stop 16 40 33 --- 20 01 55 50.7 194.4 0.6 8.9 101 140 16 38 34 16 40 33 J1930+1532 20 01 55 52.0 191.9 0.5 7.4 -19 140 No stop 16 42 33 =1928+154 20 03 56 51.9 192.7 0.5 7.9 101 142 16 40 34 16 43 13 W51 20 04 36 50.6 195.4 0.7 9.5 21 142 16 43 13 16 45 13 --- 20 06 36 50.6 196.2 0.7 10.0 120 144 16 43 14 16 45 53 J1930+1532 20 07 16 51.8 194.0 0.6 8.7 21 144 16 45 53 16 47 53 =1928+154 20 09 16 51.8 194.8 0.6 9.1 120 146 16 45 54 Schedule for TORUN (Code Tr ) Page 6 How do O-type forming stars accrete their mass? 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 23 Oct 2015 Day 296 --- 16 47 53 W51 20 09 16 50.4 197.2 0.7 10.6 -19 146 No stop 16 49 53 --- 20 11 17 50.4 197.9 0.8 11.0 101 148 16 47 54 16 49 53 J1930+1532 20 11 17 51.7 195.5 0.7 9.6 -19 148 No stop 16 51 53 =1928+154 20 13 17 51.6 196.3 0.7 10.1 101 150 16 49 54 16 51 53 W51 20 13 17 50.3 198.7 0.8 11.5 -19 150 No stop 16 53 53 --- 20 15 17 50.2 199.4 0.8 11.9 101 152 16 51 54 16 53 53 J1930+1532 20 15 17 51.5 197.1 0.7 10.5 -19 152 No stop 16 55 53 =1928+154 20 17 18 51.4 197.8 0.8 11.0 101 154 16 53 54 16 56 33 W51 20 17 58 50.0 200.4 0.9 12.5 21 154 16 56 33 16 58 33 --- 20 19 58 49.9 201.2 0.9 12.9 120 156 16 56 34 16 59 13 J1930+1532 20 20 38 51.3 199.1 0.8 11.8 22 156 16 59 13 17 01 13 =1928+154 20 22 39 51.2 199.8 0.9 12.2 120 158 16 59 14 17 05 22 J2202+4216 20 26 49 70.7 114.0 -1.6 -47.9 62 158 17 05 22 17 13 22 =VR422201 20 34 50 71.8 117.1 -1.5 -46.3 480 165 17 05 23 17 17 55 W51 20 39 24 48.7 208.1 1.2 17.0 77 165 17 17 55 17 22 55 --- 20 44 25 48.3 209.9 1.3 18.0 300 170 17 17 56 17 23 35 J1930+1532 20 45 05 49.8 208.1 1.2 17.0 21 170 17 23 35 17 25 35 =1928+154 20 47 05 49.7 208.8 1.3 17.5 120 172 17 23 36 17 25 35 W51 20 47 05 48.1 210.8 1.4 18.5 -19 172 No stop 17 27 35 --- 20 49 06 48.0 211.5 1.4 18.9 101 174 17 25 36 17 27 35 J1930+1532 20 49 06 49.5 209.5 1.3 17.9 -19 174 No stop 17 29 35 =1928+154 20 51 06 49.4 210.2 1.3 18.3 101 176 17 27 36 17 29 35 W51 20 51 06 47.8 212.2 1.4 19.3 -19 176 No stop 17 31 35 --- 20 53 06 47.7 212.8 1.5 19.7 101 178 17 29 36 17 31 35 J1930+1532 20 53 06 49.2 210.9 1.4 18.7 -19 178 No stop 17 33 35 =1928+154 20 55 07 49.0 211.6 1.4 19.1 101 180 17 31 36 17 34 15 W51 20 55 47 47.4 213.7 1.5 20.2 21 180 17 34 15 17 36 15 --- 20 57 47 47.3 214.4 1.6 20.5 120 182 17 34 16 17 36 55 J1930+1532 20 58 27 48.8 212.7 1.4 19.7 21 182 17 36 55 17 38 55 =1928+154 21 00 27 48.6 213.4 1.5 20.1 120 184 17 36 56 Schedule for TORUN (Code Tr ) Page 7 How do O-type forming stars accrete their mass? 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 23 Oct 2015 Day 296 --- 17 38 55 W51 21 00 27 47.0 215.3 1.6 21.0 -20 184 No stop 17 40 55 --- 21 02 28 46.9 216.0 1.6 21.4 100 186 17 38 56 17 40 55 J1930+1532 21 02 28 48.4 214.1 1.5 20.5 -19 186 No stop 17 42 55 =1928+154 21 04 28 48.3 214.8 1.5 20.8 101 187 17 40 56 17 42 55 W51 21 04 28 46.7 216.6 1.7 21.7 -20 187 No stop 17 44 55 --- 21 06 28 46.5 217.3 1.7 22.1 100 189 17 42 56 17 44 55 J1930+1532 21 06 28 48.1 215.5 1.6 21.2 -19 189 No stop 17 46 55 =1928+154 21 08 29 47.9 216.1 1.6 21.6 101 191 17 44 56 17 47 35 W51 21 09 09 46.3 218.1 1.7 22.5 20 191 17 47 35 17 49 35 --- 21 11 09 46.1 218.8 1.8 22.9 120 193 17 47 36 17 50 15 J1930+1532 21 11 49 47.6 217.3 1.7 22.2 20 193 17 50 15 17 52 15 =1928+154 21 13 50 47.4 217.9 1.7 22.5 120 195 17 50 16 17 52 15 W51 21 13 50 45.8 219.7 1.8 23.3 -20 195 No stop 17 54 15 --- 21 15 50 45.6 220.3 1.9 23.7 100 197 17 52 16 17 54 15 J1930+1532 21 15 50 47.3 218.6 1.7 22.9 -20 197 No stop 17 56 15 =1928+154 21 17 50 47.1 219.2 1.8 23.2 100 199 17 54 16 17 56 15 W51 21 17 50 45.4 220.9 1.9 24.0 -20 199 No stop 17 58 15 --- 21 19 51 45.2 221.6 1.9 24.3 100 201 17 56 16 17 58 15 J1930+1532 21 19 51 46.9 219.9 1.8 23.6 -20 201 No stop 18 00 15 =1928+154 21 21 51 46.7 220.5 1.8 23.9 100 203 17 58 16 18 00 55 W51 21 22 31 45.0 222.4 2.0 24.7 20 203 18 00 55 18 02 55 --- 21 24 31 44.8 223.0 2.0 25.0 120 205 18 00 56 18 03 35 J1930+1532 21 25 11 46.4 221.6 1.9 24.4 20 205 18 03 35 18 05 35 =1928+154 21 27 12 46.2 222.2 1.9 24.8 120 207 18 03 36 18 10 12 J2202+4216 21 31 49 78.0 150.7 -0.5 -23.5 115 207 18 10 12 18 18 12 =VR422201 21 39 50 78.6 157.5 -0.4 -18.1 480 214 18 10 13 18 23 07 W51 21 44 47 42.6 229.1 2.3 28.0 139 214 18 23 07 18 28 07 --- 21 49 48 42.0 230.5 2.4 28.6 300 219 18 23 08 18 28 47 J1930+1532 21 50 28 43.6 229.3 2.3 28.2 20 219 18 28 47 18 30 47 =1928+154 21 52 28 43.4 229.9 2.3 28.5 120 221 18 28 48 Schedule for TORUN (Code Tr ) Page 8 How do O-type forming stars accrete their mass? 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 23 Oct 2015 Day 296 --- 18 30 47 W51 21 52 28 41.7 231.3 2.5 28.9 -20 221 No stop 18 32 47 --- 21 54 28 41.4 231.8 2.5 29.2 100 223 18 30 48 18 32 47 J1930+1532 21 54 28 43.2 230.5 2.4 28.7 -20 223 No stop 18 34 47 =1928+154 21 56 29 43.0 231.0 2.4 29.0 100 225 18 32 48 18 34 47 W51 21 56 29 41.2 232.4 2.5 29.4 -20 225 No stop 18 36 47 --- 21 58 29 41.0 233.0 2.6 29.7 100 227 18 34 48 18 36 47 J1930+1532 21 58 29 42.7 231.6 2.4 29.3 -20 227 No stop 18 38 47 =1928+154 22 00 29 42.5 232.2 2.5 29.5 100 229 18 36 48 18 39 27 W51 22 01 09 40.6 233.7 2.6 30.0 20 229 18 39 27 18 41 27 --- 22 03 10 40.4 234.3 2.6 30.2 120 231 18 39 28 18 42 07 J1930+1532 22 03 50 42.1 233.1 2.5 29.9 20 231 18 42 07 18 44 07 =1928+154 22 05 50 41.8 233.7 2.6 30.2 120 233 18 42 08 18 44 07 W51 22 05 50 40.1 235.0 2.7 30.5 -20 233 No stop 18 46 07 --- 22 07 50 39.8 235.5 2.7 30.8 100 235 18 44 08 18 46 07 J1930+1532 22 07 50 41.6 234.3 2.6 30.4 -20 235 No stop 18 48 07 =1928+154 22 09 51 41.4 234.8 2.6 30.6 100 237 18 46 08 18 48 07 W51 22 09 51 39.6 236.1 2.8 31.0 -21 237 No stop 18 50 07 --- 22 11 51 39.3 236.6 2.8 31.2 99 238 18 48 08 18 50 07 J1930+1532 22 11 51 41.1 235.4 2.7 30.9 -20 238 No stop 18 52 07 =1928+154 22 13 51 40.9 235.9 2.7 31.1 100 240 18 50 08 18 52 47 W51 22 14 32 39.0 237.3 2.8 31.5 19 240 18 52 47 18 54 47 --- 22 16 32 38.7 237.9 2.9 31.7 120 242 18 52 48 18 55 27 J1930+1532 22 17 12 40.4 236.8 2.8 31.5 20 242 18 55 27 18 57 27 =1928+154 22 19 12 40.2 237.4 2.8 31.7 120 244 18 55 28 18 57 27 W51 22 19 12 38.4 238.6 2.9 32.0 -21 244 No stop 18 59 27 --- 22 21 13 38.1 239.1 2.9 32.2 99 246 18 57 28 18 59 27 J1930+1532 22 21 13 39.9 237.9 2.8 31.9 -20 246 No stop 19 01 27 =1928+154 22 23 13 39.7 238.4 2.9 32.1 100 248 18 59 28 19 01 27 W51 22 23 13 37.9 239.6 3.0 32.4 -21 248 No stop 19 03 27 --- 22 25 13 37.6 240.1 3.0 32.5 99 250 19 01 28 Schedule for TORUN (Code Tr ) Page 9 How do O-type forming stars accrete their mass? 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 23 Oct 2015 Day 296 --- 19 03 27 J1930+1532 22 25 13 39.4 239.0 2.9 32.3 -20 250 No stop 19 05 27 =1928+154 22 27 14 39.2 239.5 2.9 32.5 100 252 19 03 28 19 06 07 W51 22 27 54 37.3 240.8 3.1 32.8 19 252 19 06 07 19 08 07 --- 22 29 54 37.0 241.3 3.1 33.0 120 254 19 06 08 19 08 47 J1930+1532 22 30 34 38.7 240.4 3.0 32.8 20 254 19 08 47 19 10 47 =1928+154 22 32 35 38.5 240.9 3.0 33.0 120 256 19 08 48 19 15 06 J2202+4216 22 36 54 77.9 210.9 0.6 24.7 97 256 19 15 06 19 23 06 =VR422201 22 44 55 77.2 217.0 0.7 29.3 480 263 19 15 07 19 27 30 W51 22 49 20 34.4 246.1 3.4 34.6 90 263 19 27 30 19 31 00 --- 22 52 50 33.9 247.0 3.5 34.8 210 267 19 27 31 19 31 40 J1930+1532 22 53 30 35.7 246.1 3.4 34.8 20 267 19 31 40 19 33 40 =1928+154 22 55 31 35.4 246.6 3.4 34.9 120 269 19 31 41 19 33 40 W51 22 55 31 33.5 247.6 3.5 35.0 -21 269 No stop 19 35 40 --- 22 57 31 33.3 248.1 3.6 35.1 99 271 19 33 41 19 35 40 J1930+1532 22 57 31 35.1 247.1 3.4 35.0 -21 271 No stop 19 37 40 =1928+154 22 59 31 34.8 247.6 3.5 35.2 99 273 19 35 41 19 37 40 W51 22 59 31 33.0 248.6 3.6 35.3 -21 273 No stop 19 39 40 --- 23 01 32 32.7 249.0 3.6 35.4 99 275 19 37 41 19 39 40 J1930+1532 23 01 32 34.5 248.1 3.5 35.3 -21 275 No stop 19 41 40 =1928+154 23 03 32 34.3 248.5 3.5 35.5 99 276 19 39 41 19 42 20 W51 23 04 12 32.3 249.7 3.7 35.6 19 276 19 42 20 19 44 20 --- 23 06 12 32.0 250.1 3.7 35.7 120 278 19 42 21 19 45 00 J1930+1532 23 06 53 33.8 249.3 3.6 35.7 19 278 19 45 00 19 47 00 =1928+154 23 08 53 33.5 249.8 3.6 35.8 120 280 19 45 01 19 47 00 W51 23 08 53 31.7 250.7 3.7 35.9 -21 280 No stop 19 49 00 --- 23 10 53 31.4 251.2 3.8 36.0 99 282 19 47 01 19 49 00 J1930+1532 23 10 53 33.2 250.3 3.7 35.9 -21 282 No stop 19 51 00 =1928+154 23 12 54 32.9 250.7 3.7 36.0 99 284 19 49 01 19 51 00 W51 23 12 54 31.1 251.7 3.8 36.1 -21 284 No stop 19 53 00 --- 23 14 54 30.8 252.1 3.8 36.2 99 286 19 51 01 Schedule for TORUN (Code Tr ) Page 10 How do O-type forming stars accrete their mass? 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 23 Oct 2015 Day 296 --- 19 53 00 J1930+1532 23 14 54 32.7 251.2 3.7 36.2 -21 286 No stop 19 55 00 =1928+154 23 16 54 32.4 251.7 3.8 36.3 99 288 19 53 01 19 55 40 W51 23 17 34 30.4 252.7 3.9 36.3 19 288 19 55 40 19 57 40 --- 23 19 35 30.1 253.2 3.9 36.4 120 290 19 55 41 19 58 20 J1930+1532 23 20 15 31.9 252.4 3.8 36.5 19 290 19 58 20 20 00 20 =1928+154 23 22 15 31.6 252.9 3.8 36.6 120 292 19 58 21 20 00 20 W51 23 22 15 29.8 253.8 4.0 36.6 -21 292 No stop 20 02 20 --- 23 24 15 29.5 254.2 4.0 36.7 99 294 20 00 21 20 02 20 J1930+1532 23 24 15 31.3 253.3 3.9 36.7 -21 294 No stop 20 04 20 =1928+154 23 26 16 31.0 253.8 3.9 36.8 99 296 20 02 21 20 04 20 W51 23 26 16 29.2 254.7 4.0 36.8 -21 296 No stop 20 06 20 --- 23 28 16 28.9 255.1 4.1 36.8 99 298 20 04 21 20 06 20 J1930+1532 23 28 16 30.7 254.2 3.9 36.9 -21 298 No stop 20 08 20 =1928+154 23 30 16 30.5 254.7 4.0 37.0 99 300 20 06 21 20 09 00 W51 23 30 57 28.5 255.7 4.1 37.0 19 300 20 09 00 20 11 00 --- 23 32 57 28.2 256.2 4.1 37.0 120 301 20 09 01 20 11 40 J1930+1532 23 33 37 30.0 255.4 4.0 37.1 19 301 20 11 40 20 13 40 =1928+154 23 35 37 29.7 255.9 4.1 37.2 120 303 20 11 41 20 16 45 J2202+4216 23 38 43 70.9 245.5 1.6 47.7 17 303 20 16 45 20 24 45 =VR422201 23 46 45 69.7 248.4 1.7 49.1 480 311 20 16 46 20 28 03 W51 23 50 03 25.7 259.8 4.4 37.6 19 311 20 28 03 20 31 33 --- 23 53 33 25.2 260.6 4.5 37.7 210 314 20 28 04 20 32 13 J1930+1532 23 54 13 27.0 259.9 4.4 37.9 19 314 20 32 13 20 34 13 =1928+154 23 56 14 26.7 260.3 4.4 37.9 120 316 20 32 14 20 34 13 W51 23 56 14 24.8 261.2 4.5 37.8 -21 316 No stop 20 36 43 --- 23 58 44 24.4 261.7 4.6 37.9 129 319 20 34 14 20 36 43 J1930+1532 23 58 44 26.3 260.9 4.5 38.0 -21 319 No stop 20 38 43 =1928+154 00 00 44 26.0 261.3 4.5 38.0 99 321 20 36 44 20 38 43 W51 00 00 44 24.1 262.1 4.6 37.9 -21 321 No stop 20 41 13 --- 00 03 15 23.7 262.6 4.6 38.0 129 323 20 38 44 Schedule for TORUN (Code Tr ) Page 11 How do O-type forming stars accrete their mass? 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 23 Oct 2015 Day 296 --- 20 41 13 J1930+1532 00 03 15 25.6 261.8 4.5 38.1 -21 323 No stop 20 43 13 =1928+154 00 05 15 25.3 262.2 4.6 38.1 99 325 20 41 14 20 43 53 W51 00 05 55 23.3 263.2 4.7 38.0 19 325 20 43 53 20 46 23 --- 00 08 26 23.0 263.7 4.7 38.1 150 327 20 43 54 20 47 03 J1930+1532 00 09 06 24.7 263.0 4.6 38.2 19 327 20 47 03 20 49 03 =1928+154 00 11 06 24.4 263.5 4.7 38.3 120 329 20 47 04 20 49 03 W51 00 11 06 22.6 264.2 4.8 38.1 -21 329 No stop 20 51 33 --- 00 13 36 22.2 264.8 4.8 38.2 129 332 20 49 04 20 51 33 J1930+1532 00 13 36 24.1 264.0 4.7 38.3 -21 332 No stop 20 53 33 =1928+154 00 15 37 23.8 264.4 4.7 38.3 99 334 20 51 34 20 53 33 W51 00 15 37 21.9 265.2 4.9 38.2 -21 334 No stop 20 56 03 --- 00 18 07 21.5 265.7 4.9 38.2 129 336 20 53 34 20 56 03 J1930+1532 00 18 07 23.4 264.9 4.8 38.4 -21 336 No stop 20 58 03 =1928+154 00 20 08 23.1 265.3 4.8 38.4 99 338 20 56 04 20 58 43 W51 00 20 48 21.1 266.2 4.9 38.2 19 338 20 58 43 21 01 13 --- 00 23 18 20.7 266.7 5.0 38.3 150 340 20 58 44 21 01 53 J1930+1532 00 23 58 22.5 266.1 4.9 38.5 19 340 21 01 53 21 03 53 =1928+154 00 25 58 22.2 266.5 4.9 38.5 120 342 21 01 54 21 03 53 W51 00 25 58 20.3 267.3 5.0 38.3 -21 342 No stop 21 06 23 --- 00 28 29 20.0 267.8 5.1 38.3 129 345 21 03 54 21 06 23 J1930+1532 00 28 29 21.8 267.0 4.9 38.5 -21 345 No stop 21 08 23 =1928+154 00 30 29 21.5 267.4 5.0 38.5 99 347 21 06 24 21 08 23 W51 00 30 29 19.7 268.2 5.1 38.3 -21 347 No stop 21 10 53 --- 00 33 00 19.3 268.7 5.1 38.3 129 349 21 08 24 21 10 53 J1930+1532 00 33 00 21.2 267.9 5.0 38.5 -21 349 No stop 21 12 53 =1928+154 00 35 00 20.9 268.3 5.1 38.5 99 351 21 10 54 21 13 33 W51 00 35 40 18.9 269.2 5.2 38.3 19 351 21 13 33 21 16 03 --- 00 38 10 18.5 269.7 5.2 38.3 150 353 21 13 34 21 16 43 J1930+1532 00 38 51 20.3 269.1 5.1 38.6 19 353 21 16 43 21 18 43 =1928+154 00 40 51 20.0 269.5 5.2 38.6 120 355 21 16 44 Schedule for TORUN (Code Tr ) Page 12 How do O-type forming stars accrete their mass? 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 23 Oct 2015 Day 296 --- 21 21 50 J2202+4216 00 43 59 61.4 264.4 2.7 54.0 18 355 21 21 50 21 29 50 =VR422201 00 52 00 60.2 266.1 2.8 54.2 480 363 21 21 51 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess315.M128 --- 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: 6 Station: TORUN Total bit rate: 128 Format: MARK5B Bits per sample: 2 Sample rate: 4.000 Number of channels: 16 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 5900.00 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 5 1 5 2 6 2 6 3 7 3 7 4 8 4 8 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: 7 Based on FREQ, BW, and/or DOPPLER in schedule. Used with PCAL = off LO sum= 6664.12 6664.12 6664.12 6664.12 6668.12 6668.12 6668.12 6668.12 6672.12 6672.12 6672.12 6672.12 6676.12 6676.12 6676.12 6676.12 BBC fr= 764.12 764.12 764.12 764.12 768.12 768.12 768.12 768.12 772.12 772.12 772.12 772.12 776.12 776.12 776.12 776.12 Bandwd= 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 Matching frequency sets: 7 10 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) * W51 19 21 24.339697 * 19 23 42.000000 19 24 25.201954 0.00 14 24 56.76822 * 14 30 50.00000 14 33 03.33748 0.00 From catalog imbedded in main SCHED input file. Doppler based on LSR frame and radio definition. Velocities: 57.00 57.00 57.00 57.00 57.00 57.00 57.00 57.00 57.00 57.00 57.00 57.00 57.00 57.00 3C286 13 28 49.657758 * 13 31 08.288051 13 31 50.190076 0.18 * J1331+3030 30 45 58.64059 * 30 30 32.95924 30 25 49.46524 0.17 1328+307 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc J1331+30 GSFC 2015a astro solution, unpublished 225 observations. Doppler based on other sources. 1928+154 19 28 36.092074 * 19 30 52.766999 19 31 35.706903 0.07 * J1930+1532 15 26 11.96602 * 15 32 34.42741 15 34 57.17433 0.11 J1930+15 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc GSFC 2015a astro solution, unpublished 132 observations. Doppler based on other sources. VR422201 22 00 39.362505 * 22 02 43.291372 22 03 23.728543 0.00 * J2202+4216 42 02 08.59077 * 42 16 39.97990 42 21 37.02033 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 W51 sess315.M128 1 2 3 4 5 6 7 8 2.708 110.741 J1331+3030 sess315.M128 1 2 3 4 5 6 7 8 0.183 8.247 J1930+1532 sess315.M128 1 2 3 4 5 6 7 8 2.333 94.151 J2202+4216 sess315.M128 1 2 3 4 5 6 7 8 1.067 45.599 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) W51 86.4 J1331+3030 42.2 J1930+1532 88.3 J2202+4216 121.9 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