COVER INFORMATION Station: YEBES40M (Code Ys ) Experiment: How do O-type forming stars accrete their mass? Exp. Code: EG073A Schedule Version: 2.00 Processed by SCHED version: 10.20 Release of about July 12, 2012 PI: Ciriaco Goddi Address: JIVE POSTBUS 2 7990 AA Dwingelooo Netherlands Phone: +31 (0)521 596 548 EMAIL: goddi@jive.nl Fax: Phone during observation: +31 (0)521 596 548 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. Phase-cal OFF Schedule for YEBES40M (Code Ys ) 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 ---------------------------------------------------------------------------------------- --- Wed 29 May 2013 Day 149 --- Next scan frequencies: 6667.58 6667.58 6667.58 6667.58 6671.58 6671.58 6671.58 6671.58 6675.58 6675.58 6675.58 6675.58 6679.58 6679.58 6679.58 6679.58 Next BBC frequencies: 757.58 757.58 757.58 757.58 761.58 761.58 761.58 761.58 765.58 765.58 765.58 765.58 769.58 769.58 769.58 769.58 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 23 00 00 J2202+4216 15 18 10 19.1 50.1 -6.8 -52.1 0 0 23 00 00 23 08 00 =BLLAC 15 26 11 20.3 51.1 -6.6 -53.1 480 8 23 00 01 23 17 30 J1331+3030 15 35 43 63.0 257.9 2.1 59.6 350 8 23 17 30 23 28 30 =3C286 15 46 44 60.9 260.4 2.2 60.4 660 18 23 17 31 23 38 00 W51 15 56 16 38.0 104.4 -3.5 -49.5 398 18 23 38 00 23 45 00 --- 16 03 17 39.3 105.8 -3.4 -49.1 420 25 23 38 01 23 45 40 J1930+1532 16 03 57 38.8 103.5 -3.5 -50.1 23 25 23 45 40 23 47 40 =1928+154 16 05 58 39.2 103.9 -3.4 -50.0 120 27 23 45 41 23 47 40 W51 16 05 58 39.8 106.4 -3.3 -48.9 -17 27 No stop 23 49 40 --- 16 07 58 40.2 106.8 -3.3 -48.7 103 29 23 47 41 23 49 40 J1930+1532 16 07 58 39.5 104.3 -3.4 -49.9 -17 29 No stop 23 51 40 =1928+154 16 09 58 39.9 104.7 -3.4 -49.7 103 31 23 49 41 23 51 40 W51 16 09 58 40.5 107.2 -3.2 -48.6 -18 31 No stop 23 53 40 --- 16 11 59 40.9 107.7 -3.2 -48.4 102 33 23 51 41 23 53 40 J1930+1532 16 11 59 40.3 105.1 -3.3 -49.6 -18 33 No stop 23 55 40 =1928+154 16 13 59 40.6 105.5 -3.3 -49.5 102 35 23 53 41 23 56 20 W51 16 14 39 41.4 108.2 -3.2 -48.2 22 35 23 56 20 23 58 20 --- 16 16 39 41.7 108.7 -3.1 -48.1 120 37 23 56 21 --- Start: Wed 29 May 2013 Day 149 -- Stop: Thu 30 May 2013 Day 150 --- 23 59 00 J1930+1532 16 17 19 41.2 106.2 -3.2 -49.3 22 37 23 59 00 00 01 00 =1928+154 16 19 20 41.6 106.7 -3.2 -49.1 120 39 23 59 01 00 01 00 W51 16 19 20 42.2 109.2 -3.1 -47.9 -18 39 No stop 00 03 00 --- 16 21 20 42.6 109.7 -3.1 -47.7 102 41 00 01 01 00 03 00 J1930+1532 16 21 20 42.0 107.1 -3.2 -49.0 -18 41 No stop 00 05 00 =1928+154 16 23 20 42.3 107.5 -3.1 -48.8 102 43 00 03 01 Schedule for YEBES40M (Code Ys ) 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 ---------------------------------------------------------------------------------------- --- Thu 30 May 2013 Day 150 --- 00 05 00 W51 16 23 20 42.9 110.1 -3.0 -47.5 -18 43 No stop 00 07 00 --- 16 25 21 43.3 110.6 -3.0 -47.3 102 45 00 05 01 00 07 00 J1930+1532 16 25 21 42.7 107.9 -3.1 -48.7 -18 45 No stop 00 09 00 =1928+154 16 27 21 43.1 108.4 -3.1 -48.5 102 46 00 07 01 00 09 40 W51 16 28 01 43.8 111.2 -2.9 -47.1 22 46 00 09 40 00 11 40 --- 16 30 02 44.1 111.6 -2.9 -46.9 120 48 00 09 41 00 12 20 J1930+1532 16 30 42 43.7 109.1 -3.0 -48.2 22 48 00 12 20 00 14 20 =1928+154 16 32 42 44.0 109.6 -3.0 -48.0 120 50 00 12 21 00 14 20 W51 16 32 42 44.6 112.3 -2.9 -46.6 -18 50 No stop 00 16 20 --- 16 34 42 44.9 112.7 -2.8 -46.4 102 52 00 14 21 00 16 20 J1930+1532 16 34 42 44.4 110.0 -2.9 -47.9 -18 52 No stop 00 18 20 =1928+154 16 36 43 44.7 110.5 -2.9 -47.7 102 54 00 16 21 00 18 20 W51 16 36 43 45.3 113.2 -2.8 -46.2 -18 54 No stop 00 20 20 --- 16 38 43 45.6 113.7 -2.8 -46.0 102 56 00 18 21 00 20 20 J1930+1532 16 38 43 45.1 110.9 -2.9 -47.5 -18 56 No stop 00 22 20 =1928+154 16 40 43 45.4 111.4 -2.8 -47.3 102 58 00 20 21 00 23 00 W51 16 41 23 46.1 114.3 -2.7 -45.7 22 58 00 23 00 00 25 00 --- 16 43 24 46.5 114.8 -2.7 -45.5 120 60 00 23 01 00 25 40 J1930+1532 16 44 04 46.0 112.2 -2.8 -46.9 22 60 00 25 40 00 27 40 =1928+154 16 46 04 46.4 112.7 -2.8 -46.7 120 62 00 25 41 00 30 48 J2202+4216 16 49 13 33.3 60.1 -5.2 -63.1 121 62 00 30 48 00 38 48 =BLLAC 16 57 14 34.7 60.9 -5.1 -64.0 480 70 00 30 49 00 42 13 W51 17 00 40 49.4 119.3 -2.4 -43.2 132 70 00 42 13 00 46 13 --- 17 04 41 50.0 120.4 -2.3 -42.6 240 74 00 42 14 00 46 53 J1930+1532 17 05 21 49.7 117.5 -2.4 -44.4 22 74 00 46 53 00 48 53 =1928+154 17 07 21 50.0 118.1 -2.4 -44.1 120 75 00 46 54 00 48 53 W51 17 07 21 50.5 121.1 -2.3 -42.2 -18 75 No stop 00 50 53 --- 17 09 21 50.8 121.7 -2.2 -41.9 102 77 00 48 54 00 50 53 J1930+1532 17 09 21 50.4 118.6 -2.4 -43.9 -18 77 No stop 00 52 53 =1928+154 17 11 22 50.7 119.1 -2.3 -43.6 102 79 00 50 54 Schedule for YEBES40M (Code Ys ) 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 ---------------------------------------------------------------------------------------- --- Thu 30 May 2013 Day 150 --- 00 52 53 W51 17 11 22 51.1 122.3 -2.2 -41.6 -18 79 No stop 00 54 53 --- 17 13 22 51.4 122.9 -2.2 -41.3 102 81 00 52 54 00 54 53 J1930+1532 17 13 22 51.0 119.7 -2.3 -43.3 -18 81 No stop 00 56 53 =1928+154 17 15 22 51.4 120.3 -2.3 -43.0 102 83 00 54 54 00 57 33 W51 17 16 02 51.9 123.6 -2.1 -40.8 22 83 00 57 33 00 59 33 --- 17 18 03 52.2 124.2 -2.1 -40.5 120 85 00 57 34 01 00 13 J1930+1532 17 18 43 51.9 121.2 -2.2 -42.4 22 85 01 00 13 01 02 13 =1928+154 17 20 43 52.2 121.8 -2.2 -42.1 120 87 01 00 14 01 02 13 W51 17 20 43 52.6 125.1 -2.1 -40.0 -18 87 No stop 01 04 13 --- 17 22 43 52.9 125.7 -2.0 -39.6 102 89 01 02 14 01 04 13 J1930+1532 17 22 43 52.6 122.4 -2.1 -41.8 -18 89 No stop 01 06 13 =1928+154 17 24 44 52.9 123.0 -2.1 -41.4 102 91 01 04 14 01 06 13 W51 17 24 44 53.2 126.3 -2.0 -39.3 -18 91 No stop 01 08 13 --- 17 26 44 53.5 126.9 -2.0 -38.9 102 93 01 06 14 01 08 13 J1930+1532 17 26 44 53.2 123.6 -2.1 -41.1 -18 93 No stop 01 10 13 =1928+154 17 28 44 53.5 124.2 -2.0 -40.7 102 95 01 08 14 01 10 53 W51 17 29 25 53.9 127.8 -1.9 -38.4 22 95 01 10 53 01 12 53 --- 17 31 25 54.2 128.4 -1.9 -38.0 120 97 01 10 54 01 13 33 J1930+1532 17 32 05 54.0 125.2 -2.0 -40.1 22 97 01 13 33 01 15 33 =1928+154 17 34 05 54.4 125.9 -2.0 -39.7 120 99 01 13 34 01 15 33 W51 17 34 05 54.6 129.3 -1.8 -37.4 -18 99 No stop 01 17 33 --- 17 36 06 54.9 130.0 -1.8 -37.0 102 101 01 15 34 01 17 33 J1930+1532 17 36 06 54.7 126.5 -1.9 -39.4 -18 101 No stop 01 19 33 =1928+154 17 38 06 55.0 127.2 -1.9 -39.0 102 103 01 17 34 01 19 33 W51 17 38 06 55.2 130.7 -1.8 -36.6 -19 103 No stop 01 21 33 --- 17 40 06 55.5 131.3 -1.7 -36.1 101 105 01 19 34 01 21 33 J1930+1532 17 40 06 55.3 127.8 -1.9 -38.6 -19 105 No stop 01 23 33 =1928+154 17 42 07 55.6 128.5 -1.8 -38.1 101 106 01 21 34 01 24 13 W51 17 42 47 55.9 132.3 -1.7 -35.5 21 106 01 24 13 01 26 13 --- 17 44 47 56.2 133.0 -1.7 -35.1 120 108 01 24 14 Schedule for YEBES40M (Code Ys ) 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 ---------------------------------------------------------------------------------------- --- Thu 30 May 2013 Day 150 --- 01 26 53 J1930+1532 17 45 27 56.1 129.6 -1.8 -37.4 21 108 01 26 53 01 28 53 =1928+154 17 47 28 56.4 130.3 -1.7 -37.0 120 110 01 26 54 01 32 27 J2202+4216 17 51 02 43.8 65.9 -4.2 -69.9 134 110 01 32 27 01 40 27 =BLLAC 17 59 03 45.2 66.6 -4.1 -70.7 480 118 01 32 28 01 44 21 W51 18 02 58 58.5 139.8 -1.4 -30.4 147 118 01 44 21 01 48 21 --- 18 06 59 59.0 141.5 -1.3 -29.3 240 122 01 44 22 01 49 01 J1930+1532 18 07 39 59.1 137.8 -1.4 -32.0 21 122 01 49 01 01 51 01 =1928+154 18 09 39 59.4 138.6 -1.4 -31.4 120 124 01 49 02 01 51 01 W51 18 09 39 59.3 142.6 -1.2 -28.5 -19 124 No stop 01 53 01 --- 18 11 40 59.6 143.4 -1.2 -27.9 101 126 01 51 02 01 53 01 J1930+1532 18 11 40 59.6 139.4 -1.3 -30.9 -19 126 No stop 01 55 01 =1928+154 18 13 40 59.9 140.3 -1.3 -30.3 101 128 01 53 02 01 55 01 W51 18 13 40 59.8 144.3 -1.2 -27.3 -19 128 No stop 01 57 01 --- 18 15 40 60.0 145.1 -1.1 -26.7 101 130 01 55 02 01 57 01 J1930+1532 18 15 40 60.1 141.1 -1.3 -29.7 -19 130 No stop 01 59 01 =1928+154 18 17 41 60.3 141.9 -1.2 -29.1 101 132 01 57 02 01 59 41 W51 18 18 21 60.3 146.3 -1.1 -25.8 21 132 01 59 41 02 01 41 --- 18 20 21 60.5 147.2 -1.1 -25.2 120 134 01 59 42 02 02 21 J1930+1532 18 21 01 60.7 143.4 -1.2 -28.1 21 134 02 02 21 02 04 21 =1928+154 18 23 01 61.0 144.3 -1.1 -27.4 120 135 02 02 22 02 04 21 W51 18 23 01 60.8 148.4 -1.0 -24.3 -19 135 No stop 02 06 21 --- 18 25 02 61.0 149.3 -1.0 -23.6 101 137 02 04 22 02 06 21 J1930+1532 18 25 02 61.2 145.1 -1.1 -26.8 -19 137 No stop 02 08 21 =1928+154 18 27 02 61.4 146.0 -1.1 -26.1 101 139 02 06 22 02 08 21 W51 18 27 02 61.2 150.2 -1.0 -23.0 -19 139 No stop 02 10 21 --- 18 29 02 61.4 151.1 -0.9 -22.3 101 141 02 08 22 02 10 21 J1930+1532 18 29 02 61.6 147.0 -1.0 -25.5 -19 141 No stop 02 12 21 =1928+154 18 31 03 61.8 147.9 -1.0 -24.8 101 143 02 10 22 02 13 01 W51 18 31 43 61.6 152.4 -0.9 -21.3 21 143 02 13 01 02 15 01 --- 18 33 43 61.8 153.4 -0.8 -20.6 120 145 02 13 02 Schedule for YEBES40M (Code Ys ) 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 ---------------------------------------------------------------------------------------- --- Thu 30 May 2013 Day 150 --- 02 15 41 J1930+1532 18 34 23 62.1 149.4 -1.0 -23.7 21 145 02 15 41 02 17 41 =1928+154 18 36 24 62.3 150.4 -0.9 -22.9 120 147 02 15 42 02 17 41 W51 18 36 24 62.0 154.7 -0.8 -19.6 -19 147 No stop 02 19 41 --- 18 38 24 62.2 155.6 -0.8 -18.9 101 149 02 17 42 02 19 41 J1930+1532 18 38 24 62.5 151.4 -0.9 -22.2 -19 149 No stop 02 21 41 =1928+154 18 40 24 62.7 152.3 -0.9 -21.5 101 151 02 19 42 02 21 41 W51 18 40 24 62.3 156.6 -0.7 -18.2 -19 151 No stop 02 23 41 --- 18 42 25 62.5 157.6 -0.7 -17.4 101 153 02 21 42 02 23 41 J1930+1532 18 42 25 62.9 153.3 -0.8 -20.8 -19 153 No stop 02 25 41 =1928+154 18 44 25 63.0 154.3 -0.8 -20.0 101 155 02 23 42 02 26 21 W51 18 45 05 62.6 159.0 -0.7 -16.4 21 155 02 26 21 02 28 21 --- 18 47 05 62.8 160.0 -0.6 -15.6 120 157 02 26 22 02 29 01 J1930+1532 18 47 46 63.3 156.0 -0.7 -18.7 21 157 02 29 01 02 31 01 =1928+154 18 49 46 63.4 157.0 -0.7 -17.9 120 159 02 29 02 02 35 08 J2202+4216 18 53 53 54.9 71.1 -3.2 -76.6 145 159 02 35 08 02 43 08 =BLLAC 19 01 54 56.4 71.6 -3.0 -77.4 480 166 02 35 09 02 47 37 W51 19 06 24 63.7 170.2 -0.3 -7.7 157 166 02 47 37 02 52 37 --- 19 11 25 63.9 172.9 -0.2 -5.6 300 171 02 47 38 02 53 17 J1930+1532 19 12 05 64.7 169.0 -0.3 -8.7 21 171 02 53 17 02 55 17 =1928+154 19 14 06 64.8 170.1 -0.3 -7.8 120 173 02 53 18 02 55 17 W51 19 14 06 63.9 174.3 -0.2 -4.4 -19 173 No stop 02 57 17 --- 19 16 06 64.0 175.5 -0.1 -3.6 101 175 02 55 18 02 57 17 J1930+1532 19 16 06 64.8 171.2 -0.3 -6.9 -19 175 No stop 02 59 17 =1928+154 19 18 06 64.9 172.4 -0.2 -6.0 101 177 02 57 18 02 59 17 W51 19 18 06 64.0 176.6 -0.1 -2.7 -19 177 No stop 03 01 17 --- 19 20 07 64.0 177.7 -0.1 -1.8 101 179 02 59 18 03 01 17 J1930+1532 19 20 07 64.9 173.5 -0.2 -5.1 -19 179 No stop 03 03 17 =1928+154 19 22 07 65.0 174.6 -0.2 -4.2 101 181 03 01 18 03 03 57 W51 19 22 47 64.0 179.1 0.0 -0.7 21 181 03 03 57 03 05 57 --- 19 24 47 64.0 180.2 0.0 0.2 120 183 03 03 58 Schedule for YEBES40M (Code Ys ) 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 ---------------------------------------------------------------------------------------- --- Thu 30 May 2013 Day 150 --- 03 06 37 J1930+1532 19 25 27 65.0 176.5 -0.1 -2.7 21 183 03 06 37 03 08 37 =1928+154 19 27 28 65.0 177.7 -0.1 -1.8 120 185 03 06 38 03 08 37 W51 19 27 28 64.0 181.7 0.1 1.4 -19 185 No stop 03 10 37 --- 19 29 28 64.0 182.8 0.1 2.2 101 187 03 08 38 03 10 37 J1930+1532 19 29 28 65.0 178.8 0.0 -0.9 -19 187 No stop 03 12 37 =1928+154 19 31 28 65.0 180.0 0.0 0.0 101 189 03 10 38 03 12 37 W51 19 31 28 64.0 183.9 0.1 3.1 -19 189 No stop 03 14 37 --- 19 33 29 63.9 185.0 0.2 4.0 101 191 03 12 38 03 14 37 J1930+1532 19 33 29 65.0 181.1 0.0 0.9 -19 191 No stop 03 16 37 =1928+154 19 35 29 65.0 182.3 0.1 1.8 101 193 03 14 38 03 17 17 W51 19 36 09 63.9 186.5 0.2 5.1 21 193 03 17 17 03 19 17 --- 19 38 09 63.8 187.6 0.2 6.0 120 195 03 17 18 03 19 57 J1930+1532 19 38 50 65.0 184.2 0.1 3.3 21 195 03 19 57 03 21 57 =1928+154 19 40 50 65.0 185.3 0.2 4.2 120 196 03 19 58 03 21 57 W51 19 40 50 63.8 189.1 0.3 7.1 -19 196 No stop 03 23 57 --- 19 42 50 63.7 190.1 0.3 8.0 101 198 03 21 58 03 23 57 J1930+1532 19 42 50 64.9 186.4 0.2 5.1 -19 198 No stop 03 25 57 =1928+154 19 44 51 64.9 187.6 0.2 6.0 101 200 03 23 58 03 25 57 W51 19 44 51 63.6 191.2 0.3 8.8 -19 200 No stop 03 27 57 --- 19 46 51 63.6 192.3 0.4 9.6 101 202 03 25 58 03 27 57 J1930+1532 19 46 51 64.8 188.7 0.3 6.9 -19 202 No stop 03 29 57 =1928+154 19 48 51 64.8 189.8 0.3 7.7 101 204 03 27 58 03 30 37 W51 19 49 31 63.4 193.7 0.4 10.7 21 204 03 30 37 03 32 37 --- 19 51 32 63.3 194.8 0.5 11.6 120 206 03 30 38 03 33 17 J1930+1532 19 52 12 64.6 191.7 0.3 9.2 22 206 03 33 17 03 35 17 =1928+154 19 54 12 64.6 192.8 0.4 10.1 120 208 03 33 18 03 39 52 J2202+4216 19 58 48 66.7 75.2 -2.1 -83.9 142 208 03 39 52 03 47 52 =BLLAC 20 06 49 68.2 75.6 -1.9 -84.9 480 216 03 39 53 03 52 47 W51 20 11 45 62.0 205.1 0.8 19.4 152 216 03 52 47 03 57 47 --- 20 16 45 61.6 207.5 0.9 21.3 300 221 03 52 48 Schedule for YEBES40M (Code Ys ) 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 ---------------------------------------------------------------------------------------- --- Thu 30 May 2013 Day 150 --- 03 58 27 J1930+1532 20 17 25 63.1 205.1 0.8 19.5 22 221 03 58 27 04 00 27 =1928+154 20 19 26 63.0 206.1 0.8 20.3 120 223 03 58 28 04 00 27 W51 20 19 26 61.4 208.7 0.9 22.2 -18 223 No stop 04 02 27 --- 20 21 26 61.2 209.7 1.0 22.9 102 225 04 00 28 04 02 27 J1930+1532 20 21 26 62.8 207.1 0.8 21.1 -18 225 No stop 04 04 27 =1928+154 20 23 26 62.6 208.1 0.9 21.8 102 226 04 02 28 04 04 27 W51 20 23 26 61.0 210.6 1.0 23.6 -18 226 No stop 04 06 27 --- 20 25 27 60.8 211.5 1.0 24.2 102 228 04 04 28 04 06 27 J1930+1532 20 25 27 62.4 209.0 0.9 22.5 -17 228 No stop 04 08 27 =1928+154 20 27 27 62.2 210.0 0.9 23.2 103 230 04 06 28 04 09 07 W51 20 28 07 60.5 212.7 1.1 25.1 23 230 04 09 07 04 11 07 --- 20 30 08 60.3 213.6 1.1 25.8 120 232 04 09 08 04 11 47 J1930+1532 20 30 48 61.9 211.6 1.0 24.4 23 232 04 11 47 04 13 47 =1928+154 20 32 48 61.7 212.5 1.0 25.1 120 234 04 11 48 04 13 47 W51 20 32 48 60.0 214.8 1.1 26.6 -17 234 No stop 04 15 47 --- 20 34 48 59.8 215.6 1.2 27.2 103 236 04 13 48 04 15 47 J1930+1532 20 34 48 61.5 213.4 1.1 25.8 -17 236 No stop 04 17 47 =1928+154 20 36 49 61.3 214.3 1.1 26.4 103 238 04 15 48 04 17 47 W51 20 36 49 59.6 216.5 1.2 27.8 -17 238 No stop 04 19 47 --- 20 38 49 59.4 217.3 1.2 28.4 103 240 04 17 48 04 19 47 J1930+1532 20 38 49 61.1 215.2 1.1 27.1 -17 240 No stop 04 21 47 =1928+154 20 40 49 60.9 216.1 1.2 27.7 103 242 04 19 48 04 22 27 W51 20 41 29 59.1 218.4 1.3 29.2 23 242 04 22 27 04 24 27 --- 20 43 30 58.8 219.3 1.3 29.8 120 244 04 22 28 04 25 07 J1930+1532 20 44 10 60.5 217.5 1.2 28.7 23 244 04 25 07 04 27 07 =1928+154 20 46 10 60.2 218.4 1.2 29.3 120 246 04 25 08 04 27 07 W51 20 46 10 58.5 220.3 1.4 30.5 -17 246 No stop 04 29 07 --- 20 48 10 58.2 221.1 1.4 31.1 103 248 04 27 08 04 29 07 J1930+1532 20 48 10 60.0 219.2 1.3 29.9 -17 248 No stop 04 31 07 =1928+154 20 50 11 59.8 220.1 1.3 30.5 103 250 04 29 08 Schedule for YEBES40M (Code Ys ) 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 ---------------------------------------------------------------------------------------- --- Thu 30 May 2013 Day 150 --- 04 31 07 W51 20 50 11 58.0 221.9 1.4 31.6 -17 250 No stop 04 33 07 --- 20 52 11 57.7 222.7 1.5 32.2 103 252 04 31 08 04 33 07 J1930+1532 20 52 11 59.5 220.9 1.3 31.1 -17 252 No stop 04 35 07 =1928+154 20 54 11 59.3 221.7 1.4 31.7 103 254 04 33 08 04 35 47 W51 20 54 52 57.4 223.7 1.5 32.9 23 254 04 35 47 04 37 47 --- 20 56 52 57.1 224.5 1.5 33.4 120 255 04 35 48 04 38 27 J1930+1532 20 57 32 58.8 223.0 1.4 32.6 23 255 04 38 27 04 40 27 =1928+154 20 59 32 58.6 223.8 1.5 33.1 120 257 04 38 28 04 44 51 J2202+4216 21 03 57 78.7 75.9 -1.0 -94.3 101 257 04 44 51 04 52 51 =BLLAC 21 11 58 80.2 75.1 -0.9 -96.4 480 265 04 44 52 04 57 21 W51 21 16 30 54.3 231.3 1.9 37.8 100 265 04 57 21 05 00 51 --- 21 20 00 53.8 232.5 1.9 38.5 210 269 04 57 22 05 01 31 J1930+1532 21 20 41 55.6 231.4 1.8 38.1 23 269 05 01 31 05 03 31 =1928+154 21 22 41 55.3 232.1 1.9 38.5 120 270 05 01 32 05 03 31 W51 21 22 41 53.4 233.3 2.0 39.0 -17 270 No stop 05 05 31 --- 21 24 41 53.1 233.9 2.0 39.4 103 272 05 03 32 05 05 31 J1930+1532 21 24 41 55.0 232.8 1.9 38.9 -17 272 No stop 05 07 31 =1928+154 21 26 42 54.7 233.4 1.9 39.3 103 274 05 05 32 05 07 31 W51 21 26 42 52.8 234.6 2.0 39.8 -17 274 No stop 05 09 31 --- 21 28 42 52.5 235.2 2.1 40.1 103 276 05 07 32 05 09 31 J1930+1532 21 28 42 54.4 234.1 2.0 39.7 -17 276 No stop 05 11 31 =1928+154 21 30 42 54.1 234.7 2.0 40.1 103 278 05 09 32 05 12 11 W51 21 31 22 52.1 236.0 2.1 40.6 23 278 05 12 11 05 14 11 --- 21 33 23 51.8 236.6 2.2 40.9 120 280 05 12 12 05 14 51 J1930+1532 21 34 03 53.6 235.7 2.0 40.7 23 280 05 14 51 05 16 51 =1928+154 21 36 03 53.2 236.3 2.1 41.1 120 282 05 14 52 05 16 51 W51 21 36 03 51.3 237.4 2.2 41.4 -17 282 No stop 05 18 51 --- 21 38 03 51.0 237.9 2.2 41.7 103 284 05 16 52 05 18 51 J1930+1532 21 38 03 52.9 236.9 2.1 41.4 -17 284 No stop 05 20 51 =1928+154 21 40 04 52.6 237.5 2.1 41.7 103 286 05 18 52 Schedule for YEBES40M (Code Ys ) 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 ---------------------------------------------------------------------------------------- --- Thu 30 May 2013 Day 150 --- 05 20 51 W51 21 40 04 50.7 238.5 2.3 42.0 -17 286 No stop 05 22 51 --- 21 42 04 50.4 239.1 2.3 42.3 103 288 05 20 52 05 22 51 J1930+1532 21 42 04 52.3 238.1 2.2 42.1 -17 288 No stop 05 24 51 =1928+154 21 44 04 52.0 238.7 2.2 42.4 103 290 05 22 52 05 25 31 W51 21 44 45 49.9 239.8 2.3 42.8 23 290 05 25 31 05 27 31 --- 21 46 45 49.6 240.4 2.4 43.0 120 292 05 25 32 05 28 11 J1930+1532 21 47 25 51.4 239.7 2.3 42.9 23 292 05 28 11 05 30 11 =1928+154 21 49 25 51.1 240.2 2.3 43.2 120 294 05 28 12 05 30 11 W51 21 49 25 49.1 241.1 2.4 43.4 -17 294 No stop 05 32 11 --- 21 51 26 48.8 241.6 2.5 43.7 103 296 05 30 12 05 32 11 J1930+1532 21 51 26 50.8 240.8 2.3 43.5 -17 296 No stop 05 34 11 =1928+154 21 53 26 50.4 241.3 2.4 43.8 103 298 05 32 12 05 34 11 W51 21 53 26 48.5 242.2 2.5 44.0 -17 298 No stop 05 36 11 --- 21 55 26 48.1 242.7 2.5 44.2 103 299 05 34 12 05 36 11 J1930+1532 21 55 26 50.1 241.9 2.4 44.1 -17 299 No stop 05 38 11 =1928+154 21 57 27 49.7 242.4 2.4 44.4 103 301 05 36 12 05 38 51 W51 21 58 07 47.7 243.4 2.6 44.6 23 301 05 38 51 05 40 51 --- 22 00 07 47.3 243.9 2.6 44.8 120 303 05 38 52 05 41 31 J1930+1532 22 00 47 49.2 243.3 2.5 44.8 23 303 05 41 31 05 43 31 =1928+154 22 02 47 48.8 243.8 2.5 45.1 120 305 05 41 32 05 46 36 J2202+4216 22 05 53 88.1 345.3 0.0 D 164.9 61 305 05 46 36 05 54 36 =BLLAC 22 13 54 87.3 313.3 0.2 131.5 0 313 05 46 37 05 57 53 W51 22 17 12 44.4 248.0 2.9 46.7 116 313 05 57 53 06 01 23 --- 22 20 42 43.8 248.8 2.9 47.1 210 316 05 57 54 06 02 03 J1930+1532 22 21 22 45.6 248.4 2.8 47.2 23 316 06 02 03 06 04 03 =1928+154 22 23 23 45.3 248.9 2.9 47.4 120 318 06 02 04 06 04 03 W51 22 23 23 43.3 249.4 3.0 47.3 -17 318 No stop 06 06 33 --- 22 25 53 42.8 250.0 3.0 47.6 133 321 06 04 04 06 06 33 J1930+1532 22 25 53 44.8 249.4 2.9 47.6 -17 321 No stop 06 08 33 =1928+154 22 27 53 44.5 249.9 2.9 47.8 103 323 06 06 34 Schedule for YEBES40M (Code Ys ) 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 ---------------------------------------------------------------------------------------- --- Thu 30 May 2013 Day 150 --- 06 08 33 W51 22 27 53 42.5 250.4 3.1 47.7 -17 323 No stop 06 11 03 --- 22 30 24 42.0 251.0 3.1 47.9 133 325 06 08 34 06 11 03 J1930+1532 22 30 24 44.0 250.4 3.0 48.0 -17 325 No stop 06 13 03 =1928+154 22 32 24 43.6 250.9 3.0 48.2 103 327 06 11 04 06 13 43 W51 22 33 04 41.5 251.6 3.1 48.2 23 327 06 13 43 06 16 13 --- 22 35 35 41.1 252.1 3.2 48.4 150 329 06 13 44 06 16 53 J1930+1532 22 36 15 43.0 251.7 3.1 48.5 23 329 06 16 53 06 18 53 =1928+154 22 38 15 42.6 252.2 3.1 48.7 120 331 06 16 54 06 18 53 W51 22 38 15 40.6 252.7 3.2 48.6 -17 331 No stop 06 21 23 --- 22 40 45 40.2 253.2 3.3 48.7 133 334 06 18 54 06 21 23 J1930+1532 22 40 45 42.1 252.7 3.2 48.9 -17 334 No stop 06 23 23 =1928+154 22 42 46 41.8 253.1 3.2 49.0 103 336 06 21 24 06 23 23 W51 22 42 46 39.8 253.6 3.3 48.9 -17 336 No stop 06 25 53 --- 22 45 16 39.3 254.1 3.3 49.1 133 338 06 23 24 06 25 53 J1930+1532 22 45 16 41.3 253.7 3.2 49.2 -17 338 No stop 06 27 53 =1928+154 22 47 16 41.0 254.1 3.3 49.4 103 340 06 25 54 06 28 33 W51 22 47 57 38.8 254.7 3.4 49.2 23 340 06 28 33 06 31 03 --- 22 50 27 38.4 255.2 3.4 49.4 150 343 06 28 34 06 31 43 J1930+1532 22 51 07 40.2 254.9 3.3 49.6 23 343 06 31 43 06 33 43 =1928+154 22 53 07 39.9 255.3 3.4 49.7 120 344 06 31 44 06 33 43 W51 22 53 07 37.9 255.7 3.5 49.6 -17 344 No stop 06 36 13 --- 22 55 38 37.4 256.2 3.5 49.7 133 347 06 33 44 06 36 13 J1930+1532 22 55 38 39.4 255.8 3.4 49.9 -17 347 No stop 06 38 13 =1928+154 22 57 38 39.0 256.2 3.4 50.0 103 349 06 36 14 06 38 13 W51 22 57 38 37.1 256.6 3.6 49.8 -17 349 No stop 06 40 43 --- 23 00 09 36.6 257.1 3.6 49.9 133 351 06 38 14 06 40 43 J1930+1532 23 00 09 38.6 256.7 3.5 50.2 -17 351 No stop 06 42 43 =1928+154 23 02 09 38.2 257.1 3.5 50.3 103 353 06 40 44 06 43 23 W51 23 02 49 36.1 257.6 3.6 50.1 23 353 06 43 23 06 45 53 --- 23 05 19 35.6 258.1 3.7 50.2 150 356 06 43 24 Schedule for YEBES40M (Code Ys ) 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 ---------------------------------------------------------------------------------------- --- Thu 30 May 2013 Day 150 --- 06 46 33 J1930+1532 23 05 59 37.5 257.8 3.6 50.5 23 356 06 46 33 06 48 33 =1928+154 23 08 00 37.1 258.2 3.6 50.6 120 358 06 46 34 06 51 41 J2202+4216 23 11 08 77.2 283.7 1.1 92.4 132 358 06 51 41 06 59 41 =BLLAC 23 19 09 75.7 283.5 1.3 90.9 480 365 06 51 42 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess213.M128 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: 128 Format: MARK5B Bits per sample: 2 Sample rate: 4.000 Number of channels: 16 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 5910.00 5910.00 5910.00 5910.00 5910.00 5910.00 5910.00 5910.00 5910.00 5910.00 5910.00 5910.00 5910.00 5910.00 5910.00 5910.00 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= L L U U L L U U L L U U L L U U 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: 8 Based on FREQ, BW, and/or DOPPLER in schedule. Used pcal sets: 1 LO sum= 6667.58 6667.58 6667.58 6667.58 6671.58 6671.58 6671.58 6671.58 6675.58 6675.58 6675.58 6675.58 6679.58 6679.58 6679.58 6679.58 BBC fr= 757.58 757.58 757.58 757.58 761.58 761.58 761.58 761.58 765.58 765.58 765.58 765.58 769.58 769.58 769.58 769.58 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: 8 The following pulse cal sets were used with this setup: Pulse cal detection set: 1 PCAL = OFF PCALXB1= S1 S2 S3 S4 S5 S6 S7 S8 PCALXB2= M1 M2 M3 M4 M5 M6 M7 M8 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, 10, 12, 14, 16, 18, 20, 22, 24, 26, 28, 30, 32 barrel=roll_off SOURCES USED IN RECORDING SCANS -- How do O-type forming stars accrete their mass? 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) * W51 19 21 24.339697 * 19 23 42.000000 19 24 20.631048 0.00 14 24 56.76822 * 14 30 50.00000 14 32 28.19778 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 2.708 scan and 68.260 baseline hours in setup: sess213.M128 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 * J1331+3030 13 28 49.657778 * 13 31 08.288070 13 31 46.894376 0.20 3C286 30 45 58.64061 * 30 30 32.95925 30 26 28.42257 0.19 1328+307 /aps3/sched10.2/catalogs/sources.vlba J1331+30 rfc_2012b Petrov, 2012, unpublished 542 observations Doppler based on other sources. 0.183 scan and 5.133 baseline hours in setup: sess213.M128 Frequency sets (dups not shown): 1 2 3 4 5 6 7 8 * J1930+1532 19 28 36.092068 * 19 30 52.766993 19 31 31.111973 0.15 1928+154 15 26 11.96581 * 15 32 34.42720 15 34 20.15178 0.16 J1930+15 /aps3/sched10.2/catalogs/sources.vlba rfc_2012b Petrov, 2012, unpublished 139 observations Doppler based on other sources. 2.333 scan and 57.968 baseline hours in setup: sess213.M128 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 17.790226 0.14 BLLAC 42 02 08.59073 * 42 16 39.97987 42 20 26.42851 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. 1.067 scan and 27.999 baseline hours in setup: sess213.M128 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) W51 123.7 J1331+3030 112.7 J1930+1532 121.7 J2202+4216 80.0 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