COVER INFORMATION Station: IRBENE16 (Code Ib ) Experiment: A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel Exp. Code: EM117N Schedule Version: 2.00 Processed by SCHED version: 11.40 Release 11.4. March 14, 2015 PI: L. Moscadelli Address: Osservatorio Astrofisico di Arcetri Via E.Fermi 5 I-50125, Firenze Italy Phone: +39 055 2752220 EMAIL: mosca@arcetri.astro.it Fax: +39 055 220039 Phone during observation: +39 055 2752220 Observing mode: Polarization observations of 1 source at 6.7 GHz (128 Mb/s Notes: phase-cal OFF source = G25.65+1.05 Schedule for IRBENE16 (Code Ib ) Page 2 A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel 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 3 Mar 2018 Day 62 --- Next scan frequencies: 6665.52 6665.52 6665.52 6665.52 6669.52 6669.52 6669.52 6669.52 6673.52 6673.52 6673.52 6673.52 6677.52 6677.52 6677.52 6677.52 Next BBC frequencies: 565.52 565.52 565.52 565.52 569.52 569.52 569.52 569.52 573.52 573.52 573.52 573.52 577.52 577.52 577.52 577.52 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 02 30 00 J2202+4216 14 40 42 25.4-310.1 -7.4 -33.7 0 0 02 30 00 02 38 00 =VR422201 14 48 43 26.2-308.7 -7.2 -34.5 480 8 02 30 01 02 45 35 J1331+3030 14 56 19 59.2-142.7 1.4 22.1 370 8 02 45 35 02 50 35 =3C286 15 01 20 58.8-140.8 1.5 23.2 300 13 02 45 36 02 51 05 J1331+3030 15 01 50 58.7-140.6 1.5 23.3 27 13 02 51 05 02 59 05 =3C286 15 09 51 58.0-137.6 1.6 24.8 480 20 02 51 06 03 03 31 3C345 15 14 18 67.1-228.7 -1.5 -31.6 217 20 03 03 31 03 13 31 --- 15 24 20 68.1-224.3 -1.3 -29.2 600 30 03 03 32 03 18 11 J2202+4216 15 29 01 30.6-301.9 -6.6 -38.0 238 30 03 18 11 03 26 11 =VR422201 15 37 02 31.5-300.5 -6.4 -38.7 480 38 03 18 12 03 30 06 J1821-0502 15 40 58 19.5-223.1 -2.7 -21.6 194 38 03 30 06 03 35 06 =1818-050 15 45 58 19.9-221.9 -2.6 -21.1 300 43 03 30 07 03 35 06 G25.65+1.05 15 45 58 17.8-224.7 -2.8 -22.3 -4 43 No stop 03 37 06 --- 15 47 59 18.0-224.2 -2.8 -22.1 116 44 03 35 07 03 37 51 J1821-0502 15 48 44 20.2-221.2 -2.6 -20.8 41 44 03 37 51 03 40 41 =1818-050 15 51 34 20.4-220.5 -2.5 -20.5 170 47 03 37 52 03 40 41 G25.65+1.05 15 51 34 18.4-223.4 -2.7 -21.7 -4 47 No stop 03 42 41 --- 15 53 35 18.6-222.9 -2.7 -21.5 116 49 03 40 42 03 42 41 J1821-0502 15 53 35 20.6-220.0 -2.5 -20.2 -4 49 No stop 03 45 41 =1818-050 15 56 35 20.9-219.2 -2.4 -19.9 176 52 03 42 42 03 45 41 G25.65+1.05 15 56 35 18.8-222.1 -2.6 -21.2 -4 52 No stop 03 47 41 --- 15 58 35 19.0-221.6 -2.6 -21.0 116 54 03 45 42 03 48 26 J1821-0502 15 59 21 21.1-218.5 -2.4 -19.6 41 54 03 48 26 03 51 16 =1818-050 16 02 11 21.3-217.8 -2.3 -19.3 170 57 03 48 27 03 51 16 G25.65+1.05 16 02 11 19.3-220.8 -2.6 -20.6 -4 57 No stop 03 53 16 --- 16 04 11 19.5-220.3 -2.5 -20.4 116 59 03 51 17 Schedule for IRBENE16 (Code Ib ) Page 3 A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel 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 3 Mar 2018 Day 62 --- 03 53 16 J1821-0502 16 04 11 21.5-217.3 -2.3 -19.1 -4 59 No stop 03 56 16 =1818-050 16 07 12 21.7-216.6 -2.2 -18.7 176 62 03 53 17 03 56 16 G25.65+1.05 16 07 12 19.8-219.5 -2.5 -20.1 -4 62 No stop 03 58 16 --- 16 09 12 19.9-219.0 -2.4 -19.9 116 63 03 56 17 03 58 16 J1821-0502 16 09 12 21.9-216.0 -2.2 -18.5 -4 63 No stop 04 01 16 =1818-050 16 12 13 22.1-215.3 -2.2 -18.1 176 66 03 58 17 04 01 16 G25.65+1.05 16 12 13 20.2-218.3 -2.4 -19.5 -4 66 No stop 04 03 16 --- 16 14 13 20.3-217.8 -2.4 -19.3 116 68 04 01 17 04 04 01 J1821-0502 16 14 58 22.3-214.6 -2.1 -17.8 40 68 04 04 01 04 06 51 =1818-050 16 17 49 22.6-213.8 -2.1 -17.5 170 71 04 04 02 04 06 51 G25.65+1.05 16 17 49 20.6-216.9 -2.3 -18.9 -5 71 No stop 04 08 51 --- 16 19 49 20.8-216.4 -2.3 -18.7 115 73 04 06 52 04 08 51 J1821-0502 16 19 49 22.7-213.3 -2.0 -17.2 -5 73 No stop 04 11 51 =1818-050 16 22 49 22.9-212.5 -2.0 -16.8 175 76 04 08 52 04 15 51 J2202+4216 16 26 50 37.5-292.1 -5.6 -42.3 197 76 04 15 51 04 23 51 =VR422201 16 34 51 38.5-290.7 -5.5 -42.8 480 84 04 15 52 04 28 01 J1821-0502 16 39 02 24.0-208.3 -1.7 -14.8 206 84 04 28 01 04 31 01 =1818-050 16 42 03 24.2-207.5 -1.7 -14.4 180 86 04 28 02 04 31 01 G25.65+1.05 16 42 03 22.4-210.7 -1.9 -16.0 -5 86 No stop 04 33 01 --- 16 44 03 22.6-210.2 -1.9 -15.7 115 88 04 31 02 04 33 01 J1821-0502 16 44 03 24.3-207.0 -1.6 -14.1 -5 88 No stop 04 36 01 =1818-050 16 47 03 24.5-206.2 -1.6 -13.7 175 91 04 33 02 04 36 01 G25.65+1.05 16 47 03 22.8-209.4 -1.8 -15.3 -5 91 No stop 04 38 01 --- 16 49 04 22.9-208.9 -1.8 -15.1 115 93 04 36 02 04 38 01 J1821-0502 16 49 04 24.6-205.7 -1.6 -13.5 -5 93 No stop 04 41 01 =1818-050 16 52 04 24.8-204.9 -1.5 -13.1 175 96 04 38 02 04 41 01 G25.65+1.05 16 52 04 23.1-208.1 -1.7 -14.7 -5 96 No stop 04 43 01 --- 16 54 05 23.2-207.6 -1.7 -14.4 115 98 04 41 02 04 43 46 J1821-0502 16 54 50 25.0-204.1 -1.5 -12.7 40 98 04 43 46 04 46 36 =1818-050 16 57 40 25.1-203.4 -1.4 -12.3 170 101 04 43 47 Schedule for IRBENE16 (Code Ib ) Page 4 A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel 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 3 Mar 2018 Day 62 --- 04 46 36 G25.65+1.05 16 57 40 23.4-206.6 -1.6 -14.0 -5 101 No stop 04 48 36 --- 16 59 40 23.6-206.1 -1.6 -13.7 115 103 04 46 37 04 48 36 J1821-0502 16 59 40 25.2-202.8 -1.4 -12.1 -5 103 No stop 04 51 36 =1818-050 17 02 41 25.4-202.0 -1.3 -11.6 175 106 04 48 37 04 51 36 G25.65+1.05 17 02 41 23.7-205.3 -1.5 -13.3 -5 106 No stop 04 53 36 --- 17 04 41 23.9-204.8 -1.5 -13.1 115 108 04 51 37 04 53 36 J1821-0502 17 04 41 25.5-201.5 -1.3 -11.4 -5 108 No stop 04 56 36 =1818-050 17 07 42 25.6-200.6 -1.2 -10.9 175 110 04 53 37 04 56 36 G25.65+1.05 17 07 42 24.0-204.0 -1.5 -12.7 -5 110 No stop 04 58 36 --- 17 09 42 24.1-203.4 -1.4 -12.4 115 112 04 56 37 04 59 21 J1821-0502 17 10 27 25.7-199.9 -1.2 -10.6 40 112 04 59 21 05 02 11 =1818-050 17 13 18 25.9-199.1 -1.1 -10.2 170 115 04 59 22 05 02 11 G25.65+1.05 17 13 18 24.3-202.5 -1.4 -11.9 -5 115 No stop 05 04 11 --- 17 15 18 24.4-201.9 -1.3 -11.6 115 117 05 02 12 05 04 11 J1821-0502 17 15 18 26.0-198.6 -1.1 -9.9 -5 117 No stop 05 07 11 =1818-050 17 18 19 26.1-197.8 -1.1 -9.5 175 120 05 04 12 05 11 26 J2202+4216 17 22 34 44.7-282.2 -4.7 -45.2 209 120 05 11 26 05 19 26 =VR422201 17 30 36 45.7-280.7 -4.5 -45.5 480 128 05 11 27 05 23 46 J1821-0502 17 34 56 26.7-193.2 -0.8 -7.1 214 128 05 23 46 05 26 46 =1818-050 17 37 57 26.8-192.3 -0.7 -6.6 180 131 05 23 47 05 26 46 G25.65+1.05 17 37 57 25.4-195.8 -1.0 -8.5 -5 131 No stop 05 28 46 --- 17 39 57 25.5-195.3 -0.9 -8.2 115 133 05 26 47 05 28 46 J1821-0502 17 39 57 26.8-191.8 -0.7 -6.3 -5 133 No stop 05 31 46 =1818-050 17 42 58 26.9-191.0 -0.7 -5.9 175 135 05 28 47 05 31 46 G25.65+1.05 17 42 58 25.6-194.5 -0.9 -7.7 -5 135 No stop 05 33 46 --- 17 44 58 25.6-193.9 -0.8 -7.4 115 137 05 31 47 05 33 46 J1821-0502 17 44 58 27.0-190.4 -0.6 -5.6 -5 137 No stop 05 36 46 =1818-050 17 47 58 27.0-189.6 -0.6 -5.1 175 140 05 33 47 05 36 46 G25.65+1.05 17 47 58 25.7-193.1 -0.8 -7.0 -5 140 No stop 05 38 46 --- 17 49 59 25.8-192.5 -0.8 -6.7 115 142 05 36 47 Schedule for IRBENE16 (Code Ib ) Page 5 A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel 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 3 Mar 2018 Day 62 --- 05 39 31 J1821-0502 17 50 44 27.1-188.8 -0.5 -4.7 40 142 05 39 31 05 42 21 =1818-050 17 53 34 27.1-188.0 -0.5 -4.3 170 145 05 39 32 05 42 21 G25.65+1.05 17 53 34 25.9-191.5 -0.7 -6.2 -5 145 No stop 05 44 21 --- 17 55 35 26.0-191.0 -0.7 -5.9 115 147 05 42 22 05 44 21 J1821-0502 17 55 35 27.2-187.4 -0.4 -4.0 -5 147 No stop 05 47 21 =1818-050 17 58 35 27.2-186.6 -0.4 -3.5 175 150 05 44 22 05 47 21 G25.65+1.05 17 58 35 26.0-190.2 -0.6 -5.5 -5 150 No stop 05 49 21 --- 18 00 35 26.1-189.6 -0.6 -5.2 115 152 05 47 22 05 49 21 J1821-0502 18 00 35 27.3-186.0 -0.4 -3.2 -5 152 No stop 05 52 21 =1818-050 18 03 36 27.3-185.2 -0.3 -2.8 175 155 05 49 22 05 52 21 G25.65+1.05 18 03 36 26.1-188.8 -0.5 -4.7 -5 155 No stop 05 54 21 --- 18 05 36 26.2-188.2 -0.5 -4.4 115 157 05 52 22 05 55 06 J1821-0502 18 06 21 27.3-184.4 -0.3 -2.4 40 157 05 55 06 05 57 56 =1818-050 18 09 12 27.4-183.6 -0.2 -2.0 170 159 05 55 07 05 57 56 G25.65+1.05 18 09 12 26.2-187.2 -0.4 -3.9 -5 159 No stop 05 59 56 --- 18 11 12 26.3-186.7 -0.4 -3.6 115 161 05 57 57 05 59 56 J1821-0502 18 11 12 27.4-183.1 -0.2 -1.7 -5 161 No stop 06 02 56 =1818-050 18 14 13 27.4-182.2 -0.1 -1.2 175 164 05 59 57 06 07 26 J2202+4216 18 18 43 52.1-271.3 -3.7 -46.5 222 164 06 07 26 06 15 26 =VR422201 18 26 45 53.2-269.7 -3.6 -46.6 480 172 06 07 27 06 20 06 J1821-0502 18 31 25 27.4-177.4 0.2 1.4 231 172 06 20 06 06 23 06 =1818-050 18 34 26 27.4-176.6 0.2 1.9 180 175 06 20 07 06 23 06 G25.65+1.05 18 34 26 26.5-180.2 -0.0 -0.1 -5 175 No stop 06 25 06 --- 18 36 26 26.5-179.7 0.0 0.2 115 177 06 23 07 06 25 06 J1821-0502 18 36 26 27.3-176.0 0.2 2.2 -5 177 No stop 06 28 06 =1818-050 18 39 27 27.3-175.1 0.3 2.6 175 180 06 25 07 06 28 06 G25.65+1.05 18 39 27 26.5-178.8 0.1 0.6 -5 180 No stop 06 30 06 --- 18 41 27 26.4-178.3 0.1 0.9 115 181 06 28 07 06 30 06 J1821-0502 18 41 27 27.3-174.6 0.3 2.9 -5 181 No stop 06 33 06 =1818-050 18 44 28 27.2-173.7 0.4 3.4 175 184 06 30 07 Schedule for IRBENE16 (Code Ib ) Page 6 A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel 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 3 Mar 2018 Day 62 --- 06 33 06 G25.65+1.05 18 44 28 26.4-177.5 0.2 1.4 -5 184 No stop 06 35 06 --- 18 46 28 26.4-176.9 0.2 1.7 115 186 06 33 07 06 35 51 J1821-0502 18 47 13 27.2-173.0 0.4 3.8 40 186 06 35 51 06 38 41 =1818-050 18 50 04 27.2-172.2 0.5 4.2 170 189 06 35 52 06 38 41 G25.65+1.05 18 50 04 26.4-175.9 0.2 2.2 -5 189 No stop 06 40 41 --- 18 52 04 26.4-175.3 0.3 2.5 115 191 06 38 42 06 40 41 J1821-0502 18 52 04 27.1-171.6 0.5 4.5 -5 191 No stop 06 43 41 =1818-050 18 55 04 27.1-170.8 0.5 4.9 175 194 06 40 42 06 43 41 G25.65+1.05 18 55 04 26.3-174.5 0.3 3.0 -5 194 No stop 06 45 41 --- 18 57 05 26.3-174.0 0.4 3.3 115 196 06 43 42 06 45 41 J1821-0502 18 57 05 27.0-170.2 0.6 5.2 -5 196 No stop 06 48 41 =1818-050 19 00 05 26.9-169.4 0.6 5.7 175 199 06 45 42 06 48 41 G25.65+1.05 19 00 05 26.3-173.1 0.4 3.7 -5 199 No stop 06 50 41 --- 19 02 06 26.2-172.6 0.4 4.0 115 201 06 48 42 06 51 26 J1821-0502 19 02 51 26.9-168.6 0.7 6.1 40 201 06 51 26 06 54 16 =1818-050 19 05 41 26.8-167.8 0.7 6.5 170 203 06 51 27 06 54 16 G25.65+1.05 19 05 41 26.2-171.6 0.5 4.5 -5 203 No stop 06 56 16 --- 19 07 41 26.1-171.0 0.5 4.8 115 205 06 54 17 06 56 16 J1821-0502 19 07 41 26.7-167.3 0.8 6.8 -5 205 No stop 06 59 16 =1818-050 19 10 42 26.6-166.4 0.8 7.3 175 208 06 56 17 07 04 06 J2202+4216 19 15 33 59.7-258.3 -2.8 -45.3 241 208 07 04 06 07 12 06 =VR422201 19 23 34 60.7-256.2 -2.7 -44.8 480 216 07 04 07 07 17 06 J1821-0502 19 28 35 26.0-161.5 1.1 9.8 250 216 07 17 06 07 20 06 =1818-050 19 31 35 25.9-160.7 1.2 10.2 180 219 07 17 07 07 20 06 G25.65+1.05 19 31 35 25.4-164.5 0.9 8.3 -5 219 No stop 07 22 06 --- 19 33 36 25.4-163.9 1.0 8.6 115 221 07 20 07 07 22 06 J1821-0502 19 33 36 25.8-160.2 1.2 10.5 -5 221 No stop 07 25 06 =1818-050 19 36 36 25.6-159.4 1.2 10.9 175 224 07 22 07 07 25 06 G25.65+1.05 19 36 36 25.3-163.1 1.0 9.0 -5 224 No stop 07 27 06 --- 19 38 36 25.2-162.6 1.1 9.3 115 226 07 25 07 Schedule for IRBENE16 (Code Ib ) Page 7 A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel 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 3 Mar 2018 Day 62 --- 07 27 06 J1821-0502 19 38 36 25.5-158.8 1.3 11.2 -5 226 No stop 07 30 06 =1818-050 19 41 37 25.4-158.0 1.3 11.6 175 228 07 27 07 07 30 06 G25.65+1.05 19 41 37 25.0-161.7 1.1 9.7 -5 228 No stop 07 32 06 --- 19 43 37 25.0-161.2 1.1 10.0 115 230 07 30 07 07 32 51 J1821-0502 19 44 22 25.2-157.3 1.4 12.0 40 230 07 32 51 07 35 41 =1818-050 19 47 13 25.1-156.5 1.4 12.4 170 233 07 32 52 07 35 41 G25.65+1.05 19 47 13 24.8-160.2 1.2 10.5 -5 233 No stop 07 37 41 --- 19 49 13 24.7-159.7 1.2 10.8 115 235 07 35 42 07 37 41 J1821-0502 19 49 13 25.0-155.9 1.5 12.7 -5 235 No stop 07 40 41 =1818-050 19 52 14 24.8-155.1 1.5 13.1 175 238 07 37 42 07 40 41 G25.65+1.05 19 52 14 24.6-158.9 1.3 11.2 -5 238 No stop 07 42 41 --- 19 54 14 24.5-158.3 1.3 11.5 115 240 07 40 42 07 42 41 J1821-0502 19 54 14 24.7-154.6 1.5 13.4 -5 240 No stop 07 45 41 =1818-050 19 57 15 24.5-153.8 1.6 13.8 175 243 07 42 42 07 45 41 G25.65+1.05 19 57 15 24.3-157.5 1.4 11.9 -5 243 No stop 07 47 41 --- 19 59 15 24.2-157.0 1.4 12.2 115 245 07 45 42 07 48 26 J1821-0502 20 00 00 24.4-153.1 1.6 14.1 40 245 07 48 26 07 51 16 =1818-050 20 02 50 24.2-152.3 1.7 14.5 170 247 07 48 27 07 51 16 G25.65+1.05 20 02 50 24.0-156.1 1.5 12.6 -5 247 No stop 07 53 16 --- 20 04 51 23.9-155.5 1.5 12.9 115 249 07 51 17 07 53 16 J1821-0502 20 04 51 24.1-151.8 1.7 14.7 -5 249 No stop 07 56 16 =1818-050 20 07 51 23.9-151.0 1.8 15.1 175 252 07 53 17 08 01 26 J2202+4216 20 13 02 66.9-240.8 -1.8 -39.3 261 252 08 01 26 08 09 26 =VR422201 20 21 03 67.8-237.8 -1.7 -37.9 480 260 08 01 27 08 14 26 J1821-0502 20 26 04 22.6-146.3 2.1 17.4 252 260 08 14 26 08 17 26 =1818-050 20 29 05 22.4-145.5 2.1 17.8 180 263 08 14 27 08 17 26 G25.65+1.05 20 29 05 22.4-149.2 1.9 16.0 -5 263 No stop 08 19 26 --- 20 31 05 22.3-148.7 1.9 16.3 115 265 08 17 27 08 19 26 J1821-0502 20 31 05 22.2-145.0 2.1 18.0 -5 265 No stop 08 22 26 =1818-050 20 34 06 22.0-144.2 2.2 18.4 175 268 08 19 27 Schedule for IRBENE16 (Code Ib ) Page 8 A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel 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 3 Mar 2018 Day 62 --- 08 22 26 G25.65+1.05 20 34 06 22.1-147.9 2.0 16.7 -5 268 No stop 08 24 26 --- 20 36 06 21.9-147.4 2.0 16.9 115 270 08 22 27 08 24 26 J1821-0502 20 36 06 21.8-143.7 2.2 18.6 -5 270 No stop 08 27 26 =1818-050 20 39 06 21.6-142.9 2.3 18.9 175 273 08 24 27 08 27 26 G25.65+1.05 20 39 06 21.7-146.6 2.1 17.3 -5 273 No stop 08 29 26 --- 20 41 07 21.5-146.1 2.1 17.5 115 275 08 27 27 08 30 11 J1821-0502 20 41 52 21.4-142.2 2.3 19.3 40 275 08 30 11 08 33 01 =1818-050 20 44 42 21.1-141.5 2.4 19.6 170 277 08 30 12 08 33 01 G25.65+1.05 20 44 42 21.3-145.2 2.2 17.9 -5 277 No stop 08 35 01 --- 20 46 43 21.1-144.7 2.2 18.2 115 279 08 33 02 08 35 01 J1821-0502 20 46 43 20.9-141.0 2.4 19.8 -5 279 No stop 08 38 01 =1818-050 20 49 43 20.7-140.3 2.5 20.1 175 282 08 35 02 08 38 01 G25.65+1.05 20 49 43 20.9-143.9 2.2 18.5 -5 282 No stop 08 40 01 --- 20 51 43 20.7-143.4 2.3 18.8 115 284 08 38 02 08 40 01 J1821-0502 20 51 43 20.5-139.8 2.5 20.4 -5 284 No stop 08 43 01 =1818-050 20 54 44 20.3-139.0 2.5 20.7 175 287 08 40 02 08 43 01 G25.65+1.05 20 54 44 20.5-142.6 2.3 19.1 -5 287 No stop 08 45 01 --- 20 56 44 20.3-142.1 2.4 19.3 115 289 08 43 02 08 45 46 J1821-0502 20 57 29 20.0-138.3 2.6 21.0 40 289 08 45 46 08 48 36 =1818-050 21 00 20 19.8-137.6 2.6 21.3 170 292 08 45 47 08 48 36 G25.65+1.05 21 00 20 20.0-141.2 2.4 19.7 -5 292 No stop 08 50 36 --- 21 02 20 19.8-140.7 2.5 20.0 115 294 08 48 37 08 50 36 J1821-0502 21 02 20 19.6-137.1 2.7 21.5 -5 294 No stop 08 53 36 =1818-050 21 05 21 19.3-136.4 2.7 21.8 175 296 08 50 37 08 59 01 J2202+4216 21 10 47 72.7-214.4 -0.9 -24.2 282 296 08 59 01 09 07 01 =VR422201 21 18 48 73.2-209.7 -0.7 -21.1 480 304 08 59 02 09 12 36 J1821-0502 21 24 24 17.5-131.8 3.0 23.7 294 304 09 12 36 09 15 36 =1818-050 21 27 24 17.2-131.1 3.1 24.0 180 307 09 12 37 09 15 36 G25.65+1.05 21 27 24 17.6-134.6 2.9 22.6 -5 307 No stop 09 17 36 --- 21 29 25 17.4-134.1 2.9 22.8 115 309 09 15 37 Schedule for IRBENE16 (Code Ib ) Page 9 A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel 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 3 Mar 2018 Day 62 --- 09 17 36 J1821-0502 21 29 25 17.0-130.6 3.1 24.1 -5 309 No stop 09 20 36 =1818-050 21 32 25 16.7-129.9 3.2 24.4 175 312 09 17 37 09 20 36 G25.65+1.05 21 32 25 17.1-133.4 3.0 23.1 -5 312 No stop 09 22 36 --- 21 34 25 16.9-132.9 3.0 23.3 115 314 09 20 37 09 22 36 J1821-0502 21 34 25 16.4-129.4 3.2 24.6 -5 314 No stop 09 25 36 =1818-050 21 37 26 16.1-128.7 3.3 24.9 175 317 09 22 37 09 25 36 G25.65+1.05 21 37 26 16.6-132.2 3.0 23.5 -5 317 No stop 09 27 36 --- 21 39 26 16.4-131.7 3.1 23.7 115 319 09 25 37 09 28 21 J1821-0502 21 40 11 15.8-128.0 3.3 25.1 40 319 09 28 21 09 31 11 =1818-050 21 43 02 15.5-127.4 3.3 25.3 170 321 09 28 22 09 31 11 G25.65+1.05 21 43 02 16.0-130.9 3.1 24.1 -5 321 No stop 09 33 11 --- 21 45 02 15.8-130.4 3.2 24.2 115 323 09 31 12 09 33 11 J1821-0502 21 45 02 15.3-126.9 3.4 25.5 -5 323 No stop 09 36 11 =1818-050 21 48 03 15.0-126.2 3.4 25.8 175 326 09 33 12 09 36 11 G25.65+1.05 21 48 03 15.5-129.7 3.2 24.5 -5 326 No stop 09 38 11 --- 21 50 03 15.3-129.2 3.2 24.7 115 328 09 36 12 09 38 11 J1821-0502 21 50 03 14.8-125.7 3.5 25.9 -5 328 No stop 09 41 11 =1818-050 21 53 04 14.5-125.1 3.5 26.2 175 331 09 38 12 09 41 11 G25.65+1.05 21 53 04 15.0-128.5 3.3 25.0 -5 331 No stop 09 43 11 --- 21 55 04 14.8-128.1 3.3 25.1 115 333 09 41 12 09 43 56 J1821-0502 21 55 49 14.2-124.4 3.6 26.4 40 333 09 43 56 09 46 46 =1818-050 21 58 39 13.8-123.8 3.6 26.6 170 336 09 43 57 09 46 46 G25.65+1.05 21 58 39 14.4-127.2 3.4 25.4 -5 336 No stop 09 48 46 --- 22 00 40 14.2-126.8 3.4 25.6 115 338 09 46 47 09 48 46 J1821-0502 22 00 40 13.6-123.3 3.6 26.7 -5 338 No stop 09 51 46 =1818-050 22 03 40 13.3-122.6 3.7 27.0 175 341 09 48 47 09 57 11 J2202+4216 22 09 06 74.8-176.0 0.1 2.9 291 341 09 57 11 10 05 11 =VR422201 22 17 07 74.7-170.4 0.2 6.9 480 348 09 57 12 10 10 41 J1821-0502 22 22 38 11.1-118.3 4.0 28.3 296 348 10 10 41 10 13 41 =1818-050 22 25 39 10.7-117.7 4.1 28.5 180 351 10 10 42 Schedule for IRBENE16 (Code Ib ) Page 10 A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel 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 3 Mar 2018 Day 62 --- 10 13 41 G25.65+1.05 22 25 39 11.4-121.1 3.8 27.5 -5 351 No stop 10 15 41 --- 22 27 39 11.2-120.6 3.9 27.7 115 353 10 13 42 10 15 41 J1821-0502 22 27 39 10.5-117.2 4.1 28.6 -5 353 No stop 10 18 41 =1818-050 22 30 40 10.1-116.6 4.1 28.8 175 356 10 15 42 10 18 41 G25.65+1.05 22 30 40 10.8-119.9 3.9 27.9 -5 356 No stop 10 20 41 --- 22 32 40 10.6-119.5 4.0 28.0 115 358 10 18 42 10 20 41 J1821-0502 22 32 40 9.9-116.1 4.2 28.9 -5 358 No stop 10 23 41 =1818-050 22 35 41 9.5-115.4 4.2 29.1 175 361 10 20 42 10 23 41 G25.65+1.05 22 35 41 10.3-118.8 4.0 28.2 -5 361 No stop 10 25 41 --- 22 37 41 10.0-118.4 4.0 28.3 115 363 10 23 42 10 26 26 J1821-0502 22 38 26 9.2-114.8 4.3 29.3 40 363 10 26 26 10 29 16 =1818-050 22 41 16 8.8-114.2 4.3 29.4 170 366 10 26 27 10 29 16 G25.65+1.05 22 41 16 9.6-117.6 4.1 28.6 -5 366 No stop 10 31 16 --- 22 43 17 9.4-117.1 4.1 28.7 115 367 10 29 17 10 31 16 J1821-0502 22 43 17 8.6-113.8 4.4 29.5 -5 367 No stop 10 34 16 =1818-050 22 46 17 8.2-113.1 4.4 29.7 175 370 10 31 17 10 34 16 G25.65+1.05 22 46 17 9.0-116.5 4.2 28.9 -5 370 No stop 10 36 16 --- 22 48 18 8.8-116.0 4.2 29.0 115 372 10 34 17 10 36 16 J1821-0502 22 48 18 8.0-112.7 4.4 29.8 -5 372 No stop 10 39 16 =1818-050 22 51 18 7.6-112.0 4.5 29.9 175 375 10 36 17 10 39 16 G25.65+1.05 22 51 18 8.4-115.4 4.3 29.2 -5 375 No stop 10 41 16 --- 22 53 18 8.1-114.9 4.3 29.3 115 377 10 39 17 10 42 01 J1821-0502 22 54 04 7.3-111.4 4.5 30.1 40 377 10 42 01 10 44 51 =1818-050 22 56 54 6.9-110.8 4.6 30.2 170 380 10 42 02 10 44 51 G25.65+1.05 22 56 54 7.7-114.1 4.4 29.5 -5 380 No stop 10 46 51 --- 22 58 54 7.5-113.7 4.4 29.6 115 382 10 44 52 10 46 51 J1821-0502 22 58 54 6.7-110.4 4.6 30.3 -5 382 No stop 10 49 51 =1818-050 23 01 55 6.3-109.7 4.7 30.5 175 385 10 46 52 10 54 31 J2202+4216 23 06 36 71.8-139.9 1.1 27.9 244 385 10 54 31 11 02 41 =VR422201 23 14 47 71.1-135.7 1.2 30.4 490 393 10 54 32 Schedule for IRBENE16 (Code Ib ) Page 11 A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel 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 3 Mar 2018 Day 62 --- 11 07 26 J1821-0502 23 19 33 4.0-105.9 5.0 31.2 249 393 11 07 26 11 10 26 =1818-050 23 22 33 3.6-105.3 5.0 31.3 180 395 11 07 27 11 10 26 G25.65+1.05 23 22 33 4.5-108.6 4.8 30.7 -5 395 No stop 11 12 26 --- 23 24 34 4.3-108.2 4.8 30.8 115 397 11 10 27 11 12 51 J1821-0502 23 24 59 3.3-104.8 5.0 31.4 20 397 11 12 51 11 17 51 =1818-050 23 29 59 2.7-103.7 5.1 D 31.5 0 402 11 12 52 11 22 32 J2202+4216 23 34 41 69.1-126.7 1.5 35.6 245 402 11 22 32 11 30 00 =VR422201 23 42 10 68.3-123.6 1.6 37.2 448 409 11 22 33 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess118.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: 10 Station: IRBENE16 Total bit rate: 128 Format: VDIF 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= 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 6100.00 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 9 1 9 2 10 2 10 3 11 3 11 4 12 4 12 BBC SB= L L U U L L U U L L U U L L U U IF = A1 C1 A1 C1 A1 C1 A1 C1 A1 C1 A1 C1 A1 C1 A1 C1 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= 6665.52 6665.52 6665.52 6665.52 6669.52 6669.52 6669.52 6669.52 6673.52 6673.52 6673.52 6673.52 6677.52 6677.52 6677.52 6677.52 BBC fr= 565.52 565.52 565.52 565.52 569.52 569.52 569.52 569.52 573.52 573.52 573.52 573.52 577.52 577.52 577.52 577.52 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 Track assignments are: track1= 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 12, 13, 14, 15, 16 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) * G25.65+1.05 18 31 40.145161 * 18 34 20.900000 18 35 17.910134 0.00 -06 02 05.96283 *-05 59 42.10000 -05 58 47.97160 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 41.60 41.60 41.60 41.60 41.60 41.60 41.60 41.60 41.60 41.60 3C286 13 28 49.657758 * 13 31 08.288051 13 31 58.829871 0.18 * J1331+3030 30 45 58.64059 * 30 30 32.95924 30 24 50.75498 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. * 3C345 16 41 17.606228 * 16 42 58.809966 16 43 34.977099 0.76 J1642+3948 39 54 10.81496 * 39 48 36.99402 39 46 26.14472 0.52 1641+399 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc J1642+39 GSFC 2015a astro solution, unpublished 53430 observations. Doppler based on other sources. 1818-050 18 18 32.138835 * 18 21 11.809558 18 22 08.506188 0.32 * J1821-0502 -05 03 46.86946 *-05 02 20.08539 -05 01 46.63323 0.52 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc GSFC 2015a astro solution, unpublished 107 observations. Doppler based on other sources. VR422201 22 00 39.362505 * 22 02 43.291372 22 03 26.389058 0.00 * J2202+4216 42 02 08.59077 * 42 16 39.97990 42 21 48.66404 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 G25.65+1.05sess118.M128 1 2 3 4 5 6 7 8 9 10 1.900 66.385 J1331+3030 sess118.M128 1 2 3 4 5 6 7 8 9 10 0.217 9.750 3C345 sess118.M128 1 2 3 4 5 6 7 8 9 10 0.167 7.424 J1821-0502 sess118.M128 1 2 3 4 5 6 7 8 9 10 3.319 135.126 J2202+4216 sess118.M128 1 2 3 4 5 6 7 8 9 10 1.461 52.704 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) G25.65+1.05 64.7 J1331+3030 136.5 3C345 96.7 J1821-0502 68.1 J2202+4216 50.6 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