COVER INFORMATION Station: IRBENE (Code Ir ) Experiment: A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel Exp. Code: EM117F Schedule Version: 1.00 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 = G016.58-0.05 Schedule for IRBENE (Code Ir ) 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 ---------------------------------------------------------------------------------------- --- Sun 5 Jun 2016 Day 157 --- Next scan frequencies: 6664.68 6664.68 6664.68 6664.68 6668.68 6668.68 6668.68 6668.68 6672.68 6672.68 6672.68 6672.68 6676.67 6676.67 6676.67 6676.67 Next BBC frequencies: 564.68 564.68 564.68 564.68 568.68 568.68 568.68 568.68 572.68 572.68 572.68 572.68 576.67 576.67 576.67 576.67 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 20 00 00 J1331+3030 14 26 07 61.3-155.1 0.9 15.2 0 0 20 00 00 20 10 00 =3C286 14 36 08 60.7-150.8 1.1 17.6 600 10 20 00 01 20 10 30 J1331+3030 14 36 38 60.7-150.6 1.1 17.8 27 10 20 10 30 20 20 30 =3C286 14 46 40 60.0-146.5 1.2 20.1 600 19 20 10 31 20 24 55 3C345 14 51 06 64.6-237.7 -1.9 -36.2 216 19 20 24 55 20 34 55 --- 15 01 07 65.8-234.0 -1.7 -34.4 600 29 20 24 56 20 35 25 3C345 15 01 38 65.8-233.8 -1.7 -34.3 27 29 20 35 25 20 45 25 --- 15 11 39 66.9-229.8 -1.5 -32.2 600 38 20 35 26 20 50 25 J1331+3030 15 16 40 57.4-135.0 1.7 26.1 250 38 20 50 25 21 00 25 =3C286 15 26 42 56.4-131.5 1.9 27.8 600 48 20 50 26 21 04 40 1822-173 15 30 57 6.8-221.8 -2.9 -22.0 206 48 21 04 40 21 09 40 --- 15 35 58 7.2-220.7 -2.8 -21.5 300 53 21 04 41 21 09 40 G016.58-0.05 15 35 58 10.2-220.7 -2.8 -21.2 -4 53 No stop 21 11 40 --- 15 37 59 10.4-220.2 -2.7 -21.0 116 55 21 09 41 21 12 20 1822-173 15 38 39 7.5-220.1 -2.8 -21.2 36 55 21 12 20 21 15 20 --- 15 41 39 7.7-219.4 -2.7 -20.9 180 58 21 12 21 21 15 20 G016.58-0.05 15 41 39 10.7-219.4 -2.7 -20.6 -4 58 No stop 21 17 20 --- 15 43 39 10.9-218.9 -2.6 -20.4 116 60 21 15 21 21 17 20 1822-173 15 43 39 7.9-219.0 -2.7 -20.7 -4 60 No stop 21 20 20 --- 15 46 40 8.1-218.3 -2.7 -20.4 176 62 21 17 21 21 20 20 G016.58-0.05 15 46 40 11.1-218.2 -2.6 -20.1 -4 62 No stop 21 22 20 --- 15 48 40 11.3-217.8 -2.6 -19.8 116 64 21 20 21 21 23 00 1822-173 15 49 20 8.4-217.7 -2.6 -20.1 36 64 21 23 00 21 26 00 --- 15 52 21 8.6-217.0 -2.6 -19.8 180 67 21 23 01 21 26 00 G016.58-0.05 15 52 21 11.6-216.9 -2.5 -19.4 -4 67 No stop 21 28 00 --- 15 54 21 11.7-216.5 -2.5 -19.2 116 69 21 26 01 Schedule for IRBENE (Code Ir ) 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 ---------------------------------------------------------------------------------------- --- Sun 5 Jun 2016 Day 157 --- 21 28 00 1822-173 15 54 21 8.8-216.5 -2.5 -19.6 -4 69 No stop 21 31 00 --- 15 57 22 9.0-215.9 -2.5 -19.2 176 72 21 28 01 21 31 00 G016.58-0.05 15 57 22 12.0-215.8 -2.4 -18.9 -4 72 No stop 21 33 00 --- 15 59 22 12.1-215.3 -2.4 -18.7 116 74 21 31 01 21 33 00 1822-173 15 59 22 9.2-215.4 -2.5 -19.0 -4 74 No stop 21 36 00 --- 16 02 23 9.4-214.7 -2.4 -18.7 176 77 21 33 01 21 36 00 G016.58-0.05 16 02 23 12.4-214.6 -2.3 -18.3 -4 77 No stop 21 38 00 --- 16 04 23 12.5-214.1 -2.3 -18.1 116 79 21 36 01 21 38 40 1822-173 16 05 03 9.6-214.1 -2.4 -18.4 36 79 21 38 40 21 41 40 --- 16 08 03 9.8-213.4 -2.3 -18.0 180 82 21 38 41 21 41 40 G016.58-0.05 16 08 03 12.8-213.2 -2.2 -17.7 -4 82 No stop 21 43 40 --- 16 10 04 12.9-212.8 -2.2 -17.5 116 84 21 41 41 21 43 40 1822-173 16 10 04 10.0-212.9 -2.3 -17.8 -4 84 No stop 21 46 40 --- 16 13 04 10.2-212.3 -2.2 -17.5 176 87 21 43 41 21 51 35 J1331+3030 16 18 00 50.7-115.5 2.8 34.2 244 87 21 51 35 22 01 35 =3C286 16 28 02 49.5-112.8 2.9 35.0 600 96 21 51 36 22 10 25 J2202+4216 16 36 53 38.8-290.3 -5.4 -42.9 438 96 22 10 25 22 20 25 =VR422201 16 46 55 40.0-288.6 -5.3 -43.5 600 106 22 10 26 22 29 45 1822-173 16 56 16 12.8-202.1 -1.5 -12.2 515 106 22 29 45 22 32 45 --- 16 59 17 13.0-201.4 -1.5 -11.8 180 109 22 29 46 22 32 45 G016.58-0.05 16 59 17 15.9-200.9 -1.4 -11.4 -4 109 No stop 22 34 45 --- 17 01 17 16.0-200.4 -1.3 -11.1 116 111 22 32 46 22 34 45 1822-173 17 01 17 13.1-200.9 -1.4 -11.6 -4 111 No stop 22 37 45 --- 17 04 18 13.2-200.2 -1.4 -11.2 176 113 22 34 46 22 37 45 G016.58-0.05 17 04 18 16.2-199.6 -1.3 -10.7 -4 113 No stop 22 39 45 --- 17 06 18 16.2-199.1 -1.3 -10.5 116 115 22 37 46 22 39 45 1822-173 17 06 18 13.3-199.7 -1.3 -10.9 -4 115 No stop 22 42 45 --- 17 09 18 13.4-198.9 -1.3 -10.5 176 118 22 39 46 22 42 45 G016.58-0.05 17 09 18 16.4-198.4 -1.2 -10.1 -4 118 No stop 22 44 45 --- 17 11 19 16.5-197.9 -1.2 -9.8 116 120 22 42 46 Schedule for IRBENE (Code Ir ) 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 ---------------------------------------------------------------------------------------- --- Sun 5 Jun 2016 Day 157 --- 22 45 25 1822-173 17 11 59 13.6-198.3 -1.2 -10.2 36 120 22 45 25 22 48 25 --- 17 14 59 13.7-197.6 -1.2 -9.8 180 123 22 45 26 22 48 25 G016.58-0.05 17 14 59 16.6-197.0 -1.1 -9.3 -4 123 No stop 22 50 25 --- 17 17 00 16.7-196.5 -1.1 -9.0 116 125 22 48 26 22 50 25 1822-173 17 17 00 13.8-197.1 -1.2 -9.5 -4 125 No stop 22 53 25 --- 17 20 00 13.9-196.4 -1.1 -9.1 176 128 22 50 26 22 58 50 J1331+3030 17 25 26 42.1 -98.5 3.9 38.0 274 128 22 58 50 23 06 50 =3C286 17 33 27 41.0 -96.7 4.0 38.2 480 136 22 58 51 23 12 10 1822-173 17 38 48 14.5-191.8 -0.8 -6.6 269 136 23 12 10 23 15 10 --- 17 41 49 14.6-191.0 -0.7 -6.2 180 138 23 12 11 23 15 10 G016.58-0.05 17 41 49 17.4-190.2 -0.7 -5.6 -4 138 No stop 23 17 10 --- 17 43 49 17.5-189.7 -0.6 -5.4 116 140 23 15 11 23 17 10 1822-173 17 43 49 14.6-190.5 -0.7 -5.9 -4 140 No stop 23 20 10 --- 17 46 50 14.7-189.8 -0.7 -5.5 176 143 23 17 11 23 20 10 G016.58-0.05 17 46 50 17.6-189.0 -0.6 -4.9 -4 143 No stop 23 22 10 --- 17 48 50 17.6-188.4 -0.6 -4.7 116 145 23 20 11 23 22 10 1822-173 17 48 50 14.7-189.3 -0.6 -5.2 -4 145 No stop 23 25 10 --- 17 51 50 14.8-188.6 -0.6 -4.8 176 148 23 22 11 23 25 10 G016.58-0.05 17 51 50 17.7-187.7 -0.5 -4.3 -4 148 No stop 23 27 10 --- 17 53 51 17.7-187.2 -0.5 -4.0 116 150 23 25 11 23 27 50 1822-173 17 54 31 14.8-187.9 -0.5 -4.4 36 150 23 27 50 23 30 50 --- 17 57 31 14.9-187.2 -0.5 -4.0 180 153 23 27 51 23 30 50 G016.58-0.05 17 57 31 17.7-186.2 -0.4 -3.5 -4 153 No stop 23 32 50 --- 17 59 32 17.8-185.7 -0.4 -3.2 116 155 23 30 51 23 32 50 1822-173 17 59 32 14.9-186.7 -0.5 -3.7 -4 155 No stop 23 35 50 --- 18 02 32 15.0-185.9 -0.4 -3.3 176 158 23 32 51 23 35 50 G016.58-0.05 18 02 32 17.8-185.0 -0.3 -2.8 -4 158 No stop 23 37 50 --- 18 04 33 17.8-184.5 -0.3 -2.5 116 160 23 35 51 23 37 50 1822-173 18 04 33 15.0-185.4 -0.4 -3.1 -4 160 No stop 23 40 50 --- 18 07 33 15.0-184.7 -0.3 -2.6 176 162 23 37 51 Schedule for IRBENE (Code Ir ) 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 ---------------------------------------------------------------------------------------- --- Sun 5 Jun 2016 Day 157 --- 23 40 50 G016.58-0.05 18 07 33 17.9-183.7 -0.2 -2.1 -4 162 No stop 23 42 50 --- 18 09 33 17.9-183.2 -0.2 -1.8 116 164 23 40 51 23 43 30 1822-173 18 10 13 15.1-184.0 -0.3 -2.3 36 164 23 43 30 23 46 30 --- 18 13 14 15.1-183.3 -0.2 -1.9 180 167 23 43 31 23 46 30 G016.58-0.05 18 13 14 17.9-182.3 -0.1 -1.3 -4 167 No stop 23 48 30 --- 18 15 14 17.9-181.7 -0.1 -1.0 116 169 23 46 31 23 48 30 1822-173 18 15 14 15.1-182.8 -0.2 -1.6 -4 169 No stop 23 51 30 --- 18 18 15 15.1-182.1 -0.1 -1.2 176 172 23 48 31 23 51 30 G016.58-0.05 18 18 15 17.9-181.0 -0.1 -0.5 -4 172 No stop 23 53 30 --- 18 20 15 17.9-180.5 -0.0 -0.3 116 174 23 51 31 23 53 30 1822-173 18 20 15 15.1-181.6 -0.1 -0.9 -4 174 No stop 23 56 30 --- 18 23 16 15.1-180.8 -0.1 -0.5 176 177 23 53 31 23 56 30 G016.58-0.05 18 23 16 17.9-179.7 0.0 0.2 -4 177 No stop 23 58 30 --- 18 25 16 17.9-179.2 0.1 0.4 116 179 23 56 31 --- Start: Sun 5 Jun 2016 Day 157 -- Stop: Mon 6 Jun 2016 Day 158 --- 23 59 10 1822-173 18 25 56 15.1-180.2 -0.0 -0.1 36 179 23 59 10 00 02 10 --- 18 28 57 15.1-179.4 0.0 0.3 180 182 23 59 11 00 07 50 J1331+3030 18 34 37 32.8 -83.7 5.0 38.2 290 182 00 07 50 00 15 50 =3C286 18 42 39 31.7 -82.1 5.2 38.0 480 189 00 07 51 00 21 15 1822-173 18 48 05 15.0-174.7 0.4 3.0 275 189 00 21 15 00 24 15 --- 18 51 05 15.0-173.9 0.4 3.4 180 192 00 21 16 00 24 15 G016.58-0.05 18 51 05 17.7-172.6 0.5 4.1 -4 192 No stop 00 26 15 --- 18 53 05 17.6-172.1 0.5 4.4 116 194 00 24 16 00 26 15 1822-173 18 53 05 14.9-173.5 0.4 3.7 -4 194 No stop 00 29 15 --- 18 56 06 14.9-172.7 0.5 4.1 176 197 00 26 16 00 29 15 G016.58-0.05 18 56 06 17.6-171.4 0.6 4.8 -4 197 No stop 00 31 15 --- 18 58 06 17.5-170.9 0.6 5.0 116 199 00 29 16 00 31 15 1822-173 18 58 06 14.9-172.2 0.5 4.4 -4 199 No stop 00 34 15 --- 19 01 07 14.8-171.5 0.6 4.8 176 202 00 31 16 Schedule for IRBENE (Code Ir ) 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 ---------------------------------------------------------------------------------------- --- Mon 6 Jun 2016 Day 158 --- 00 34 15 G016.58-0.05 19 01 07 17.5-170.1 0.7 5.5 -4 202 No stop 00 36 15 --- 19 03 07 17.4-169.6 0.7 5.7 116 204 00 34 16 00 36 55 1822-173 19 03 47 14.7-170.8 0.6 5.1 36 204 00 36 55 00 39 55 --- 19 06 48 14.7-170.1 0.7 5.6 180 207 00 36 56 00 39 55 G016.58-0.05 19 06 48 17.3-168.7 0.7 6.3 -4 207 No stop 00 41 55 --- 19 08 48 17.3-168.2 0.8 6.5 116 209 00 39 56 00 41 55 1822-173 19 08 48 14.6-169.6 0.7 5.8 -4 209 No stop 00 44 55 --- 19 11 49 14.6-168.8 0.8 6.2 176 212 00 41 56 00 44 55 G016.58-0.05 19 11 49 17.2-167.4 0.8 6.9 -4 212 No stop 00 46 55 --- 19 13 49 17.1-166.9 0.9 7.2 116 213 00 44 56 00 46 55 1822-173 19 13 49 14.5-168.4 0.8 6.5 -4 213 No stop 00 49 55 --- 19 16 49 14.4-167.6 0.8 6.9 176 216 00 46 56 00 49 55 G016.58-0.05 19 16 49 17.0-166.1 0.9 7.6 -4 216 No stop 00 51 55 --- 19 18 50 17.0-165.6 0.9 7.9 116 218 00 49 56 00 52 35 1822-173 19 19 30 14.3-167.0 0.9 7.3 36 218 00 52 35 00 55 35 --- 19 22 30 14.2-166.2 0.9 7.7 180 221 00 52 36 00 55 35 G016.58-0.05 19 22 30 16.9-164.7 1.0 8.4 -4 221 No stop 00 57 35 --- 19 24 31 16.8-164.2 1.0 8.7 116 223 00 55 36 00 57 35 1822-173 19 24 31 14.2-165.7 1.0 8.0 -4 223 No stop 01 00 35 --- 19 27 31 14.1-165.0 1.0 8.4 176 226 00 57 36 01 00 35 G016.58-0.05 19 27 31 16.7-163.5 1.1 9.1 -4 226 No stop 01 02 35 --- 19 29 31 16.6-163.0 1.1 9.3 116 228 01 00 36 01 02 35 1822-173 19 29 31 14.0-164.5 1.0 8.6 -4 228 No stop 01 05 35 --- 19 32 32 13.9-163.8 1.1 9.0 176 231 01 02 36 01 11 00 J1331+3030 19 37 58 24.5 -71.3 6.1 36.1 276 231 01 11 00 01 19 00 =3C286 19 45 59 23.5 -69.8 6.2 35.7 480 238 01 11 01 01 24 15 1822-173 19 51 15 13.1-159.3 1.4 11.5 267 238 01 24 15 01 27 15 --- 19 54 16 13.0-158.5 1.5 11.9 180 241 01 24 16 01 27 15 G016.58-0.05 19 54 16 15.4-156.9 1.5 12.6 -4 241 No stop 01 29 15 --- 19 56 16 15.3-156.4 1.6 12.8 116 243 01 27 16 Schedule for IRBENE (Code Ir ) 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 ---------------------------------------------------------------------------------------- --- Mon 6 Jun 2016 Day 158 --- 01 29 15 1822-173 19 56 16 12.9-158.1 1.5 12.1 -4 243 No stop 01 32 15 --- 19 59 16 12.7-157.3 1.5 12.5 176 246 01 29 16 01 32 15 G016.58-0.05 19 59 16 15.2-155.6 1.6 13.2 -4 246 No stop 01 34 15 --- 20 01 17 15.1-155.1 1.7 13.5 116 248 01 32 16 01 34 15 1822-173 20 01 17 12.6-156.9 1.6 12.8 -4 248 No stop 01 37 15 --- 20 04 17 12.4-156.2 1.6 13.1 176 251 01 34 16 01 37 15 G016.58-0.05 20 04 17 14.9-154.4 1.7 13.9 -4 251 No stop 01 39 15 --- 20 06 17 14.8-153.9 1.7 14.1 116 253 01 37 16 01 39 55 1822-173 20 06 58 12.3-155.5 1.7 13.5 36 253 01 39 55 01 42 55 --- 20 09 58 12.1-154.8 1.7 13.8 180 256 01 39 56 01 42 55 G016.58-0.05 20 09 58 14.6-153.0 1.8 14.6 -4 256 No stop 01 44 55 --- 20 11 58 14.4-152.5 1.8 14.8 116 258 01 42 56 01 44 55 1822-173 20 11 58 12.0-154.3 1.8 14.1 -4 258 No stop 01 47 55 --- 20 14 59 11.8-153.6 1.8 14.5 176 261 01 44 56 01 47 55 G016.58-0.05 20 14 59 14.2-151.8 1.9 15.2 -4 261 No stop 01 49 55 --- 20 16 59 14.1-151.3 1.9 15.4 116 262 01 47 56 01 49 55 1822-173 20 16 59 11.7-153.1 1.8 14.7 -4 262 No stop 01 52 55 --- 20 20 00 11.5-152.4 1.9 15.1 176 265 01 49 56 01 52 55 G016.58-0.05 20 20 00 13.9-150.6 2.0 15.8 -4 265 No stop 01 54 55 --- 20 22 00 13.8-150.1 2.0 16.0 116 267 01 52 56 01 55 35 1822-173 20 22 40 11.4-151.8 1.9 15.4 36 267 01 55 35 01 58 35 --- 20 25 41 11.2-151.1 2.0 15.8 180 270 01 55 36 01 58 35 G016.58-0.05 20 25 41 13.5-149.3 2.1 16.5 -4 270 No stop 02 00 35 --- 20 27 41 13.4-148.8 2.1 16.7 116 272 01 58 36 02 00 35 1822-173 20 27 41 11.0-150.6 2.0 16.0 -4 272 No stop 02 03 35 --- 20 30 41 10.8-149.9 2.1 16.4 176 275 02 00 36 02 03 35 G016.58-0.05 20 30 41 13.2-148.1 2.1 17.1 -4 275 No stop 02 05 35 --- 20 32 42 13.0-147.6 2.2 17.3 116 277 02 03 36 02 06 15 1822-173 20 33 22 10.7-149.3 2.1 16.7 36 277 02 06 15 02 09 15 --- 20 36 22 10.4-148.6 2.2 17.0 180 280 02 06 16 Schedule for IRBENE (Code Ir ) 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 ---------------------------------------------------------------------------------------- --- Mon 6 Jun 2016 Day 158 --- 02 14 30 J1331+3030 20 41 38 16.8 -59.2 7.2 32.3 268 280 02 14 30 02 22 30 =3C286 20 49 40 15.9 -57.7 7.3 31.7 480 287 02 14 31 02 27 35 1822-173 20 54 45 9.1-144.4 2.5 19.1 258 287 02 27 35 02 30 35 --- 20 57 46 8.8-143.7 2.5 19.4 180 290 02 27 36 02 30 35 G016.58-0.05 20 57 46 11.1-141.7 2.6 20.1 -4 290 No stop 02 32 35 --- 20 59 46 10.9-141.2 2.6 20.3 116 292 02 30 36 02 32 35 1822-173 20 59 46 8.7-143.2 2.6 19.7 -4 292 No stop 02 35 35 --- 21 02 47 8.4-142.5 2.6 20.0 176 295 02 32 36 02 35 35 G016.58-0.05 21 02 47 10.7-140.5 2.7 20.6 -4 295 No stop 02 37 35 --- 21 04 47 10.5-140.1 2.7 20.8 116 297 02 35 36 02 37 35 1822-173 21 04 47 8.3-142.1 2.6 20.2 -4 297 No stop 02 40 35 --- 21 07 48 8.0-141.4 2.7 20.5 176 300 02 37 36 02 40 35 G016.58-0.05 21 07 48 10.2-139.4 2.8 21.1 -4 300 No stop 02 42 35 --- 21 09 48 10.1-138.9 2.8 21.4 116 302 02 40 36 02 43 16 1822-173 21 10 29 7.8-140.8 2.7 20.8 37 302 02 43 16 02 46 16 --- 21 13 29 7.5-140.1 2.8 21.1 180 305 02 43 17 02 46 16 G016.58-0.05 21 13 29 9.7-138.1 2.9 21.7 -4 305 No stop 02 48 16 --- 21 15 30 9.6-137.6 2.9 21.9 116 307 02 46 17 02 48 16 1822-173 21 15 30 7.4-139.7 2.8 21.3 -4 307 No stop 02 51 16 --- 21 18 30 7.1-139.0 2.9 21.6 176 310 02 48 17 02 51 16 G016.58-0.05 21 18 30 9.3-136.9 2.9 22.2 -4 310 No stop 02 53 16 --- 21 20 31 9.1-136.5 3.0 22.4 116 312 02 51 17 02 53 16 1822-173 21 20 31 6.9-138.6 2.9 21.8 -4 312 No stop 02 56 16 --- 21 23 31 6.7-137.9 2.9 22.1 176 314 02 53 17 02 56 16 G016.58-0.05 21 23 31 8.8-135.8 3.0 22.7 -4 314 No stop 02 58 16 --- 21 25 31 8.6-135.4 3.1 22.9 116 316 02 56 17 02 58 57 1822-173 21 26 13 6.4-137.3 3.0 22.4 37 316 02 58 57 03 01 57 --- 21 29 13 6.1-136.6 3.0 22.7 180 319 02 58 58 03 01 57 G016.58-0.05 21 29 13 8.3-134.5 3.1 23.3 -4 319 No stop 03 03 57 --- 21 31 13 8.1-134.1 3.2 23.5 116 321 03 01 58 Schedule for IRBENE (Code Ir ) 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 ---------------------------------------------------------------------------------------- --- Mon 6 Jun 2016 Day 158 --- 03 03 57 1822-173 21 31 13 6.0-136.2 3.1 22.9 -4 321 No stop 03 06 57 --- 21 34 14 5.7-135.5 3.1 23.2 176 324 03 03 58 03 06 57 G016.58-0.05 21 34 14 7.8-133.4 3.2 23.7 -4 324 No stop 03 08 57 --- 21 36 14 7.6-133.0 3.2 23.9 116 326 03 06 58 03 09 38 1822-173 21 36 55 5.4-134.9 3.2 23.4 37 326 03 09 38 03 12 38 --- 21 39 56 5.1-134.3 3.2 23.7 180 329 03 09 39 03 17 38 J1331+3030 21 44 57 10.0 -47.1 8.2 27.1 254 329 03 17 38 03 25 08 =3C286 21 52 28 9.3 -45.6 8.3 26.4 450 336 03 17 39 03 32 58 G016.58-0.05 22 00 19 5.1-127.6 3.6 26.0 425 336 03 32 58 03 34 58 --- 22 02 19 4.9-127.2 3.7 D 26.2 0 338 03 32 59 04 23 18 3C84 22 50 47 45.5-279.4 -4.5 -45.0 2817 338 04 23 18 04 32 18 --- 22 59 49 46.7-277.7 -4.4 -45.3 540 347 04 23 19 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess216.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: 11 Station: IRBENE 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= 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 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: 11 Based on FREQ, BW, and/or DOPPLER in schedule. Used with PCAL = off LO sum= 6664.68 6664.68 6664.68 6664.68 6668.68 6668.68 6668.68 6668.68 6672.68 6672.68 6672.68 6672.68 6676.67 6676.67 6676.67 6676.67 BBC fr= 564.68 564.68 564.68 564.68 568.68 568.68 568.68 568.68 572.68 572.68 572.68 572.68 576.67 576.67 576.67 576.67 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: 11 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) * G016.58-0.05 18 18 18.082109 * 18 21 09.137000 18 22 06.299153 0.00 -14 33 14.85453 *-14 31 48.68500 -14 31 08.56980 0.00 From catalog imbedded in main SCHED input file. Doppler based on LSR frame and radio definition. Velocities: 62.11 62.11 62.11 62.11 62.11 62.11 62.11 62.11 62.11 62.11 62.11 62.11 62.11 62.11 * 3C84 03 16 29.567263 * 03 19 48.160094 03 20 51.992012 1.30 J0319+4130 41 19 51.91701 * 41 30 42.10413 41 33 57.39012 2.69 0316+413 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc J0319+41 GSFC 2015a astro solution, unpublished 10208 observations. Doppler based on other sources. 3C286 13 28 49.657758 * 13 31 08.288051 13 31 54.114921 0.18 * J1331+3030 30 45 58.64059 * 30 30 32.95924 30 25 41.42465 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 33.434982 0.76 J1642+3948 39 54 10.81496 * 39 48 36.99402 39 46 58.13981 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. * 1822-173 18 22 42.013862 * 18 25 36.532313 18 26 34.824174 0.23 J1825-1718 -17 20 35.28837 *-17 18 49.84725 -17 18 02.96003 0.41 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc GSFC 2015a astro solution, unpublished 76 observations. Doppler based on other sources. VR422201 22 00 39.362505 * 22 02 43.291372 22 03 24.820358 0.00 * J2202+4216 42 02 08.59077 * 42 16 39.97990 42 21 15.85553 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 G016.58-0.0sess216.M128 1 2 3 4 5 6 7 8 9 11 1.833 73.263 3C84 sess216.M128 1 2 3 4 5 6 7 8 11 0.150 6.750 J1331+3030 sess216.M128 1 2 3 4 5 6 7 8 9 11 1.325 61.342 3C345 sess216.M128 1 2 3 4 5 6 7 8 9 11 0.333 18.333 1822-173 sess216.M128 1 2 3 4 5 6 7 8 9 11 3.193 137.396 J2202+4216 sess216.M128 1 3 4 5 6 7 8 11 0.167 6.000 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) G016.58-0.05 158.5 3C84 27.8 J1331+3030 107.4 3C345 117.4 1822-173 158.6 J2202+4216 84.3 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