COVER INFORMATION Station: IRBENE16 (Code Ib ) Experiment: Inclination Dependences of Optical-UV Broad Emission Line Profiles in Qu Exp. Code: EK038A Schedule Version: 3.00 Processed by SCHED version: 11.40 Release 11.4. March 14, 2015 PI: Jun Yi Koay Address: Institute of Astronomy and Astrophysics, Academia Sinica No.1, Sec. 4, Roosevelt Rd, Taipei, 10617 Taiwan Phone: +886909426947 EMAIL: jykoay@asiaa.sinica.edu.tw Fax: Phone during observation: +886909426947 Observing mode: 6cm EVN/MKV Notes: Schedule for IRBENE16 (Code Ib ) Page 2 Inclination Dependences of Optical-UV Broad Emission Line Profiles in Qu 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 ---------------------------------------------------------------------------------------- --- Tue 6 Mar 2018 Day 65 --- Next scan frequencies: 4942.49 4942.49 4942.49 4942.49 4974.49 4974.49 4974.49 4974.49 5006.49 5006.49 5006.49 5006.49 5038.49 5038.49 5038.49 5038.49 Next BBC frequencies: 842.49 842.49 842.49 842.49 874.49 874.49 874.49 874.49 906.49 906.49 906.49 906.49 938.49 938.49 938.49 938.49 Next scan bandwidths: 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 08 00 00 3C454.3 20 23 26 40.0-230.3 -2.5 -25.4 0 0 08 00 00 08 04 40 --- 20 28 06 40.5-228.9 -2.4 -24.9 280 36 08 00 01 08 06 20 J2349+0534 20 29 47 25.2-237.6 -3.3 -27.1 89 36 08 06 20 08 07 50 =2346+052 20 31 17 25.4-237.2 -3.3 -26.9 90 48 08 06 21 08 07 50 2345+061 20 31 17 26.2-237.4 -3.3 -27.1 -3 48 No stop 08 11 20 --- 20 34 47 26.6-236.5 -3.2 -26.8 207 75 08 07 51 08 11 20 J2349+0534 20 34 47 25.8-236.3 -3.3 -26.7 -3 75 No stop 08 12 50 =2346+052 20 36 18 25.9-236.0 -3.2 -26.5 87 86 08 11 21 08 12 50 2345+061 20 36 18 26.8-236.2 -3.2 -26.6 -3 86 No stop 08 16 20 --- 20 39 48 27.2-235.3 -3.2 -26.3 207 113 08 12 51 08 16 20 J2349+0534 20 39 48 26.3-235.1 -3.2 -26.2 -3 113 No stop 08 17 50 =2346+052 20 41 18 26.5-234.7 -3.1 -26.1 87 125 08 16 21 08 19 20 J0009+1513 20 42 49 32.8-244.6 -3.5 -30.2 82 125 08 19 20 08 20 50 =0007+149 20 44 19 33.0-244.3 -3.4 -30.1 90 137 08 19 21 08 20 50 0017+154 20 44 19 32.1-247.2 -3.6 -30.9 -4 137 No stop 08 24 20 --- 20 47 50 32.5-246.3 -3.6 -30.7 206 164 08 20 51 08 24 20 J0009+1513 20 47 50 33.4-243.4 -3.4 -29.8 -4 164 No stop 08 25 50 =0007+149 20 49 20 33.6-243.0 -3.4 -29.7 86 175 08 24 21 08 25 50 0017+154 20 49 20 32.7-246.0 -3.5 -30.6 -4 175 No stop 08 29 20 --- 20 52 50 33.1-245.1 -3.5 -30.4 206 202 08 25 51 08 30 10 J0009+1513 20 53 41 34.1-241.9 -3.3 -29.4 46 202 08 30 10 08 31 40 =0007+149 20 55 11 34.3-241.5 -3.3 -29.3 90 214 08 30 11 08 31 40 0017+154 20 55 11 33.4-244.5 -3.4 -30.2 -4 214 No stop 08 35 10 --- 20 58 41 33.8-243.6 -3.4 -30.0 206 241 08 31 41 08 35 10 J0009+1513 20 58 41 34.7-240.6 -3.2 -29.0 -4 241 No stop 08 36 40 =0007+149 21 00 12 34.9-240.3 -3.2 -28.9 86 252 08 35 11 Schedule for IRBENE16 (Code Ib ) Page 3 Inclination Dependences of Optical-UV Broad Emission Line Profiles in Qu 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 ---------------------------------------------------------------------------------------- --- Tue 6 Mar 2018 Day 65 --- 08 36 40 0017+154 21 00 12 34.0-243.3 -3.4 -29.9 -4 252 No stop 08 40 10 --- 21 03 42 34.4-242.4 -3.3 -29.6 206 280 08 36 41 08 40 10 J0009+1513 21 03 42 35.3-239.4 -3.1 -28.6 -5 280 No stop 08 41 40 =0007+149 21 05 12 35.5-239.0 -3.1 -28.5 85 291 08 40 11 08 43 20 J2349+0534 21 06 53 29.2-228.2 -2.7 -23.7 92 291 08 43 20 08 44 50 =2346+052 21 08 23 29.3-227.8 -2.7 -23.5 90 303 08 43 21 08 44 50 2345+061 21 08 23 30.2-228.0 -2.7 -23.6 -3 303 No stop 08 48 20 --- 21 11 54 30.5-227.0 -2.6 -23.3 207 330 08 44 51 08 48 20 J2349+0534 21 11 54 29.7-226.9 -2.6 -23.2 -3 330 No stop 08 49 50 =2346+052 21 13 24 29.8-226.5 -2.6 -23.0 87 341 08 48 21 08 49 50 2345+061 21 13 24 30.7-226.6 -2.6 -23.1 -3 341 No stop 08 53 20 --- 21 16 54 31.0-225.7 -2.5 -22.7 207 368 08 49 51 08 53 20 J2349+0534 21 16 54 30.1-225.5 -2.6 -22.6 -3 368 No stop 08 54 50 =2346+052 21 18 25 30.3-225.1 -2.5 -22.5 87 380 08 53 21 08 56 20 J0009+1513 21 19 55 37.1-235.1 -2.8 -27.1 82 380 08 56 20 08 57 50 =0007+149 21 21 25 37.3-234.7 -2.8 -27.0 90 392 08 56 21 08 57 50 0017+154 21 21 25 36.5-237.8 -3.0 -28.1 -5 392 No stop 09 01 20 --- 21 24 56 36.9-236.9 -2.9 -27.8 205 419 08 57 51 09 01 20 J0009+1513 21 24 56 37.7-233.7 -2.8 -26.6 -5 419 No stop 09 02 50 =0007+149 21 26 26 37.8-233.3 -2.7 -26.5 85 430 09 01 21 09 02 50 0017+154 21 26 26 37.1-236.5 -2.9 -27.7 -5 430 No stop 09 06 20 --- 21 29 56 37.4-235.5 -2.9 -27.4 205 457 09 02 51 09 07 10 J0009+1513 21 30 47 38.3-232.1 -2.7 -26.0 45 457 09 07 10 09 08 40 =0007+149 21 32 17 38.4-231.7 -2.6 -25.9 90 469 09 07 11 09 08 40 0017+154 21 32 17 37.7-234.9 -2.8 -27.1 -5 469 No stop 09 12 10 --- 21 35 47 38.1-233.9 -2.8 -26.8 205 496 09 08 41 09 12 10 J0009+1513 21 35 47 38.8-230.7 -2.6 -25.5 -5 496 No stop 09 13 40 =0007+149 21 37 18 39.0-230.3 -2.6 -25.3 85 508 09 12 11 09 13 40 0017+154 21 37 18 38.2-233.5 -2.7 -26.6 -5 508 No stop 09 17 10 --- 21 40 48 38.6-232.6 -2.7 -26.3 205 535 09 13 41 Schedule for IRBENE16 (Code Ib ) Page 4 Inclination Dependences of Optical-UV Broad Emission Line Profiles in Qu 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 ---------------------------------------------------------------------------------------- --- Tue 6 Mar 2018 Day 65 --- 09 17 10 J0009+1513 21 40 48 39.3-229.3 -2.5 -24.9 -5 535 No stop 09 18 40 =0007+149 21 42 18 39.5-228.9 -2.5 -24.8 85 546 09 17 11 09 20 20 J2349+0534 21 43 59 32.6-218.2 -2.1 -19.5 92 546 09 20 20 09 21 50 =2346+052 21 45 29 32.7-217.8 -2.1 -19.3 90 558 09 20 21 09 21 50 2345+061 21 45 29 33.5-217.9 -2.1 -19.4 -3 558 No stop 09 25 20 --- 21 49 00 33.8-216.9 -2.0 -18.9 207 585 09 21 51 09 25 20 J2349+0534 21 49 00 33.0-216.8 -2.0 -18.8 -3 585 No stop 09 26 50 =2346+052 21 50 30 33.1-216.4 -2.0 -18.6 87 596 09 25 21 09 26 50 2345+061 21 50 30 34.0-216.4 -2.0 -18.7 -3 596 No stop 09 30 20 --- 21 54 00 34.2-215.4 -1.9 -18.2 207 623 09 26 51 09 30 20 J2349+0534 21 54 00 33.4-215.4 -1.9 -18.2 -3 623 No stop 09 31 50 =2346+052 21 55 31 33.5-214.9 -1.9 -18.0 87 635 09 30 21 09 33 20 J0009+1513 21 57 01 40.9-224.6 -2.2 -23.0 82 635 09 33 20 09 34 50 =0007+149 21 58 31 41.1-224.2 -2.2 -22.8 90 647 09 33 21 09 34 50 0017+154 21 58 31 40.4-227.6 -2.4 -24.3 -5 647 No stop 09 38 20 --- 22 02 02 40.8-226.5 -2.3 -23.9 205 674 09 34 51 09 38 20 J0009+1513 22 02 02 41.4-223.2 -2.1 -22.4 -5 674 No stop 09 39 50 =0007+149 22 03 32 41.5-222.7 -2.1 -22.2 85 685 09 38 21 09 39 50 0017+154 22 03 32 40.9-226.1 -2.3 -23.7 -5 685 No stop 09 43 20 --- 22 07 03 41.3-225.1 -2.2 -23.2 205 712 09 39 51 09 44 10 J0009+1513 22 07 53 41.9-221.4 -2.0 -21.6 45 712 09 44 10 09 45 40 =0007+149 22 09 23 42.0-221.0 -2.0 -21.4 90 724 09 44 11 09 45 40 0017+154 22 09 23 41.5-224.4 -2.2 -22.9 -5 724 No stop 09 49 10 --- 22 12 53 41.8-223.3 -2.1 -22.5 205 751 09 45 41 09 49 10 J0009+1513 22 12 53 42.3-219.9 -2.0 -20.9 -5 751 No stop 09 50 40 =0007+149 22 14 24 42.5-219.4 -1.9 -20.7 85 763 09 49 11 09 50 40 0017+154 22 14 24 42.0-222.9 -2.1 -22.3 -5 763 No stop 09 54 10 --- 22 17 54 42.3-221.8 -2.1 -21.8 205 790 09 50 41 09 54 10 J0009+1513 22 17 54 42.8-218.4 -1.9 -20.2 -5 790 No stop 09 55 40 =0007+149 22 19 25 42.9-217.9 -1.9 -20.0 85 801 09 54 11 Schedule for IRBENE16 (Code Ib ) Page 5 Inclination Dependences of Optical-UV Broad Emission Line Profiles in Qu 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 ---------------------------------------------------------------------------------------- --- Tue 6 Mar 2018 Day 65 --- 09 58 10 J0237+2848 22 21 55 37.7-265.5 -4.3 -37.6 123 801 09 58 10 10 02 10 =0234+285 22 25 56 38.2-264.6 -4.2 -37.6 240 832 09 58 11 10 03 50 J2349+0534 22 27 36 35.7-205.6 -1.4 -13.5 68 832 10 03 50 10 05 20 =2346+052 22 29 06 35.7-205.2 -1.4 -13.2 90 844 10 03 51 10 05 20 2345+061 22 29 06 36.6-205.1 -1.3 -13.3 -3 844 No stop 10 08 50 --- 22 32 37 36.8-204.1 -1.3 -12.7 207 871 10 05 21 10 08 50 J2349+0534 22 32 37 35.9-204.1 -1.3 -12.7 -3 871 No stop 10 10 20 =2346+052 22 34 07 36.0-203.7 -1.3 -12.5 87 882 10 08 51 10 10 20 2345+061 22 34 07 36.9-203.6 -1.3 -12.5 -3 882 No stop 10 13 50 --- 22 37 38 37.1-202.6 -1.2 -12.0 207 909 10 10 21 10 13 50 J2349+0534 22 37 38 36.2-202.6 -1.2 -12.0 -3 909 No stop 10 15 20 =2346+052 22 39 08 36.3-202.1 -1.2 -11.7 87 921 10 13 51 10 16 50 J0009+1513 22 40 38 44.5-211.2 -1.5 -16.7 82 921 10 16 50 10 18 20 =0007+149 22 42 08 44.6-210.7 -1.5 -16.5 90 933 10 16 51 10 18 20 0017+154 22 42 08 44.3-214.3 -1.7 -18.3 -5 933 No stop 10 21 50 --- 22 45 39 44.5-213.2 -1.6 -17.8 205 960 10 18 21 10 21 50 J0009+1513 22 45 39 44.8-209.5 -1.4 -15.9 -5 960 No stop 10 23 20 =0007+149 22 47 09 44.9-209.0 -1.4 -15.7 85 971 10 21 51 10 23 20 0017+154 22 47 09 44.6-212.7 -1.6 -17.5 -5 971 No stop 10 26 50 --- 22 50 40 44.9-211.6 -1.5 -17.0 205 998 10 23 21 10 27 40 J0009+1513 22 51 30 45.2-207.6 -1.3 -14.9 45 998 10 27 40 10 29 10 =0007+149 22 53 00 45.3-207.1 -1.3 -14.7 90 1010 10 27 41 10 29 10 0017+154 22 53 00 45.1-210.8 -1.5 -16.6 -5 1010 No stop 10 32 40 --- 22 56 31 45.3-209.7 -1.4 -16.0 205 1037 10 29 11 10 32 40 J0009+1513 22 56 31 45.5-205.9 -1.2 -14.1 -5 1037 No stop 10 34 10 =0007+149 22 58 01 45.6-205.4 -1.2 -13.8 85 1049 10 32 41 10 34 10 0017+154 22 58 01 45.4-209.2 -1.4 -15.8 -5 1049 No stop 10 37 40 --- 23 01 31 45.6-208.0 -1.3 -15.2 205 1076 10 34 11 10 37 40 J0009+1513 23 01 31 45.8-204.3 -1.2 -13.2 -5 1076 No stop 10 39 10 =0007+149 23 03 02 45.9-203.8 -1.1 -12.9 85 1087 10 37 41 Schedule for IRBENE16 (Code Ib ) Page 6 Inclination Dependences of Optical-UV Broad Emission Line Profiles in Qu 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 ---------------------------------------------------------------------------------------- --- Tue 6 Mar 2018 Day 65 --- 10 40 50 J2349+0534 23 04 42 37.4-194.3 -0.8 -7.7 93 1087 10 40 50 10 42 20 =2346+052 23 06 12 37.4-193.8 -0.7 -7.4 90 1099 10 40 51 10 42 20 2345+061 23 06 12 38.3-193.7 -0.7 -7.4 -3 1099 No stop 10 45 50 --- 23 09 43 38.4-192.6 -0.7 -6.8 207 1126 10 42 21 10 45 50 J2349+0534 23 09 43 37.5-192.8 -0.7 -6.8 -3 1126 No stop 10 47 20 =2346+052 23 11 13 37.6-192.3 -0.7 -6.6 87 1137 10 45 51 10 47 20 2345+061 23 11 13 38.4-192.1 -0.6 -6.5 -3 1137 No stop 10 50 50 --- 23 14 44 38.5-191.0 -0.6 -5.9 207 1165 10 47 21 10 50 50 J2349+0534 23 14 44 37.7-191.2 -0.6 -6.0 -3 1165 No stop 10 52 20 =2346+052 23 16 14 37.7-190.7 -0.6 -5.8 87 1176 10 50 51 10 53 50 J0009+1513 23 17 44 46.6-198.7 -0.9 -10.3 83 1176 10 53 50 10 55 20 =0007+149 23 19 14 46.7-198.2 -0.9 -10.0 90 1188 10 53 51 10 55 20 0017+154 23 19 14 46.6-202.0 -1.0 -12.1 -5 1188 No stop 10 58 50 --- 23 22 45 46.8-200.8 -1.0 -11.4 205 1215 10 55 21 10 58 50 J0009+1513 23 22 45 46.8-197.0 -0.8 -9.4 -5 1215 No stop 11 00 20 =0007+149 23 24 15 46.9-196.5 -0.8 -9.1 85 1226 10 58 51 11 00 20 0017+154 23 24 15 46.9-200.3 -1.0 -11.2 -5 1226 No stop 11 03 50 --- 23 27 46 47.0-199.1 -0.9 -10.5 205 1253 11 00 21 11 04 40 J0009+1513 23 28 36 47.0-195.0 -0.7 -8.3 45 1253 11 04 40 11 06 10 =0007+149 23 30 06 47.1-194.4 -0.7 -8.0 90 1265 11 04 41 11 06 10 0017+154 23 30 06 47.1-198.3 -0.9 -10.1 -5 1265 No stop 11 09 40 --- 23 33 37 47.3-197.0 -0.8 -9.4 205 1292 11 06 11 11 09 40 J0009+1513 23 33 37 47.2-193.2 -0.6 -7.3 -5 1292 No stop 11 11 10 =0007+149 23 35 07 47.2-192.7 -0.6 -7.0 85 1304 11 09 41 11 11 10 0017+154 23 35 07 47.3-196.5 -0.8 -9.1 -5 1304 No stop 11 14 40 --- 23 38 38 47.5-195.3 -0.7 -8.5 205 1331 11 11 11 11 14 40 J0009+1513 23 38 38 47.3-191.4 -0.5 -6.3 -5 1331 No stop 11 16 10 =0007+149 23 40 08 47.4-190.9 -0.5 -6.0 85 1342 11 14 41 11 18 20 3C454.3 23 42 18 47.7-162.9 0.8 9.4 113 1342 11 18 20 11 23 00 --- 23 46 59 47.5-161.3 0.9 10.3 280 1378 11 18 21 Schedule for IRBENE16 (Code Ib ) Page 7 Inclination Dependences of Optical-UV Broad Emission Line Profiles in Qu 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 ---------------------------------------------------------------------------------------- --- Tue 6 Mar 2018 Day 65 --- 11 24 40 J2349+0534 23 48 39 38.1-180.5 -0.0 -0.3 87 1378 11 24 40 11 26 10 =2346+052 23 50 09 38.1-180.0 -0.0 -0.0 90 1390 11 24 41 11 26 10 2345+061 23 50 09 39.0-179.8 0.0 0.1 -3 1390 No stop 11 29 40 --- 23 53 40 38.9-178.6 0.1 0.7 207 1417 11 26 11 11 29 40 J2349+0534 23 53 40 38.1-178.9 0.1 0.6 -3 1417 No stop 11 31 10 =2346+052 23 55 10 38.1-178.4 0.1 0.8 87 1429 11 29 41 11 31 10 2345+061 23 55 10 38.9-178.2 0.1 1.0 -3 1429 No stop 11 34 40 --- 23 58 41 38.9-177.0 0.2 1.6 207 1456 11 31 11 11 34 40 J2349+0534 23 58 41 38.1-177.3 0.1 1.4 -3 1456 No stop 11 36 10 =2346+052 00 00 11 38.1-176.9 0.2 1.7 87 1467 11 34 41 11 37 40 J0009+1513 00 01 41 47.7-183.2 -0.1 -1.8 82 1467 11 37 40 11 39 10 =0007+149 00 03 12 47.7-182.7 -0.1 -1.5 90 1479 11 37 41 11 39 10 0017+154 00 03 12 48.1-186.5 -0.3 -3.6 -5 1479 No stop 11 42 40 --- 00 06 42 48.1-185.3 -0.2 -2.9 205 1506 11 39 11 11 42 40 J0009+1513 00 06 42 47.8-181.4 -0.1 -0.8 -5 1506 No stop 11 44 10 =0007+149 00 08 12 47.8-180.9 -0.0 -0.5 85 1517 11 42 41 11 44 10 0017+154 00 08 12 48.1-184.7 -0.2 -2.6 -5 1517 No stop 11 47 40 --- 00 11 43 48.2-183.5 -0.2 -1.9 205 1545 11 44 11 11 48 30 J0009+1513 00 12 33 47.8-179.3 0.0 0.4 45 1545 11 48 30 11 50 00 =0007+149 00 14 03 47.8-178.8 0.1 0.7 90 1556 11 48 31 11 50 00 0017+154 00 14 03 48.2-182.6 -0.1 -1.5 -5 1556 No stop 11 53 30 --- 00 17 34 48.2-181.4 -0.1 -0.8 205 1583 11 50 01 11 53 30 J0009+1513 00 17 34 47.7-177.5 0.1 1.4 -5 1583 No stop 11 55 00 =0007+149 00 19 04 47.7-177.0 0.1 1.7 85 1595 11 53 31 11 55 00 0017+154 00 19 04 48.2-180.8 -0.0 -0.5 -5 1595 No stop 11 58 30 --- 00 22 35 48.2-179.5 0.0 0.3 205 1622 11 55 01 11 58 30 J0009+1513 00 22 35 47.7-175.7 0.2 2.4 -5 1622 No stop 12 00 00 =0007+149 00 24 05 47.7-175.2 0.2 2.7 85 1633 11 58 31 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess118.C1024 --- 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: 12 Station: IRBENE16 Total bit rate: 1024 Format: VDIF Bits per sample: 2 Sample rate: 32.000 Number of channels: 16 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 4100.00 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 3 11 3 11 5 13 5 13 7 15 7 15 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 B1 D1 B1 D1 B1 D1 B1 D1 The following frequency sets based on these setups were used. Frequency Set: 4 Setup file default. Used with PCAL = off LO sum= 4942.49 4942.49 4942.49 4942.49 4974.49 4974.49 4974.49 4974.49 5006.49 5006.49 5006.49 5006.49 5038.49 5038.49 5038.49 5038.49 BBC fr= 842.49 842.49 842.49 842.49 874.49 874.49 874.49 874.49 906.49 906.49 906.49 906.49 938.49 938.49 938.49 938.49 Bandwd= 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 16.00 Matching frequency sets: 4 13 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) * 3C454.3 22 51 29.519738 * 22 53 57.747938 22 54 49.718147 0.67 J2253+1608 15 52 54.34810 * 16 08 53.56093 16 14 32.45539 0.70 2251+158 From catalog imbedded in main SCHED input file. J2253+16 GSFC 2015a astro solution, unpublished 40748 observations. 2346+052 23 46 47.611401 * 23 49 21.051510 23 50 14.898581 0.12 * J2349+0534 05 17 59.10038 * 05 34 39.87237 05 40 31.81999 0.26 From catalog imbedded in main SCHED input file. GSFC 2015a astro solution, unpublished 94 observations. 0007+149 00 07 09.036608 * 00 09 43.468697 00 10 37.772311 0.39 * J0009+1513 14 56 56.51284 * 15 13 37.90554 15 19 30.76853 0.76 From catalog imbedded in main SCHED input file. rfc_2015a Petrov, 2015, unpublished. 28 observations * 2345+061 23 45 58.408106 * 23 48 31.770600 23 49 25.594727 0.00 06 08 19.20677 * 06 24 59.78084 06 30 51.76196 0.00 From catalog imbedded in main SCHED input file. Target * 0017+154 00 17 49.906527 * 00 20 25.223501 00 21 19.872341 0.00 15 24 16.13804 * 15 40 54.71900 15 46 46.46550 0.00 From catalog imbedded in main SCHED input file. Target 0234+285 02 34 55.589590 * 02 37 52.405677 02 38 55.326095 0.00 * J0237+2848 28 35 11.40776 * 28 48 08.99001 28 52 42.97458 0.00 J0237+28 /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc GSFC 2015a astro solution, unpublished 54650 observations. 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 3C454.3 sess118.C1024 1 2 3 4 5 6 7 8 9 12 14 15 + 0.156 16.411 J2349+0534 sess118.C1024 1 2 3 4 5 6 7 8 9 12 14 15 + 0.450 43.718 J0009+1513 sess118.C1024 1 2 3 4 5 6 7 8 9 12 14 15 + 0.750 73.792 2345+061 sess118.C1024 1 2 3 4 5 6 7 8 9 12 14 15 + 0.700 73.645 0017+154 sess118.C1024 1 2 3 4 5 6 7 8 9 12 14 15 + 1.400 146.182 J0237+2848 sess118.C1024 1 2 3 4 5 6 7 8 9 12 14 15 + 0.067 8.000 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) 3C454.3 22.1 J2349+0534 15.5 J0009+1513 26.1 2345+061 16.0 0017+154 28.1 J0237+2848 61.3 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