  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel
 Exp. Code:  EM117M  


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 = G012.68-0.18
 
 

Schedule for HART      (Code Hh )                                   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
----------------------------------------------------------------------------------------

 --- Fri   2 Mar 2018   Day  61 ---

 Next scan frequencies:  6665.15  6665.15  6665.15  6665.15  6669.15  6669.15  6669.15  6669.15
                         6673.15  6673.15  6673.15  6673.15  6677.15  6677.15  6677.15  6677.15
 Next BBC frequencies:    155.15   155.15   155.15   155.15   159.15   159.15   159.15   159.15
                          163.15   163.15   163.15   163.15   167.15   167.15   167.15   167.15
 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  J1331+3030   15 00 06  29.9 338.1  1.5       0.0     0        0   02 30 00
02 40 00  =3C286       15 10 08  29.0 335.8  1.6       0.0   600       10   02 30 01

02 40 30  J1331+3030   15 10 38  28.9 335.7  1.6       0.0     9       10   02 40 30
02 50 30  =3C286       15 20 40  28.0 333.5  1.8       0.0   600       19   02 40 31

02 54 50  3C345        15 25 00  21.8  16.2 -1.3       0.0   138       19   02 54 50
03 04 50  ---          15 35 02  22.4  14.2 -1.1       0.0   600       29   02 54 51

03 05 20  3C345        15 35 32  22.4  14.1 -1.1       0.0     9       29   03 05 20
03 15 20  ---          15 45 34  23.0  12.1 -1.0       0.0   600       39   03 05 21

03 20 40  J1331+3030   15 50 55  24.6 327.3  2.3       0.0   196       39   03 20 40
03 29 50  =3C286       16 00 06  23.5 325.5  2.5       0.0   550       48   03 20 41

03 34 20  J1832-2039   16 04 37  55.6  89.1 -2.5       0.0    94       48   03 34 20
03 39 20  =1829-207    16 09 38  56.7  88.6 -2.4       0.0   300       52   03 34 21

03 39 20 G012.68-0.18  16 09 38  60.0  81.2 -2.1       0.0   -36       52   No stop 
03 41 20  ---          16 11 38  60.4  80.9 -2.1       0.0    84       54   03 39 21

03 42 10  J1832-2039   16 12 28  57.3  88.2 -2.3       0.0    14       54   03 42 10
03 45 00  =1829-207    16 15 19  58.0  87.9 -2.3       0.0   170       57   03 42 11

03 45 00 G012.68-0.18  16 15 19  61.2  80.2 -2.0       0.0   -36       57   No stop 
03 47 00  ---          16 17 19  61.7  79.9 -2.0       0.0    84       59   03 45 01

03 47 00  J1832-2039   16 17 19  58.4  87.6 -2.3       0.0   -36       59   No stop 
03 50 00  =1829-207    16 20 19  59.1  87.3 -2.2       0.0   144       62   03 47 01

03 50 00 G012.68-0.18  16 20 19  62.3  79.3 -1.9       0.0   -36       62   No stop 
03 52 00  ---          16 22 20  62.8  78.9 -1.9       0.0    84       64   03 50 01

03 52 50  J1832-2039   16 23 10  59.7  86.9 -2.2       0.0    14       64   03 52 50
03 55 40  =1829-207    16 26 00  60.4  86.5 -2.1       0.0   170       67   03 52 51

03 55 40 G012.68-0.18  16 26 00  63.6  78.2 -1.8       0.0   -36       67   No stop 
03 57 40  ---          16 28 01  64.0  77.8 -1.8       0.0    84       68   03 55 41
Schedule for HART      (Code Hh )                                   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
----------------------------------------------------------------------------------------

 --- Fri   2 Mar 2018   Day  61 ---

03 57 40  J1832-2039   16 28 01  60.8  86.3 -2.1       0.0   -36       68   No stop 
04 00 40  =1829-207    16 31 01  61.5  85.8 -2.0       0.0   144       71   03 57 41

04 00 40 G012.68-0.18  16 31 01  64.7  77.2 -1.7       0.0   -36       71   No stop 
04 02 40  ---          16 33 01  65.1  76.7 -1.7       0.0    84       73   04 00 41

04 02 40  J1832-2039   16 33 01  62.0  85.6 -2.0       0.0   -36       73   No stop 
04 05 40  =1829-207    16 36 02  62.6  85.1 -2.0       0.0   144       76   04 02 41

04 05 40 G012.68-0.18  16 36 02  65.8  76.1 -1.6       0.0   -36       76   No stop 
04 07 40  ---          16 38 02  66.2  75.6 -1.6       0.0    84       78   04 05 41

04 08 30  J1832-2039   16 38 52  63.3  84.7 -1.9       0.0    14       78   04 08 30
04 11 20  =1829-207    16 41 43  63.9  84.3 -1.9       0.0   170       81   04 08 31

04 11 20 G012.68-0.18  16 41 43  67.0  74.7 -1.6       0.0   -36       81   No stop 
04 13 20  ---          16 43 43  67.5  74.2 -1.5       0.0    84       83   04 11 21

04 13 20  J1832-2039   16 43 43  64.4  84.0 -1.8       0.0   -36       83   No stop 
04 16 20  =1829-207    16 46 44  65.0  83.5 -1.8       0.0   144       86   04 13 21

04 21 35  J1331+3030   16 52 00  16.1 316.6  3.3       0.0   136       86   04 21 35
04 29 35  =3C286       17 00 01  14.9 315.3  3.5       0.0   480       93   04 21 36

04 57 45  J1832-2039   17 28 16  74.2  74.0 -1.1       0.0  1514       93   04 57 45
05 00 45  =1829-207    17 31 16  74.8  73.0 -1.0       0.0   180       96   04 57 46

05 00 45 G012.68-0.18  17 31 16  77.2  54.3 -0.7       0.0   -36       96   No stop 
05 02 45  ---          17 33 16  77.5  52.9 -0.7       0.0    84       98   05 00 46

05 02 45  J1832-2039   17 33 16  75.3  72.3 -1.0       0.0   -36       98   No stop 
05 05 45  =1829-207    17 36 17  75.9  71.1 -0.9       0.0   144      101   05 02 46

05 05 45 G012.68-0.18  17 36 17  78.1  50.6 -0.6       0.0   -36      101   No stop 
05 07 45  ---          17 38 17  78.4  49.0 -0.6       0.0    84      103   05 05 46

05 07 45  J1832-2039   17 38 17  76.3  70.3 -0.9       0.0   -36      103   No stop 
05 10 45  =1829-207    17 41 18  77.0  69.0 -0.9       0.0   144      106   05 07 46

05 10 45 G012.68-0.18  17 41 18  78.9  46.4 -0.6       0.0   -36      106   No stop 
05 12 45  ---          17 43 18  79.2  44.6 -0.5       0.0    84      108   05 10 46

05 13 35  J1832-2039   17 44 08  77.6  67.6 -0.8       0.0    14      108   05 13 35
05 16 25  =1829-207    17 46 59  78.2  66.1 -0.8       0.0   170      111   05 13 36
Schedule for HART      (Code Hh )                                   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
----------------------------------------------------------------------------------------

 --- Fri   2 Mar 2018   Day  61 ---

05 16 25 G012.68-0.18  17 46 59  79.8  40.9 -0.5       0.0   -36      111   No stop 
05 18 25  ---          17 48 59  80.1  38.7 -0.4       0.0    84      113   05 16 26

05 18 25  J1832-2039   17 48 59  78.6  65.0 -0.7       0.0   -36      113   No stop 
05 21 25  =1829-207    17 51 59  79.2  63.2 -0.7       0.0   144      115   05 18 26

05 40 05  J1832-2039   18 10 43  82.6  45.8 -0.4       0.0  1098      115   05 40 05
05 43 05  =1829-207    18 13 43  83.1  41.5 -0.3       0.0   180      118   05 40 06

05 43 05 G012.68-0.18  18 13 43  82.1   2.1 -0.0       0.0   -36      118   No stop 
05 45 05  ---          18 15 43  82.1 358.7  0.0       0.0    84      120   05 43 06

05 45 05  J1832-2039   18 15 43  83.4  38.4 -0.3       0.0   -36      120   No stop 
05 48 05  =1829-207    18 18 44  83.8  33.2 -0.2       0.0   144      123   05 45 06

05 48 05 G012.68-0.18  18 18 44  82.1 353.5  0.1       0.0   -36      123   No stop 
05 50 05  ---          18 20 44  82.0 350.0  0.1       0.0    84      125   05 48 06

05 50 05  J1832-2039   18 20 44  84.0  29.4 -0.2       0.0   -36      125   No stop 
05 53 05  =1829-207    18 23 45  84.3  23.1 -0.2       0.0   144      128   05 50 06

05 53 05 G012.68-0.18  18 23 45  81.9 345.0  0.1       0.0   -36      128   No stop 
05 55 05  ---          18 25 45  81.7 341.8  0.2       0.0    84      130   05 53 06

05 55 55  J1832-2039   18 26 35  84.5  16.6 -0.1       0.0    14      130   05 55 55
05 58 45  =1829-207    18 29 26  84.7   9.7 -0.1       0.0   170      133   05 55 56

05 58 45 G012.68-0.18  18 29 26  81.4 336.2  0.2       0.0   -36      133   No stop 
06 00 45  ---          18 31 26  81.3 333.3  0.3       0.0    84      135   05 58 46

06 00 45  J1832-2039   18 31 26  84.7   4.6 -0.0       0.0   -36      135   No stop 
06 03 45  =1829-207    18 34 26  84.8 356.9  0.0       0.0   144      138   06 00 46

06 03 45 G012.68-0.18  18 34 26  80.9 329.2  0.3       0.0   -36      138   No stop 
06 05 45  ---          18 36 27  80.7 326.6  0.4       0.0    84      139   06 03 46

06 05 45  J1832-2039   18 36 27  84.7 351.8  0.1       0.0   -36      139   No stop 
06 08 45  =1829-207    18 39 27  84.6 344.5  0.1       0.0   144      142   06 05 46

06 08 45 G012.68-0.18  18 39 27  80.3 323.0  0.4       0.0   -36      142   No stop 
06 10 45  ---          18 41 28  80.0 320.7  0.4       0.0    84      144   06 08 46

06 11 35  J1832-2039   18 42 18  84.4 337.9  0.2       0.0    14      144   06 11 35
06 14 25  =1829-207    18 45 08  84.1 331.9  0.2       0.0   170      147   06 11 36
Schedule for HART      (Code Hh )                                   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
----------------------------------------------------------------------------------------

 --- Fri   2 Mar 2018   Day  61 ---

06 14 25 G012.68-0.18  18 45 08  79.5 316.9  0.5       0.0   -36      147   No stop 
06 16 25  ---          18 47 08  79.2 314.9  0.5       0.0    84      149   06 14 26

06 16 25  J1832-2039   18 47 08  83.9 328.0  0.2       0.0   -36      149   No stop 
06 19 25  =1829-207    18 50 09  83.5 322.6  0.3       0.0   144      152   06 16 26

06 19 25 G012.68-0.18  18 50 09  78.7 312.2  0.6       0.0   -36      152   No stop 
06 21 25  ---          18 52 09  78.3 310.5  0.6       0.0    84      154   06 19 26

06 21 25  J1832-2039   18 52 09  83.2 319.4  0.3       0.0   -36      154   No stop 
06 24 25  =1829-207    18 55 10  82.7 315.0  0.4       0.0   144      157   06 21 26

06 24 25 G012.68-0.18  18 55 10  77.8 308.2  0.7       0.0   -36      157   No stop 
06 26 25  ---          18 57 10  77.5 306.7  0.7       0.0    84      159   06 24 26

06 27 15  J1832-2039   18 58 00  82.3 311.4  0.4       0.0    14      159   06 27 15
06 30 05  =1829-207    19 00 51  81.8 308.2  0.5       0.0   170      161   06 27 16

06 49 30  J1832-2039   19 20 19  78.0 293.4  0.8       0.0  1143      161   06 49 30
06 52 20  =1829-207    19 23 09  77.4 292.0  0.8       0.0   170      164   06 49 31

06 52 20 G012.68-0.18  19 23 09  72.4 293.0  1.1       0.0   -36      164   No stop 
06 54 20  ---          19 25 10  71.9 292.3  1.2       0.0    84      166   06 52 21

06 54 20  J1832-2039   19 25 10  77.0 291.1  0.9       0.0   -36      166   No stop 
06 57 20  =1829-207    19 28 10  76.3 289.7  0.9       0.0   144      169   06 54 21

06 57 20 G012.68-0.18  19 28 10  71.3 291.2  1.2       0.0   -36      169   No stop 
06 59 20  ---          19 30 11  70.9 290.5  1.3       0.0    84      171   06 57 21

06 59 20  J1832-2039   19 30 11  75.9 288.9  0.9       0.0   -36      171   No stop 
07 02 20  =1829-207    19 33 11  75.3 287.8  1.0       0.0   144      174   06 59 21

07 02 20 G012.68-0.18  19 33 11  70.3 289.5  1.3       0.0   -36      174   No stop 
07 04 20  ---          19 35 11  69.8 288.9  1.3       0.0    84      176   07 02 21

07 05 10  J1832-2039   19 36 01  74.7 286.7  1.0       0.0    14      176   07 05 10
07 08 00  =1829-207    19 38 52  74.1 285.8  1.1       0.0   170      178   07 05 11

07 08 00 G012.68-0.18  19 38 52  69.0 287.8  1.4       0.0   -36      178   No stop 
07 10 00  ---          19 40 52  68.6 287.2  1.4       0.0    84      180   07 08 01

07 10 00  J1832-2039   19 40 52  73.6 285.2  1.1       0.0   -36      180   No stop 
07 13 00  =1829-207    19 43 53  73.0 284.3  1.2       0.0   144      183   07 10 01
Schedule for HART      (Code Hh )                                   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
----------------------------------------------------------------------------------------

 --- Fri   2 Mar 2018   Day  61 ---

07 13 00 G012.68-0.18  19 43 53  68.0 286.4  1.5       0.0   -36      183   No stop 
07 15 00  ---          19 45 53  67.5 285.9  1.5       0.0    84      185   07 13 01

07 15 00  J1832-2039   19 45 53  72.5 283.7  1.2       0.0   -36      185   No stop 
07 18 00  =1829-207    19 48 54  71.9 282.9  1.3       0.0   144      188   07 15 01

07 18 00 G012.68-0.18  19 48 54  66.9 285.1  1.6       0.0   -36      188   No stop 
07 20 00  ---          19 50 54  66.4 284.6  1.6       0.0    84      190   07 18 01

07 20 50  J1832-2039   19 51 44  71.2 282.1  1.3       0.0    14      190   07 20 50
07 23 40  =1829-207    19 54 35  70.6 281.5  1.4       0.0   170      193   07 20 51

07 23 40 G012.68-0.18  19 54 35  65.6 283.8  1.7       0.0   -36      193   No stop 
07 25 40  ---          19 56 35  65.2 283.3  1.7       0.0    84      195   07 23 41

07 25 40  J1832-2039   19 56 35  70.2 281.0  1.4       0.0   -36      195   No stop 
07 28 40  =1829-207    19 59 35  69.5 280.3  1.4       0.0   144      198   07 25 41

07 28 40 G012.68-0.18  19 59 35  64.5 282.7  1.7       0.0   -36      198   No stop 
07 30 40  ---          20 01 36  64.1 282.3  1.8       0.0    84      200   07 28 41

07 30 40  J1832-2039   20 01 36  69.1 279.9  1.5       0.0   -36      200   No stop 
07 33 40  =1829-207    20 04 36  68.4 279.3  1.5       0.0   144      202   07 30 41

07 52 50  J1832-2039   20 23 49  64.1 275.9  1.8       0.0  1128      202   07 52 50
07 55 50  =1829-207    20 26 50  63.4 275.4  1.9       0.0   180      205   07 52 51

07 55 50 G012.68-0.18  20 26 50  58.5 277.7  2.2       0.0   -36      205   No stop 
07 57 50  ---          20 28 50  58.1 277.4  2.2       0.0    84      207   07 55 51

07 57 50  J1832-2039   20 28 50  63.0 275.1  1.9       0.0   -36      207   No stop 
08 00 50  =1829-207    20 31 51  62.3 274.7  2.0       0.0   144      210   07 57 51

08 00 50 G012.68-0.18  20 31 51  57.4 276.9  2.3       0.0   -36      210   No stop 
08 02 50  ---          20 33 51  57.0 276.6  2.3       0.0    84      212   08 00 51

08 02 50  J1832-2039   20 33 51  61.9 274.4  2.0       0.0   -36      212   No stop 
08 05 50  =1829-207    20 36 51  61.2 274.0  2.1       0.0   144      215   08 02 51

08 05 50 G012.68-0.18  20 36 51  56.3 276.2  2.4       0.0   -36      215   No stop 
08 07 50  ---          20 38 52  55.8 275.9  2.4       0.0    84      217   08 05 51

08 08 40  J1832-2039   20 39 42  60.6 273.6  2.1       0.0    14      217   08 08 40
08 11 30  =1829-207    20 42 32  59.9 273.2  2.2       0.0   170      220   08 08 41
Schedule for HART      (Code Hh )                                   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
----------------------------------------------------------------------------------------

 --- Fri   2 Mar 2018   Day  61 ---

08 11 30 G012.68-0.18  20 42 32  55.0 275.4  2.5       0.0   -36      220   No stop 
08 13 30  ---          20 44 33  54.6 275.1  2.5       0.0    84      222   08 11 31

08 13 30  J1832-2039   20 44 33  59.5 272.9  2.2       0.0   -36      222   No stop 
08 16 30  =1829-207    20 47 33  58.8 272.6  2.2       0.0   144      224   08 13 31

08 16 30 G012.68-0.18  20 47 33  53.9 274.7  2.5       0.0   -36      224   No stop 
08 18 30  ---          20 49 34  53.4 274.4  2.6       0.0    84      226   08 16 31

08 18 30  J1832-2039   20 49 34  58.3 272.3  2.3       0.0   -36      226   No stop 
08 21 30  =1829-207    20 52 34  57.7 271.9  2.3       0.0   144      229   08 18 31

08 21 30 G012.68-0.18  20 52 34  52.8 274.0  2.6       0.0   -36      229   No stop 
08 23 30  ---          20 54 34  52.3 273.8  2.7       0.0    84      231   08 21 31

08 24 20  J1832-2039   20 55 24  57.0 271.6  2.4       0.0    14      231   08 24 20
08 27 10  =1829-207    20 58 15  56.4 271.3  2.4       0.0   170      234   08 24 21

08 27 10 G012.68-0.18  20 58 15  51.5 273.3  2.7       0.0   -36      234   No stop 
08 29 10  ---          21 00 15  51.0 273.1  2.8       0.0    84      236   08 27 11

08 29 10  J1832-2039   21 00 15  55.9 271.0  2.5       0.0   -36      236   No stop 
08 32 10  =1829-207    21 03 16  55.3 270.7  2.5       0.0   144      239   08 29 11

08 32 10 G012.68-0.18  21 03 16  50.4 272.7  2.8       0.0   -36      239   No stop 
08 34 10  ---          21 05 16  49.9 272.4  2.8       0.0    84      241   08 32 11

08 35 00  J1832-2039   21 06 06  54.6 270.4  2.5       0.0    14      241   08 35 00
08 37 50  =1829-207    21 08 57  54.0 270.1  2.6       0.0   170      243   08 35 01

08 56 30  J1832-2039   21 27 40  49.8 268.1  2.9       0.0  1098      243   08 56 30
08 59 20  =1829-207    21 30 30  49.1 267.8  3.0       0.0   170      246   08 56 31

08 59 20 G012.68-0.18  21 30 30  44.2 269.6  3.3       0.0   -36      246   No stop 
09 01 20  ---          21 32 31  43.8 269.4  3.3       0.0    84      248   08 59 21

09 01 20  J1832-2039   21 32 31  48.7 267.6  3.0       0.0   -36      248   No stop 
09 04 20  =1829-207    21 35 31  48.0 267.3  3.0       0.0   144      251   09 01 21

09 04 20 G012.68-0.18  21 35 31  43.1 269.0  3.3       0.0   -36      251   No stop 
09 06 20  ---          21 37 31  42.7 268.8  3.4       0.0    84      253   09 04 21

09 06 20  J1832-2039   21 37 31  47.6 267.1  3.1       0.0   -36      253   No stop 
09 09 20  =1829-207    21 40 32  46.9 266.8  3.1       0.0   144      256   09 06 21
Schedule for HART      (Code Hh )                                   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
----------------------------------------------------------------------------------------

 --- Fri   2 Mar 2018   Day  61 ---

09 09 20 G012.68-0.18  21 40 32  42.0 268.5  3.4       0.0   -36      256   No stop 
09 11 20  ---          21 42 32  41.5 268.3  3.5       0.0    84      258   09 09 21

09 12 10  J1832-2039   21 43 22  46.2 266.6  3.2       0.0    14      258   09 12 10
09 15 00  =1829-207    21 46 13  45.6 266.3  3.2       0.0   170      261   09 12 11

09 15 00 G012.68-0.18  21 46 13  40.7 267.9  3.5       0.0   -36      261   No stop 
09 17 00  ---          21 48 13  40.3 267.7  3.6       0.0    84      262   09 15 01

09 17 00  J1832-2039   21 48 13  45.2 266.1  3.2       0.0   -36      262   No stop 
09 20 00  =1829-207    21 51 14  44.5 265.8  3.3       0.0   144      265   09 17 01

09 20 00 G012.68-0.18  21 51 14  39.6 267.4  3.6       0.0   -36      265   No stop 
09 22 00  ---          21 53 14  39.1 267.2  3.6       0.0    84      267   09 20 01

09 22 00  J1832-2039   21 53 14  44.0 265.6  3.3       0.0   -36      267   No stop 
09 25 00  =1829-207    21 56 14  43.4 265.4  3.4       0.0   144      270   09 22 01

09 25 00 G012.68-0.18  21 56 14  38.5 266.9  3.7       0.0   -36      270   No stop 
09 27 00  ---          21 58 15  38.0 266.7  3.7       0.0    84      272   09 25 01

09 27 50  J1832-2039   21 59 05  42.7 265.1  3.4       0.0    14      272   09 27 50
09 30 40  =1829-207    22 01 55  42.1 264.8  3.5       0.0   170      275   09 27 51

09 30 40 G012.68-0.18  22 01 55  37.2 266.4  3.8       0.0   -36      275   No stop 
09 32 40  ---          22 03 56  36.7 266.2  3.8       0.0    84      277   09 30 41

09 32 40  J1832-2039   22 03 56  41.6 264.7  3.5       0.0   -36      277   No stop 
09 35 40  =1829-207    22 06 56  41.0 264.4  3.6       0.0   144      280   09 32 41

09 35 40 G012.68-0.18  22 06 56  36.0 265.9  3.9       0.0   -36      280   No stop 
09 37 40  ---          22 08 57  35.6 265.7  3.9       0.0    84      282   09 35 41

09 38 30  J1832-2039   22 09 47  40.3 264.1  3.6       0.0    14      282   09 38 30
09 41 20  =1829-207    22 12 37  39.7 263.9  3.7       0.0   170      284   09 38 31

09 58 50  J1832-2039   22 30 10  35.8 262.3  3.9       0.0  1028      284   09 58 50
10 01 40  =1829-207    22 33 00  35.1 262.1  4.0       0.0   170      287   09 58 51

10 01 40 G012.68-0.18  22 33 00  30.2 263.4  4.3       0.0   -36      287   No stop 
10 03 40  ---          22 35 01  29.8 263.2  4.3       0.0    84      289   10 01 41

10 03 40  J1832-2039   22 35 01  34.7 261.9  4.0       0.0   -36      289   No stop 
10 06 40  =1829-207    22 38 01  34.0 261.6  4.1       0.0   144      292   10 03 41
Schedule for HART      (Code Hh )                                   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
----------------------------------------------------------------------------------------

 --- Fri   2 Mar 2018   Day  61 ---

10 06 40 G012.68-0.18  22 38 01  29.1 262.9  4.4       0.0   -36      292   No stop 
10 08 40  ---          22 40 02  28.6 262.7  4.4       0.0    84      294   10 06 41

10 08 40  J1832-2039   22 40 02  33.6 261.5  4.1       0.0   -36      294   No stop 
10 11 40  =1829-207    22 43 02  32.9 261.2  4.2       0.0   144      297   10 08 41

10 11 40 G012.68-0.18  22 43 02  28.0 262.4  4.5       0.0   -36      297   No stop 
10 13 40  ---          22 45 02  27.5 262.2  4.5       0.0    84      299   10 11 41

10 14 30  J1832-2039   22 45 53  32.3 261.0  4.2       0.0    14      299   10 14 30
10 17 20  =1829-207    22 48 43  31.7 260.7  4.3       0.0   170      301   10 14 31

10 17 20 G012.68-0.18  22 48 43  26.7 261.9  4.6       0.0   -36      301   No stop 
10 19 20  ---          22 50 43  26.3 261.7  4.6       0.0    84      303   10 17 21

10 19 20  J1832-2039   22 50 43  31.2 260.5  4.3       0.0   -36      303   No stop 
10 22 20  =1829-207    22 53 44  30.5 260.3  4.3       0.0   144      306   10 19 21

10 22 20 G012.68-0.18  22 53 44  25.6 261.4  4.6       0.0   -36      306   No stop 
10 24 20  ---          22 55 44  25.1 261.3  4.7       0.0    84      308   10 22 21

10 24 20  J1832-2039   22 55 44  30.1 260.1  4.4       0.0   -36      308   No stop 
10 27 20  =1829-207    22 58 45  29.4 259.8  4.4       0.0   144      311   10 24 21

10 27 20 G012.68-0.18  22 58 45  24.5 261.0  4.7       0.0   -36      311   No stop 
10 29 20  ---          23 00 45  24.0 260.8  4.8       0.0    84      313   10 27 21

10 30 10  J1832-2039   23 01 35  28.8 259.6  4.5       0.0    14      313   10 30 10
10 33 00  =1829-207    23 04 26  28.2 259.4  4.5       0.0   170      316   10 30 11

10 33 00 G012.68-0.18  23 04 26  23.2 260.4  4.8       0.0   -36      316   No stop 
10 35 00  ---          23 06 26  22.8 260.3  4.9       0.0    84      318   10 33 01

10 35 00  J1832-2039   23 06 26  27.7 259.2  4.6       0.0   -36      318   No stop 
10 38 00  =1829-207    23 09 26  27.1 258.9  4.6       0.0   144      321   10 35 01

10 38 00 G012.68-0.18  23 09 26  22.1 260.0  4.9       0.0   -36      321   No stop 
10 40 00  ---          23 11 27  21.7 259.8  4.9       0.0    84      323   10 38 01

10 40 50  J1832-2039   23 12 17  26.4 258.7  4.7       0.0    14      323   10 40 50
10 43 40  =1829-207    23 15 07  25.8 258.4  4.7       0.0   170      325   10 40 51

11 04 50  J1832-2039   23 36 21  21.2 256.6  5.1       0.0  1248      325   11 04 50
11 07 50  =1829-207    23 39 21  20.5 256.3  5.1       0.0   180      328   11 04 51
Schedule for HART      (Code Hh )                                   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
----------------------------------------------------------------------------------------

 --- Fri   2 Mar 2018   Day  61 ---

11 07 50 G012.68-0.18  23 39 21  15.5 257.2  5.4       0.0   -36      328   No stop 
11 09 50  ---          23 41 22  15.1 257.0  5.4       0.0    84      330   11 07 51

11 09 50  J1832-2039   23 41 22  20.1 256.1  5.1       0.0   -36      330   No stop 
11 12 50  =1829-207    23 44 22  19.4 255.8  5.2       0.0   144      333   11 09 51

11 12 50 G012.68-0.18  23 44 22  14.4 256.7  5.5       0.0   -36      333   No stop 
11 14 50  ---          23 46 22  14.0 256.5  5.5       0.0    84      335   11 12 51

11 14 50  J1832-2039   23 46 22  19.0 255.7  5.2       0.0   -36      335   No stop 
11 17 50  =1829-207    23 49 23  18.3 255.4  5.3       0.0   144      338   11 14 51

11 17 50 G012.68-0.18  23 49 23  13.3 256.2  5.6       0.0   -36      338   No stop 
11 19 50  ---          23 51 23  12.9 256.0  5.6       0.0    84      340   11 17 51

11 20 40  J1832-2039   23 52 13  17.7 255.1  5.3       0.0    14      340   11 20 40
11 23 30  =1829-207    23 55 04  17.1 254.9  5.4       0.0   170      342   11 20 41

11 23 30 G012.68-0.18  23 55 04  12.1 255.7  5.7       0.0   -36      342   No stop 
11 25 30  ---          23 57 04  11.6 255.5  5.7       0.0    84      344   11 23 31

11 25 30  J1832-2039   23 57 04  16.6 254.7  5.4       0.0   -36      344   No stop 
11 30 00  =1829-207    00 01 35  15.7 254.3  5.5       0.0   234      349   11 25 31


SETUP FILE INFORMATION:
   NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings.


 ======== Setup file: sess118.M128
   Matching groups in /home/guest/rmc/SCHED/sched11.4/catalogs/freq_RDBE.dat:
     hh5cm           Values confirmed by E-mail Jonathan Quick 20140219 (CR)
    ****** Only   16.00 of   32.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:    5         Station: HART              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=   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00
             6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00
   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:   9  Based on FREQ, BW, and/or DOPPLER in schedule.  Used with PCAL = off
    **** Warning  Only    16.00 MHz of    32.00 MHz in scheduled channels is within IFs.
   LO sum=   6665.15  6665.15  6665.15  6665.15  6669.15  6669.15  6669.15  6669.15
             6673.15  6673.15  6673.15  6673.15  6677.15  6677.15  6677.15  6677.15
   BBC fr=    155.15   155.15   155.15   155.15   159.15   159.15   159.15   159.15
              163.15   163.15   163.15   163.15   167.15   167.15   167.15   167.15
   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:   9

   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)

 * G012.68-0.18      18 10 59.237691   * 18 13 54.750000     18 14 57.111308       0.00
                    -18 02 40.99379    *-18 01 46.57000     -18 01 20.11352        0.00
                     From catalog imbedded in main SCHED input file.
                     Doppler based on LSR frame and radio definition.  Velocities:
                         57.50    57.50    57.50    57.50    57.50    57.50    57.50    57.50
                         57.50    57.50    57.50    57.50    57.50    57.50

 * 3C84              03 16 29.567263   * 03 19 48.160094     03 20 59.268816       1.30
   J0319+4130        41 19 51.91701    * 41 30 42.10413      41 34 34.42351        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 58.810467       0.18
 * J1331+3030        30 45 58.64059    * 30 30 32.95924      30 24 50.67443        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 34.945371       0.76
   J1642+3948        39 54 10.81496    * 39 48 36.99402      39 46 26.20896        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.

   1829-207          18 29 12.261812   * 18 32 11.046476     18 33 14.447938       0.28
 * J1832-2039       -20 42 02.03615    *-20 39 48.20378     -20 38 52.65825        0.41
                     /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
                     GSFC 2015a astro solution, unpublished    110 observations.
                     Doppler based on other sources.

   VR422201          22 00 39.362505   * 22 02 43.291372     22 03 26.383956       0.00
 * J2202+4216        42 02 08.59077    * 42 16 39.97990      42 21 48.94604        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
  G012.68-0.1sess118.M128          1 2 3 4 5 6 7 8 9 10              1.867    51.408
  3C84       sess118.M128          1 2 3 4 5 6 7 8 10                0.131     4.700
  J1331+3030 sess118.M128          1 2 3 4 5 6 7 8 9 10              1.258    46.797
  3C345      sess118.M128          1 2 3 4 5 6 7 8 9 10              0.333    14.951
  J1832-2039 sess118.M128          1 2 3 4 5 6 7 8 9 10              3.197    96.840
  J2202+4216 sess118.M128          2 3 4 5 6 7 8 10                  0.158     4.433


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) 
   G012.68-0.18        68.2
   3C84                78.2
   J1331+3030         136.0
   3C345               96.3
   J1832-2039          63.9
   J2202+4216          50.8

  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 

