  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel
 Exp. Code:  EM117A  


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 = 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
----------------------------------------------------------------------------------------

 --- Sat  27 Feb 2016   Day  58 ---

 Next scan frequencies:  6665.14  6665.14  6665.14  6665.14  6669.13  6669.13  6669.13  6669.13
                         6673.13  6673.13  6673.13  6673.13  6677.13  6677.13  6677.13  6677.13
 Next BBC frequencies:    155.14   155.14   155.14   155.14   159.13   159.13   159.13   159.13
                          163.13   163.13   163.13   163.13   167.13   167.13   167.13   167.13
 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   14 46 15  30.9 341.3  1.2       0.0     0        0   02 30 00
02 40 00  =3C286       14 56 16  30.2 339.0  1.4       0.0   600       10   02 30 01

02 40 30  J1331+3030   14 56 46  30.1 338.8  1.4       0.0     9       10   02 40 30
02 50 30  =3C286       15 06 48  29.3 336.6  1.6       0.0   600       19   02 40 31

02 54 50  3C345        15 11 09  20.9  18.8 -1.5       0.0   138       19   02 54 50
03 04 50  ---          15 21 10  21.6  16.9 -1.4       0.0   600       29   02 54 51

03 05 20  3C345        15 21 40  21.6  16.8 -1.4       0.0     9       29   03 05 20
03 15 20  ---          15 31 42  22.2  14.8 -1.2       0.0   600       38   03 05 21

03 20 20  J1331+3030   15 36 43  26.3 330.1  2.1       0.0   176       38   03 20 20
03 30 20  =3C286       15 46 45  25.1 328.1  2.2       0.0   600       48   03 20 21

03 34 50  J1832-2039   15 51 15  52.6  90.6 -2.7       0.0    94       48   03 34 50
03 39 50  =1829-207    15 56 16  53.7  90.1 -2.6       0.0   300       53   03 34 51

03 39 50 G012.68-0.18  15 56 16  57.0  83.3 -2.3       0.0   -36       53   No stop 
03 41 50  ---          15 58 16  57.5  83.0 -2.3       0.0    84       55   03 39 51

03 42 30  J1832-2039   15 58 57  54.3  89.8 -2.6       0.0     4       55   03 42 30
03 45 30  =1829-207    16 01 57  55.0  89.4 -2.5       0.0   180       58   03 42 31

03 45 30 G012.68-0.18  16 01 57  58.3  82.5 -2.2       0.0   -36       58   No stop 
03 47 30  ---          16 03 57  58.7  82.1 -2.2       0.0    84       60   03 45 31

03 47 30  J1832-2039   16 03 57  55.5  89.2 -2.5       0.0   -36       60   No stop 
03 50 30  =1829-207    16 06 58  56.1  88.9 -2.4       0.0   144       62   03 47 31

03 50 30 G012.68-0.18  16 06 58  59.4  81.6 -2.1       0.0   -36       62   No stop 
03 52 30  ---          16 08 58  59.9  81.3 -2.1       0.0    84       64   03 50 31

03 53 10  J1832-2039   16 09 38  56.7  88.6 -2.4       0.0     4       64   03 53 10
03 56 10  =1829-207    16 12 39  57.4  88.2 -2.3       0.0   180       67   03 53 11

03 56 10 G012.68-0.18  16 12 39  60.7  80.7 -2.0       0.0   -36       67   No stop 
03 58 10  ---          16 14 39  61.1  80.3 -2.0       0.0    84       69   03 56 11
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
----------------------------------------------------------------------------------------

 --- Sat  27 Feb 2016   Day  58 ---

03 58 10  J1832-2039   16 14 39  57.9  88.0 -2.3       0.0   -36       69   No stop 
04 01 10  =1829-207    16 17 40  58.5  87.6 -2.3       0.0   144       72   03 58 11

04 01 10 G012.68-0.18  16 17 40  61.8  79.8 -2.0       0.0   -36       72   No stop 
04 03 10  ---          16 19 40  62.2  79.4 -1.9       0.0    84       74   04 01 11

04 03 10  J1832-2039   16 19 40  59.0  87.3 -2.2       0.0   -36       74   No stop 
04 06 10  =1829-207    16 22 40  59.7  86.9 -2.2       0.0   144       77   04 03 11

04 06 10 G012.68-0.18  16 22 40  62.9  78.8 -1.9       0.0   -36       77   No stop 
04 08 10  ---          16 24 41  63.3  78.5 -1.8       0.0    84       79   04 06 11

04 08 50  J1832-2039   16 25 21  60.3  86.6 -2.1       0.0     4       79   04 08 50
04 11 50  =1829-207    16 28 21  60.9  86.2 -2.1       0.0   180       82   04 08 51

04 11 50 G012.68-0.18  16 28 21  64.1  77.7 -1.8       0.0   -36       82   No stop 
04 13 50  ---          16 30 22  64.6  77.3 -1.7       0.0    84       84   04 11 51

04 13 50  J1832-2039   16 30 22  61.4  85.9 -2.0       0.0   -36       84   No stop 
04 16 50  =1829-207    16 33 22  62.1  85.5 -2.0       0.0   144       87   04 13 51

04 21 20  J1331+3030   16 37 53  18.2 318.8  3.1       0.0    91       87   04 21 20
04 31 20  =3C286       16 47 55  16.7 317.2  3.3       0.0   600       96   04 21 21

04 58 20  J1832-2039   17 14 59  71.3  77.8 -1.3       0.0  1444       96   04 58 20
05 01 20  =1829-207    17 17 59  72.0  77.0 -1.3       0.0   180       99   04 58 21

05 01 20 G012.68-0.18  17 17 59  74.7  62.0 -0.9       0.0   -36       99   No stop 
05 03 20  ---          17 20 00  75.1  61.0 -0.9       0.0    84      101   05 01 21

05 03 20  J1832-2039   17 20 00  72.4  76.5 -1.2       0.0   -36      101   No stop 
05 06 20  =1829-207    17 23 00  73.1  75.6 -1.2       0.0   144      104   05 03 21

05 06 20 G012.68-0.18  17 23 00  75.6  59.4 -0.9       0.0   -36      104   No stop 
05 08 20  ---          17 25 01  76.0  58.2 -0.8       0.0    84      106   05 06 21

05 08 20  J1832-2039   17 25 01  73.5  75.0 -1.1       0.0   -36      106   No stop 
05 11 20  =1829-207    17 28 01  74.2  74.0 -1.1       0.0   144      109   05 08 21

05 11 20 G012.68-0.18  17 28 01  76.6  56.4 -0.8       0.0   -36      109   No stop 
05 13 20  ---          17 30 01  77.0  55.1 -0.7       0.0    84      111   05 11 21

05 14 00  J1832-2039   17 30 42  74.7  73.1 -1.0       0.0     4      111   05 14 00
05 17 00  =1829-207    17 33 42  75.4  72.1 -1.0       0.0   180      113   05 14 01
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
----------------------------------------------------------------------------------------

 --- Sat  27 Feb 2016   Day  58 ---

05 17 00 G012.68-0.18  17 33 42  77.6  52.5 -0.7       0.0   -36      113   No stop 
05 19 00  ---          17 35 42  78.0  51.0 -0.7       0.0    84      115   05 17 01

05 19 00  J1832-2039   17 35 42  75.8  71.3 -1.0       0.0   -36      115   No stop 
05 22 00  =1829-207    17 38 43  76.5  70.1 -0.9       0.0   144      118   05 19 01

05 41 00  J1832-2039   17 57 46  80.3  59.0 -0.6       0.0  1118      118   05 41 00
05 44 00  =1829-207    18 00 47  80.9  56.5 -0.5       0.0   180      121   05 41 01

05 44 00 G012.68-0.18  18 00 47  81.5  23.2 -0.2       0.0   -36      121   No stop 
05 46 00  ---          18 02 47  81.7  20.2 -0.2       0.0    84      123   05 44 01

05 46 00  J1832-2039   18 02 47  81.3  54.6 -0.5       0.0   -36      123   No stop 
05 49 00  =1829-207    18 05 47  81.8  51.5 -0.5       0.0   144      126   05 46 01

05 49 00 G012.68-0.18  18 05 47  81.9  15.4 -0.2       0.0   -36      126   No stop 
05 51 00  ---          18 07 48  82.0  12.1 -0.1       0.0    84      128   05 49 01

05 51 00  J1832-2039   18 07 48  82.2  49.3 -0.4       0.0   -36      128   No stop 
05 54 00  =1829-207    18 10 48  82.7  45.5 -0.4       0.0   144      131   05 51 01

05 54 00 G012.68-0.18  18 10 48  82.1   7.0 -0.1       0.0   -36      131   No stop 
05 56 00  ---          18 12 48  82.1   3.5 -0.0       0.0    84      133   05 54 01

05 56 40  J1832-2039   18 13 29  83.1  41.7 -0.3       0.0     4      133   05 56 40
05 59 40  =1829-207    18 16 29  83.5  37.0 -0.3       0.0   180      136   05 56 41

05 59 40 G012.68-0.18  18 16 29  82.1 357.2  0.0       0.0   -36      136   No stop 
06 01 40  ---          18 18 29  82.1 353.7  0.1       0.0    84      137   05 59 41

06 01 40  J1832-2039   18 18 29  83.8  33.4 -0.2       0.0   -36      137   No stop 
06 04 40  =1829-207    18 21 30  84.1  27.6 -0.2       0.0   144      140   06 01 41

06 04 40 G012.68-0.18  18 21 30  82.0 348.6  0.1       0.0   -36      140   No stop 
06 06 40  ---          18 23 30  81.9 345.3  0.1       0.0    84      142   06 04 41

06 06 40  J1832-2039   18 23 30  84.3  23.4 -0.2       0.0   -36      142   No stop 
06 09 40  =1829-207    18 26 31  84.5  16.5 -0.1       0.0   144      145   06 06 41

06 09 40 G012.68-0.18  18 26 31  81.7 340.5  0.2       0.0   -36      145   No stop 
06 11 40  ---          18 28 31  81.5 337.4  0.2       0.0    84      147   06 09 41

06 12 20  J1832-2039   18 29 11  84.7  10.0 -0.1       0.0     4      147   06 12 20
06 15 20  =1829-207    18 32 12  84.8   2.4 -0.0       0.0   180      150   06 12 21
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
----------------------------------------------------------------------------------------

 --- Sat  27 Feb 2016   Day  58 ---

06 15 20 G012.68-0.18  18 32 12  81.2 332.1  0.3       0.0   -36      150   No stop 
06 17 20  ---          18 34 12  80.9 329.4  0.3       0.0    84      152   06 15 21

06 17 20  J1832-2039   18 34 12  84.8 357.3  0.0       0.0   -36      152   No stop 
06 20 20  =1829-207    18 37 12  84.7 349.7  0.1       0.0   144      155   06 17 21

06 20 20 G012.68-0.18  18 37 12  80.6 325.5  0.4       0.0   -36      155   No stop 
06 22 20  ---          18 39 13  80.3 323.1  0.4       0.0    84      157   06 20 21

06 22 20  J1832-2039   18 39 13  84.6 344.8  0.1       0.0   -36      157   No stop 
06 25 20  =1829-207    18 42 13  84.4 337.8  0.2       0.0   144      160   06 22 21

06 25 20 G012.68-0.18  18 42 13  79.9 319.8  0.5       0.0   -36      160   No stop 
06 27 20  ---          18 44 14  79.6 317.7  0.5       0.0    84      162   06 25 21

06 28 00  J1832-2039   18 44 54  84.1 332.1  0.2       0.0     4      162   06 28 00
06 31 00  =1829-207    18 47 54  83.8 326.3  0.2       0.0   180      164   06 28 01

06 49 50  J1832-2039   19 06 47  80.7 302.4  0.6       0.0  1108      164   06 49 50
06 52 50  =1829-207    19 09 48  80.1 300.0  0.6       0.0   180      167   06 49 51

06 52 50 G012.68-0.18  19 09 48  75.0 299.0  0.9       0.0   -36      167   No stop 
06 54 50  ---          19 11 48  74.6 298.0  0.9       0.0    84      169   06 52 51

06 54 50  J1832-2039   19 11 48  79.7 298.6  0.6       0.0   -36      169   No stop 
06 57 50  =1829-207    19 14 49  79.1 296.6  0.7       0.0   144      172   06 54 51

06 57 50 G012.68-0.18  19 14 49  74.0 296.5  1.0       0.0   -36      172   No stop 
06 59 50  ---          19 16 49  73.6 295.6  1.0       0.0    84      174   06 57 51

06 59 50  J1832-2039   19 16 49  78.7 295.3  0.7       0.0   -36      174   No stop 
07 02 50  =1829-207    19 19 49  78.1 293.6  0.8       0.0   144      177   06 59 51

07 02 50 G012.68-0.18  19 19 49  73.0 294.3  1.1       0.0   -36      177   No stop 
07 04 50  ---          19 21 50  72.6 293.5  1.1       0.0    84      179   07 02 51

07 05 30  J1832-2039   19 22 30  77.5 292.3  0.8       0.0     4      179   07 05 30
07 08 30  =1829-207    19 25 30  76.9 290.8  0.9       0.0   180      182   07 05 31

07 08 30 G012.68-0.18  19 25 30  71.9 292.1  1.2       0.0   -36      182   No stop 
07 10 30  ---          19 27 31  71.4 291.4  1.2       0.0    84      184   07 08 31

07 10 30  J1832-2039   19 27 31  76.5 290.0  0.9       0.0   -36      184   No stop 
07 13 30  =1829-207    19 30 31  75.8 288.7  1.0       0.0   144      187   07 10 31
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
----------------------------------------------------------------------------------------

 --- Sat  27 Feb 2016   Day  58 ---

07 13 30 G012.68-0.18  19 30 31  70.8 290.4  1.3       0.0   -36      187   No stop 
07 15 30  ---          19 32 32  70.4 289.7  1.3       0.0    84      188   07 13 31

07 15 30  J1832-2039   19 32 32  75.4 288.0  1.0       0.0   -36      188   No stop 
07 18 30  =1829-207    19 35 32  74.8 286.9  1.0       0.0   144      191   07 15 31

07 18 30 G012.68-0.18  19 35 32  69.7 288.8  1.3       0.0   -36      191   No stop 
07 20 30  ---          19 37 32  69.3 288.2  1.4       0.0    84      193   07 18 31

07 21 10  J1832-2039   19 38 12  74.2 286.0  1.1       0.0     4      193   07 21 10
07 24 10  =1829-207    19 41 13  73.5 285.0  1.1       0.0   180      196   07 21 11

07 24 10 G012.68-0.18  19 41 13  68.5 287.1  1.4       0.0   -36      196   No stop 
07 26 10  ---          19 43 13  68.1 286.6  1.5       0.0    84      198   07 24 11

07 26 10  J1832-2039   19 43 13  73.1 284.4  1.2       0.0   -36      198   No stop 
07 29 10  =1829-207    19 46 14  72.4 283.6  1.2       0.0   144      201   07 26 11

07 29 10 G012.68-0.18  19 46 14  67.4 285.8  1.5       0.0   -36      201   No stop 
07 31 10  ---          19 48 14  67.0 285.3  1.6       0.0    84      203   07 29 11

07 31 10  J1832-2039   19 48 14  72.0 283.0  1.3       0.0   -36      203   No stop 
07 34 10  =1829-207    19 51 15  71.3 282.2  1.3       0.0   144      206   07 31 11

07 52 50  J1832-2039   20 09 58  67.2 278.2  1.6       0.0  1098      206   07 52 50
07 55 50  =1829-207    20 12 58  66.5 277.7  1.7       0.0   180      209   07 52 51

07 55 50 G012.68-0.18  20 12 58  61.6 280.0  2.0       0.0   -36      209   No stop 
07 57 50  ---          20 14 58  61.1 279.7  2.0       0.0    84      211   07 55 51

07 57 50  J1832-2039   20 14 58  66.1 277.3  1.7       0.0   -36      211   No stop 
08 00 50  =1829-207    20 17 59  65.4 276.8  1.7       0.0   144      213   07 57 51

08 00 50 G012.68-0.18  20 17 59  60.5 279.1  2.1       0.0   -36      213   No stop 
08 02 50  ---          20 19 59  60.0 278.8  2.1       0.0    84      215   08 00 51

08 02 50  J1832-2039   20 19 59  65.0 276.5  1.8       0.0   -36      215   No stop 
08 05 50  =1829-207    20 23 00  64.3 276.0  1.8       0.0   144      218   08 02 51

08 05 50 G012.68-0.18  20 23 00  59.3 278.3  2.1       0.0   -36      218   No stop 
08 07 50  ---          20 25 00  58.9 278.0  2.2       0.0    84      220   08 05 51

08 08 30  J1832-2039   20 25 40  63.7 275.6  1.9       0.0     4      220   08 08 30
08 11 30  =1829-207    20 28 41  63.0 275.1  1.9       0.0   180      223   08 08 31
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
----------------------------------------------------------------------------------------

 --- Sat  27 Feb 2016   Day  58 ---

08 11 30 G012.68-0.18  20 28 41  58.1 277.4  2.2       0.0   -36      223   No stop 
08 13 30  ---          20 30 41  57.6 277.1  2.3       0.0    84      225   08 11 31

08 13 30  J1832-2039   20 30 41  62.6 274.8  2.0       0.0   -36      225   No stop 
08 16 30  =1829-207    20 33 42  61.9 274.4  2.0       0.0   144      228   08 13 31

08 16 30 G012.68-0.18  20 33 42  57.0 276.6  2.3       0.0   -36      228   No stop 
08 18 30  ---          20 35 42  56.5 276.3  2.3       0.0    84      230   08 16 31

08 18 30  J1832-2039   20 35 42  61.4 274.1  2.0       0.0   -36      230   No stop 
08 21 30  =1829-207    20 38 42  60.8 273.7  2.1       0.0   144      233   08 18 31

08 21 30 G012.68-0.18  20 38 42  55.8 275.9  2.4       0.0   -36      233   No stop 
08 23 30  ---          20 40 43  55.4 275.6  2.4       0.0    84      235   08 21 31

08 24 10  J1832-2039   20 41 23  60.2 273.3  2.1       0.0     4      235   08 24 10
08 27 10  =1829-207    20 44 23  59.5 273.0  2.2       0.0   180      237   08 24 11

08 27 10 G012.68-0.18  20 44 23  54.6 275.1  2.5       0.0   -36      237   No stop 
08 29 10  ---          20 46 24  54.1 274.8  2.5       0.0    84      239   08 27 11

08 29 10  J1832-2039   20 46 24  59.0 272.7  2.2       0.0   -36      239   No stop 
08 32 10  =1829-207    20 49 24  58.4 272.3  2.3       0.0   144      242   08 29 11

08 32 10 G012.68-0.18  20 49 24  53.4 274.4  2.6       0.0   -36      242   No stop 
08 34 10  ---          20 51 24  53.0 274.2  2.6       0.0    84      244   08 32 11

08 34 50  J1832-2039   20 52 05  57.8 272.0  2.3       0.0     4      244   08 34 50
08 37 50  =1829-207    20 55 05  57.1 271.6  2.4       0.0   180      247   08 34 51

08 56 20  J1832-2039   21 13 38  52.9 269.5  2.7       0.0  1088      247   08 56 20
08 59 20  =1829-207    21 16 39  52.2 269.2  2.7       0.0   180      250   08 56 21

08 59 20 G012.68-0.18  21 16 39  47.3 271.1  3.0       0.0   -36      250   No stop 
09 01 20  ---          21 18 39  46.9 270.9  3.1       0.0    84      252   08 59 21

09 01 20  J1832-2039   21 18 39  51.8 269.0  2.8       0.0   -36      252   No stop 
09 04 20  =1829-207    21 21 39  51.1 268.7  2.8       0.0   144      255   09 01 21

09 04 20 G012.68-0.18  21 21 39  46.2 270.5  3.1       0.0   -36      255   No stop 
09 06 20  ---          21 23 40  45.7 270.3  3.1       0.0    84      257   09 04 21

09 06 20  J1832-2039   21 23 40  50.7 268.5  2.8       0.0   -36      257   No stop 
09 09 20  =1829-207    21 26 40  50.0 268.2  2.9       0.0   144      260   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
----------------------------------------------------------------------------------------

 --- Sat  27 Feb 2016   Day  58 ---

09 09 20 G012.68-0.18  21 26 40  45.1 270.0  3.2       0.0   -36      260   No stop 
09 11 20  ---          21 28 41  44.6 269.8  3.2       0.0    84      262   09 09 21

09 12 01  J1832-2039   21 29 22  49.4 267.9  2.9       0.0     5      262   09 12 01
09 15 01  =1829-207    21 32 22  48.7 267.6  3.0       0.0   180      264   09 12 02

09 15 01 G012.68-0.18  21 32 22  43.8 269.4  3.3       0.0   -36      264   No stop 
09 17 01  ---          21 34 22  43.3 269.2  3.3       0.0    84      266   09 15 02

09 17 01  J1832-2039   21 34 22  48.2 267.4  3.0       0.0   -36      266   No stop 
09 20 01  =1829-207    21 37 23  47.6 267.1  3.1       0.0   144      269   09 17 02

09 20 01 G012.68-0.18  21 37 23  42.7 268.8  3.4       0.0   -36      269   No stop 
09 22 01  ---          21 39 23  42.2 268.6  3.4       0.0    84      271   09 20 02

09 22 01  J1832-2039   21 39 23  47.1 266.9  3.1       0.0   -36      271   No stop 
09 25 01  =1829-207    21 42 24  46.4 266.7  3.2       0.0   144      274   09 22 02

09 25 01 G012.68-0.18  21 42 24  41.5 268.3  3.5       0.0   -36      274   No stop 
09 27 01  ---          21 44 24  41.1 268.1  3.5       0.0    84      276   09 25 02

09 27 42  J1832-2039   21 45 05  45.8 266.4  3.2       0.0     5      276   09 27 42
09 30 42  =1829-207    21 48 06  45.2 266.1  3.2       0.0   180      279   09 27 43

09 30 42 G012.68-0.18  21 48 06  40.3 267.7  3.6       0.0   -36      279   No stop 
09 32 42  ---          21 50 06  39.8 267.5  3.6       0.0    84      281   09 30 43

09 32 42  J1832-2039   21 50 06  44.7 265.9  3.3       0.0   -36      281   No stop 
09 35 42  =1829-207    21 53 07  44.0 265.6  3.3       0.0   144      284   09 32 43

09 35 42 G012.68-0.18  21 53 07  39.1 267.2  3.6       0.0   -36      284   No stop 
09 37 42  ---          21 55 07  38.7 267.0  3.7       0.0    84      286   09 35 43

09 38 23  J1832-2039   21 55 48  43.4 265.4  3.4       0.0     5      286   09 38 23
09 41 23  =1829-207    21 58 49  42.8 265.1  3.4       0.0   180      288   09 38 24

09 58 33  J1832-2039   22 16 01  38.9 263.6  3.7       0.0  1008      288   09 58 33
10 01 33  =1829-207    22 19 02  38.2 263.3  3.8       0.0   180      291   09 58 34

10 01 33 G012.68-0.18  22 19 02  33.3 264.7  4.1       0.0   -36      291   No stop 
10 03 33  ---          22 21 02  32.9 264.5  4.1       0.0    84      293   10 01 34

10 03 33  J1832-2039   22 21 02  37.8 263.1  3.8       0.0   -36      293   No stop 
10 06 33  =1829-207    22 24 03  37.1 262.9  3.8       0.0   144      296   10 03 34
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
----------------------------------------------------------------------------------------

 --- Sat  27 Feb 2016   Day  58 ---

10 06 33 G012.68-0.18  22 24 03  32.2 264.2  4.2       0.0   -36      296   No stop 
10 08 33  ---          22 26 03  31.7 264.0  4.2       0.0    84      298   10 06 34

10 08 33  J1832-2039   22 26 03  36.7 262.7  3.9       0.0   -36      298   No stop 
10 11 33  =1829-207    22 29 03  36.0 262.4  3.9       0.0   144      301   10 08 34

10 11 33 G012.68-0.18  22 29 03  31.1 263.7  4.2       0.0   -36      301   No stop 
10 13 33  ---          22 31 04  30.6 263.6  4.3       0.0    84      303   10 11 34

10 14 13  J1832-2039   22 31 44  35.4 262.2  4.0       0.0     4      303   10 14 13
10 17 13  =1829-207    22 34 44  34.7 261.9  4.0       0.0   180      306   10 14 14

10 17 13 G012.68-0.18  22 34 44  29.8 263.2  4.3       0.0   -36      306   No stop 
10 19 13  ---          22 36 45  29.4 263.0  4.4       0.0    84      308   10 17 14

10 19 13  J1832-2039   22 36 45  34.3 261.8  4.1       0.0   -36      308   No stop 
10 22 13  =1829-207    22 39 45  33.6 261.5  4.1       0.0   144      311   10 19 14

10 22 13 G012.68-0.18  22 39 45  28.7 262.7  4.4       0.0   -36      311   No stop 
10 24 13  ---          22 41 46  28.2 262.5  4.4       0.0    84      312   10 22 14

10 24 13  J1832-2039   22 41 46  33.2 261.3  4.1       0.0   -36      312   No stop 
10 27 13  =1829-207    22 44 46  32.5 261.1  4.2       0.0   144      315   10 24 14

10 27 13 G012.68-0.18  22 44 46  27.6 262.3  4.5       0.0   -36      315   No stop 
10 29 13  ---          22 46 46  27.1 262.1  4.5       0.0    84      317   10 27 14

10 29 53  J1832-2039   22 47 26  31.9 260.8  4.2       0.0     4      317   10 29 53
10 32 53  =1829-207    22 50 27  31.2 260.6  4.3       0.0   180      320   10 29 54

10 32 53 G012.68-0.18  22 50 27  26.3 261.7  4.6       0.0   -36      320   No stop 
10 34 53  ---          22 52 27  25.9 261.5  4.6       0.0    84      322   10 32 54

10 34 53  J1832-2039   22 52 27  30.8 260.4  4.3       0.0   -36      322   No stop 
10 37 53  =1829-207    22 55 28  30.1 260.1  4.4       0.0   144      325   10 34 54

10 37 53 G012.68-0.18  22 55 28  25.2 261.3  4.7       0.0   -36      325   No stop 
10 39 53  ---          22 57 28  24.7 261.1  4.7       0.0    84      327   10 37 54

10 40 33  J1832-2039   22 58 08  29.5 259.9  4.4       0.0     4      327   10 40 33
10 43 33  =1829-207    23 01 09  28.9 259.6  4.5       0.0   180      330   10 40 34

11 04 43  J1832-2039   23 22 22  24.2 257.8  4.8       0.0  1248      330   11 04 43
11 07 43  =1829-207    23 25 23  23.5 257.5  4.9       0.0   180      333   11 04 44
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
----------------------------------------------------------------------------------------

 --- Sat  27 Feb 2016   Day  58 ---

11 07 43 G012.68-0.18  23 25 23  18.6 258.5  5.2       0.0   -36      333   No stop 
11 09 43  ---          23 27 23  18.1 258.3  5.2       0.0    84      335   11 07 44

11 09 43  J1832-2039   23 27 23  23.1 257.3  4.9       0.0   -36      335   No stop 
11 12 43  =1829-207    23 30 24  22.4 257.1  5.0       0.0   144      337   11 09 44

11 12 43 G012.68-0.18  23 30 24  17.5 258.0  5.3       0.0   -36      337   No stop 
11 14 43  ---          23 32 24  17.0 257.8  5.3       0.0    84      339   11 12 44

11 14 43  J1832-2039   23 32 24  22.0 256.9  5.0       0.0   -36      339   No stop 
11 17 43  =1829-207    23 35 24  21.3 256.6  5.0       0.0   144      342   11 14 44

11 17 43 G012.68-0.18  23 35 24  16.4 257.5  5.3       0.0   -36      342   No stop 
11 19 43  ---          23 37 25  15.9 257.3  5.4       0.0    84      344   11 17 44

11 20 23  J1832-2039   23 38 05  20.7 256.4  5.1       0.0     4      344   11 20 23
11 23 23  =1829-207    23 41 05  20.1 256.1  5.1       0.0   180      347   11 20 24

11 23 23 G012.68-0.18  23 41 05  15.1 257.0  5.4       0.0   -36      347   No stop 
11 25 23  ---          23 43 06  14.7 256.8  5.5       0.0    84      349   11 23 24

11 25 23  J1832-2039   23 43 06  19.7 255.9  5.2       0.0   -36      349   No stop 
11 29 53  =1829-207    23 47 36  18.7 255.5  5.2       0.0   234      353   11 25 24


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


 ======== Setup file: sess116.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: 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=   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=   6665.14  6665.14  6665.14  6665.14  6669.13  6669.13  6669.13  6669.13
             6673.13  6673.13  6673.13  6673.13  6677.13  6677.13  6677.13  6677.13
   BBC fr=    155.14   155.14   155.14   155.14   159.13   159.13   159.13   159.13
              163.13   163.13   163.13   163.13   167.13   167.13   167.13   167.13
   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=  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)

 * G012.68-0.18      18 10 59.237691   * 18 13 54.750000     18 14 50.683477       0.00
                    -18 02 40.99379    *-18 01 46.57000     -18 01 19.53498        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 52.276392       1.30
   J0319+4130        41 19 51.91701    * 41 30 42.10413      41 34 09.42345        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 53.636002       0.18
 * J1331+3030        30 45 58.64059    * 30 30 32.95924      30 25 24.85410        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 31.125669       0.76
   J1642+3948        39 54 10.81496    * 39 48 36.99402      39 46 40.96182        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 07.898771       0.28
 * J1832-2039       -20 42 02.03615    *-20 39 48.20378     -20 38 55.03370        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 22.032751       0.00
 * J2202+4216        42 02 08.59077    * 42 16 39.97990      42 21 19.67288        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
  G012.68-0.1sess116.M128          1 2 3 4 5 6 7 8 9                 1.867    54.003
  3C84       sess116.M128          1 2 3 4 5 6 7 8                   0.133     4.800
  J1331+3030 sess116.M128          1 2 3 4 5 6 7 8 9                 1.317    49.300
  3C345      sess116.M128          1 2 3 4 5 6 7 8 9                 0.333    15.000
  J1832-2039 sess116.M128          1 2 3 4 5 6 7 8 9                 3.258   105.633
  J2202+4216 sess116.M128          1 3 4 5 6 7 8                     0.167     4.538


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        64.7
   3C84                81.4
   J1331+3030         134.2
   3C345               94.6
   J1832-2039          60.4
   J2202+4216          51.5

  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 

