  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel
 Exp. Code:  EM117C  


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 = IRAS18264-1152
 
 

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
----------------------------------------------------------------------------------------

 --- Mon  29 Feb 2016   Day  60 ---

 Next scan frequencies:  6665.38  6665.38  6665.38  6665.38  6669.38  6669.38  6669.38  6669.38
                         6673.38  6673.38  6673.38  6673.38  6677.38  6677.38  6677.38  6677.38
 Next BBC frequencies:    155.38   155.38   155.38   155.38   159.38   159.38   159.38   159.38
                          163.38   163.38   163.38   163.38   167.38   167.38   167.38   167.38
 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 45 35  J1331+3030   15 09 45  29.0 335.9  1.6       0.0     0        0   02 45 35
02 50 35  =3C286       15 14 46  28.5 334.8  1.7       0.0   300        5   02 45 36

02 51 00  J1331+3030   15 15 11  28.5 334.7  1.7       0.0     4        5   02 51 00
02 59 00  =3C286       15 23 13  27.7 333.0  1.9       0.0   480       12   02 51 01

03 03 35  3C345        15 27 48  22.0  15.6 -1.3       0.0   153       12   03 03 35
03 13 35  ---          15 37 50  22.6  13.6 -1.1       0.0   600       22   03 03 36

03 29 45  J1825-1718   15 54 03  53.7  84.1 -2.5       0.0   829       22   03 29 45
03 34 45  =1822-173    15 59 03  54.8  83.4 -2.5       0.0   300       27   03 29 46

03 34 45 IRAS18264-11  15 59 03  51.8  75.6 -2.5       0.0   -38       27   No stop 
03 36 45  ---          16 01 04  52.2  75.3 -2.5       0.0    82       29   03 34 46

03 37 25  J1825-1718   16 01 44  55.4  83.0 -2.4       0.0     2       29   03 37 25
03 40 25  =1822-173    16 04 44  56.1  82.6 -2.4       0.0   180       32   03 37 26

03 40 25 IRAS18264-11  16 04 44  53.0  74.6 -2.4       0.0   -38       32   No stop 
03 42 25  ---          16 06 45  53.4  74.2 -2.4       0.0    82       34   03 40 26

03 42 25  J1825-1718   16 06 45  56.5  82.3 -2.3       0.0   -38       34   No stop 
03 45 25  =1822-173    16 09 45  57.2  81.8 -2.3       0.0   142       37   03 42 26

03 45 25 IRAS18264-11  16 09 45  54.1  73.6 -2.3       0.0   -38       37   No stop 
03 47 25  ---          16 11 45  54.5  73.2 -2.3       0.0    82       38   03 45 26

03 48 00  J1825-1718   16 12 21  57.7  81.4 -2.2       0.0    -3       38   03 48 00
03 51 00  =1822-173    16 15 21  58.4  80.9 -2.2       0.0   177       41   03 48 01

03 51 00 IRAS18264-11  16 15 21  55.3  72.5 -2.2       0.0   -38       41   No stop 
03 53 00  ---          16 17 21  55.7  72.1 -2.2       0.0    82       43   03 51 01

03 53 00  J1825-1718   16 17 21  58.9  80.6 -2.2       0.0   -38       43   No stop 
03 56 00  =1822-173    16 20 22  59.5  80.0 -2.1       0.0   142       46   03 53 01

03 56 00 IRAS18264-11  16 20 22  56.4  71.4 -2.2       0.0   -38       46   No stop 
03 58 00  ---          16 22 22  56.8  71.0 -2.1       0.0    82       48   03 56 01
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
----------------------------------------------------------------------------------------

 --- Mon  29 Feb 2016   Day  60 ---

03 58 00  J1825-1718   16 22 22  60.0  79.7 -2.1       0.0   -38       48   No stop 
04 01 00  =1822-173    16 25 23  60.6  79.1 -2.0       0.0   142       51   03 58 01

04 01 00 IRAS18264-11  16 25 23  57.4  70.3 -2.1       0.0   -38       51   No stop 
04 03 00  ---          16 27 23  57.9  69.9 -2.0       0.0    82       53   04 01 01

04 03 40  J1825-1718   16 28 03  61.2  78.6 -2.0       0.0     2       53   04 03 40
04 06 40  =1822-173    16 31 04  61.9  78.1 -1.9       0.0   180       56   04 03 41

04 06 40 IRAS18264-11  16 31 04  58.6  69.0 -2.0       0.0   -38       56   No stop 
04 08 40  ---          16 33 04  59.1  68.5 -2.0       0.0    82       58   04 06 41

04 08 40  J1825-1718   16 33 04  62.3  77.7 -1.9       0.0   -38       58   No stop 
04 11 40  =1822-173    16 36 04  63.0  77.0 -1.8       0.0   142       61   04 08 41

04 28 25  J1825-1718   16 52 52  66.6  73.1 -1.6       0.0   983       61   04 28 25
04 31 25  =1822-173    16 55 53  67.3  72.3 -1.5       0.0   180       63   04 28 26

04 31 25 IRAS18264-11  16 55 53  63.7  62.1 -1.6       0.0   -38       63   No stop 
04 33 25  ---          16 57 53  64.1  61.4 -1.5       0.0    82       65   04 31 26

04 33 25  J1825-1718   16 57 53  67.7  71.8 -1.5       0.0   -38       65   No stop 
04 36 25  =1822-173    17 00 54  68.4  70.9 -1.4       0.0   142       68   04 33 26

04 36 25 IRAS18264-11  17 00 54  64.7  60.4 -1.5       0.0   -38       68   No stop 
04 38 25  ---          17 02 54  65.1  59.7 -1.5       0.0    82       70   04 36 26

04 38 25  J1825-1718   17 02 54  68.8  70.3 -1.4       0.0   -38       70   No stop 
04 41 25  =1822-173    17 05 54  69.4  69.4 -1.3       0.0   142       73   04 38 26

04 41 25 IRAS18264-11  17 05 54  65.7  58.6 -1.4       0.0   -38       73   No stop 
04 43 25  ---          17 07 55  66.1  57.9 -1.4       0.0    82       75   04 41 26

04 44 05  J1825-1718   17 08 35  70.0  68.5 -1.3       0.0     2       75   04 44 05
04 47 05  =1822-173    17 11 35  70.6  67.5 -1.2       0.0   180       78   04 44 06

04 47 05 IRAS18264-11  17 11 35  66.8  56.4 -1.3       0.0   -38       78   No stop 
04 49 05  ---          17 13 36  67.1  55.6 -1.3       0.0    82       80   04 47 06

04 49 05  J1825-1718   17 13 36  71.0  66.7 -1.2       0.0   -38       80   No stop 
04 52 05  =1822-173    17 16 36  71.6  65.6 -1.2       0.0   142       83   04 49 06

04 52 05 IRAS18264-11  17 16 36  67.7  54.4 -1.2       0.0   -38       83   No stop 
04 54 05  ---          17 18 36  68.0  53.5 -1.2       0.0    82       85   04 52 06
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
----------------------------------------------------------------------------------------

 --- Mon  29 Feb 2016   Day  60 ---

04 54 05  J1825-1718   17 18 36  72.1  64.8 -1.1       0.0   -38       85   No stop 
04 57 05  =1822-173    17 21 37  72.7  63.6 -1.1       0.0   142       87   04 54 06

04 57 05 IRAS18264-11  17 21 37  68.6  52.1 -1.1       0.0   -38       87   No stop 
04 59 05  ---          17 23 37  68.9  51.2 -1.1       0.0    82       89   04 57 06

04 59 45  J1825-1718   17 24 17  73.2  62.4 -1.0       0.0     2       89   04 59 45
05 02 45  =1822-173    17 27 18  73.8  61.0 -1.0       0.0   180       92   04 59 46

05 02 45 IRAS18264-11  17 27 18  69.6  49.4 -1.0       0.0   -38       92   No stop 
05 04 45  ---          17 29 18  69.9  48.4 -1.0       0.0    82       94   05 02 46

05 04 45  J1825-1718   17 29 18  74.2  60.0 -1.0       0.0   -38       94   No stop 
05 07 45  =1822-173    17 32 19  74.8  58.4 -0.9       0.0   142       97   05 04 46

05 24 50  J1825-1718   17 49 26  77.8  46.9 -0.6       0.0  1003       97   05 24 50
05 27 50  =1822-173    17 52 27  78.3  44.3 -0.6       0.0   180      100   05 24 51

05 27 50 IRAS18264-11  17 52 27  73.4  34.0 -0.6       0.0   -38      100   No stop 
05 29 50  ---          17 54 27  73.6  32.5 -0.6       0.0    82      102   05 27 51

05 29 50  J1825-1718   17 54 27  78.6  42.5 -0.5       0.0   -38      102   No stop 
05 32 50  =1822-173    17 57 28  79.1  39.6 -0.5       0.0   142      105   05 29 51

05 32 50 IRAS18264-11  17 57 28  74.0  30.2 -0.5       0.0   -38      105   No stop 
05 34 50  ---          17 59 28  74.2  28.6 -0.5       0.0    82      107   05 32 51

05 34 50  J1825-1718   17 59 28  79.4  37.5 -0.5       0.0   -38      107   No stop 
05 37 50  =1822-173    18 02 29  79.8  34.2 -0.4       0.0   142      110   05 34 51

05 37 50 IRAS18264-11  18 02 29  74.5  26.2 -0.5       0.0   -38      110   No stop 
05 39 50  ---          18 04 29  74.7  24.5 -0.4       0.0    82      112   05 37 51

05 40 32  J1825-1718   18 05 11  80.1  31.1 -0.4       0.0     4      112   05 40 32
05 43 32  =1822-173    18 08 12  80.4  27.3 -0.3       0.0   180      114   05 40 33

05 43 32 IRAS18264-11  18 08 12  75.0  21.2 -0.4       0.0   -38      114   No stop 
05 45 32  ---          18 10 12  75.2  19.4 -0.3       0.0    82      116   05 43 33

05 45 32  J1825-1718   18 10 12  80.6  24.6 -0.3       0.0   -38      116   No stop 
05 48 32  =1822-173    18 13 12  80.9  20.5 -0.2       0.0   142      119   05 45 33

05 48 32 IRAS18264-11  18 13 12  75.4  16.6 -0.3       0.0   -38      119   No stop 
05 50 32  ---          18 15 13  75.5  14.7 -0.2       0.0    82      121   05 48 33
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
----------------------------------------------------------------------------------------

 --- Mon  29 Feb 2016   Day  60 ---

05 50 32  J1825-1718   18 15 13  81.0  17.6 -0.2       0.0   -38      121   No stop 
05 53 32  =1822-173    18 18 13  81.2  13.1 -0.1       0.0   142      124   05 50 33

05 53 32 IRAS18264-11  18 18 13  75.7  11.8 -0.2       0.0   -38      124   No stop 
05 55 32  ---          18 20 14  75.7   9.9 -0.2       0.0    82      126   05 53 33

05 56 14  J1825-1718   18 20 56  81.3   8.9 -0.1       0.0     4      126   05 56 14
05 59 14  =1822-173    18 23 56  81.4   4.1 -0.0       0.0   180      129   05 56 15

05 59 14 IRAS18264-11  18 23 56  75.9   6.2 -0.1       0.0   -38      129   No stop 
06 01 14  ---          18 25 56  75.9   4.2 -0.1       0.0    82      131   05 59 15

06 01 14  J1825-1718   18 25 56  81.4   1.0 -0.0       0.0   -38      131   No stop 
06 04 14  =1822-173    18 28 57  81.4 356.1  0.0       0.0   142      134   06 01 15

06 21 44  J1825-1718   18 46 30  80.2 330.7  0.3       0.0  1028      134   06 21 44
06 24 44  =1822-173    18 49 30  79.9 327.0  0.4       0.0   180      137   06 21 45

06 24 44 IRAS18264-11  18 49 30  75.2 341.1  0.3       0.0   -38      137   No stop 
06 26 44  ---          18 51 31  75.1 339.3  0.4       0.0    82      138   06 24 45

06 26 44  J1825-1718   18 51 31  79.6 324.7  0.4       0.0   -38      138   No stop 
06 29 44  =1822-173    18 54 31  79.2 321.5  0.5       0.0   142      141   06 26 45

06 29 44 IRAS18264-11  18 54 31  74.8 336.6  0.4       0.0   -38      141   No stop 
06 31 44  ---          18 56 31  74.6 334.9  0.4       0.0    82      143   06 29 45

06 31 44  J1825-1718   18 56 31  78.9 319.5  0.5       0.0   -38      143   No stop 
06 34 44  =1822-173    18 59 32  78.5 316.6  0.5       0.0   142      146   06 31 45

06 34 44 IRAS18264-11  18 59 32  74.3 332.4  0.5       0.0   -38      146   No stop 
06 36 44  ---          19 01 32  74.1 330.8  0.5       0.0    82      148   06 34 45

06 37 29  J1825-1718   19 02 17  78.1 314.2  0.6       0.0     7      148   06 37 29
06 40 29  =1822-173    19 05 18  77.6 311.7  0.6       0.0   180      151   06 37 30

06 40 29 IRAS18264-11  19 05 18  73.7 327.8  0.6       0.0   -38      151   No stop 
06 42 29  ---          19 07 18  73.4 326.3  0.6       0.0    82      153   06 40 30

06 42 29  J1825-1718   19 07 18  77.2 310.2  0.7       0.0   -38      153   No stop 
06 45 29  =1822-173    19 10 19  76.7 308.0  0.7       0.0   142      156   06 42 30

06 45 29 IRAS18264-11  19 10 19  73.0 324.2  0.7       0.0   -38      156   No stop 
06 47 29  ---          19 12 19  72.8 322.8  0.7       0.0    82      158   06 45 30
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
----------------------------------------------------------------------------------------

 --- Mon  29 Feb 2016   Day  60 ---

06 47 29  J1825-1718   19 12 19  76.3 306.7  0.8       0.0   -38      158   No stop 
06 50 29  =1822-173    19 15 20  75.8 304.7  0.8       0.0   142      161   06 47 30

06 50 29 IRAS18264-11  19 15 20  72.4 320.7  0.8       0.0   -38      161   No stop 
06 52 29  ---          19 17 20  72.1 319.5  0.8       0.0    82      162   06 50 30

06 53 14  J1825-1718   19 18 05  75.3 303.1  0.9       0.0     7      162   06 53 14
06 56 14  =1822-173    19 21 05  74.7 301.4  0.9       0.0   180      165   06 53 15

06 56 14 IRAS18264-11  19 21 05  71.5 317.1  0.8       0.0   -38      165   No stop 
06 58 14  ---          19 23 06  71.2 315.9  0.9       0.0    82      167   06 56 15

06 58 14  J1825-1718   19 23 06  74.3 300.4  0.9       0.0   -38      167   No stop 
07 01 14  =1822-173    19 26 06  73.7 298.9  1.0       0.0   142      170   06 58 15

07 06 09  J2202+4216   19 31 02  13.2  27.9 -2.5       0.0   149      170   07 06 09
07 14 09  =VR422201    19 39 03  14.1  26.7 -2.4       0.0   480      178   07 06 10

07 19 14  J1825-1718   19 44 09  70.1 291.6  1.3       0.0   159      178   07 19 14
07 22 14  =1822-173    19 47 10  69.4 290.6  1.3       0.0   180      181   07 19 15

07 22 14 IRAS18264-11  19 47 10  67.0 304.2  1.3       0.0   -38      181   No stop 
07 24 14  ---          19 49 10  66.7 303.4  1.3       0.0    82      183   07 22 15

07 24 14  J1825-1718   19 49 10  69.0 290.0  1.4       0.0   -38      183   No stop 
07 27 14  =1822-173    19 52 11  68.4 289.1  1.4       0.0   142      186   07 24 15

07 27 14 IRAS18264-11  19 52 11  66.1 302.2  1.4       0.0   -38      186   No stop 
07 29 14  ---          19 54 11  65.7 301.4  1.4       0.0    82      187   07 27 15

07 29 14  J1825-1718   19 54 11  67.9 288.5  1.5       0.0   -38      187   No stop 
07 32 14  =1822-173    19 57 11  67.3 287.7  1.5       0.0   142      190   07 29 15

07 32 14 IRAS18264-11  19 57 11  65.1 300.4  1.5       0.0   -38      190   No stop 
07 34 14  ---          19 59 12  64.7 299.7  1.5       0.0    82      192   07 32 15

07 34 59  J1825-1718   19 59 57  66.7 286.9  1.6       0.0     7      192   07 34 59
07 37 59  =1822-173    20 02 57  66.0 286.2  1.6       0.0   180      195   07 35 00

07 37 59 IRAS18264-11  20 02 57  64.0 298.4  1.5       0.0   -38      195   No stop 
07 39 59  ---          20 04 58  63.6 297.7  1.6       0.0    82      197   07 38 00

07 39 59  J1825-1718   20 04 58  65.6 285.7  1.6       0.0   -38      197   No stop 
07 42 59  =1822-173    20 07 58  65.0 284.9  1.7       0.0   142      200   07 40 00
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
----------------------------------------------------------------------------------------

 --- Mon  29 Feb 2016   Day  60 ---

07 42 59 IRAS18264-11  20 07 58  63.0 296.8  1.6       0.0   -38      200   No stop 
07 44 59  ---          20 09 58  62.6 296.2  1.7       0.0    82      202   07 43 00

07 44 59  J1825-1718   20 09 58  64.5 284.5  1.7       0.0   -38      202   No stop 
07 47 59  =1822-173    20 12 59  63.9 283.8  1.8       0.0   142      205   07 45 00

07 47 59 IRAS18264-11  20 12 59  62.0 295.3  1.7       0.0   -38      205   No stop 
07 49 59  ---          20 14 59  61.6 294.7  1.7       0.0    82      207   07 48 00

07 50 44  J1825-1718   20 15 44  63.3 283.2  1.8       0.0     7      207   07 50 44
07 53 44  =1822-173    20 18 45  62.6 282.6  1.9       0.0   180      210   07 50 45

07 53 44 IRAS18264-11  20 18 45  60.8 293.7  1.8       0.0   -38      210   No stop 
07 55 44  ---          20 20 45  60.4 293.1  1.8       0.0    82      212   07 53 45

07 55 44  J1825-1718   20 20 45  62.2 282.2  1.9       0.0   -38      212   No stop 
07 58 44  =1822-173    20 23 46  61.5 281.6  2.0       0.0   142      214   07 55 45

08 03 54  J2202+4216   20 28 57  18.4  18.2 -1.6       0.0   164      214   08 03 54
08 11 54  =VR422201    20 36 58  18.9  16.7 -1.4       0.0   480      222   08 03 55

08 17 09  J1825-1718   20 42 14  57.4 278.4  2.3       0.0   169      222   08 17 09
08 20 09  =1822-173    20 45 14  56.7 277.9  2.3       0.0   180      225   08 17 10

08 20 09 IRAS18264-11  20 45 14  55.2 287.4  2.3       0.0   -38      225   No stop 
08 22 09  ---          20 47 15  54.8 287.0  2.3       0.0    82      227   08 20 10

08 22 09  J1825-1718   20 47 15  56.3 277.6  2.3       0.0   -38      227   No stop 
08 25 09  =1822-173    20 50 15  55.6 277.1  2.4       0.0   142      230   08 22 10

08 25 09 IRAS18264-11  20 50 15  54.1 286.4  2.3       0.0   -38      230   No stop 
08 27 09  ---          20 52 15  53.7 286.0  2.4       0.0    82      232   08 25 10

08 27 09  J1825-1718   20 52 15  55.2 276.8  2.4       0.0   -38      232   No stop 
08 30 09  =1822-173    20 55 16  54.5 276.4  2.5       0.0   142      235   08 27 10

08 30 09 IRAS18264-11  20 55 16  53.1 285.5  2.4       0.0   -38      235   No stop 
08 32 09  ---          20 57 16  52.6 285.1  2.5       0.0    82      237   08 30 10

08 32 54  J1825-1718   20 58 01  53.9 276.0  2.5       0.0     7      237   08 32 54
08 35 54  =1822-173    21 01 02  53.2 275.6  2.6       0.0   180      239   08 32 55

08 35 54 IRAS18264-11  21 01 02  51.8 284.4  2.5       0.0   -38      239   No stop 
08 37 54  ---          21 03 02  51.4 284.0  2.5       0.0    82      241   08 35 55
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
----------------------------------------------------------------------------------------

 --- Mon  29 Feb 2016   Day  60 ---

08 37 54  J1825-1718   21 03 02  52.8 275.3  2.6       0.0   -38      241   No stop 
08 40 54  =1822-173    21 06 03  52.1 274.9  2.7       0.0   142      244   08 37 55

08 40 54 IRAS18264-11  21 06 03  50.7 283.5  2.6       0.0   -38      244   No stop 
08 42 54  ---          21 08 03  50.3 283.2  2.6       0.0    82      246   08 40 55

08 42 54  J1825-1718   21 08 03  51.6 274.6  2.7       0.0   -38      246   No stop 
08 45 54  =1822-173    21 11 03  51.0 274.2  2.7       0.0   142      249   08 42 55

08 45 54 IRAS18264-11  21 11 03  49.6 282.6  2.7       0.0   -38      249   No stop 
08 47 54  ---          21 13 04  49.2 282.3  2.7       0.0    82      251   08 45 55

08 48 39  J1825-1718   21 13 49  50.4 273.9  2.8       0.0     7      251   08 48 39
08 51 39  =1822-173    21 16 49  49.7 273.5  2.8       0.0   180      254   08 48 40

08 51 39 IRAS18264-11  21 16 49  48.3 281.7  2.8       0.0   -38      254   No stop 
08 53 39  ---          21 18 50  47.9 281.4  2.8       0.0    82      256   08 51 40

08 53 39  J1825-1718   21 18 50  49.2 273.2  2.9       0.0   -38      256   No stop 
08 56 39  =1822-173    21 21 50  48.6 272.9  2.9       0.0   142      259   08 53 40

09 01 54  J2202+4216   21 27 06  21.2   7.2 -0.6       0.0   169      259   09 01 54
09 09 54  =VR422201    21 35 07  21.4   5.6 -0.5       0.0   480      266   09 01 55

09 15 19  J1825-1718   21 40 33  44.3 270.7  3.2       0.0   179      266   09 15 19
09 18 19  =1822-173    21 43 34  43.7 270.4  3.3       0.0   180      269   09 15 20

09 18 19 IRAS18264-11  21 43 34  42.4 277.8  3.2       0.0   -38      269   No stop 
09 20 19  ---          21 45 34  42.0 277.5  3.3       0.0    82      271   09 18 20

09 20 19  J1825-1718   21 45 34  43.2 270.1  3.3       0.0   -38      271   No stop 
09 23 19  =1822-173    21 48 35  42.5 269.8  3.4       0.0   142      274   09 20 20

09 23 19 IRAS18264-11  21 48 35  41.3 277.1  3.3       0.0   -38      274   No stop 
09 25 19  ---          21 50 35  40.9 276.8  3.3       0.0    82      276   09 23 20

09 25 19  J1825-1718   21 50 35  42.1 269.6  3.4       0.0   -38      276   No stop 
09 28 19  =1822-173    21 53 35  41.4 269.3  3.5       0.0   142      279   09 25 20

09 28 19 IRAS18264-11  21 53 35  40.2 276.4  3.4       0.0   -38      279   No stop 
09 30 19  ---          21 55 36  39.7 276.2  3.4       0.0    82      281   09 28 20

09 31 04  J1825-1718   21 56 21  40.8 269.0  3.5       0.0     7      281   09 31 04
09 34 04  =1822-173    21 59 21  40.1 268.7  3.5       0.0   180      284   09 31 05
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
----------------------------------------------------------------------------------------

 --- Mon  29 Feb 2016   Day  60 ---

09 34 04 IRAS18264-11  21 59 21  38.9 275.7  3.5       0.0   -38      284   No stop 
09 36 04  ---          22 01 22  38.4 275.4  3.5       0.0    82      286   09 34 05

09 36 04  J1825-1718   22 01 22  39.7 268.5  3.6       0.0   -38      286   No stop 
09 39 04  =1822-173    22 04 22  39.0 268.1  3.6       0.0   142      288   09 36 05

09 39 04 IRAS18264-11  22 04 22  37.8 275.0  3.6       0.0   -38      288   No stop 
09 41 04  ---          22 06 23  37.3 274.8  3.6       0.0    82      290   09 39 05

09 41 04  J1825-1718   22 06 23  38.5 267.9  3.7       0.0   -38      290   No stop 
09 44 04  =1822-173    22 09 23  37.9 267.6  3.7       0.0   142      293   09 41 05

09 44 04 IRAS18264-11  22 09 23  36.6 274.4  3.7       0.0   -38      293   No stop 
09 46 04  ---          22 11 23  36.2 274.2  3.7       0.0    82      295   09 44 05

09 46 49  J1825-1718   22 12 09  37.2 267.3  3.8       0.0     7      295   09 46 49
09 49 49  =1822-173    22 15 09  36.6 267.0  3.8       0.0   180      298   09 46 50

09 49 49 IRAS18264-11  22 15 09  35.4 273.7  3.8       0.0   -38      298   No stop 
09 51 49  ---          22 17 09  34.9 273.5  3.8       0.0    82      300   09 49 50

09 51 49  J1825-1718   22 17 09  36.1 266.8  3.8       0.0   -38      300   No stop 
09 54 49  =1822-173    22 20 10  35.4 266.5  3.9       0.0   142      303   09 51 50

09 59 59  J2202+4216   22 25 21  21.6 355.6  0.4       0.0   164      303   09 59 59
10 07 59  =VR422201    22 33 22  21.4 354.1  0.5       0.0   480      311   10 00 00

10 13 09  J1825-1718   22 38 33  31.3 264.7  4.2       0.0   164      311   10 13 09
10 16 09  =1822-173    22 41 33  30.6 264.5  4.3       0.0   180      313   10 13 10

10 16 09 IRAS18264-11  22 41 33  29.4 270.7  4.2       0.0   -38      313   No stop 
10 18 09  ---          22 43 34  29.0 270.5  4.2       0.0    82      315   10 16 10

10 18 09  J1825-1718   22 43 34  30.2 264.3  4.3       0.0   -38      315   No stop 
10 21 09  =1822-173    22 46 34  29.5 264.0  4.3       0.0   142      318   10 18 10

10 21 09 IRAS18264-11  22 46 34  28.3 270.1  4.3       0.0   -38      318   No stop 
10 23 09  ---          22 48 34  27.8 269.9  4.3       0.0    82      320   10 21 10

10 23 09  J1825-1718   22 48 34  29.1 263.8  4.4       0.0   -38      320   No stop 
10 26 09  =1822-173    22 51 35  28.4 263.5  4.4       0.0   142      323   10 23 10

10 26 09 IRAS18264-11  22 51 35  27.2 269.6  4.4       0.0   -38      323   No stop 
10 28 09  ---          22 53 35  26.7 269.4  4.4       0.0    82      325   10 26 10
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
----------------------------------------------------------------------------------------

 --- Mon  29 Feb 2016   Day  60 ---

10 28 49  J1825-1718   22 54 15  27.8 263.2  4.5       0.0     2      325   10 28 49
10 31 49  =1822-173    22 57 16  27.1 262.9  4.5       0.0   180      328   10 28 50

10 31 49 IRAS18264-11  22 57 16  25.9 269.0  4.5       0.0   -38      328   No stop 
10 33 49  ---          22 59 16  25.4 268.8  4.5       0.0    82      330   10 31 50

10 33 49  J1825-1718   22 59 16  26.7 262.8  4.5       0.0   -38      330   No stop 
10 36 49  =1822-173    23 02 17  26.0 262.5  4.6       0.0   142      333   10 33 50

10 36 49 IRAS18264-11  23 02 17  24.8 268.5  4.5       0.0   -38      333   No stop 
10 38 49  ---          23 04 17  24.3 268.2  4.6       0.0    82      335   10 36 50

10 38 49  J1825-1718   23 04 17  25.6 262.3  4.6       0.0   -38      335   No stop 
10 41 49  =1822-173    23 07 18  24.9 262.0  4.7       0.0   142      337   10 38 50

10 41 49 IRAS18264-11  23 07 18  23.6 267.9  4.6       0.0   -38      337   No stop 
10 43 49  ---          23 09 18  23.2 267.7  4.7       0.0    82      339   10 41 50

10 44 29  J1825-1718   23 09 58  24.3 261.7  4.7       0.0     2      339   10 44 29
10 47 29  =1822-173    23 12 58  23.6 261.5  4.8       0.0   180      342   10 44 30

10 47 29 IRAS18264-11  23 12 58  22.4 267.3  4.7       0.0   -38      342   No stop 
10 49 29  ---          23 14 59  21.9 267.1  4.7       0.0    82      344   10 47 30

10 49 29  J1825-1718   23 14 59  23.2 261.3  4.8       0.0   -38      344   No stop 
10 52 29  =1822-173    23 17 59  22.5 261.0  4.9       0.0   142      347   10 49 30

10 56 49  J2202+4216   23 22 20  19.4 344.7  1.3       0.0   114      347   10 56 49
11 02 49  =VR422201    23 28 21  19.0 343.5  1.4       0.0   360      353   10 56 50

11 07 04  J1825-1718   23 32 37  19.3 259.6  5.1       0.0   109      353   11 07 04
11 10 04  =1822-173    23 35 37  18.6 259.3  5.2       0.0   180      356   11 07 05

11 10 04 IRAS18264-11  23 35 37  17.3 265.0  5.1       0.0   -38      356   No stop 
11 12 04  ---          23 37 38  16.8 264.8  5.1       0.0    82      358   11 10 05

11 12 29  J1825-1718   23 38 03  18.1 259.1  5.2       0.0   -13      358   11 12 29
11 17 29  =1822-173    23 43 03  17.0 258.6  5.3       0.0   287      362   11 12 30

11 22 14  J2202+4216   23 47 49  17.6 340.0  1.7       0.0   139      362   11 22 14
11 30 00  =VR422201    23 55 36  17.0 338.7  1.9       0.0   466      370   11 22 15


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:  10  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=   6665.38  6665.38  6665.38  6665.38  6669.38  6669.38  6669.38  6669.38
             6673.38  6673.38  6673.38  6673.38  6677.38  6677.38  6677.38  6677.38
   BBC fr=    155.38   155.38   155.38   155.38   159.38   159.38   159.38   159.38
              163.38   163.38   163.38   163.38   167.38   167.38   167.38   167.38
   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:  10

   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)

 * IRAS18264-11      18 26 26.649085   * 18 29 14.360000     18 30 07.761228       0.00
                    -11 52 23.96488    *-11 50 22.50000     -11 49 36.15358        0.00
                     From catalog imbedded in main SCHED input file.
                     Doppler based on LSR frame and radio definition.  Velocities:
                         46.80    46.80    46.80    46.80    46.80    46.80    46.80    46.80
                         46.80    46.80    46.80    46.80    46.80    46.80

   3C286             13 28 49.657758   * 13 31 08.288051     13 31 53.678223       0.18
 * J1331+3030        30 45 58.64059    * 30 30 32.95924      30 25 24.99919        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 31.191092       0.76
   J1642+3948        39 54 10.81496    * 39 48 36.99402      39 46 40.88951        0.52
   1641+399          /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
   J1642+39          GSFC 2015a astro solution, unpublished  53430 observations.
                     Doppler based on other sources.

   1822-173          18 22 42.013862   * 18 25 36.532313     18 26 32.125105       0.23
 * J1825-1718       -17 20 35.28837    *-17 18 49.84725     -17 18 06.77707        0.41
                     /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
                     GSFC 2015a astro solution, unpublished     76 observations.
                     Doppler based on other sources.

   VR422201          22 00 39.362505   * 22 02 43.291372     22 03 22.050139       0.00
 * J2202+4216        42 02 08.59077    * 42 16 39.97990      42 21 19.17747        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
  IRAS18264-1sess116.M128          1 2 3 4 5 6 8 9 10                1.900    60.265
  J1331+3030 sess116.M128          1 2 3 4 5 6 8 9 10                0.217     9.750
  3C345      sess116.M128          1 2 3 4 5 6 8 9 10                0.167     7.500
  J1825-1718 sess116.M128          1 2 3 4 5 6 8 9 10                3.367   116.671
  J2202+4216 sess116.M128          1 2 3 4 5 6 8 9 10                1.429    50.892


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) 
   IRAS18264-11        63.2
   J1331+3030         135.2
   3C345               95.6
   J1825-1718          63.9
   J2202+4216          51.1

  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 

