  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: A 3-D View of high-mass star formation: gas Kinematics and Magnetic Fiel
 Exp. Code:  EM117B  


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 = G25.65+1.05
 
 

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

 --- Sun  28 Feb 2016   Day  59 ---

 Next scan frequencies:  6665.50  6665.50  6665.50  6665.50  6669.50  6669.50  6669.50  6669.50
                         6673.50  6673.50  6673.50  6673.50  6677.50  6677.50  6677.50  6677.50
 Next BBC frequencies:    155.50   155.50   155.50   155.50   159.50   159.50   159.50   159.50
                          163.50   163.50   163.50   163.50   167.50   167.50   167.50   167.50
 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 05 49  29.4 336.8  1.6       0.0     0        0   02 45 35
02 50 35  =3C286       15 10 50  28.9 335.7  1.6       0.0   300        5   02 45 36

02 51 05  J1331+3030   15 11 20  28.9 335.5  1.7       0.0     9        5   02 51 05
02 59 05  =3C286       15 19 21  28.1 333.8  1.8       0.0   480       12   02 51 06

03 03 31  3C345        15 23 48  21.8  16.4 -1.3       0.0   144       12   03 03 31
03 13 31  ---          15 33 49  22.4  14.4 -1.2       0.0   600       22   03 03 32

03 30 06  J1821-0502   15 50 27  48.2  66.6 -2.5       0.0   878       22   03 30 06
03 35 06  =1818-050    15 55 28  49.2  65.6 -2.4       0.0   300       27   03 30 07

03 35 06  G25.65+1.05  15 55 28  47.0  69.5 -2.7       0.0   -33       27   No stop 
03 37 06  ---          15 57 28  47.4  69.1 -2.6       0.0    87       29   03 35 07

03 37 41  J1821-0502   15 58 03  49.8  65.0 -2.4       0.0     1       29   03 37 41
03 40 41  =1818-050    16 01 04  50.4  64.3 -2.3       0.0   180       32   03 37 42

03 40 41  G25.65+1.05  16 01 04  48.2  68.3 -2.6       0.0   -33       32   No stop 
03 42 41  ---          16 03 04  48.6  67.9 -2.5       0.0    87       34   03 40 42

03 42 41  J1821-0502   16 03 04  50.8  63.9 -2.3       0.0   -34       34   No stop 
03 45 41  =1818-050    16 06 05  51.4  63.2 -2.3       0.0   146       37   03 42 42

03 45 41  G25.65+1.05  16 06 05  49.2  67.3 -2.5       0.0   -33       37   No stop 
03 47 41  ---          16 08 05  49.7  66.9 -2.5       0.0    87       38   03 45 42

03 48 16  J1821-0502   16 08 40  51.9  62.5 -2.2       0.0     1       38   03 48 16
03 51 16  =1818-050    16 11 41  52.5  61.8 -2.2       0.0   180       41   03 48 17

03 51 16  G25.65+1.05  16 11 41  50.4  66.1 -2.4       0.0   -33       41   No stop 
03 53 16  ---          16 13 41  50.8  65.7 -2.4       0.0    87       43   03 51 17

03 53 16  J1821-0502   16 13 41  52.9  61.3 -2.1       0.0   -34       43   No stop 
03 56 16  =1818-050    16 16 41  53.5  60.5 -2.1       0.0   146       46   03 53 17

03 56 16  G25.65+1.05  16 16 41  51.4  65.0 -2.3       0.0   -33       46   No stop 
03 58 16  ---          16 18 42  51.8  64.5 -2.3       0.0    87       48   03 56 17
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
----------------------------------------------------------------------------------------

 --- Sun  28 Feb 2016   Day  59 ---

03 58 16  J1821-0502   16 18 42  53.9  60.0 -2.1       0.0   -34       48   No stop 
04 01 16  =1818-050    16 21 42  54.5  59.2 -2.0       0.0   146       51   03 58 17

04 01 16  G25.65+1.05  16 21 42  52.4  63.8 -2.2       0.0   -33       51   No stop 
04 03 16  ---          16 23 43  52.8  63.3 -2.2       0.0    87       53   04 01 17

04 03 51  J1821-0502   16 24 18  55.0  58.5 -2.0       0.0     1       53   04 03 51
04 06 51  =1818-050    16 27 18  55.5  57.7 -1.9       0.0   180       56   04 03 52

04 06 51  G25.65+1.05  16 27 18  53.6  62.5 -2.1       0.0   -33       56   No stop 
04 08 51  ---          16 29 18  54.0  62.0 -2.1       0.0    87       58   04 06 52

04 08 51  J1821-0502   16 29 18  55.9  57.1 -1.9       0.0   -34       58   No stop 
04 11 51  =1818-050    16 32 19  56.5  56.2 -1.8       0.0   146       61   04 08 52

04 28 01  J1821-0502   16 48 32  59.4  51.0 -1.6       0.0   948       61   04 28 01
04 31 01  =1818-050    16 51 32  59.9  49.9 -1.5       0.0   180       63   04 28 02

04 31 01  G25.65+1.05  16 51 32  58.2  55.7 -1.7       0.0   -33       63   No stop 
04 33 01  ---          16 53 32  58.6  55.0 -1.7       0.0    87       65   04 31 02

04 33 01  J1821-0502   16 53 32  60.3  49.2 -1.5       0.0   -34       65   No stop 
04 36 01  =1818-050    16 56 33  60.8  48.1 -1.4       0.0   146       68   04 33 02

04 36 01  G25.65+1.05  16 56 33  59.2  54.1 -1.6       0.0   -33       68   No stop 
04 38 01  ---          16 58 33  59.5  53.4 -1.6       0.0    87       70   04 36 02

04 38 01  J1821-0502   16 58 33  61.1  47.3 -1.4       0.0   -34       70   No stop 
04 41 01  =1818-050    17 01 34  61.6  46.1 -1.3       0.0   146       73   04 38 02

04 41 01  G25.65+1.05  17 01 34  60.1  52.4 -1.6       0.0   -33       73   No stop 
04 43 01  ---          17 03 34  60.4  51.7 -1.5       0.0    87       75   04 41 02

04 43 36  J1821-0502   17 04 09  62.0  45.1 -1.3       0.0     1       75   04 43 36
04 46 36  =1818-050    17 07 10  62.5  43.8 -1.2       0.0   180       78   04 43 37

04 46 36  G25.65+1.05  17 07 10  61.0  50.4 -1.5       0.0   -33       78   No stop 
04 48 36  ---          17 09 10  61.4  49.6 -1.4       0.0    87       80   04 46 37

04 48 36  J1821-0502   17 09 10  62.8  43.0 -1.2       0.0   -34       80   No stop 
04 51 36  =1818-050    17 12 10  63.3  41.7 -1.2       0.0   146       83   04 48 37

04 51 36  G25.65+1.05  17 12 10  61.9  48.5 -1.4       0.0   -33       83   No stop 
04 53 36  ---          17 14 11  62.2  47.7 -1.4       0.0    87       85   04 51 37
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
----------------------------------------------------------------------------------------

 --- Sun  28 Feb 2016   Day  59 ---

04 53 36  J1821-0502   17 14 11  63.6  40.8 -1.1       0.0   -34       85   No stop 
04 56 36  =1818-050    17 17 11  64.0  39.4 -1.1       0.0   146       87   04 53 37

04 56 36  G25.65+1.05  17 17 11  62.7  46.5 -1.3       0.0   -33       87   No stop 
04 58 36  ---          17 19 12  63.1  45.6 -1.3       0.0    87       89   04 56 37

04 59 11  J1821-0502   17 19 47  64.4  38.2 -1.0       0.0     1       89   04 59 11
05 02 11  =1818-050    17 22 47  64.8  36.7 -1.0       0.0   180       92   04 59 12

05 02 11  G25.65+1.05  17 22 47  63.6  44.1 -1.2       0.0   -33       92   No stop 
05 04 11  ---          17 24 48  63.9  43.2 -1.2       0.0    87       94   05 02 12

05 04 11  J1821-0502   17 24 48  65.0  35.7 -1.0       0.0   -34       94   No stop 
05 07 11  =1818-050    17 27 48  65.4  34.2 -0.9       0.0   146       97   05 04 12

05 23 46  J1821-0502   17 44 26  67.3  24.9 -0.6       0.0   973       97   05 23 46
05 26 46  =1818-050    17 47 26  67.6  23.1 -0.6       0.0   180      100   05 23 47

05 26 46  G25.65+1.05  17 47 26  67.1  31.9 -0.8       0.0   -33      100   No stop 
05 28 46  ---          17 49 27  67.3  30.7 -0.8       0.0    87      102   05 26 47

05 28 46  J1821-0502   17 49 27  67.7  21.9 -0.5       0.0   -34      102   No stop 
05 31 46  =1818-050    17 52 27  68.0  20.0 -0.5       0.0   146      105   05 28 47

05 31 46  G25.65+1.05  17 52 27  67.6  29.0 -0.7       0.0   -33      105   No stop 
05 33 46  ---          17 54 27  67.8  27.8 -0.7       0.0    87      107   05 31 47

05 33 46  J1821-0502   17 54 27  68.1  18.7 -0.5       0.0   -34      107   No stop 
05 36 46  =1818-050    17 57 28  68.3  16.8 -0.4       0.0   146      110   05 33 47

05 36 46  G25.65+1.05  17 57 28  68.1  26.0 -0.6       0.0   -33      110   No stop 
05 38 46  ---          17 59 28  68.3  24.7 -0.6       0.0    87      112   05 36 47

05 39 21  J1821-0502   18 00 03  68.5  15.1 -0.4       0.0     1      112   05 39 21
05 42 21  =1818-050    18 03 04  68.7  13.1 -0.3       0.0   180      114   05 39 22

05 42 21  G25.65+1.05  18 03 04  68.7  22.5 -0.5       0.0   -33      114   No stop 
05 44 21  ---          18 05 04  68.8  21.2 -0.5       0.0    87      116   05 42 22

05 44 21  J1821-0502   18 05 04  68.7  11.7 -0.3       0.0   -34      116   No stop 
05 47 21  =1818-050    18 08 05  68.9   9.7 -0.2       0.0   146      119   05 44 22

05 47 21  G25.65+1.05  18 08 05  69.1  19.2 -0.5       0.0   -33      119   No stop 
05 49 21  ---          18 10 05  69.2  17.8 -0.4       0.0    87      121   05 47 22
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
----------------------------------------------------------------------------------------

 --- Sun  28 Feb 2016   Day  59 ---

05 49 21  J1821-0502   18 10 05  68.9   8.3 -0.2       0.0   -34      121   No stop 
05 52 21  =1818-050    18 13 05  69.0   6.2 -0.1       0.0   146      124   05 49 22

05 52 21  G25.65+1.05  18 13 05  69.4  15.8 -0.4       0.0   -33      124   No stop 
05 54 21  ---          18 15 06  69.5  14.4 -0.3       0.0    87      126   05 52 22

05 54 56  J1821-0502   18 15 41  69.1   4.4 -0.1       0.0     1      126   05 54 56
05 57 56  =1818-050    18 18 41  69.1   2.3 -0.1       0.0   180      129   05 54 57

05 57 56  G25.65+1.05  18 18 41  69.7  11.9 -0.3       0.0   -33      129   No stop 
05 59 56  ---          18 20 42  69.8  10.5 -0.2       0.0    87      131   05 57 57

05 59 56  J1821-0502   18 20 42  69.1   0.9 -0.0       0.0   -34      131   No stop 
06 02 56  =1818-050    18 23 42  69.1 358.8  0.0       0.0   146      134   05 59 57

06 20 06  J1821-0502   18 40 55  68.7 347.0  0.3       0.0  1008      134   06 20 06
06 23 06  =1818-050    18 43 55  68.5 345.0  0.4       0.0   180      137   06 20 07

06 23 06  G25.65+1.05  18 43 55  70.0 353.7  0.1       0.0   -33      137   No stop 
06 25 06  ---          18 45 56  69.9 352.2  0.2       0.0    87      138   06 23 07

06 25 06  J1821-0502   18 45 56  68.4 343.7  0.4       0.0   -34      138   No stop 
06 28 06  =1818-050    18 48 56  68.2 341.7  0.4       0.0   146      141   06 25 07

06 28 06  G25.65+1.05  18 48 56  69.8 350.1  0.2       0.0   -33      141   No stop 
06 30 06  ---          18 50 57  69.7 348.6  0.3       0.0    87      143   06 28 07

06 30 06  J1821-0502   18 50 57  68.0 340.4  0.5       0.0   -34      143   No stop 
06 33 06  =1818-050    18 53 57  67.8 338.6  0.5       0.0   146      146   06 30 07

06 33 06  G25.65+1.05  18 53 57  69.6 346.5  0.3       0.0   -33      146   No stop 
06 35 06  ---          18 55 57  69.5 345.1  0.3       0.0    87      148   06 33 07

06 35 41  J1821-0502   18 56 33  67.6 337.0  0.6       0.0     1      148   06 35 41
06 38 41  =1818-050    18 59 33  67.3 335.1  0.6       0.0   180      151   06 35 42

06 38 41  G25.65+1.05  18 59 33  69.3 342.7  0.4       0.0   -33      151   No stop 
06 40 41  ---          19 01 33  69.1 341.3  0.4       0.0    87      153   06 38 42

06 40 41  J1821-0502   19 01 33  67.1 334.0  0.7       0.0   -34      153   No stop 
06 43 41  =1818-050    19 04 34  66.8 332.2  0.7       0.0   146      156   06 40 42

06 43 41  G25.65+1.05  19 04 34  68.9 339.3  0.5       0.0   -33      156   No stop 
06 45 41  ---          19 06 34  68.7 338.0  0.5       0.0    87      158   06 43 42
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
----------------------------------------------------------------------------------------

 --- Sun  28 Feb 2016   Day  59 ---

06 45 41  J1821-0502   19 06 34  66.6 331.1  0.7       0.0   -34      158   No stop 
06 48 41  =1818-050    19 09 35  66.2 329.4  0.8       0.0   146      161   06 45 42

06 48 41  G25.65+1.05  19 09 35  68.5 336.1  0.6       0.0   -33      161   No stop 
06 50 41  ---          19 11 35  68.3 334.9  0.6       0.0    87      162   06 48 42

06 51 16  J1821-0502   19 12 10  65.9 328.0  0.8       0.0     1      162   06 51 16
06 54 16  =1818-050    19 15 11  65.6 326.4  0.9       0.0   180      165   06 51 17

06 54 16  G25.65+1.05  19 15 11  67.9 332.7  0.7       0.0   -33      165   No stop 
06 56 16  ---          19 17 11  67.7 331.5  0.7       0.0    87      167   06 54 17

06 56 16  J1821-0502   19 17 11  65.3 325.4  0.9       0.0   -34      167   No stop 
06 59 16  =1818-050    19 20 11  64.9 323.8  1.0       0.0   146      170   06 56 17

07 04 06  J2202+4216   19 25 02  12.6  28.8 -2.6       0.0   153      170   07 04 06
07 12 06  =VR422201    19 33 04  13.5  27.6 -2.5       0.0   480      178   07 04 07

07 17 06  J1821-0502   19 38 04  62.3 315.7  1.3       0.0   161      178   07 17 06
07 20 06  =1818-050    19 41 05  61.8 314.5  1.3       0.0   180      181   07 17 07

07 20 06  G25.65+1.05  19 41 05  64.6 318.9  1.1       0.0   -33      181   No stop 
07 22 06  ---          19 43 05  64.3 317.9  1.1       0.0    87      183   07 20 07

07 22 06  J1821-0502   19 43 05  61.5 313.7  1.4       0.0   -34      183   No stop 
07 25 06  =1818-050    19 46 06  61.0 312.5  1.4       0.0   146      186   07 22 07

07 25 06  G25.65+1.05  19 46 06  63.9 316.6  1.2       0.0   -33      186   No stop 
07 27 06  ---          19 48 06  63.6 315.7  1.2       0.0    87      187   07 25 07

07 27 06  J1821-0502   19 48 06  60.7 311.7  1.4       0.0   -34      187   No stop 
07 30 06  =1818-050    19 51 06  60.2 310.6  1.5       0.0   146      190   07 27 07

07 30 06  G25.65+1.05  19 51 06  63.1 314.4  1.3       0.0   -33      190   No stop 
07 32 06  ---          19 53 07  62.8 313.6  1.3       0.0    87      192   07 30 07

07 32 41  J1821-0502   19 53 42  59.7 309.7  1.5       0.0     1      192   07 32 41
07 35 41  =1818-050    19 56 42  59.2 308.6  1.6       0.0   180      195   07 32 42

07 35 41  G25.65+1.05  19 56 42  62.2 312.1  1.4       0.0   -33      195   No stop 
07 37 41  ---          19 58 43  61.8 311.4  1.4       0.0    87      197   07 35 42

07 37 41  J1821-0502   19 58 43  58.9 307.9  1.6       0.0   -34      197   No stop 
07 40 41  =1818-050    20 01 43  58.3 306.9  1.7       0.0   146      200   07 37 42
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
----------------------------------------------------------------------------------------

 --- Sun  28 Feb 2016   Day  59 ---

07 40 41  G25.65+1.05  20 01 43  61.3 310.2  1.4       0.0   -33      200   No stop 
07 42 41  ---          20 03 44  61.0 309.5  1.5       0.0    87      202   07 40 42

07 42 41  J1821-0502   20 03 44  58.0 306.3  1.7       0.0   -34      202   No stop 
07 45 41  =1818-050    20 06 44  57.4 305.3  1.7       0.0   146      205   07 42 42

07 45 41  G25.65+1.05  20 06 44  60.4 308.4  1.5       0.0   -33      205   No stop 
07 47 41  ---          20 08 44  60.1 307.7  1.6       0.0    87      207   07 45 42

07 48 16  J1821-0502   20 09 19  56.9 304.5  1.8       0.0     1      207   07 48 16
07 51 16  =1818-050    20 12 20  56.4 303.6  1.8       0.0   180      210   07 48 17

07 51 16  G25.65+1.05  20 12 20  59.4 306.5  1.6       0.0   -33      210   No stop 
07 53 16  ---          20 14 20  59.1 305.8  1.7       0.0    87      212   07 51 17

07 53 16  J1821-0502   20 14 20  56.0 303.0  1.9       0.0   -34      212   No stop 
07 56 16  =1818-050    20 17 21  55.4 302.2  1.9       0.0   146      214   07 53 17

08 01 26  J2202+4216   20 22 32  17.9  19.3 -1.7       0.0   173      214   08 01 26
08 09 26  =VR422201    20 30 33  18.5  17.9 -1.5       0.0   480      222   08 01 27

08 14 26  J1821-0502   20 35 34  51.9 297.4  2.2       0.0   161      222   08 14 26
08 17 26  =1818-050    20 38 34  51.3 296.7  2.3       0.0   180      225   08 14 27

08 17 26  G25.65+1.05  20 38 34  54.5 298.7  2.1       0.0   -33      225   No stop 
08 19 26  ---          20 40 35  54.1 298.2  2.1       0.0    87      227   08 17 27

08 19 26  J1821-0502   20 40 35  50.9 296.2  2.3       0.0   -34      227   No stop 
08 22 26  =1818-050    20 43 35  50.3 295.5  2.4       0.0   146      230   08 19 27

08 22 26  G25.65+1.05  20 43 35  53.5 297.4  2.1       0.0   -33      230   No stop 
08 24 26  ---          20 45 35  53.1 296.9  2.2       0.0    87      232   08 22 27

08 24 26  J1821-0502   20 45 35  49.8 295.1  2.4       0.0   -34      232   No stop 
08 27 26  =1818-050    20 48 36  49.2 294.4  2.4       0.0   146      235   08 24 27

08 27 26  G25.65+1.05  20 48 36  52.5 296.2  2.2       0.0   -33      235   No stop 
08 29 26  ---          20 50 36  52.1 295.7  2.3       0.0    87      237   08 27 27

08 30 01  J1821-0502   20 51 11  48.7 293.9  2.5       0.0     1      237   08 30 01
08 33 01  =1818-050    20 54 12  48.1 293.2  2.5       0.0   180      239   08 30 02

08 33 01  G25.65+1.05  20 54 12  51.3 294.9  2.3       0.0   -33      239   No stop 
08 35 01  ---          20 56 12  50.9 294.4  2.4       0.0    87      241   08 33 02
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
----------------------------------------------------------------------------------------

 --- Sun  28 Feb 2016   Day  59 ---

08 35 01  J1821-0502   20 56 12  47.7 292.8  2.6       0.0   -34      241   No stop 
08 38 01  =1818-050    20 59 13  47.0 292.2  2.6       0.0   146      244   08 35 02

08 38 01  G25.65+1.05  20 59 13  50.3 293.8  2.4       0.0   -33      244   No stop 
08 40 01  ---          21 01 13  49.9 293.3  2.4       0.0    87      246   08 38 02

08 40 01  J1821-0502   21 01 13  46.6 291.8  2.7       0.0   -34      246   No stop 
08 43 01  =1818-050    21 04 13  46.0 291.2  2.7       0.0   146      249   08 40 02

08 43 01  G25.65+1.05  21 04 13  49.3 292.7  2.5       0.0   -33      249   No stop 
08 45 01  ---          21 06 14  48.8 292.3  2.5       0.0    87      251   08 43 02

08 45 36  J1821-0502   21 06 49  45.5 290.7  2.7       0.0     1      251   08 45 36
08 48 36  =1818-050    21 09 49  44.8 290.2  2.8       0.0   180      254   08 45 37

08 48 36  G25.65+1.05  21 09 49  48.1 291.6  2.6       0.0   -33      254   No stop 
08 50 36  ---          21 11 50  47.7 291.2  2.6       0.0    87      256   08 48 37

08 50 36  J1821-0502   21 11 50  44.4 289.8  2.8       0.0   -34      256   No stop 
08 53 36  =1818-050    21 14 50  43.8 289.3  2.9       0.0   146      259   08 50 37

08 59 01  J2202+4216   21 20 16  21.0   8.5 -0.7       0.0   188      259   08 59 01
09 07 01  =VR422201    21 28 17  21.3   6.9 -0.6       0.0   480      266   08 59 02

09 12 36  J1821-0502   21 33 53  39.7 286.0  3.2       0.0   196      266   09 12 36
09 15 36  =1818-050    21 36 54  39.0 285.5  3.2       0.0   180      269   09 12 37

09 15 36  G25.65+1.05  21 36 54  42.3 286.6  3.0       0.0   -33      269   No stop 
09 17 36  ---          21 38 54  41.9 286.3  3.1       0.0    87      271   09 15 37

09 17 36  J1821-0502   21 38 54  38.6 285.2  3.3       0.0   -34      271   No stop 
09 20 36  =1818-050    21 41 55  37.9 284.8  3.3       0.0   146      274   09 17 37

09 20 36  G25.65+1.05  21 41 55  41.3 285.8  3.1       0.0   -33      274   No stop 
09 22 36  ---          21 43 55  40.8 285.4  3.1       0.0    87      276   09 20 37

09 22 36  J1821-0502   21 43 55  37.5 284.5  3.4       0.0   -34      276   No stop 
09 25 36  =1818-050    21 46 55  36.8 284.0  3.4       0.0   146      279   09 22 37

09 25 36  G25.65+1.05  21 46 55  40.2 285.0  3.2       0.0   -33      279   No stop 
09 27 36  ---          21 48 56  39.7 284.6  3.2       0.0    87      281   09 25 37

09 28 11  J1821-0502   21 49 31  36.3 283.6  3.5       0.0     1      281   09 28 11
09 31 11  =1818-050    21 52 31  35.6 283.2  3.5       0.0   180      284   09 28 12
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
----------------------------------------------------------------------------------------

 --- Sun  28 Feb 2016   Day  59 ---

09 31 11  G25.65+1.05  21 52 31  38.9 284.1  3.3       0.0   -33      284   No stop 
09 33 11  ---          21 54 32  38.5 283.8  3.3       0.0    87      286   09 31 12

09 33 11  J1821-0502   21 54 32  35.2 282.9  3.5       0.0   -34      286   No stop 
09 36 11  =1818-050    21 57 32  34.5 282.4  3.6       0.0   146      288   09 33 12

09 36 11  G25.65+1.05  21 57 32  37.9 283.3  3.4       0.0   -33      288   No stop 
09 38 11  ---          21 59 33  37.4 283.0  3.4       0.0    87      290   09 36 12

09 38 11  J1821-0502   21 59 33  34.1 282.2  3.6       0.0   -34      290   No stop 
09 41 11  =1818-050    22 02 33  33.4 281.7  3.7       0.0   146      293   09 38 12

09 41 11  G25.65+1.05  22 02 33  36.8 282.6  3.5       0.0   -33      293   No stop 
09 43 11  ---          22 04 33  36.3 282.3  3.5       0.0    87      295   09 41 12

09 43 46  J1821-0502   22 05 08  32.8 281.4  3.7       0.0     1      295   09 43 46
09 46 46  =1818-050    22 08 09  32.2 281.0  3.8       0.0   180      298   09 43 47

09 46 46  G25.65+1.05  22 08 09  35.5 281.8  3.5       0.0   -33      298   No stop 
09 48 46  ---          22 10 09  35.1 281.5  3.6       0.0    87      300   09 46 47

09 48 46  J1821-0502   22 10 09  31.7 280.7  3.8       0.0   -34      300   No stop 
09 51 46  =1818-050    22 13 10  31.1 280.3  3.9       0.0   146      303   09 48 47

09 57 11  J2202+4216   22 18 36  21.7 357.0  0.3       0.0   188      303   09 57 11
10 05 11  =VR422201    22 26 37  21.5 355.4  0.4       0.0   480      311   09 57 12

10 10 41  J1821-0502   22 32 08  26.9 277.8  4.2       0.0   191      311   10 10 41
10 13 41  =1818-050    22 35 08  26.2 277.5  4.2       0.0   180      313   10 10 42

10 13 41  G25.65+1.05  22 35 08  29.5 278.2  4.0       0.0   -33      313   No stop 
10 15 41  ---          22 37 09  29.1 277.9  4.0       0.0    87      315   10 13 42

10 15 41  J1821-0502   22 37 09  25.7 277.2  4.3       0.0   -34      315   No stop 
10 18 41  =1818-050    22 40 09  25.1 276.9  4.3       0.0   146      318   10 15 42

10 18 41  G25.65+1.05  22 40 09  28.4 277.5  4.1       0.0   -33      318   No stop 
10 20 41  ---          22 42 10  28.0 277.3  4.1       0.0    87      320   10 18 42

10 20 41  J1821-0502   22 42 10  24.6 276.6  4.3       0.0   -34      320   No stop 
10 23 41  =1818-050    22 45 10  23.9 276.3  4.4       0.0   146      323   10 20 42

10 23 41  G25.65+1.05  22 45 10  27.3 276.9  4.2       0.0   -33      323   No stop 
10 25 41  ---          22 47 10  26.9 276.7  4.2       0.0    87      325   10 23 42
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
----------------------------------------------------------------------------------------

 --- Sun  28 Feb 2016   Day  59 ---

10 26 16  J1821-0502   22 47 45  23.4 275.9  4.4       0.0     1      325   10 26 16
10 29 16  =1818-050    22 50 46  22.7 275.6  4.5       0.0   180      328   10 26 17

10 29 16  G25.65+1.05  22 50 46  26.1 276.2  4.3       0.0   -33      328   No stop 
10 31 16  ---          22 52 46  25.6 276.0  4.3       0.0    87      330   10 29 17

10 31 16  J1821-0502   22 52 46  22.2 275.4  4.5       0.0   -34      330   No stop 
10 34 16  =1818-050    22 55 47  21.6 275.0  4.6       0.0   146      333   10 31 17

10 34 16  G25.65+1.05  22 55 47  24.9 275.6  4.3       0.0   -33      333   No stop 
10 36 16  ---          22 57 47  24.5 275.4  4.4       0.0    87      335   10 34 17

10 36 16  J1821-0502   22 57 47  21.1 274.8  4.6       0.0   -34      335   No stop 
10 39 16  =1818-050    23 00 48  20.4 274.4  4.6       0.0   146      337   10 36 17

10 39 16  G25.65+1.05  23 00 48  23.8 275.0  4.4       0.0   -33      337   No stop 
10 41 16  ---          23 02 48  23.4 274.8  4.5       0.0    87      339   10 39 17

10 41 51  J1821-0502   23 03 23  19.9 274.1  4.7       0.0     1      339   10 41 51
10 44 51  =1818-050    23 06 23  19.2 273.8  4.7       0.0   180      342   10 41 52

10 44 51  G25.65+1.05  23 06 23  22.6 274.4  4.5       0.0   -33      342   No stop 
10 46 51  ---          23 08 24  22.1 274.1  4.6       0.0    87      344   10 44 52

10 46 51  J1821-0502   23 08 24  18.7 273.5  4.8       0.0   -34      344   No stop 
10 49 51  =1818-050    23 11 24  18.1 273.2  4.8       0.0   146      347   10 46 52

10 54 41  J2202+4216   23 16 15  19.7 345.8  1.2       0.0   153      347   10 54 41
11 02 41  =VR422201    23 24 16  19.2 344.3  1.3       0.0   480      355   10 54 42

11 07 26  J1821-0502   23 29 02  14.1 271.2  5.1       0.0   146      355   11 07 26
11 10 26  =1818-050    23 32 03  13.4 270.9  5.2       0.0   180      358   11 07 27

11 10 26  G25.65+1.05  23 32 03  16.8 271.5  4.9       0.0   -33      358   No stop 
11 12 26  ---          23 34 03  16.3 271.2  5.0       0.0    87      360   11 10 27

11 12 51  J1821-0502   23 34 28  12.9 270.6  5.2       0.0    -9      360   11 12 51
11 17 51  =1818-050    23 39 29  11.8 270.1  5.3       0.0   291      364   11 12 52

11 22 40  J2202+4216   23 44 19  17.9 340.7  1.7       0.0   152      364   11 22 40
11 30 00  =VR422201    23 51 40  17.3 339.4  1.8       0.0   440      371   11 22 41


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=   6665.50  6665.50  6665.50  6665.50  6669.50  6669.50  6669.50  6669.50
             6673.50  6673.50  6673.50  6673.50  6677.50  6677.50  6677.50  6677.50
   BBC fr=    155.50   155.50   155.50   155.50   159.50   159.50   159.50   159.50
              163.50   163.50   163.50   163.50   167.50   167.50   167.50   167.50
   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)

 * G25.65+1.05       18 31 40.145161   * 18 34 20.900000     18 35 12.025539       0.00
                    -06 02 05.96283    *-05 59 42.10000     -05 58 50.47653        0.00
                     From catalog imbedded in main SCHED input file.
                     Doppler based on LSR frame and radio definition.  Velocities:
                         41.60    41.60    41.60    41.60    41.60    41.60    41.60    41.60
                         41.60    41.60    41.60    41.60    41.60    41.60

   3C286             13 28 49.657758   * 13 31 08.288051     13 31 53.656563       0.18
 * J1331+3030        30 45 58.64059    * 30 30 32.95924      30 25 24.92879        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 31.157818       0.76
   J1642+3948        39 54 10.81496    * 39 48 36.99402      39 46 40.92272        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.

   1818-050          18 18 32.138835   * 18 21 11.809558     18 22 02.659645       0.32
 * J1821-0502       -05 03 46.86946    *-05 02 20.08539     -05 01 47.03899        0.52
                     /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
                     GSFC 2015a astro solution, unpublished    107 observations.
                     Doppler based on other sources.

   VR422201          22 00 39.362505   * 22 02 43.291372     22 03 22.040381       0.00
 * J2202+4216        42 02 08.59077    * 42 16 39.97990      42 21 19.41844        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
  G25.65+1.05sess116.M128          1 2 3 4 5 6 8 9 10                1.900    65.677
  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     7.485
  J1821-0502 sess116.M128          1 2 3 4 5 6 8 9 10                3.367   137.209
  J2202+4216 sess116.M128          1 2 3 4 5 6 8 9 10                1.456    51.767


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) 
   G25.65+1.05         61.4
   J1331+3030         134.7
   3C345               95.1
   J1821-0502          64.8
   J2202+4216          51.3

  Barry Clark estimates from predictions by Ketan Desai of IPM scattering sizes 
  that the Sun will cause amplitude reductions on the  longest VLBA baselines 
  at a solar distance of 60deg F^(-0.6) where F is in GHz. 
  For common VLBI bands, this is: 
       327 MHz        117. deg 
       610 MHz         81. deg 
       1.6 GHz         45. deg 
       2.3 GHz         36. deg 
       5.0 GHz         23. deg 
       8.4 GHz         17. deg 
      15.0 GHz         12. deg 
      22.0 GHz          9. deg 
      43.0 GHz          6. deg 

