  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: Dominant heating mechanism in ULIRGs
 Exp. Code:  EP064K  


Schedule Version:       1.00                                              
Processed by SCHED version:   8.10  Bug fixs and minor enhancements       

PI:       Miguel A. Perez-Torres                                          

Address:  IAA - CSIC                                                      
          C/ Camino Bajo de Huetor, 50                                    
          18008 Granada, Spain                                            
                                                                          

Phone:    +34-958230644                                                   
EMAIL:    torres@iaa.es                                                   
Fax:      +34-958814530                                                   
Phone during observation: +34-665252538                                   

Observing mode: 1024 Mbps                                                 

Notes:    6-hr of 1-Gb/s, phase-ref of IRAS 07251-0248 with EVN+MERLIN    
          Third epoch obs-ns at 6cm                                       
                                                                          
                                                                          

Schedule for SHANGHAI  (Code Sh )                                   Page   2
               Dominant heating mechanism in ULIRGs
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
         For disks, the footages are really the GBytes
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)   SYNC
----------------------------------------------------------------------------------------

 --- Thu  18 Mar 2010   Day  77 ---

 Next scan frequencies:  4942.49  4942.49  4942.49  4942.49  4974.49  4974.49
                         4974.49  4974.49  5006.49  5006.49  5006.49  5006.49
                         5038.49  5038.49  5038.49  5038.49
 Next BBC frequencies:    742.49   742.49   742.49   742.49   774.49   774.49
                          774.49   774.49   806.49   806.49   806.49   806.49
                          838.49   838.49   838.49   838.49
 Next scan bandwidths:     16.00    16.00    16.00    16.00    16.00    16.00
                           16.00    16.00    16.00    16.00    16.00    16.00
                           16.00    16.00    16.00    16.00

15 00 00  J0730-0241   10 49 03  32.1 243.7  3.3      50.2     0   1  1      0  15 00 00
15 01 20  =0727-025    10 50 23  31.8 244.0  3.3      50.4    80   F  1     10  15 00 01

15 01 20  IRAS0725     10 50 23  31.1 244.3  3.4      50.6    -3   1  1     10  No stop 
15 05 10  ---          10 54 14  30.4 245.0  3.4      51.0   227   F  1     40  15 01 21

15 05 10  J0730-0241   10 54 14  31.1 244.7  3.4      50.8    -3   1  1     40  No stop 
15 06 30  =0727-025    10 55 34  30.8 244.9  3.4      50.9    77   F  1     50  15 05 11

15 06 30  IRAS0725     10 55 34  30.1 245.2  3.5      51.1    -3   1  1     50  No stop 
15 10 20  ---          10 59 25  29.4 245.9  3.5      51.5   227   F  1     80  15 06 31

15 10 20  J0730-0241   10 59 25  30.1 245.6  3.5      51.3    -3   1  1     80  No stop 
15 11 40  =0727-025    11 00 45  29.8 245.9  3.5      51.5    77   F  1     90  15 10 21

15 11 40  IRAS0725     11 00 45  29.1 246.1  3.5      51.6    -3   1  1     90  No stop 
15 15 30  ---          11 04 36  28.4 246.8  3.6      52.0   227   F  1    120  15 11 41

15 16 30  J0730-0241   11 05 36  28.8 246.7  3.6      51.9    57   1  1    120  15 16 30
15 17 50  =0727-025    11 06 56  28.6 246.9  3.6      52.1    80   F  1    130  15 16 31

15 17 50  IRAS0725     11 06 56  27.9 247.2  3.6      52.2    -3   1  1    130  No stop 
15 21 40  ---          11 10 47  27.1 247.9  3.7      52.6   227   F  1    160  15 17 51

15 21 40  J0730-0241   11 10 47  27.8 247.6  3.7      52.4    -3   1  1    160  No stop 
15 23 00  =0727-025    11 12 07  27.6 247.8  3.7      52.6    77   F  1    170  15 21 41

15 23 00  IRAS0725     11 12 07  26.9 248.1  3.7      52.7    -3   1  1    170  No stop 
15 26 50  ---          11 15 57  26.1 248.8  3.8      53.1   227   F  1    200  15 23 01

15 26 50  J0730-0241   11 15 57  26.8 248.5  3.7      52.9    -3   1  1    200  No stop 
15 28 10  =0727-025    11 17 18  26.5 248.7  3.8      53.0    77   F  1    210  15 26 51
Schedule for SHANGHAI  (Code Sh )                                   Page   3
               Dominant heating mechanism in ULIRGs
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
         For disks, the footages are really the GBytes
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)   SYNC
----------------------------------------------------------------------------------------

 --- Thu  18 Mar 2010   Day  77 ---

15 28 10  IRAS0725     11 17 18  25.8 249.0  3.8      53.2    -3   1  1    210  No stop 
15 32 00  ---          11 21 08  25.1 249.6  3.9      53.5   227   F  1    240  15 28 11

15 33 00  J0730-0241   11 22 08  25.6 249.5  3.9      53.4    57   1  1    240  15 33 00
15 34 20  =0727-025    11 23 29  25.3 249.7  3.9      53.5    80   F  1    250  15 33 01

15 34 20  IRAS0725     11 23 29  24.6 250.0  3.9      53.7    -3   1  1    250  No stop 
15 38 10  ---          11 27 19  23.8 250.6  4.0      54.0   227   F  1    280  15 34 21

15 38 10  J0730-0241   11 27 19  24.5 250.4  3.9      53.8    -3   1  1    280  No stop 
15 39 30  =0727-025    11 28 39  24.2 250.6  4.0      54.0    77   F  1    290  15 38 11

15 39 30  IRAS0725     11 28 39  23.5 250.8  4.0      54.1    -3   1  1    290  No stop 
15 43 20  ---          11 32 30  22.8 251.5  4.1      54.4   227   F  1    320  15 39 31

15 43 20  J0730-0241   11 32 30  23.5 251.2  4.0      54.2    -3   1  1    320  No stop 
15 44 40  =0727-025    11 33 50  23.2 251.4  4.0      54.3    77   F  1    330  15 43 21

15 44 40  IRAS0725     11 33 50  22.5 251.7  4.1      54.5    -3   1  1    330  No stop 
15 48 30  ---          11 37 41  21.7 252.3  4.2      54.7   227   F  1    360  15 44 41

15 49 30  J0730-0241   11 38 41  22.2 252.2  4.1      54.7    57   1  1    360  15 49 30
15 50 50  =0727-025    11 40 01  21.9 252.4  4.2      54.8    80   F  1    370  15 49 31

15 50 50  IRAS0725     11 40 01  21.2 252.6  4.2      54.9    -3   1  1    370  No stop 
15 54 40  ---          11 43 52  20.5 253.2  4.3      55.2   227   F  1    400  15 50 51

15 54 40  J0730-0241   11 43 52  21.2 253.0  4.2      55.1    -3   1  1    400  No stop 
15 56 00  =0727-025    11 45 12  20.9 253.2  4.2      55.1    77   F  1    410  15 54 41

15 56 00  IRAS0725     11 45 12  20.2 253.4  4.3      55.3    -3   1  1    410  No stop 
15 59 50  ---          11 49 03  19.4 254.0  4.3      55.5   227   F  1    440  15 56 01

15 59 50  J0730-0241   11 49 03  20.1 253.8  4.3      55.4    -3   1  1    440  No stop 
16 01 10  =0727-025    11 50 23  19.8 254.0  4.3      55.5    77   F  1    450  15 59 51

16 01 10  IRAS0725     11 50 23  19.1 254.2  4.4      55.6    -3   1  1    450  No stop 
16 05 00  ---          11 54 14  18.3 254.8  4.4      55.8   227   F  1    480  16 01 11

16 06 00  J0730-0241   11 55 14  18.8 254.7  4.4      55.8    57   1  1    480  16 06 00
16 07 20  =0727-025    11 56 34  18.5 254.9  4.4      55.9    80   F  1    490  16 06 01

16 07 20  IRAS0725     11 56 34  17.8 255.1  4.5      56.0    -3   1  1    490  No stop 
16 11 10  ---          12 00 25  17.0 255.7  4.5      56.2   227   F  1    520  16 07 21
Schedule for SHANGHAI  (Code Sh )                                   Page   4
               Dominant heating mechanism in ULIRGs
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
         For disks, the footages are really the GBytes
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)   SYNC
----------------------------------------------------------------------------------------

 --- Thu  18 Mar 2010   Day  77 ---

16 11 10  J0730-0241   12 00 25  17.7 255.5  4.5      56.1    -3   1  1    520  No stop 
16 12 30  =0727-025    12 01 45  17.5 255.7  4.5      56.2    77   F  1    530  16 11 11

16 12 30  IRAS0725     12 01 45  16.8 255.9  4.6      56.2    -3   1  1    530  No stop 
16 16 20  ---          12 05 36  16.0 256.4  4.6      56.5   227   F  1    560  16 12 31

16 16 20  J0730-0241   12 05 36  16.7 256.2  4.6      56.4    -3   1  1    560  No stop 
16 17 40  =0727-025    12 06 56  16.4 256.4  4.6      56.4    77   F  1    570  16 16 21

16 17 40  IRAS0725     12 06 56  15.7 256.6  4.6      56.5    -3   1  1    570  No stop 
16 21 30  ---          12 10 46  14.9 257.2  4.7      56.7   227   F  1    600  16 17 41

16 22 30  J0730-0241   12 11 47  15.4 257.1  4.7      56.7    57   1  1    600  16 22 30
16 23 50  =0727-025    12 13 07  15.1 257.3  4.7      56.7    80   F  1    610  16 22 31

16 23 50  IRAS0725     12 13 07  14.4 257.5  4.7      56.8    -3   1  1    610  No stop 
16 27 40  ---          12 16 57  13.6 258.0  4.8      57.0   227   F  1    640  16 23 51

16 27 40  J0730-0241   12 16 57  14.3 257.8  4.8      56.9    -3   1  1    640  No stop 
16 29 00  =0727-025    12 18 18  14.0 258.0  4.8      57.0    77   F  1    650  16 27 41

16 29 00  IRAS0725     12 18 18  13.3 258.2  4.8      57.1    -3   1  1    650  No stop 
16 32 50  ---          12 22 08  12.5 258.8  4.9      57.2   227   F  1    680  16 29 01

16 32 50  J0730-0241   12 22 08  13.2 258.6  4.9      57.2    -3   1  1    680  No stop 
16 34 10  =0727-025    12 23 28  12.9 258.7  4.9      57.2    77   F  1    690  16 32 51

16 34 10  IRAS0725     12 23 28  12.2 258.9  4.9      57.3    -3   1  1    690  No stop 
16 38 00  ---          12 27 19  11.4 259.5  5.0      57.5   227   F  1    720  16 34 11

16 39 00  J0730-0241   12 28 19  11.9 259.4  5.0      57.4    57   1  1    720  16 39 00
16 40 20  =0727-025    12 29 39  11.6 259.6  5.0      57.5    80   F  1    730  16 39 01

16 40 20  IRAS0725     12 29 39  10.9 259.8  5.0      57.5    -3   1  1    730  No stop 
16 44 00  ---          12 33 20  10.1 260.3  5.1      57.7   217   F  1    759  16 40 21

16 44 00  J0730-0241   12 33 20  10.9 260.1  5.0      57.6    -3   1  1    759  No stop 
16 45 20  =0727-025    12 34 40  10.6 260.3  5.1      57.7    77   F  1    769  16 44 01

16 45 20  IRAS0725     12 34 40   9.9 260.5  5.1      57.7    -3   1  1    769  No stop 
16 49 00  ---          12 38 21   9.1 261.0  5.2      57.9   217   F  1    797  16 45 21

16 49 00  J0730-0241   12 38 21   9.8 260.8  5.1      57.8    -3   1  1    797  No stop 
16 50 20  =0727-025    12 39 41   9.5 261.0  5.1      57.8    77   F  1    808  16 49 01
Schedule for SHANGHAI  (Code Sh )                                   Page   5
               Dominant heating mechanism in ULIRGs
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
         For disks, the footages are really the GBytes
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)   SYNC
----------------------------------------------------------------------------------------

 --- Thu  18 Mar 2010   Day  77 ---

16 50 20  IRAS0725     12 39 41   8.8 261.1  5.2      57.9    -3   1  1    808  No stop 
16 54 00  ---          12 43 22   8.0 261.6  5.3      58.0   217   F  1    836  16 50 21

16 55 00  J0730-0241   12 44 22   8.5 261.6  5.2      58.0    57   1  1    836  16 55 00
16 56 20  =0727-025    12 45 42   8.2 261.8  5.2      58.0    80   F  1    846  16 55 01

16 56 20  IRAS0725     12 45 42   7.5 261.9  5.3      58.1    -3   1  1    846  No stop 
17 00 00  ---          12 49 23   6.8 262.4  5.4      58.2   217   F  1    875  16 56 21

17 00 00  J0730-0241   12 49 23   7.5 262.3  5.3      58.1    -3   1  1    875  No stop 
17 01 20  =0727-025    12 50 43   7.2 262.4  5.3      58.2    77   F  1    885  17 00 01

17 01 20  IRAS0725     12 50 43   6.5 262.6  5.4      58.2    -3   1  1    885  No stop 
17 05 00  ---          12 54 24   5.7 263.1  5.4      58.3   217   F  1    913  17 01 21

17 05 00  J0730-0241   12 54 24   6.4 262.9  5.4      58.3    -3   1  1    913  No stop 
17 06 20  =0727-025    12 55 44   6.1 263.1  5.4      58.3    77   F  1    924  17 05 01

17 06 20  IRAS0725     12 55 44   5.4 263.3  5.5      58.4    -3   1  1    924  No stop 
17 10 00  ---          12 59 24   4.6 263.8  5.5  D   58.5     0   F  1    952  17 06 21

17 11 00  J0730-0241   13 00 25   5.1 263.7  5.5      58.4    58   1  1    952  17 11 00
17 12 20  =0727-025    13 01 45   4.8 263.9  5.5  D   58.5     0   F  1    963  17 11 01

17 23 20  J0854+2006   13 12 47  31.7 275.6  4.3      65.1   613   1  1    963  17 23 20
17 28 50  =0851+202    13 18 17  30.5 276.3  4.4      65.0   330   F  1   1005  17 23 21

17 28 50  4C39.25      13 18 17  42.9 296.3  3.8      81.1   -23   1  1   1005  No stop 
17 34 20  ---          13 23 48  41.9 296.5  3.9      80.4   307   F  1   1048  17 28 51

20 53 20  3C286        16 43 21  49.1 282.0  3.2      76.3 11923   1  1   1048  20 53 20
21 00 00  ---          16 50 02  47.8 282.5  3.3      75.9   400   F  1   1099  20 53 21


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


 Setup file: ep064k.6cm
   Matches group sh6cm in /home/cristina/sched_8.1/catalogs/freq.dat
    Update freq. range AnTao 22Mar08

   Setup group:    9         Station: SHANGHAI          Total bit rate: 1024
   Format: MKIV1:2           Bits per sample: 2         Sample rate: 32.000
   Number of channels: 16                               Speedup factor:   0.50

   Disk used to record data.

   1st LO=   4200.00   4200.00   4200.00   4200.00   4200.00   4200.00   4200.00   4200.00
             4200.00   4200.00   4200.00   4200.00   4200.00   4200.00   4200.00   4200.00
   Net SB=         L         L         U         U         L         L         U         U
                   L         L         U         U         L         L         U         U
   Pol.  =      RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
                RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
   BBC   =         1         2         1         2         3         4         3         4
                   5         6         5         6         7         8         7         8
   BBC SB=         L         L         U         U         L         L         U         U
                   L         L         U         U         L         L         U         U
   IF    =        C         A         C         A         C         A         C         A 
                  C         A         C         A         C         A         C         A 

  The following frequency sets based on this setup were used.

   Frequency Set:   9  Setup file default.  Used pcal sets:   1
   LO sum=    4942.49   4942.49   4942.49   4942.49   4974.49   4974.49   4974.49   4974.49
              5006.49   5006.49   5006.49   5006.49   5038.49   5038.49   5038.49   5038.49
   BBC fr=     742.49    742.49    742.49    742.49    774.49    774.49    774.49    774.49
               806.49    806.49    806.49    806.49    838.49    838.49    838.49    838.49
   Bandwd=     16.000    16.000    16.000    16.000    16.000    16.000    16.000    16.000
               16.000    16.000    16.000    16.000    16.000    16.000    16.000    16.000

  The following pulse cal sets were used with this setup:

   Pulse cal detection set:   1  PCAL = 1MHZ
    PCALXB1=   S1    S3    S5    S7    S9    S11   S13   S15
    PCALXB2=   S2    S4    S6    S8    S10   S12   S14   S16
    PCALFR1=   490   510   490   510   490   510   490   510
    PCALFR2=   490   510   490   510   490   510   490   510

   Track assignments are: 
    track1=   2, 10, 18, 26,  3, 11, 19, 27, 66, 74, 82, 90, 67, 75, 83, 91
    barrel=roll_off 
 SOURCE LIST -- Dominant heating mechanism in ULIRGs
     Catalog positions marked with *. 
     Precession of date coordinates is based on stop time of first scan.
     Names used in schedule marked with *. 
     Short names used in VLA and SNAP files marked with +. 
     Observation date used in B1950/J2000 coordinate conversion (PRECDATE):  1979.900
     No adjustments are made for rates (DRA, DDEC).
     Scan hours are for recording scans only. 
     Baseline hours are only counted for scans above horizon at both ends.

   Source                         Source position (RA/Dec)                        Error
                        (B1950)             (J2000)             (Date)            (mas)

 * IRAS0725          07 25 06.977760   * 07 27 37.613044     07 28 09.871382       0.00
                    -02 48 45.42650    *-02 54 54.19322     -02 56 19.01571        0.00
                     From catalog imbedded in main SCHED input file.
                        3.839 scan hours,    164.303 baseline hours above horizon.

 * J0730-0241        07 27 54.982193   * 07 30 25.877603     07 30 58.204316       0.29
   0727-025         -02 35 04.77201    *-02 41 24.90408     -02 42 52.06267        0.55
                     /home/cristina/sched_8.1/catalogs/sources.vlba
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro
                        1.483 scan hours,     51.877 baseline hours above horizon.

 * J0854+2006        08 51 57.250618   * 08 54 48.874930     08 55 26.023144       0.21
   0851+202          20 17 58.41742    * 20 06 30.64087      20 04 03.81258        0.40
   J0854+20          /home/cristina/sched_8.1/catalogs/sources.vlba
   OJ287             VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro
                        0.092 scan hours,      4.568 baseline hours above horizon.

   J0927+3902        09 23 55.319214   * 09 27 03.013935     09 27 43.927725       0.26
   0923+392          39 15 23.56647    * 39 02 20.85187      38 59 37.42205        0.40
 * 4C39.25           /home/cristina/sched_8.1/catalogs/sources.vlba
   J0927+39          VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro
                        0.092 scan hours,      3.839 baseline hours above horizon.

   J1331+3030        13 28 49.657764   * 13 31 08.288056     13 31 38.899248       0.36
 * 3C286             30 45 58.64058    * 30 30 32.95922      30 27 05.78820        0.47
   1328+307          /home/cristina/sched_8.1/catalogs/sources.vlba
   J1331+30          VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro
                        0.111 scan hours,      3.167 baseline hours above horizon.



  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) 
   IRAS0725           113.8
   J0730-0241         114.5
   J0854+2006         132.6
   4C39.25            129.4
   3C286              142.2

  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 

