  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: 3C48
 Exp. Code:  EA033   


Schedule Version:       1.00                                              
Processed by SCHED version:   6.01  Release: Late March 2005              

PI:       T.An                                                            

Address:  Shanghai Astronomical Observatory                               
          Nandan Road 80                                                  
          Shanghai                                                        
          CHINA                                                           

Phone:    +8621 64386191                                                  
EMAIL:    antao@shao.ac.cn                                                
Fax:      +8621 64384618                                                  
Phone during observation: +8621 57651763                                  

Observing mode: EVN+MERLIN, 3C48 at 18cm (256 Mb/s)                       

Notes:                                                                    
                                                                          
                                                                          
                                                                          

Schedule for HART      (Code Hh )                                   Page   2
               3C48
  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.
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Tue   7 Jun 2005   Day 158 ---

 Next scan frequencies:  1637.99  1637.99  1645.99  1645.99  1653.99  1653.99
                         1661.99  1661.99
 Next BBC frequencies:    127.99   127.99   135.99   135.99   143.99   143.99
                          151.99   151.99
 Next scan bandwidths:      8.00     8.00     8.00     8.00     8.00     8.00
                            8.00     8.00

02 00 00  3C48         20 53 02   0.2  52.4 -4.7  D    0.0     0   1  1      0  02 00 00
02 22 00  ---          21 15 06   4.1  49.9 -4.4  D    0.0     0   F  1  17600

02 23 00  3C48         21 16 06   4.2  49.8 -4.4  D    0.0    36   1  2  17600  02 23 00
02 45 00  ---          21 38 10   7.9  47.0 -4.0  D    0.0     0   R  1      0

02 46 00  3C48         21 39 10   8.1  46.9 -4.0       0.0    36   1  3      0  02 46 00
03 08 00  ---          22 01 13  11.6  43.9 -3.6       0.0  1320   F  1  17600

03 09 00  3C48         22 02 14  11.8  43.7 -3.6       0.0    36   1  4  17600  03 09 00
03 31 00  ---          22 24 17  15.1  40.4 -3.2       0.0  1320   R  1      0

03 32 00  3C48         22 25 17  15.3  40.3 -3.2       0.0    36   1  5      0  03 32 00
03 54 00  ---          22 47 21  18.3  36.7 -2.8       0.0  1320   F  1  17600

03 55 00  3C48         22 48 21  18.5  36.5 -2.8       0.0    36   1  6  17600  03 55 00
04 17 00  ---          23 10 25  21.3  32.6 -2.5       0.0  1320   R  1      0

04 18 00  3C48         23 11 25  21.4  32.4 -2.4       0.0    36   1  7      0  04 18 00
04 40 00  ---          23 33 29  23.9  28.2 -2.1       0.0  1320   F  1  17600

04 41 00  3C48         23 34 29  24.0  28.0 -2.1       0.0    36   1  8  17600  04 41 00
05 03 00  ---          23 56 32  26.2  23.5 -1.7       0.0  1320   R  1      0

05 04 00  DA193        23 57 33 -15.9  53.0 -6.0  D    0.0   -92   1  9      0  05 04 00
05 15 00  ---          00 08 34 -14.0  52.2 -5.8  D    0.0     0   F  1   8800

05 17 00  3C48         00 10 35  27.4  20.5 -1.5       0.0   -37   1  9   8800  05 17 00
05 28 00  ---          00 21 36  28.2  18.1 -1.3       0.0   623   F  1  17600

05 29 00  3C48         00 22 37  28.3  17.9 -1.3       0.0    36   1 10  17600  05 29 00
05 51 00  ---          00 44 40  29.6  12.8 -0.9       0.0  1320   R  1      0

05 52 00  3C48         00 45 40  29.6  12.6 -0.9       0.0    36   1 11      0  05 52 00
06 14 00  ---          01 07 44  30.5   7.3 -0.5       0.0  1320   F  1  17600
Schedule for HART      (Code Hh )                                   Page   3
               3C48
  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.
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Tue   7 Jun 2005   Day 158 ---

06 15 00  3C48         01 08 44  30.5   7.1 -0.5       0.0    36   1 12  17600  06 15 00
06 37 00  ---          01 30 48  30.9   1.7 -0.1       0.0  1320   R  1      0

06 47 35  3C138        01 41 25  21.7  57.6 -3.7       0.0   502   1 13      0  06 47 35
06 58 35  ---          01 52 27  23.7  55.9 -3.5       0.0   660   F  1   8800
        Source only    7.6 degrees from the Sun.

06 58 35  DA193        01 52 27   3.3  42.2 -4.1  D    0.0   -73   1 13   8800  06 58 35
07 09 35  ---          02 03 29   4.9  40.9 -3.9  D    0.0     0   F  1  17600

07 14 26  3C48         02 08 20  30.5 352.6  0.5       0.0   132   1 14  17600  07 14 26
07 36 26  ---          02 30 24  29.6 347.4  0.9       0.0  1320   R  1      0

-----------  Tape Change ------------

07 51 26  3C48         02 45 26  28.8 343.9  1.1       0.0   865   1  1      0  07 51 26
08 13 26  ---          03 07 30  27.2 339.0  1.5       0.0  1320   F  1  17600

08 14 26  3C48         03 08 30  27.1 338.8  1.5       0.0    36   1  2  17600  08 14 26
08 36 26  ---          03 30 33  25.1 334.1  1.9       0.0  1320   R  1      0

08 41 17  3C138        03 35 26  40.3  34.1 -1.8       0.0   155   1  3      0  08 41 17
08 52 17  ---          03 46 27  41.6  31.1 -1.6       0.0   660   F  1   8800
        Source only    7.6 degrees from the Sun.

08 52 17  DA193        03 46 27  17.7  25.6 -2.2       0.0   -73   1  3   8800  08 52 17
09 03 17  ---          03 57 29  18.7  23.6 -2.0       0.0   587   F  1  17600

09 11 07  3C48         04 05 20  21.3 327.4  2.5       0.0   310   1  4  17600  09 11 07
09 33 07  ---          04 27 24  18.5 323.5  2.8       0.0  1320   R  1      0

09 34 07  3C48         04 28 24  18.4 323.3  2.8       0.0    36   1  5      0  09 34 07
09 56 07  ---          04 50 27  15.3 319.8  3.2       0.0  1320   F  1  17600

09 57 07  3C48         04 51 28  15.1 319.6  3.2       0.0    36   1  6  17600  09 57 07
10 19 07  ---          05 13 31  11.8 316.3  3.6       0.0  1320   R  1      0

10 25 44  3C138        05 20 10  47.5   0.5  0.0       0.0   262   1  7      0  10 25 44
10 36 44  ---          05 31 11  47.4 356.6  0.2       0.0   660   F  1   8800
        Source only    7.6 degrees from the Sun.

10 36 44  DA193        05 31 11  24.0   5.2 -0.4       0.0   -73   1  7   8800  10 36 44
10 47 44  ---          05 42 13  24.2   2.9 -0.2       0.0   587   F  1  17600
Schedule for HART      (Code Hh )                                   Page   4
               3C48
  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.
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Tue   7 Jun 2005   Day 158 ---

10 57 08  3C48         05 51 39   5.6 311.2  4.2  D    0.0   403   1  8  17600  10 57 08
11 19 08  ---          06 13 42   1.8 308.6  4.6  D    0.0     0   R  1      0

11 20 08  3C48         06 14 43   1.6 308.5  4.6  D    0.0    36   1  9      0  11 20 08
11 42 08  ---          06 36 46  -2.3 306.1  5.0  D    0.0     0   F  1  17600

11 48 35  3C138        06 43 14  43.0 332.7  1.4       0.0   251   1 10  17600  11 48 35
11 59 35  ---          06 54 15  41.8 329.6  1.5       0.0   660   R  1   8800
        Source only    7.6 degrees from the Sun.

11 59 35  DA193        06 54 15  22.9 347.9  1.0       0.0   -73   1 10   8800  11 59 35
12 10 35  ---          07 05 17  22.3 345.7  1.2       0.0   587   R  1      0

12 11 35  3C48         07 06 17  -7.8 303.2  5.5  D    0.0   -96   1 11      0  12 11 35
12 33 35  ---          07 28 21 -12.0 301.3  5.8  D    0.0     0   F  1  17600

12 34 35  3C48         07 29 21 -12.2 301.2  5.9  D    0.0    36   1 12  17600  12 34 35
12 56 35  ---          07 51 25 -16.4 299.4  6.2  D    0.0     0   R  1      0

13 02 06  3C138        07 56 57  33.1 314.1  2.6       0.0   206   1 13      0  13 02 06
13 13 06  ---          08 07 59  31.3 311.9  2.8       0.0   660   F  1   8800
        Source only    7.6 degrees from the Sun.

13 13 06  DA193        08 07 59  17.4 334.0  2.2       0.0   -73   1 13   8800  13 13 06
13 24 06  ---          08 19 00  16.3 332.1  2.4       0.0   587   F  1  17600

13 26 06  3C48         08 21 01 -22.3 297.3  6.7  D    0.0   -11   1 14  17600  13 26 06
13 34 06  ---          08 29 02 -23.9 296.8  6.9  D    0.0     0   R  1  11200

13 48 53  3C286        08 43 52   1.1  55.0 -4.8  D    0.0   541   1 14  11200  13 48 53
13 59 53  ---          08 54 54   3.1  53.7 -4.6  D    0.0     0   R  1   2400


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


 Setup file: ea033.18cm
   Matches group hh18cm in /home/vlbi/sched/catalogs/freq.dat
    Values confirmed by E-mail Jonathan Quick 291100 (CR)

   Setup group:   10         Station: HART              Total bit rate:  256
   Format: MKIV1:2           Bits per sample: 2         Sample rate: 16.000
   Number of channels:  8    Passes/head pos:   1       Speedup factor:   1.00

   Tape speeds: Low density - 270.000 ips,  High density - 160.00 ips
   Time per pass for  17600 ft, High density tapes is: 00:22:00

   1st LO=   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00
   Net SB=         U         U         U         U         U         U         U         U
   Pol.  =      RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
   BBC   =         2         1         4         3         6         5         8         7
   BBC SB=         U         U         U         U         U         U         U         U
   IF    =        2N        1N        2N        1N        2N        1N        2N        1N

  The following frequency sets based on this setup were used.

   Frequency Set:  10  Setup file default.  No pcal detection.
   LO sum=    1637.99   1637.99   1645.99   1645.99   1653.99   1653.99   1661.99   1661.99
   BBC fr=     127.99    127.99    135.99    135.99    143.99    143.99    151.99    151.99
   Bandwd=      8.000     8.000     8.000     8.000     8.000     8.000     8.000     8.000

   Track assignments are: 
    track1=   2, 10, 18, 26,  3, 11, 19, 27
    barrel=roll_off 
 SOURCE LIST -- 3C48
     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)

   J0137+3309        01 34 49.826428   * 01 37 41.299494     01 37 58.240862       0.90
   0134+329          32 54 20.25964    * 33 09 35.13382      33 11 04.85479        0.91
 * 3C48              /home/vlbi/sched/catalogs/sources.vlba
   J0137+33          VLBA Calib Srcs - GSFC sols. - catalog 2004f_astro
                        8.017 scan hours,    286.509 baseline hours above horizon.

   J0521+1638        05 18 16.514154   * 05 21 09.886036     05 21 26.865476       0.58
   0518+165          16 35 26.83434    * 16 38 22.05180      16 38 46.19998        0.76
 * 3C138             /home/vlbi/sched/catalogs/sources.vlba
   J0521+16          VLBA Calib Srcs - GSFC sols. - catalog 2004f_astro
                        0.917 scan hours,     34.832 baseline hours above horizon.

   J0555+3948        05 52 01.407172   * 05 55 30.805614     05 55 51.310111       0.26
   0552+398          39 48 21.94585    * 39 48 49.16500      39 49 00.30450        0.40
 * DA193             /home/vlbi/sched/catalogs/sources.vlba
   J0555+39          VLBA Calib Srcs - GSFC sols. - catalog 2004f_astro
                        1.100 scan hours,     34.346 baseline hours above horizon.

   J1331+3030        13 28 49.657757   * 13 31 08.288049     13 31 24.176855       0.37
   1328+307          30 45 58.64062    * 30 30 32.95926      30 28 58.46438        0.47
 * 3C286             /home/vlbi/sched/catalogs/sources.vlba
   J1331+30          VLBA Calib Srcs - GSFC sols. - catalog 2004f_astro
                        0.183 scan hours,      5.133 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) 
   3C48                45.8
   3C138                7.6
   DA193               20.5
   3C286              106.6

  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 

