USNO Analysis Report for I18011 ($18JAN11XU) 
       This report is a contributed analysis report that does not correspond to 
       the database maintained by the IVS Data Centers for this session.  
   (Analyzed by Christopher Dieck, US Naval Observatory.
    Spoolfile source: interactive nuSolve analysis.) 

Problems: The SVETLOE data was very noisy, as it has been for most of the recent Thursday INT1s in which it participated. Only 4 scans from each SVETLOE baseline are included.

Number of observations rejected during correlation:    1
      Scan 011-1914: Error code G on S-Band. (SV baseline)

Number of observations not usable by the software:     3
      Scan 011-1855: FQ = 0 on  S-Band due to low SNR, source 1636+473 (KV baseline)
      Scan 011-1927: FQ = 0 on  X-Band due to low SNR, source 2209+236 (KV baseline)
      Scan 011-1927: FQ = 0 on  X-Band due to low SNR, source 2209+236 (KS baseline)

Number of observations rejected during analysis:      15
    Noisy SVETLOE scans that are deselected
      Observation  3, SVETLOE:WETTZELL, 0955+476, 18:30:20, which fits at -1309.46 +/- 13.16 ps.
      Observation  6,    KOKEE:SVETLOE, 1800+440, 18:35:17, which fits at  3699.46 +/- 70.74 ps.
      Observation  7, SVETLOE:WETTZELL, 1800+440, 18:35:17, which fits at -3784.88 +/- 15.76 ps.
      Observation  9,    KOKEE:SVETLOE,    3C371, 18:38:05, which fits at  7283.53 +/- 80.68 ps.
      Observation 10, SVETLOE:WETTZELL,    3C371, 18:38:05, which fits at   689.29 +/- 15.01 ps.
      Observation 13,    KOKEE:SVETLOE, 1418+546, 18:43:56, which fits at  3670.87 +/- 89.59 ps.
      Observation 14, SVETLOE:WETTZELL, 1418+546, 18:43:56, which fits at  2651.60 +/-  8.43 ps.
      Observation 17,    KOKEE:SVETLOE, 1300+580, 18:47:10, which fits at -2104.07 +/- 73.38 ps.
      Observation 18, SVETLOE:WETTZELL, 1300+580, 18:47:10, which fits at -5777.27 +/- 16.22 ps.
      Observation 29,    KOKEE:SVETLOE, 0716+714. 19:05:30, which fits at  5580.91 +/- 70.47 ps.
      Observation 30, SVETLOE:WETTZELL, 0716+714. 19:05:30, which fits at  2255.97 +/- 13.79 ps.
      Observation 34,    KOKEE:SVETLOE, 1800+440, 19:11:49, which fits at -7871.27 +/- 71.33 ps.
      Observation 37,    KOKEE:SVETLOE, 2113+293, 19:15:29, which fits at -4248.61 +/- 73.68 ps.
      Observation 45, SVETLOE:WETTZELL, 2209+236, 19:27:44, which fits at  9219.75 +/- 15.27 ps.

    Outliers:
      Observation 12,   KOKEE:WETTZELL, 1418+546, 18:43:56, which fits at   285.73 +/- 76.66 ps.

Other comments: None. 

Parameterization: 
   8 parameters: 
     UT1 offset 
     atmosphere offset for:
         KOKEE SVETLOE WETTZELL
     clock offset (0), first order term (1), and/or second order term (2) for:
         KOKEE (0,1) SVETLOE (0,1)

Clock breaks: None

Session Statistics 

  Observations:       45 scheduled 
                      44 correlated (included in the database) 
                      41 recoverable (usable in Solve/nuSolve) 
                      26 used
  Session fit:        15.526 ps
  UT1 formal error:    5.82 microsec 

Source Performance 

                    Number of Observations

                Scheduled  Correlated*    Used    

  0716+714              4           4        2
  0800+618              1           1        1
  0920+390              1           1        1
  0955+476              3           3        2
  1144+402              3           3        3
  1300+580              3           3        1
  1418+546              6           6        3
  NGC6251               3           3        3
  1636+473              2           2        1
  1803+784              1           1        1
  1800+440              6           6        3
  3C371                 3           3        1
  2113+293              3           2        1
  2141+175              1           1        1
  2144+092              1           1        1
  2209+236              3           3        0
  2229+695              1           1        1
  ------------  ---------  ----------   ------
  Source Total         45          44       26

 * Correlated means included in the database. 
   Please note that the number of recoverable (usable) observations 
   cannot be broken down by source for Intensive solutions.