Contents.
      planet: 7 - Uranus
  satellites: U1-Ariel     : 3,
              U2-Umbriel   : 2,
              U3-Titania   : 5,
              U4-Oberon    : 5
total number: 15
        type: absolute
       dates: 1963-1963
 observatory: 083 - Golosseevo-Kiev

Reference.
    Shatokhina S. V. (2012)
    Astrometric positions of the external planets and their satellites.
    On-line Data Catalog: DBGPA 3/07. Originally published in: http://gua.db.ukr-vo.org/starcatalogs.php?whc=unp.
    2012apep__cat_____S

Informations.
           relative to: absolute
       reference frame: astrometric
       center of frame: geocenter
      epoch of equinox: ICRF/J2000.0
            time scale: UTC
             reduction: ACT catalog
           coordinates: absolute
      diff. refraction: no information
              receptor: photographic
             telescope: 400/5500 double long-focus astrograph (DLFA)
             observers: M.L.Divinsky, O.M.Izhakevich, L.M.Kizyun, A.S.Kotovich, A.M.Kuryanova, I.M.Ledovska, R.F.Lisyakova,
                        S.P.Mayor, G.V.Moroz, A.B.Onegina, E.M.Sereda, Yu.K.Filipov, S.V.Shatokhina
data included in standard data file: no

Comments.
  The residuals (O-C) were obtained by comparing the positions with the theoretical ones provided by Horizons On-Line Ephemeris System (JPL).

Format.
  1. Observed satellite number (N): 1 - U1, 2 - U2, 3 - U3, 4 - U4
  2. Number of the plate
  3. Year   of the date of observation
  4. Month  of the date of observation
  5. Day    of the date of observation with decimals
  6. Hour   of right ascension (alpha, h)
  7. Minute of right ascension (alpha, m)
  8. Second of right ascension (alpha, s) with decimals
  9. Degree of declination (delta, deg)
 10. Minute of declination (delta, '  )
 11. Second of declination (delta, '' ) with decimals
 12. Residual (O-C) in alpha (arcseconds)
 13. Residual (O-C) in delta (arcseconds)

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N Plate Year   Day         alpha         delta          O-C   O-C
             Month         h  m  s      deg ' ''        alpha delta
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