Table 3: The table lists the ecliptic coordinates of the asteroid's spin axis direction $(\lambda_{\rm p},~ \beta_{\rm p})$, its sidereal rotation period P, the span of observations in years, the number of oppositions  $N_{\rm opp}$, the number of lightcurves  $N_{\rm lc}$, and the rms residual of the fit.
Asteroid \(\lambda_{\rm p}\) \(\beta_{\rm p}\) P Years of obs. $N_{\rm opp}$ $N_{\rm lc}$ rms
  [deg] [deg] [hr]       [mag]
(110) Lydia 331 -61 10.92580 1958-2003 4 26 0.011
  149 -55          
(125) Liberatrix 280 +74 3.968199 1981-2005 7 34 0.024
  95 +68          
(130) Elektra 65 -88 5.224664 1980-2003 11 54 0.013
(165) Loreley 346 +29 7.22667 1981-2006 6 29 0.015
(196) Philomela 276 -49 8.332827 1964-2006 8 27 0.013
  111 -41          
(218) Bianca 305 +17 6.33717 1979-2005 10 50 0.015
  121 -10          
(306) Unitas 79 -35 8.73875 1979-2003 5 15 0.015
  254 -18          
(423) Diotima 351 +4 4.775377 1981-2006 10 48 0.017
(776) Berbericia 347 +12 7.66701 1977-2006 8 36 0.012
(944) Hidalgo 281 +5 10.058634 1976-2004 4 14 0.013

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