\\ Species Tag:        &   29006 & Name:&  CO-17         
\\ Version:            &       2 & & Carbon monoxide,
\\ Date:       & Aug. 1997       & & $^{17}$O isotope
\\ Contributor:& H. S. P. M\"uller & &
\\             &                 & &
\\ Lines Listed:       &      50 & Q(300.0)=&      111.678
\\ Freq. (GHz) $<$     &    5532 & Q(225.0)=&       83.828
\\ Max. J:             &      50 & Q(150.0)=&       55.987
\\ LOGSTR0=            &   -12.5 & Q(75.00)=&       28.157
\\ LOGSTR1=            &   -12.5 & Q(37.50)=&       14.248
\\ Isotope Corr.:      &  -3.432 & Q(18.75)=&        7.298
\\ Egy. (cm$^{-1}$) $>$&     0.0 & Q(9.375)=&        3.831
\\ $\mu_a$ = & 0.11034           & A=&
\\ $\mu_b$ = &                   & B=& 56179.990
\\ $\mu_c$ = &                   & C=&
\headend
 
The experimental measurements were reported by (1) M. Winnewisser, B. P.
Winnewisser, and G. Winnewisser, in 1985, "Molecular Astrophysics, Series C"
(G. H. F. Diercksen, W. F. Huebner, and P. W. Langhoff, Eds.), Vol. 157,
pp. 375 -- 402. Reidel, Dordrecht. No hyperfine splittings due to $^{17}$O
have been reported in this study. Hyperfine splittings for the J = 1 -- 0
transition were reported in (2)
F. J. Lovas and E. Tiemann, 1974, J. Phys. Chem. Ref. Data {\bf 3}, 609-770.
The experimental line positions and uncertainties, the logarithmic line
strengths, and the quantum numbers $F'+1/2$ and $F''+1/2$, are \\
  112358.7200  0.1000 -5.6952  2  3   \\
  112358.9800  0.0200 -5.3942  4  3   \\
  112360.0160  0.0200 -5.5191  3  3   \\
The dipole moment and dipole centrifugal corrections are taken from (3)
D. Goorvitch, 1994, Astrophys.\ J. Suppl.\ {\bf 95}, 535. Additional
rotational lines up to R(60) from (3) were included in the fit.