\\ Species Tag:        &   57001 & Name:&  C-13CS 
\\ Version:            &       1 & & Dicarbon monosulfide
\\ Date:       &Nov. 1993         & & $^{13}$CCS, X $^3\Sigma^-$  
\\ Contributor:&  E. A. Cohen   & &
\\             &                 & &
\\ Lines Listed:       &    1013 & Q(300.0)=&     5953.713
\\ Freq. (GHz) $<$     &    1232 & Q(225.0)=&     4438.003
\\ Max. J:             &      99 & Q(150.0)=&     2922.894
\\ LOGSTR0=            &    -8.0 & Q(75.00)=&     1410.246
\\ LOGSTR1=            &    -6.0 & Q(37.50)=&      658.455
\\ Isotope Corr.:      &   -1.955& Q(18.75)=&      290.244
\\ Egy. (cm$^{-1}$) $>$&     0.0 & Q(9.375)=&      117.819
\\ $\mu_a$ = &2.9                & A=&
\\ $\mu_b$ = &                   & B=&6188.08655(51)
\\ $\mu_c$ = &                   & C=&
\headend
The measurements were taken from S. Yamamoto {\it et al.}, 1990, Astrophys.\ J.
{\bf 361}, 318.  The dipole moment was quoted in this paper from an
{\it ab initio} calculation by A. Murakami.  Uniform weighting of the
reported measurements reproduces the molecular parameters given
in the referenced paper.  An assigned uncertainty of 30 kHz for each 
measured line produces approximately the same $1\sigma$
uncertainties for calculated transitions as reported in the reference.
Note that $N$ is not a good quantum number and that in this calculation
the naming of the $N_J=2_1$ and $0_1$ is the reverse of that in the reference.
Yamamoto {\it et al.}, report 9 individual hyperfine components due to
the $^{13}$C splitting and 17 unresolved doublets.  As a result the
measured frequencies have not been merged.  Only calculated frequencies are
listed.