\\ Species Tag:        &   49002 & Name:&  O3-asym-O-17   
\\ Version:            &       2 & & Ozone, 
\\ Date:       &  Mar. 1984      & &  asymmetric
\\ Contributor:&  E. A. Cohen    & &  $^{17}$O isotope
\\             &                 & & 
\\ Lines Listed:       &   52613 & Q(300.0)=&    42098.453 
\\ Freq. (GHz) $<$     &    4681 & Q(225.0)=&    27331.975 
\\ Max. J:             &      77 & Q(150.0)=&    14876.039 
\\ LOGSTR0=            &    -8.6 & Q(75.00)=&     5268.769 
\\ LOGSTR1=            &    -8.3 & Q(37.50)=&     1873.796 
\\ Isotope Corr.:      &  -3.131 & Q(18.75)=&      672.414 
\\ Egy. (cm$^{-1}$) $>$&     0.0 & Q(9.375)=&      246.163 
\\ $\mu_a$ = & 0.0037            & A=& 105491.1
\\ $\mu_b$ = & 0.5337            & B=&  12951.3
\\ $\mu_c$ = &                   & C=&  11508.0
\headend 

The spectra are from E. A. Cohen, K. W. Hillig II, and H. M. Pickett,
1995, J. Mol.\ Struct.\ {\bf 352/353,} 273, as well as the more recently
measured $32_{2,30}-32_{1,31}$ transition near 426012 MHz.   The
calculation fixes centrifugal distortion constants beyond the sextic terms 
to those of the parent species with the exception of the coefficients of 
$P_a^{2n}$ which are assumed to be proportional to $A^n$.  The dipole moments 
are  assumed values based on the structure and the value for
the parent species, however centrifugal corrections have not been applied. 
Where several experimental lines have the same frequency,
the uncertainties refer to the center of a blended feature, not to the
individual components.