\\ Species Tag:        &   48004 & Name:&  O3            
\\ Version:            &       4 & &Ozone,
\\ Date:       &  Nov 2005       & &ground vibrational 
\\ Contributor:&  B. J. Drouin   & &state
\\             &  H. M. Pickett  & &
\\ Lines Listed:       &    7133 & Q(300.0)=&     3553.040
\\ Freq. (GHz) $<$     &    8908 & Q(225.0)=&     2230.489
\\ Max. J:             &      80 & Q(150.0)=&     1198.671
\\ LOGSTR0=            &    -9.8 & Q(75.00)=&      423.448
\\ LOGSTR1=            &   -10.0 & Q(37.50)=&      150.038
\\ Isotope Corr.:      &     0.0 & Q(18.75)=&       53.297
\\ Egy. (cm$^{-1}$) $>$&     0.0 & Q(9.375)=&       19.037
\\ $\mu_a$ = &                   & A=&106536.224
\\ $\mu_b$ = &    0.5337         & B=&13349.254
\\ $\mu_c$ = &                   & C=&11834.361
\headend

The ozone spectrum was fitted using the microwave, millimeter, far-infrared,
and infrared transitions given in H. M. Pickett {\it et al.}, (1985), J. Mol.\ 
Spect.\ {\bf 110}, 186, H. M. Pickett {\it et al.}, (1988), J. Mol.\ 
Spect.\ {\bf 128}, 151, De Natale {\it et al.}, (1997), Appl.\ Op.\ {\bf 36}, 8526, and
Colmont {\it et al.}, (2005), J.\ Mol.\ Spec.\ {\bf 233}, 203. The dipole moment is 
from K. M. Mack and J. S. Muenter, (1977)
J.\ Chem.\ Phys.\ {\bf 66}, 15.  Line strengths were calculated using 
Herman Wallis parameters fitted to match intensities from a model Hamiltonian 
in which the ground state and the three fundamentals 
were coupled with theoretical matrix elements, and infrared transition 
dipoles were allowed to mix with the permanent dipole.
This treatment gives the correct perturbation of the rotational intensities 
due to centrifugal distortion.  Comparisons of calculated intensities agree within 2$\sigma$ to those of M. Birk, G. Wagner and J-M. Flaud, (1994), J. Mol. Spec. {\bf 163}, 245-261.  The partition includes contributions from 
all vibrational states.