  We present Giant Metrewave Radio Telescope (GMRT) observations of OH
absorption in B3~1504+377 ($z \sim 0.673$) and PKS 1413+135 ($z \sim 0.247$).
OH has now been detected in absorption towards four intermediate redshift
systems, viz. the lensing galaxies towards B~0218+357 ($z \sim 0.685$; Kanekar
et al. 2001) and 1830-211 ($z \sim 0.886$; Chengalur et al. 1999), in addition
to the two systems listed above. All four systems also give rise to well
studied millimetre wavelength molecular line absorption from a host of
molecules, including HCO$^+$. Comparing our OH data with these millimetre line
transitions, we find that the linear correlation between $N_{\rm OH}$ and
$N_{\rm HCO^+}$ found in molecular clouds in the Milky Way (Liszt & Lucas 1996)
persists out to $z \sim 1$. It has been suggested (Liszt & Lucas 1999) that OH
is a good tracer of ${\rm H_2}$, with $N_{\rm H_2}/N_{\rm OH} \approx 10^7$
under a variety of physical conditions. We use this relationship to estimate
$N_{\rm H_2}$ in these absorbers. The estimated $N_{\rm H_2}$ is $\ga 10^{22}$
in all four cases and substantially different from estimates based on CO
observations.
