The z=0.8596 Damped Lyman Alpha Absorbing Galaxy Toward PKS 0454+039

We present {\it Hubble Space Telescope} and ground–based data on the $z_{abs}=0.8596$ metal line absorption system along the line of sight to PKS 0454+0356. The system is a moderate redshift damped Lyman alpha system, with $\mathrm{N}(\mathrm{H}\mathrm{I})=(5.7\pm 0.3)\times {10}^{20}$~cm${}^{-2}$ as measured from the {\it Faint Object Spectrograph} spectrum. We also present ground–based images which we use to identify the galaxy which most probably gives rise to the damped system; the most likely candidate is relatively underluminous by QSO absorber standards ($M_B\sim -19.0$ for $q_0=0.5$ and $H_0=50$ \kms Mpc${}^{-1}$), and lies $\sim 8.5h^{-1}$ kpc in projection from the QSO sightline. Ground–based measurements of Zn~II, Cr~II, and Fe~II absorption lines from this system allow us to infer abundances of [Zn/H]=$-1.1$, [Cr/H]=$-1.2$, and [Fe/H]=$-1.2$, indicating overall metallicity similar to damped systems at $z>2$, and that the depletion of Cr and Fe onto dust grains may be even {\it less} important than in many of the high redshift systems of comparable metallicity. Limits previously placed on the 21-cm optical depth in the $z=0.8596$ system, together with our new N(H~I) measurement, suggest a very high spin temperature for the H~I, $T_S>>580$ K.