  We compute the $^{63}$Ga(p,$\gamma$)$^{64}$Ge and
$^{64}$Ge(p,$\gamma$)$^{65}$As thermonuclear reaction rates using the latest
experimental input supplemented with theoretical nuclear spectroscopic
information. The experimental input consists of the latest proton thresholds of
$^{64}$Ge and $^{65}$As, and the nuclear spectroscopic information of
$^{65}$As, whereas the theoretical nuclear spectroscopic information for
$^{64}$Ge and $^{65}$As are deduced from the full pf-shell space
configuration-interaction shell-model calculations with the GXPF1A Hamiltonian.
Both thermonuclear reaction rates are determined with known uncertainties at
the energies that correspond to the Gamow windows of the temperature regime
relevant to Type I X-ray bursts, covering the typical temperature range of the
thermonuclear runaway of the GS 1826$-$24 periodic bursts and SAX
J1808.4$-$3658 photospheric radius expansion bursts.
