A systematic study of the \ensuremath{\alpha} decay of $^{181\mathrm{\ensuremath{-}}186}\mathrm{Au}$ utilizing an on-line isotope separator has revealed several \ensuremath{\alpha} groups and resulted in the observation of the \ensuremath{\alpha} decay of $^{186}\mathrm{Au}$ and $^{185}\mathrm{Pt}$. By simultaneous measurement of \ensuremath{\gamma}-ray and x-ray spectra and use of known EC/${\mathrm{\ensuremath{\beta}}}^{+}$ decay schemes, \ensuremath{\alpha}-decay branching ratios and hindrance factors were deduced for each \ensuremath{\alpha} transition. In $^{185}\mathrm{Au}$ and $^{183}\mathrm{Au}$ the ground state is known to be dominated by the 5/${2}^{\mathrm{\ensuremath{-}}}$,1/2[541] configuration associated with the ${\mathit{h}}_{9/2}$ intruder from above the Z=82 closed shell. Thus, the unhindered \ensuremath{\alpha} decay of these parents identify levels in the Ir daughters which also are dominated by the ${\mathit{h}}_{9/2}$ orbital. Several previously unknown low-lying \ensuremath{\gamma}-ray transitions were observed in the Ir daughters by means of \ensuremath{\alpha}-\ensuremath{\gamma} coincidence measurements. The hindrance factor for the \ensuremath{\alpha} decay of $^{181}\mathrm{Au}$ to the 5/${2}^{\mathrm{\ensuremath{-}}}$,1/2[541] ground state of $^{177}\mathrm{Ir}$ suggests that the ground state of $^{181}\mathrm{Au}$ has a different configuration than those of $^{183}\mathrm{Au}$ and $^{185}\mathrm{Au}$.
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