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A subset of Post-AGB (PAGB) objects are the highly luminous RV Taurivariables that show similarities to Type-II Cepheids. By using a sample ofknown RV Tauri stars from the Magellanic Clouds we are able to determine periodluminosity relationships (PLRs) in various bands that have been used todetermine the luminosities of their Galactic counterparts. We have gathered allavailable photometry in order to generate an SED for each object and determinethe total integrated flux. This total flux combined with a calculated orinferred intrinsic luminosity leads to a distance (Vickers et al. 2015). Thisdistance catalogue has allowed us to begin to constrain the physical parametersof this poorly understood evolutionary phase and to determine links betweenthese physical characteristics as a function of their stellar population.

A homogeneous distance catalogue for Galactic RV Tauri objects