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emissionLinesPortSPECTRO Emission line kinematics results for SDSS and BOSS galaxies using GANDALF
We fit galaxies using an adaptation of the publicly available Gas AND Absorption Line Fitting (GANDALF, Sarzi et al. 2006) and penalised PiXel Fitting (pPXF, Cappellari & Emsellem 2004). Stellar population models for the continuum are from of Maraston & Strömbäck (2011) and Thomas, Maraston & Johansson (2011).