Switching between four common stellar population synthesis models produces systematic offsets of up to 0.6 dex in stellar mass and 0.4 dex in star formation rate for the same galaxies.
Figure 2: Analysis of the risk of bias in accordance with the cochrane collaboration guidelines (Sigal et al., 2007; Church et al., 2010; Lambers et al., 2008; Tomas-Carus et al., 2016; Seyedizadeh, Cheragh-Birjandi & Hamedi Nia, 2020; Johansen et al., 2017; Macdonald et al., 2021; Aylin et al., 2009; Myers et al., 2013; Balducci et al., 2010; Reid et al., 2010; Stomby et al., 2017; Callisaya et al., 2017; Newton et al., 2020; Sénéchal et al., 2013; Annibalini et al., 2017; Donyaei et al., 2024; Larose et al., 2010; Byrkjeland et al., 2015; Banitalebi et al., 2019; Sparks et al., 2013; Banitalebi et al., 2021; Kadoglou et al., 2013; De Oliveira et al., 2012; Jamshidpour, Bahrpeyma & Khatami, 2020; Delevatti et al., 2022, 2020; Kang, Ko & Baek, 2016; Ghodrati et al., 2023; Martínez-Velilla et al., 2021; Espeland et al., 2017; Szilágyi et al., 2019; Jeon et al., 2020; Cai et al., 2023; Venkataraman et al., 2019; Yue et al., 2023; Ahmad et al., 2020).
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Impact of stellar population models on the estimated physical properties of galaxies
Switching between four common stellar population synthesis models produces systematic offsets of up to 0.6 dex in stellar mass and 0.4 dex in star formation rate for the same galaxies.