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Table 5

Comparison of stellar mass estimates between our catalog and the ones derived by changing one of the model descriptions outlined in Sect. 6.

Module Δ NMAD Δ NMAD Δ NMAD
ALL StarForm AGN
IMF (Chabrier 2003 vs. Salpeter 1955) −0.244 0.362 −0.248 0.367 −0.246 0.364
SSP (Bruzual & Charlot 2003 vs. Maraston 2005) −0.258 0.382 −0.235 0.348 −0.262 0.388
SFH (delayed with extra burst vs. non parametric) 0.027 0.066 0.039 0.094 0.044 0.084
Z (metallicity fixed to solar vs. variable) −0.039 0.076 −0.040 0.073 −0.046 0.101

DustAtt (Calzetti et al. 2000 vs. Charlot & Fall 2000) −0.031 0.063 −0.024 0.063 −0.109 0.167
DustEm (Draine et al. 2014 vs. Dale et al. 2014) −0.000 0.018 −0.000 0.028 −0.000 0.049

AGN (Fritz et al. 2006 vs. no AGN) 0.004 0.018 0.007 0.024 −0.001 0.045
AGN (Fritz et al. 2006 vs. Stalevski et al. 2012, 2016) 0.001 0.006 0.003 0.007 0.005 0.030

SEDs (grzW14 vs. grzW12) −0.002 0.055 −0.009 0.071 −0.013 0.187
SEDs (grzW14 vs. grz) 0.036 0.166 0.067 0.190 0.044 0.212

Notes. The median difference (Δ), and NMAD (see Sect. 5.1 for definitions) are reported for the given change in the model considering the change in the initial mass function (IMF), single stellar population models (SSP), star formation history prescription (SFH), metallicity (Z), dust attenuation law (DustAtt), dust emission model (DustEm), and AGN models (AGN). The influence of the presence of MIR information is also reported. The metrics are derived for the entire representative sample (All) and separately for star-forming galaxies (StarForm) and AGN (including both NLs and BL AGNs).

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