Notes. ^(a)Equatorial coordinates of the continuum peak measured by Maury et al. (2019). ^(b)Internal luminosity, estimated from the Herschel Gould Belt Survey (HGBS, see André et al. 2010 and Ladjelate et al., in prep.). ^(c) Envelope mass, corrected for the assumed distance. ^(d)Peak flux density at 1.4 mm measured by Maury et al. (2019). ^(e)PA of the jet blue lobe. We adopt the values measured by Podio et al. (in prep.) from CALYPSO observations of the SiO line emission. These values are in agreement with those estimated from previous studies, e.g., Codella et al. (2014; NGC 1333-IRAS 2A), Santangelo et al. (2015; NGC 1333-IRAS AA), Podio et al. (2016; L1157) and Tokuda et al. (2014; 2016; L1521F). ^(f) References for the protostar discovery, distance and envelope mass. ^(g)Jet is asymmetric: the red-shifted lobe PA is 140°. ^(h) The distance of GF9-2 is very uncertain. Here we adopt a distance of 200 pc (Wiesemeyer et al. 1997), but another study suggests a distance of 474 pc (Zucker, priv. comm.).

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