Fig. 4

Fitted SED of SU AUR using the model parameters described in Sect. 5. Data are taken from Cutri & et al. (2012) (WISE); Høg et al. (2000) (the Tycho-2 Catalogue); Mermilliod (1991) (Johnson UBV); Morel & Magnenat (1978) (Johnson UBVRIJKLM); Ishihara et al. (2010) (AKARI/IRC mid-IR all-sky Survey – L18W+S9W); Ducati (2002) (Johnson VJKLMN); Ofek (2008) (Johnson JKH); ESA (1997) (Tycho-2.BT+.VT); Droege et al. (2006) (Cousins I; Johnson V); Monet et al. (2003) (USNO-B1.0.B1+.R1); tISAS/JAXA (2010) (AKARI/IRC mid-IR all-sky Survey – WIDEL+WIDES+N160+N60); Kharchenko (2001) (Johnson BV); Skrutskie et al. (2006) (2MASS JKsH); Hauck et al. (1990) (Johnson UBV); Andrews & Williams (2005) (450 and 850 μm filters).
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