Full SED (including synchrotron and Compton emission) of models which are roughly consistent with the broadband observations of Sgr A* (models # 20, 24, 35, and 39, see Table 1.). The observational data points and upper limits are taken from Falcke et al. (1998), An et al. (2005), Marrone et al. (2006), Melia & Falcke (2001), Doeleman et al. (2008), Schoedel et al. (2011), and the X-ray luminosity of the inner accretion flow is from Neilsen et al. (2013).