Fig. 5.
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Same as Fig. 4 but here we show the output plot generated by astroARIADNE. The synthetic photometry is shown via the cyan points; the purple diamonds show the fit points. The synthetic spectrum is a spectrum with the parameters Teff = 9500 K, log g = 3.5 and [Fe/H]= − 0.1 dex taken from Kurucz (1993). This method probes a smaller wavelength range so that no IR excess can be seen here.
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