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Fig. 11


Spectral energy distribution of two T Tauri candidates: 2XMM J223122.8+390914 (left) and 2XMM J184401.2+005455 (right). We compare the SED of the T Tauri stars with stellar atmosphere models (grey) from Castelli & Kurucz (2004) with effective temperatures 5200 K and 4000 K respectively, and log    (g) = 4.5. The optical spectra obtained at the telescope are shown as a black line, and upper limits on the magnitude are indicated with an arrow.

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