All Figures

Figure 1: Correlations: photon index versus normalization for (top left) 3C 273 (3EG J1229+0210), (bottom left) Mkn 421 (3EG J1104+3809), and (bottom right) PKS 2155-304 (3EG J2158-3023). (Top right) Equivalent width of the FeK line versus photon index for 3C273. The open square indicates the XMM-Newton data from the present work, while the filled circle represents the values from BeppoSAX observations reported in Grandi & Palumbo (2004). The points of the simultaneous BeppoSAX-XMM-Newton observation (June 2001) are tagged with a triangle, filled for BeppoSAX and open for XMM-Newton.

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In the text

Figure 2: SED of newly modelled blazars: (top, left) AO 0235+164; (top, right) PKS 1334-127; (bottom, left) PKS 1406-076; (bottom, right) PKS 1830-211, not corrected for the gravitational lensing effects. The black line is a single-zone synchrotron inverse Compton model using the input parameters listed in Table 4. In all the SED, the XMM-Newton data are indicated with black filled symbols, while the remaining symbols and lines (grey) refer to archival data. The bump at 1014-15 Hz is the assumed disk spectrum.

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In the text

	Figure 3: Updated blazar sequence, adapted from Ghisellini et al. (2002), with the addition of the new TeV BL Lacs. We mark with black filled symbols the sources analyzed in this paper, emphasizing AO 0235+164 (in quiescence and during the outburst presented in this work), PKS 1334-127, PKS 1406-076 (the fit without the X-ray detection and with the present data), and PKS 1830-211.
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In the text

Figure A.1: SED of the sources studied in this paper. We compare the XMM-Newton data (filled black symbols) to the available archival data in all bands.


In the text

Figure A.2: SED of the sources studied in this paper. We compare the XMM-Newton data (filled black symbols) to the available archival data in all bands.


In the text