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X-ray analysis and broad-band properties of [NeV]-selected type 2 AGN

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Alma Mater Studiorum · Universit`

a di Bologna

Scuola di Scienze

Dipartimento di Fisica e Astronomia

Corso di Laurea Magistrale in Astrofisica e Cosmologia

X-ray analysis and broad-band properties of

[NeV]-selected type 2 AGN

ALLEGATO B

Relatore:

Chiar.mo Prof.

Cristian Vignali

Co-relatori:

Presentata da:

Luigi Barchiesi

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Appendix B - SED fitting results

In this section we report the SED fitting results for the sources from 824548 to 910023, the SED-fitting of the other sources are in Appendix A. All the details about the sample, the SED-fitting code and the model used are explained in details in section 4.

Figure 1: SED decomposition and residuals to the best-fitting solution. Data with 1 σ confidence error are from the COSMOS2015 catalog (Laigle et al. 2016). The black line is the best-fit SED, the blue is the galactic contribution, which is composed of heated-dust emission (grey) and stellar emission (green). The green dashed line is the stellar contribution accounting for the dust extinction. The red line is the torus (AGN) emission. The reported ¯χ2 is the χ2 divided by the number of photometric points.

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Figura

Figure 1: SED decomposition and residuals to the best-fitting solution. Data with 1 σ confidence error are from the COSMOS2015 catalog (Laigle et al

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