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Fossil group origins IV Characterization of the sample and observational properties of fossil systems

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Figure

Fig. 1. Distribution of redshifts (of 34 FG candidates byleft panel), X-ray luminosities (central panel), and absolute magnitudes of the BGGs (right panel) for the sample Santos et al
Fig. 4. Spectroscopic completeness of the 25 FG candidates with eitherFOGO or SDSS spectroscopy (top panel) and success rate of the 18 FGcandidates with FOGO spectroscopy only (bottom panel) as a functionof r-band magnitude.
Fig. 5. Identification of the members of the 25 FG candidates in the redshift space. For each system we show all the galaxies in the field of view(black histogram), as well as the galaxies identified as members using the DEDICA procedure (green histogram) ass
Fig. 6. Velocity–position diagram of the sample of FG candidates. Green filled and black open circles mark the member and non-member galaxies,respectively
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