Very Luminous Galaxies (Cappi+, 2003)

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Galaxy Catalogs, Redshifts, Velocity Dispersion

Scientific paper

Three VLGs were selected from our catalogue of VLGs (see Table 1 of Paper I, Cappi et al., 1998A&A...335..779C), while a fourth galaxy satisfying the VLG definition was selected from the CfA catalogue (see Geller & Huchra, 1989Sci...246..897G); the 4 VLG fields were observed at OHP. Other 15 VLG fields were extracted from the 2dFGRS public catalogue (Cat. ), which has an overlap with the SSRS2 (Cat. ). While partially imposed by observational constraints (see below), our selection is random with respect to the VLG properties, and should be representative of the whole sample. In fact, one third of the selected VLGs are early-type galaxies, a fraction consistent with that of the total sample published in Paper I, Cappi et al. (1998A&A...335..779C).
(3 data files).

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