1939
DOI: 10.2307/40083811
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Mére et Fils

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“…The scatter of the mock samples was adjusted so that the radial variation of the peculiar velocities at large distances in the mock catalog match the observations. The derived scatter of < ∼ 0.4 mag depends on the HI line-width, and is in any case smaller than that obtained for galaxies in clusters (Giovanelli et al 1996a). A more extensive discussion of the motivation and the -7details for the adopted procedure will be presented in da Costa et al (1996).…”
Section: Analysis Of the Sfi Samplementioning
confidence: 88%
“…The scatter of the mock samples was adjusted so that the radial variation of the peculiar velocities at large distances in the mock catalog match the observations. The derived scatter of < ∼ 0.4 mag depends on the HI line-width, and is in any case smaller than that obtained for galaxies in clusters (Giovanelli et al 1996a). A more extensive discussion of the motivation and the -7details for the adopted procedure will be presented in da Costa et al (1996).…”
Section: Analysis Of the Sfi Samplementioning
confidence: 88%