Alignment of faint galaxy images - Cosmological distortion and rotation

Mathematics – Logic

Scientific paper

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Astronomical Photography, Cosmology, Galactic Structure, Anisotropy, Distortion, Ellipticity, Mass Distribution, Red Shift, Relic Radiation, Spherical Harmonics

Scientific paper

The images of 44,462 randomly chosen galaxies between 22.5 and 23.5 J apparent magnitude have been examined in 35 fields for a coherent ellipticity due to cosmological image distortion arising from inhomogeneity and anisotropy in the large-scale mass distribution of the universe. It is found that strong limits can be put on the degree of large angular scale anisotropy in cosmological models. The result for a large-scale ellipticity is null with a three-sigma upper limit of ellipticity less than 0.04 out to a redshift of 0.6, implying that the cosmological distortion is small out to redshifts of about one. Variations in the field-to-field ellipticity over the sky have a dispersion of less than 0.03. This sets a three-sigma upper limit of 0.1 for the mass overdensity contrast in clusters of 1000 Mpc size and a three-sigma upper limit to the Weyl tensor components of about 1.5 x 10 to the -20th/sq yr.

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