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Large Scale Shearing of the Universe from Ariel V X-Ray Data

Large scale X-ray background anisotropy measurements may be combined with our peculiar velocity deduced from the microwave background to search for matter perturbations within z ∼ 5, Ariel V data show a significant 12 h variation with a pole coincident, within the errors, with the microwave velocity direction. If this variation is wholly extragalactic, then it may indicate, or place limits upon, large (≳ 1019M⊙) low contrast (δρ/ρ) matter perturbations at z ∼ 1.