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We revisit the convex integration constructions for the Monge-Ampère system and prove its flexibility in dimension and codimension , up to . To our knowledge, it is the first result in which the obtained Hölder exponent is larger than but it is not contained in the full flexibility up to result. Previous various approaches, based on Kuiper’s corrugations, always led to the Hölder regularity not exceeding , while constructions based on the Nash spirals (when applicable) led to the regularity . Combining the two approaches towards an interpolation between their corresponding exponent ranges has been so far an open problem.

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