Abstract
The paper 'Investigating darkmatter substructure with pulsar timing - II. Improved limits on small-scale cosmology' was published in MNRAS, 456, 1402 (Paper II, Clark, Lewis & Scott 2016b). Due to an error in the interpretation of the timing noise in Paper I (Clark, Lewis & Scott 2016a), the limits on UCMH abundance used in Paper II were incorrect.
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