paper

Revisiting the NVSS number count dipole

arXiv:1509.02532 · doi:10.1088/1475-7516/2016/03/062

Abstract

We present a realistic modeling of the dipole component of the projected sky distribution of NVSS radio galaxies. The modeling relies on mock catalogs generated within the context of CDM cosmology, in the linear regime of structure formation. After removing the contribution from the solar motion, the mocks show that the remaining observed signal is mostly (70\%) due to structures within . The amplitude of the model signal depends on the bias factor of the NVSS mock galaxies. For sources with flux density, , the bias recipe inferred from higher order moments is consistent with the observed dipole signal at . Flux thresholds above yield a disagreement close to the level. A constant high bias, is needed to mitigate the tension to the level.

14 pages, 5 figures, 3 tables

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