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| Format: | Preprint |
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2026
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| Online Access: | https://arxiv.org/abs/2602.07389 |
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| _version_ | 1866913100388630528 |
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| author | Takeuchi, Tsutomu T. |
| author_facet | Takeuchi, Tsutomu T. |
| contents | The dipole anisotropy in galaxy and QSO number counts induced by the motion of the observer (the kinematic dipole) provides an important test of cosmological isotropy and a comparison with the Cosmic Microwave Background (CMB) dipole. Traditionally, the Ellis \& Baldwin expression,$\mathcal{A}=2+x(1+α)$, has been widely adopted, assuming power-law number counts and a single power-law spectral energy distribution (SED). Realistic surveys, however, involve a range of non-ideal effects, including diverse SEDs, finite instrumental bandpasses, non-power-law number counts, multi-band photometry and photo-$z$ selections, and direction-dependent or stochastic detection limits. In this paper, we incorporate these effects explicitly at the theoretical level and present a unified formulation of the kinematic dipole for a general parent population and a general multi-dimensional selection function. We show that the dipole amplitude is not described by a single index, but is instead given by a functional, $\mathcal{A}[\mathcal{W},f]$, defined as the Doppler response of the selection function acting on the underlying population. We demonstrate that the classical Ellis--Baldwin result is recovered as a special limiting case of this formalism, and clarify the relation between the theoretical coefficient $\mathcal{A}$ and the dipole vector estimated from finite catalogs, separating theoretical response from statistical uncertainty. This framework provides a basis for reinterpreting reported discrepancies in kinematic dipole measurements across surveys and is directly applicable to future wide-area, multi-band observations. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2602_07389 |
| institution | arXiv |
| publishDate | 2026 |
| record_format | arxiv |
| spellingShingle | A General Formulation of the Kinematic Dipole as a Functional of Selection and Source Properties: Beyond the Ellis--Baldwin Approximation Takeuchi, Tsutomu T. Cosmology and Nongalactic Astrophysics The dipole anisotropy in galaxy and QSO number counts induced by the motion of the observer (the kinematic dipole) provides an important test of cosmological isotropy and a comparison with the Cosmic Microwave Background (CMB) dipole. Traditionally, the Ellis \& Baldwin expression,$\mathcal{A}=2+x(1+α)$, has been widely adopted, assuming power-law number counts and a single power-law spectral energy distribution (SED). Realistic surveys, however, involve a range of non-ideal effects, including diverse SEDs, finite instrumental bandpasses, non-power-law number counts, multi-band photometry and photo-$z$ selections, and direction-dependent or stochastic detection limits. In this paper, we incorporate these effects explicitly at the theoretical level and present a unified formulation of the kinematic dipole for a general parent population and a general multi-dimensional selection function. We show that the dipole amplitude is not described by a single index, but is instead given by a functional, $\mathcal{A}[\mathcal{W},f]$, defined as the Doppler response of the selection function acting on the underlying population. We demonstrate that the classical Ellis--Baldwin result is recovered as a special limiting case of this formalism, and clarify the relation between the theoretical coefficient $\mathcal{A}$ and the dipole vector estimated from finite catalogs, separating theoretical response from statistical uncertainty. This framework provides a basis for reinterpreting reported discrepancies in kinematic dipole measurements across surveys and is directly applicable to future wide-area, multi-band observations. |
| title | A General Formulation of the Kinematic Dipole as a Functional of Selection and Source Properties: Beyond the Ellis--Baldwin Approximation |
| topic | Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2602.07389 |