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[ref] and later reformulated either through the tripolar spherical harmonics [ref] or the angular power spectrum [ref] [They expand the 2CF in terms of angular power spectrum and then analytically sum over angular multipoles such that only numerical integration over $k$ is required.].","intent_p":0.82,"contests_p":null},{"arxiv_id":"2407.00168","title":"Multipoles of the galaxy bispectrum on a light cone: wide-separation and relativistic corrections","url":"/paper/2407.00168","section":"Introduction","sentence":"Although the angular part of these corrections, induced as we leave the local plane-parallel limit, has been extensively studied for the case of the two-point statistics [ref] , giving rise to the so-called wide-angle corrections, their impact on the galaxy bispectrum [ref] and corrections that appear by breaking statistical homogeneity radially [ref] are much less common.","intent_p":0.94,"contests_p":null}]}],"unlabelled_sentences":25},"outgoing":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"claims":[],"thresholds":{"intent_p":0.8,"supports_p":0.95,"contests_p":0.7},"method":"Citing sentences come from each paper's LaTeX source; every \\cite marks the sentence and the works it cites. 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