{"arxiv_id":"2603.23247","incoming":{"papers":1,"sentences":1,"groups":[],"unlabelled_sentences":1},"outgoing":{"papers":50,"sentences":77,"groups":[{"kind":"extends","label":"Builds on","papers":2,"sentences":2,"quotes":[{"arxiv_id":"2503.03288","title":"A semi-cosmographic approach to study cosmological evolution in phase space","url":"/paper/2503.03288","section":"Introduction","sentence":"Building on this, we develop a semi-cosmographic framework [ref] that incorporates the two-body decaying dark matter (DDM) scenario.","intent_p":0.84,"contests_p":null},{"arxiv_id":"2506.14275","title":null,"url":"/paper/2506.14275","section":"Introduction","sentence":"Building on this, we develop a semi-cosmographic framework [ref] that incorporates the two-body decaying dark matter (DDM) scenario.","intent_p":0.84,"contests_p":null}]},{"kind":"method_or_tool","label":"Uses the method or tool of","papers":3,"sentences":3,"quotes":[{"arxiv_id":"0809.0363","title":"Estimation of Cosmological 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redshift $z$ is modelled as [ref] [equation] We have adopted the Alcock–Paczyński (AP) [ref] rescaling between the fiducial and trial cosmologies by defining [equation] where $H^f$ and $D_A^f$ are the Hubble parameter and Angular diameter distance in a fiducial cosmology, and the AP-remapped variables $(k̃,μ̃)$ are given by [equation] The redshift-space distortion parameter $β_T$ is given by [equation] Here $D_+(z)$ denotes the linear growing mode of density perturbations and $b_T(z)$ is the effective HI bias.","intent_p":0.98,"contests_p":null},{"arxiv_id":"astro-ph/0512263","title":"Cosmological Parameter Estimation Using 21 cm Radiation from the Epoch of Reionization","url":"/paper/astro-ph/0512263","section":"The 21-cm Intensity Mapping","sentence":"We model instrumental uncertainties with the standard thermal-noise power spectrum for an interferometric array [ref] .","intent_p":0.99,"contests_p":null}]},{"kind":"data_used","label":"Uses data or values 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