{"arxiv_id":"1810.06672","incoming":{"papers":7,"sentences":11,"groups":[{"kind":"method_or_tool","label":"Uses its method or tool","papers":1,"sentences":2,"quotes":[{"arxiv_id":"2106.05267","title":"Cosmological parameter forecasts by a joint 2D tomographic approach to CMB and galaxy clustering","url":"/paper/2106.05267","section":"Radio continuum galaxy surveys","sentence":"Hence, we adopt a more conservative choice for the tomography and divide EMU and SKA1 in 5 broad bins in redshift as in [ref] .","intent_p":0.94,"contests_p":null}]},{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":2,"quotes":[{"arxiv_id":"2410.00375","title":"Cross Correlating the Unresolved Gamma-Ray Background with Cosmic Large-Scale Structure from DESI: Implications for Astrophysics and Dark Matter","url":"/paper/2410.00375","section":"Misaligned AGN","sentence":"For the bias of mAGN, we use the same as in Ref. 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as suppression at small scales (see e.g., [ref] and references therein) or primordial non-Gaussianities (see e.g., [ref] ).","intent_p":0.8,"contests_p":null}]}],"unlabelled_sentences":5},"outgoing":{"papers":78,"sentences":92,"groups":[{"kind":"method_or_tool","label":"Uses the method or tool of","papers":15,"sentences":15,"quotes":[{"arxiv_id":"1805.05222","title":"The Tiered Radio Extragalactic Continuum Simulation (T-RECS)","url":"/paper/1805.05222","section":"EMU","sentence":"We use the Tiered Radio Extragalactic Continuum Simulation (T-RECS) [ref] to estimate the galaxy number density distribution as a function of redshift of both star forming galaxies (SFG) and galaxies with active galactic nucleus (AGN) and the corresponding galaxy and magnification biases.","intent_p":0.92,"contests_p":null},{"arxiv_id":"astro-ph/9603021","title":"Karhunen-Loeve eigenvalue problems in cosmology: how should we tackle large data sets?","url":"/paper/astro-ph/9603021","section":"Fisher matrix formalism","sentence":"In order to forecast the constraining power of EMU for the models discussed above, we use the Fisher matrix analysis [ref] .","intent_p":0.99,"contests_p":null},{"arxiv_id":"1810.10714","title":"Preliminary results of using k-Nearest Neighbours Regression to estimate the redshift of radio selected datasets","url":"/paper/1810.10714","section":"Introduction","sentence":"Besides considering the whole sample altogether, we also take advantage of the expected broad distribution of sources in redshift and the potential of machine-learning redshift measurements (e.g. [ref] ) and clustering-based redshifts obtained by cross correlating EMU's sample with spectroscopic catalogues [ref] (whose performance in cosmological surveys was estimated in [ref] ).","intent_p":0.85,"contests_p":null},{"arxiv_id":"1606.07434","title":"Cosmological Constraints with Clustering-Based Redshifts","url":"/paper/1606.07434","section":"Introduction","sentence":"Besides considering the whole sample altogether, we also take advantage of the expected broad distribution of sources in redshift and the potential of machine-learning redshift measurements (e.g. [ref] ) and clustering-based redshifts obtained by cross correlating EMU's sample with spectroscopic catalogues [ref] (whose performance in cosmological surveys was estimated in [ref] ).","intent_p":0.85,"contests_p":null},{"arxiv_id":"1303.4722","title":"Clustering-based redshift estimation: method and application to data","url":"/paper/1303.4722","section":"Introduction","sentence":"Besides considering the whole sample altogether, we also take advantage of the expected broad distribution of sources in redshift and the potential of machine-learning redshift measurements (e.g. [ref] ) and clustering-based redshifts obtained by cross correlating EMU's sample with spectroscopic catalogues [ref] (whose performance in cosmological surveys was estimated in [ref] 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lensing CMB power spectra from Planck [ref] , combined with BAO observations from spectroscopic galaxy surveys [ref] (except for $Λ$CDM+$μ_0$+$γ_0$, for which we use the constraints from Planck+BAO+RSD, as done in [ref] ).","intent_p":1.0,"contests_p":null},{"arxiv_id":"1607.03155","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample","url":"/paper/1607.03155","section":"Results","sentence":"In order to estimate the combined constraints with current observations, we add priors from the temperature, polarization and lensing CMB power spectra from Planck [ref] , combined with BAO observations from spectroscopic galaxy surveys [ref] (except for $Λ$CDM+$μ_0$+$γ_0$, for which we use the constraints from Planck+BAO+RSD, as done in [ref] ).","intent_p":1.0,"contests_p":null},{"arxiv_id":"1807.06209","title":"Planck 2018 results. VI. Cosmological parameters","url":"/paper/1807.06209","section":"Results","sentence":"In order to estimate the combined constraints with current observations, we add priors from the temperature, polarization and lensing CMB power spectra from Planck [ref] , combined with BAO observations from spectroscopic galaxy surveys [ref] (except for $Λ$CDM+$μ_0$+$γ_0$, for which we use the constraints from Planck+BAO+RSD, as done in [ref] ).","intent_p":1.0,"contests_p":null},{"arxiv_id":"1502.01592","title":"Planck 2015 results. XVII. Constraints on primordial non-Gaussianity","url":"/paper/1502.01592","section":"Results","sentence":"For these cases, we make use of the marginalized 68% confidence level constraints on each of the extra parameters reported in [ref] and [ref] , respectively, to the $Λ$CDM parameter covariance matrix, only in the corresponding diagonal element.","intent_p":1.0,"contests_p":null}]},{"kind":"comparison","label":"Compares with","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1811.02743","title":"Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts","url":"/paper/1811.02743","section":"Conclusions","sentence":"This result is consistent with the findings reported for the SKA Phase 1 [ref] .","intent_p":0.91,"contests_p":null}]},{"kind":"supports_this_paper","label":"Cites as support","papers":2,"sentences":2,"quotes":[{"arxiv_id":"1311.6813","title":"Lensing and time-delay contributions to galaxy correlations","url":"/paper/1311.6813","section":"Cosmological observables","sentence":"However, we do observe a significant cross correlation due to lensing contributions [ref] .","intent_p":0.97,"contests_p":null},{"arxiv_id":"1511.03049","title":"Parameter splitting in dark energy: is dark energy the same in the background and in the cosmic structures?","url":"/paper/1511.03049","section":"Modified gravity","sentence":"Moreover, consistency tests of GR using current data do not favour modifications (see e.g., [ref] ).","intent_p":0.97,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":27,"sentences":27,"quotes":[{"arxiv_id":"1106.3219","title":"EMU: Evolutionary Map of the Universe","url":"/paper/1106.3219","section":"Introduction","sentence":"EMU [ref] is an all-sky radio-continuum survey using the Australian SKA Pathfinder (ASKAP) radio telescope [ref] .","intent_p":0.85,"contests_p":null},{"arxiv_id":"1210.7521","title":"Radio Continuum Surveys with Square Kilometre Array Pathfinders","url":"/paper/1210.7521","section":"Introduction","sentence":"EMU [ref] is an all-sky radio-continuum survey using the Australian SKA Pathfinder (ASKAP) radio telescope [ref] .","intent_p":0.85,"contests_p":null},{"arxiv_id":"1807.06209","title":"Planck 2018 results. VI. Cosmological parameters","url":"/paper/1807.06209","section":"Modified gravity","sentence":"We only consider scale independent modifications of GR, but there are several possible parameterizations of $μ(z,k)$ and $γ(z,k)$ [ref] .","intent_p":0.8,"contests_p":null},{"arxiv_id":"1610.09290","title":"The Observational Future of Cosmological Scalar-Tensor Theories","url":"/paper/1610.09290","section":"Introduction","sentence":"Studies of cosmological models and beyond-$Λ$CDM parameter constraints using next generation radio surveys were spearheaded in [ref] and then followed by subsequent works such as e.g., [ref] .","intent_p":0.94,"contests_p":null},{"arxiv_id":"1712.07425","title":"Probing primordial features with next-generation photometric and radio surveys","url":"/paper/1712.07425","section":"Introduction","sentence":"Studies of cosmological models and beyond-$Λ$CDM parameter constraints using next generation radio surveys were spearheaded in [ref] and then followed by subsequent works such as e.g., [ref] .","intent_p":0.94,"contests_p":null}]}],"unlabelled_sentences":37},"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. Pith's classifier typed each sentence. A label is shown at intent probability 0.8 or more (0.95 for support), a contest at 0.7 or more. Measured accuracy against two blind model families is at https://pith.science/accuracy. The quoted sentences are the citing authors' own.","held_up":null,"_links":{"html":"https://pith.science/paper/1810.06672"}}