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([ref]) and are resummed at order $1-j$.","intent_p":0.99,"contests_p":null},{"arxiv_id":"1909.05271","title":"The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure","url":"/paper/1909.05271","section":"Biased tracers in redshift space","sentence":"To this extent, we adopt two computational strategies, a numerical one [ref] and an analytical one relying on the FFTLog decomposition of the linear power spectrum [ref] , described in appendix [ref].","intent_p":1.0,"contests_p":null},{"arxiv_id":"1609.00717","title":"Very Massive Tracers and Higher Derivative Biases","url":"/paper/1609.00717","section":"Procedure for comparing to data","sentence":"This procedure is practically the same as the one that has been implemented in [ref] for the dark matter power spectrum.","intent_p":0.93,"contests_p":null}]},{"kind":"comparison","label":"Compares with it","papers":2,"sentences":2,"quotes":[{"arxiv_id":"2112.05889","title":"Neural Network Acceleration of Large-scale Structure Theory Calculations","url":"/paper/2112.05889","section":"Comparison with Taylor Expansions","sentence":"Finally, we compare our MLP surrogate model to a Taylor series expansion, a common alternative for approximating EFT models for redshift space power spectra [ref] .","intent_p":0.87,"contests_p":null},{"arxiv_id":"1609.00349","title":"FFT-PT: Reducing the two-loop large-scale structure power spectrum to low-dimensional radial integrals","url":"/paper/1609.00349","section":"Introduction","sentence":"Although we share the same motivation and goals with Refs. 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are then used as input for the IR-resummation code [], also released with this work. implements the IR-resummation technique developed in [ref] to incorporate the leading effect of large-scale displacements on the perturbative predictions of the EFTofLSS.","intent_p":0.99,"contests_p":null},{"arxiv_id":"1406.4143","title":"The One-Loop Matter Bispectrum in the Effective Field Theory of Large Scale Structures","url":"/paper/1406.4143","section":"ResumEFT","sentence":"In a separate step, the output files from , along with $Ω_m$ and desired redshift, are then used as input for the IR-resummation code [], also released with this work. implements the IR-resummation technique developed in [ref] to incorporate the leading effect of large-scale displacements on the perturbative predictions of the EFTofLSS.","intent_p":0.99,"contests_p":null},{"arxiv_id":"1507.05326","title":"Precision Comparison of the Power Spectrum in the EFTofLSS with Simulations","url":"/paper/1507.05326","section":"The 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[ref], $χ_5^2(p)$ is the quantile function for probability $p$ of the chi-squared distribution with 5 degrees of freedom.","intent_p":0.95,"contests_p":null}]},{"kind":"comparison","label":"Compares with","papers":1,"sentences":1,"quotes":[{"arxiv_id":"1304.7849","title":"The Coyote Universe Extended: Precision Emulation of the Matter Power Spectrum","url":"/paper/1304.7849","section":"Tests","sentence":"We anticipate here that in order to obtain $P_EFT-2-loop$ within 1% of the nonlinear power spectrum obtained from the emulator code [ref] [<http://www.hep.anl.gov/cosmology/CosmicEmu/emu.html>.","intent_p":0.83,"contests_p":null}]},{"kind":"background","label":"Cites as background","papers":29,"sentences":36,"quotes":[{"arxiv_id":"1603.04826","title":"FAST-PT: a novel algorithm to calculate convolution integrals in cosmological perturbation theory","url":"/paper/1603.04826","section":": Efficient exploration of cosmology-dependence in the EFTofLSS","sentence":"Several ways to make the integration more efficient have been proposed [ref] .","intent_p":0.82,"contests_p":null},{"arxiv_id":"1208.1191","title":"RegPT: Direct and fast calculation of regularized cosmological power spectrum at two-loop order","url":"/paper/1208.1191","section":": Efficient exploration of cosmology-dependence in the EFTofLSS","sentence":"Several ways to make the integration more efficient have been proposed [ref] .","intent_p":0.82,"contests_p":null},{"arxiv_id":"1309.3308","title":"Cosmological perturbation theory at three-loop order","url":"/paper/1309.3308","section":": Efficient exploration of cosmology-dependence in the EFTofLSS","sentence":"Several ways to make the integration more efficient have been proposed [ref] .","intent_p":0.82,"contests_p":null},{"arxiv_id":"1202.3998","title":"The Shift of the Baryon Acoustic Oscillation Scale: A Simple Physical Picture","url":"/paper/1202.3998","section":": Efficient exploration of cosmology-dependence in the EFTofLSS","sentence":"Several ways to make the integration more efficient have been proposed [ref] .","intent_p":0.82,"contests_p":null},{"arxiv_id":"1512.07630","title":"Non-Gaussian Covariance of the Matter Power Spectrum in the Effective Field Theory of Large Scale Structure","url":"/paper/1512.07630","section":": Efficient exploration of cosmology-dependence in the EFTofLSS","sentence":"Several ways to make the integration more efficient have been proposed [ref] .","intent_p":0.82,"contests_p":null}]}],"unlabelled_sentences":93},"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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