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• W4308976239 abstract "We perform the first application of the wavelet scattering transform (WST) to actual galaxy observations, through a WST analysis of the BOSS DR12 CMASS dataset. We included the effects of redshift-space anisotropy, nontrivial survey geometry, systematic weights, and the Alcock-Paczynski distortion effect, following the commonly adopted steps for the power spectrum analysis. In order to capture the cosmological dependence of the WST, we use galaxy mocks obtained from the state-of-the-art ABACUSSUMMIT simulations, tuned to match the anisotropic correlation function of the BOSS CMASS sample in the redshift range $0.46<z<0.60$. Using our model for the WST coefficients, as well as for the first 2 multipoles of the galaxy power spectrum, that we use as reference, we perform a likelihood analysis of the CMASS data. We obtain the posterior probability distributions of four cosmological parameters, ${{ensuremath{omega}}_{b},{ensuremath{omega}}_{c},{n}_{s},{ensuremath{sigma}}_{8}}$, as well as the Hubble constant, derived from a fixed value of the angular size of the sound horizon at last scattering measured by the Planck satellite, all of which are marginalized over the seven nuisance parameters of the halo occupation distribution model. The WST is found to deliver a substantial improvement in the values of the predicted $1ensuremath{sigma}$ errors compared to the regular power spectrum, which are tighter by a factor of 3--5 in the case of flat and uninformative priors and by a factor of 3--8, when a big bang nucleosynthesis prior is applied on the value of ${ensuremath{omega}}_{b}$. Our results are investigative and subject to certain approximations, which we discuss in the text." @default.
• W4308976239 created "2022-11-20" @default.
• W4308976239 creator A5070286426 @default.
• W4308976239 creator A5086773080 @default.
• W4308976239 date "2022-11-14" @default.
• W4308976239 modified "2023-10-15" @default.
• W4308976239 title "Going beyond the galaxy power spectrum: An analysis of BOSS data with wavelet scattering transforms" @default.
• W4308976239 cites W1520258040 @default.
• W4308976239 cites W1943306457 @default.
• W4308976239 cites W1946283183 @default.
• W4308976239 cites W1965779302 @default.
• W4308976239 cites W1974931032 @default.
• W4308976239 cites W1984613353 @default.
• W4308976239 cites W1988002195 @default.
• W4308976239 cites W1988535164 @default.
• W4308976239 cites W1994906459 @default.
• W4308976239 cites W2030392256 @default.
• W4308976239 cites W2048074979 @default.
• W4308976239 cites W2072072671 @default.
• W4308976239 cites W2080806384 @default.
• W4308976239 cites W2088125843 @default.
• W4308976239 cites W2090094520 @default.
• W4308976239 cites W2093231248 @default.
• W4308976239 cites W2102336972 @default.
• W4308976239 cites W2102600871 @default.
• W4308976239 cites W2115328997 @default.
• W4308976239 cites W2128130302 @default.
• W4308976239 cites W2128424195 @default.
• W4308976239 cites W2130563989 @default.
• W4308976239 cites W2131279590 @default.
• W4308976239 cites W2141709306 @default.
• W4308976239 cites W2147549428 @default.
• W4308976239 cites W2150453594 @default.
• W4308976239 cites W2163031978 @default.
• W4308976239 cites W2192436647 @default.
• W4308976239 cites W2204578610 @default.
• W4308976239 cites W2205003259 @default.
• W4308976239 cites W2258945625 @default.
• W4308976239 cites W2275841288 @default.
• W4308976239 cites W2299345254 @default.
• W4308976239 cites W2416612325 @default.
• W4308976239 cites W2461007441 @default.
• W4308976239 cites W2557413462 @default.
• W4308976239 cites W2607127149 @default.
• W4308976239 cites W2611924239 @default.
• W4308976239 cites W2746743250 @default.
• W4308976239 cites W2766792342 @default.
• W4308976239 cites W2771079062 @default.
• W4308976239 cites W2787427854 @default.
• W4308976239 cites W2798718650 @default.
• W4308976239 cites W2807308604 @default.
• W4308976239 cites W2809838409 @default.
• W4308976239 cites W2888191076 @default.
• W4308976239 cites W2895688790 @default.
• W4308976239 cites W2901415485 @default.
• W4308976239 cites W2952835984 @default.
• W4308976239 cites W2972735740 @default.
• W4308976239 cites W3015636173 @default.
• W4308976239 cites W3023513537 @default.
• W4308976239 cites W3025689141 @default.
• W4308976239 cites W3035003787 @default.
• W4308976239 cites W3035201698 @default.
• W4308976239 cites W3043938721 @default.
• W4308976239 cites W3080529233 @default.
• W4308976239 cites W3084279638 @default.
• W4308976239 cites W3092142288 @default.
• W4308976239 cites W3098850972 @default.
• W4308976239 cites W3099275094 @default.
• W4308976239 cites W3099459948 @default.
• W4308976239 cites W3099859885 @default.
• W4308976239 cites W3100347567 @default.
• W4308976239 cites W3100386365 @default.
• W4308976239 cites W3101791280 @default.
• W4308976239 cites W3102014803 @default.
• W4308976239 cites W3102758612 @default.
• W4308976239 cites W3102830401 @default.
• W4308976239 cites W3103406638 @default.
• W4308976239 cites W3103711895 @default.
• W4308976239 cites W3103880752 @default.
• W4308976239 cites W3104379077 @default.
• W4308976239 cites W3104388551 @default.
• W4308976239 cites W3105204625 @default.
• W4308976239 cites W3105554724 @default.
• W4308976239 cites W3106530008 @default.
• W4308976239 cites W3111440124 @default.
• W4308976239 cites W3119251236 @default.
• W4308976239 cites W3119653973 @default.
• W4308976239 cites W3121883876 @default.
• W4308976239 cites W3125978220 @default.
• W4308976239 cites W3126379213 @default.
• W4308976239 cites W3137571780 @default.
• W4308976239 cites W3151998837 @default.
• W4308976239 cites W3179131474 @default.
• W4308976239 cites W3196144079 @default.
• W4308976239 cites W3197794916 @default.
• W4308976239 cites W3198261414 @default.
• W4308976239 cites W3200917128 @default.
• W4308976239 cites W3205632825 @default.
• W4308976239 cites W3206694873 @default.
• W4308976239 cites W3208259367 @default.

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