Improving SDSS cosmological constraints through <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>β</mml:mi></mml:mrow></mml:math>-skeleton weighted correlation functions

Abstract

The $\ensuremath{\beta}$-skeleton approach can be conveniently utilized to construct the cosmic web based on the spatial geometry distribution of galaxies, particularly in sparse samples. This method plays a key role in establishing the three-dimensional structure of the Universe and serves as a tool for quantitatively characterizing the nature of the cosmic web. This study is the first application of $\ensuremath{\beta}$-skeleton information as weights in mark weighted correlation functions (MCFs), presenting a novel statistical measure. We have applied the $\ensuremath{\beta}$-skeleton approach to the CMASS NGC galaxy samples from SDSS BOSS DR12 in the redshift interval $0.45\ensuremath{\le}z\ensuremath{\le}0.55$. Additionally, we applied this approach to three COLA cosmological simulations with different settings (${\mathrm{\ensuremath{\Omega}}}_{m}=0.25$, ${\mathrm{\ensuremath{\Omega}}}_{m}=0.31$, ${\mathrm{\ensuremath{\Omega}}}_{m}=0.4$) for comparison. We measured three MCFs, each weighted by (i) the number of neighboring galaxies around each galaxy, (ii) the average distance of each galaxy from its surrounding neighbors, and (iii) the reciprocal of the average distance of each galaxy from its surrounding neighbors. By comparing measurements and calculating corresponding ${\ensuremath{\chi}}^{2}$ statistics, we observe high sensitivity to the cosmological parameter ${\mathrm{\ensuremath{\Omega}}}_{m}$ through a joint analysis of the two-point correlation and three MCFs.