4.6 Article

Integrated trispectrum detection from BOSS DR12 NGC CMASS

出版社

IOP Publishing Ltd
DOI: 10.1088/1475-7516/2022/09/050

关键词

galaxy clustering; galaxy surveys; power spectrum; redshift surveys

资金

  1. European Union [725327]
  2. European Union's Horizon 2020 research and innovation programme ERC [725327]
  3. FEDER [PGC2018-098866-B-I00, MCIN/AEI/10.13039/501100011033]
  4. Center of Excellence Maria de Maeztu 2020-2023 award to the ICCUB [MCIN/AEI/10.13039/501100011033, CEX2019-000918-M]
  5. European Research Council (ERC) [725327] Funding Source: European Research Council (ERC)

向作者/读者索取更多资源

This study presents the first detection and quantification of the monopole and quadrupole signals of the integrated trispectrum in BOSS CMASS NGC DR12, using the Fourier transform of the four-point correlation function. The analysis confirms the presence of the physical signal in the BOSS data.
We present the first detection of the integrated trispectrum (i-trispectrum) monopole and quadrupoles signal from BOSS CMASS NGC DR12. Extending the FKP estimators formalism to the Fourier transform of the four-point correlation function, we test shot-noise subtraction, Gaussianity of the i-trispectrum data-vector, significance of the de-tection and similarity between the signal from the data and from the galaxy mock catalogues used to numerically estimate the covariance matrix. Using scales corresponding to modes from minimum kmin = 0.03 h/Mpc to maximum kmax = 0.15 h/Mpc, we find a detection in terms of distance from the null hypothesis of (10.4, 5.2, 8.3, 1.1, 3.1) a-intervals for the i-trispectrum monopole T(0) and quadrupoles (T(2000), T(0200), T(0020), T(0002)) respectively. This quantifies the presence of the physical signal of the four-points statistics on BOSS data. For completeness the same analysis is also performed for power spectrum and bispectrum, both monopoles and quadrupoles.

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