The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the configuration-space clustering wedges

By Ariel G. Sánchez, R. Scoccimarro, Martín Crocce, J. Grieb, Salvador Salazar-Albornoz, Claudio DallaVecchia, Martha Lippich, F. Beutler, J. Brownstein, C. Chuang and 14 more. 2016

152 citations recorded by the source corpus.

Citation: Sanchez, A. G., Scoccimarro, R., Crocce, M., Grieb, J. N., Salazar-Albornoz, S., Dalla Vecchia, C., . . . Zhao, G. B. (2017). The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the configuration-space clustering wedges. Monthly Notices of the Royal Astronomical Society, 464(2), 1640-1658. doi:10.1093/mnras/stw2443

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/232291e184e0c758219c1feef002caf2e300bdcb

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Citations in the corpus

The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space (2016, methodology): “Companion papers Alam et al. (2016), Beutler et al. (2017), Ross et al. (2017), Grieb et al. (2016) and Sanchez et al. (2017b) perform the BAO measurements using the same galaxy catalogue but in three redshift slices of 0.2 < z < 0.5, 0.4 < z < 0.6 and 0.5 < z < 0.75.”
Galileon gravity in light of ISW, CMB, BAO and H0 data (2017, methodology): “[100] for an example of such analysis from the BOSS survey).”
The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the quasar sample in configuration space between redshift 0.8 and 2.2 (2020, methodology): “Such a FoG treatment, which takes into account the nonlinear corrections, can also be found in Sánchez et al. (2017b), Grieb et al. (2017), Hou et al. (2018).”
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Constraining modified gravity (2016, methodology): “These measurements are optimally combined using the method described in Sánchez et al. (2017a), and are provided as correlated measurements of fσ8, DA/rs and Hrs at three different redshifts, z = 0.38, z = 0.51 and z = 0.61, which we use along with the 9 × 9 covariance matrix for these…”