Escala acústica bariônica em z_eff = 0,166 com galáxias azuis do SDSS
DOI:
https://doi.org/10.47456/Cad.Astro.v7nEspecial.53378Palabras clave:
cosmologia: estrutura em grande escala do Universo, cosmologia: observações, cosmologia: parâmetros cosmológicosResumen
Trabalho apresentado no evento As Astrocientistas: III Encontro Brasiliero de Meninas e Mulheres da Astrofísica, Cosmologia e Gravitação, realizado entre os dias 31 de março e 4 de abril de 2025.
Referencias
[1] P. J. E. Peebles e J. T. Yu, Primeval Adiabatic Perturbation in an Expanding Universe, 162, 815 (1970).
[2] R. A. Sunyaev e Y. B. Zeldovich, SmallScale Fluctuations of Relic Radiation, 7 (1), 3 (1970).
[3] D. J. Eisenstein e et al., Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies, 633 (2), 560 (2005).
[4] S. Cole e et al., The 2dF Galaxy Redshift Survey: power-spectrum analysis of the final data set and cosmological implications, 362 (2), 505 (2005).
[5] S. Alam e et al., Completed SDSS-IV extended Baryon Oscillation Spectroscopic Surcades of spectroscopic surveys at the Apache Point Observatory, 103 (8), 083533 (2021).
[6] F. Beutler e et al., The 6dF Galaxy Survey: baryon acoustic oscillations and the local Hubble constant, 416 (4), 3017 (2011).
[7] C. Blake e et al., The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations, 418 (3), 1707 (2011).
[8] M. Crocce e R. Scoccimarro, Nonlinear evolution of baryon acoustic oscillations, Physical Review D 77 (2) (2008).
[9] E. de Carvalho, A. Bernui, F. Avila, C. P. Novaes e J. P. Nogueira-Cavalcante, BAO angular scale at z eff = 0.11 with the SDSS blue galaxies, 649, A20 (2021).
[10] S. D. Landy e A. S. Szalay, Bias and Variance of Angular Correlation Functions, 412, 64 (1993).
[11] M. Jarvis, G. Bernstein e B. Jain, The skewness of the aperture mass statistic, 352 (1), 338 (2004).
[12] M. Visser, Cosmography: Cosmology without the Einstein equations, General Relativity and Gravitation 37 (9), 1541 (2005).
[13] E.-K. Li, M. Du e L. Xu, General cosmography model with spatial curvature, 491 (4), 4960 (2020).
[14] J. Liu, L. Qiao, B. Chang e L. Xu, Revisiting cosmography via Gaussian process, European Physical Journal C 83 (5), 374 (2023).
[15] E. e. a. Sánchez, Tracing the sound horizon scale with photometric redshift surveys, 411 (1), 277 (2011).
[16] P. Carter e et al., Low redshift baryon acoustic oscillation measurement from the reconstructed 6-degree field galaxy survey, 481 (2), 2371 (2018).
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Derechos de autor 2026 Hanna Lima, Rafael da Costa Nunes, Felipe Avila, Edilson Carvalho, Armando Bernui

Esta obra está bajo una licencia internacional Creative Commons Atribución 4.0.



