Constraining the dark energy models using baryon acoustic oscillations: An approach independent of H0 ⋅ rd

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Table 1.

Compilation of BAO measurements from diverse releases of surveys such as SDSS, WiggleZ, and DES.

z	D_A/r_d	σ_Data	Year	Ref.
0.11	2.607	0.138	2021	de Carvalho et al. (2021)
0.24	5.594	0.305	2016	Chuang et al. (2017)
0.32	6.636	0.11	2016	Alam et al. (2017)
0.38	7.389	0.122	2019	Beutler et al. (2017)
0.44	8.19	0.77	2012	Blake et al. (2012)
0.51	7.893	0.279	2015	Carvalho et al. (2016)
0.54	9.212	0.41	2012	Seo et al. (2012)
0.6	9.37	0.65	2012	Blake et al. (2012)
0.697	10.18	0.52	2020	Sridhar et al. (2020), Gil-Marin et al. (2020)^( * )
0.73	10.42	0.73	2012	Blake et al. (2012)
0.81	10.75	0.43	2017	Abbott et al. (2019)
0.85	10.76	0.54	2020	Tamone et al. (2020)
0.874	11.41	0.74	2020	Sridhar et al. (2020)
1.00	11.521	1.032	2019	Zhu et al. (2018)
1.480	12.18	0.32	2020	Hou et al. (2020), Gil-Marin et al. (2020), Bautista et al. (2020)^( * )
2.00	12.011	0.562	2019	Zhu et al. (2018)
2.35	10.83	0.54	2019	Blomqvist et al. (2019), du Mas des Bourboux et al. (2020)^( * )
2.4	10.5	0.34	2017	du Mas des Bourboux et al. (2017)

Notes. The values marked with ^( * ) are calculated through their covariance matrices relating D_M and D_H.

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