Constraining the CDM and Galileon models with recent cosmological data

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Table 4

Updated growth of structure data.

z	fσ₈(z)	F(z)	r	Survey	Reference

0.067	0.423 ± 0.055	–	–	6dFGRS^a	Beutler et al. (2012)
0.15	0.53 ± 0.19	–	–	SDSS MGS^b	Howlett et al. (2015)
0.32	0.384 ± 0.095	0.327 ± 0.030	0.71	BOSS LOWZ	Chuang et al. (2016)
0.44	0.413 ± 0.080	0.482 ± 0.049	0.73	WiggleZ	Blake et al. (2012)
0.57	0.441 ± 0.044	–	–	BOSS CMASS^c	Samushia et al. (2014)
0.6	0.390 ± 0.063	0.650 ± 0.053	0.74	WiggleZ	Blake et al. (2012)
0.73	0.437 ± 0.072	0.865 ± 0.073	0.85	WiggleZ	Blake et al. (2012)
0.8	0.47 ± 0.08	–	–	VIPERS^a	de la Torre et al. (2013)

Notes. Parameter r is the cross-correlation between the fσ₈(z) and F(z) measurements. Correlations between the three WiggleZ measurements also exist but are not reported here.

^(a)

The Alcock-Paczynski effect is supposed to be negligible in these analysis.

^(b)

Values of fσ₈ are corrected for the Alcock-Paczynski effect but no F(z) values are provided.

^(c)

Samushia et al. (2014) provides a F(z) measurement, but to avoid double counting with the BOSS CMASS H(z) and D_A(z) measurements in Table 3 here we used only their fσ₈(z) result marginalised over F(z).

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