Testing the spatial geometry of the Universe with TianQin: Prospect of using supermassive black hole binaries

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Table 1.

H(z) data measurement from the differential age method (I) and the radial BAO method (II).

z	H(z)( km s⁻¹ Mpc⁻¹)	Method	References
0.09	69 ± 12	I	Jimenez et al. (2003)

0.17	83 ± 8	I
0.27	77 ± 14	I
0.4	95 ± 17	I
0.9	117 ± 23	I	Simon et al. (2005)
1.3	168 ± 17	I
1.43	177 ± 18	I
1.53	140 ± 14	I
1.75	202 ± 40	I

0.48	97 ± 62	I	Stern et al. (2010)
0.88	90 ± 40	I

0.35	82.1 ± 4.9	I	Chuang & Wang (2012)

0.179	75 ± 4	I
0.199	75 ± 5	I
0.352	83 ± 14	I
0.593	104 ± 13	I
0.68	92 ± 8	I	Moresco et al. (2012)
0.781	105 ± 12	I
0.875	125 ± 17	I
1.037	154 ± 20	I

0.07	69 ± 19.6	I
0.12	68.6 ± 26.2	I
0.2	72.9 ± 29.6	I	Zhang et al. (2014)
0.28	88.8 ± 36.6	I

1.363	160 ± 33.6	I	Moresco (2015)
1.965	186.5 ± 50.4	I

0.3802	83 ± 13.5	I
0.4004	77 ± 10.2	I
0.4247	87.1 ± 11.2	I	Moresco et al. (2016)
0.4497	92.8 ± 12.9	I
0.4783	80.9 ± 9	I

0.24	79.69 ± 2.65	II	Gaztanaga et al. (2009)
0.43	86.45 ± 3.68	II

0.44	82.6 ± 7.8	II
0.6	87.9 ± 6.1	II	Blake et al. (2012)

0.73	97.3 ± 7	II

0.35	84.4 ± 7	II	Xu et al. (2013)

0.57	92.4 ± 4.5	II	Samushia et al. (2013)

2.3	224 ± 8	II	Busca et al. (2013)

2.36	226 ± 8	II	Font-Ribera et al. (2014)

2.34	222 ± 7	II	Delubac et al. (2015)

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