Built on

A. Sandage, “The Change of Redshift and Apparent Luminosity of Galaxies due to the Deceleration of Selected Expanding Universes,” Astrophys. J. 136
1962
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2002
Earlier work this paper cites.
P. -S. Corasaniti, D. Huterer and A. Melchiorri, “Exploring the Dark Energy Redshift Desert with the Sandage-Loeb Test,” Phys. Rev. D 75
2007
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A. Balbi and C. Quercellini, “The time evolution of cosmological redshift as a test of dark energy,” Mon. Not. Roy. Astron. Soc. 382
Original
2007
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H. -B. Zhang, W. Zhong, Z. H. Zhu and S. He, “Exploring holographic dark energy model with Sandage-Leob test,” Phys. Rev. D 76
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2007
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J. Liske, A. Grazian, E. Vanzella, M. Dessauges, M. Viel, L. Pasquini, M. Haehnelt and S. Cristiani et al
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2008
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2010
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A. Conley et al
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2011
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Then

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G. Hinshaw et al
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Y. Wang and S. Wang, “Distance Priors from Planck and Dark Energy Constraints from Current Data,” Phys. Rev. D 88
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2013
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M. Li, X. -D. Li, Y. -Z. Ma, X. Zhang and Z. Zhang, “Planck Constraints on Holographic Dark Energy,” JCAP 1309
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2014

Parameter estimation with Sandage-Loeb test

Geng, Jia-Jia, Zhang, Jing-Fei, Zhang, Xin

Understand

The Sandage-Loeb (SL) test directly measures the expansion rate of the universe in the redshift range of $2\lesssim z\lesssim 5$ by detecting redshift drift in the spectra of Lyman-$\alpha$ forest of distant quasars.

We discuss the impact of the future SL test data on parameter estimation for the $\Lambda$CDM, the $w$CDM, and the $w_0w_a$CDM models.
To avoid the potential inconsistency with other observational data, we take the best-fitting dark energy model constrained by the current observations as the fiducial model to produce 30 mock SL test data.
The SL test data provide an important supplement to the other dark energy probes, since they are extremely helpful in breaking the existing parameter degeneracies.

Built on

A. Sandage, “The Change of Redshift and Apparent Luminosity of Galaxies due to the Deceleration of Selected Expanding Universes,” Astrophys. J. 136
1962
Earlier work this paper cites.
A. Loeb, “Direct Measurement of Cosmological Parameters from the Cosmic Deceleration of Extragalactic Objects,” Astrophys. J. 499
1998
Earlier work this paper cites.
A. Lewis and S. Bridle, “Cosmological parameters from CMB and other data: a Monte-Carlo approach,” Phys. Rev. D 66
2002
Earlier work this paper cites.
P. -S. Corasaniti, D. Huterer and A. Melchiorri, “Exploring the Dark Energy Redshift Desert with the Sandage-Loeb Test,” Phys. Rev. D 75
2007
Earlier work this paper cites.
A. Balbi and C. Quercellini, “The time evolution of cosmological redshift as a test of dark energy,” Mon. Not. Roy. Astron. Soc. 382
Original
2007
Earlier work this paper cites.
H. -B. Zhang, W. Zhong, Z. H. Zhu and S. He, “Exploring holographic dark energy model with Sandage-Leob test,” Phys. Rev. D 76
Original
2007
Earlier work this paper cites.
J. Liske, A. Grazian, E. Vanzella, M. Dessauges, M. Viel, L. Pasquini, M. Haehnelt and S. Cristiani et al
Original
2008
Earlier work this paper cites.