# Revisit of constraints on holographic dark energy: SNLS3 dataset with the effects of time-varying β and different light-curve fitters

@article{Wang2013RevisitOC,
title={Revisit of constraints on holographic dark energy: SNLS3 dataset with the effects of time-varying $\beta$ and different light-curve fitters},
author={Shuang Wang and Jia-Jia Geng and Ying Hu and Xin Zhang},
journal={Science China Physics, Mechanics \& Astronomy},
year={2013},
volume={58},
pages={1-11}
}
• Published 1 December 2013
• Physics
• Science China Physics, Mechanics & Astronomy
Previous studies have shown that for the Supernova Legacy Survey three-year (SNLS3) data there is strong evidence for the redshift-evolution of color-luminosity parameter β of type Ia supernovae (SN Ia). In this paper, we explore the effects of varying β on the cosmological constraints of holographic dark energy (HDE) model. In addition to the SNLS3 data, we also use Planck distance prior data of cosmic microwave background (CMB), as well as galaxy clustering (GC) data extracted from Sloan…
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## References

SHOWING 1-10 OF 154 REFERENCES
SNLS3: Constraints on dark energy combining the supernova legacy survey three-year data with other probes
• Physics
• 2011
We present observational constraints on the nature of dark energy using the Supernova Legacy Survey three-year sample (SNLS3) of Guy et al. and Conley et al. We use the 472 Type Ia supernovae (SNe
The Supernova Legacy Survey: measurement of Ωm, Ω∧ and w from the first year data set. Commentary
• Physics
• 2006
We present distance measurements to 71 high redshift type Ia supernovae discovered during the first year of the 5-year Supernova Legacy Survey (SNLS). These events were detected and their multi-color
Robust Dark Energy Constraints from Supernovae, Galaxy Clustering, and 3 yr Wilkinson Microwave Anisotropy Probe Observations
• Physics
• 2006
Type Ia supernova (SN Ia), galaxy clustering, and cosmic microwave background (CMB) anisotropy data provide complementary constraints on the nature of the dark energy in the universe. We find that
Constraints on the Holographic Dark Energy Model from Type Ia Supernovae, WMAP7, Baryon Acoustic Oscillation and Redshift-Space Distortion
In this paper, we use the joint measurement of geometry and growth rate from matter density perturbations to constrain the holographic dark energy model. The geometry measurement includes type Ia
Features of holographic dark energy under combined cosmological constraints
• Physics
• 2007
We investigate the observational signatures of the holographic dark-energy models, including both the original model and a model with an interaction term between the dark energy and dark matter. We
Improved Dark Energy Constraints From ~ 100 New CfA Supernova Type Ia Light Curves
• Physics
• 2009
We combine the CfA3 supernovae Type Ia (SN Ia) sample with samples from the literature to calculate improved constraints on the dark energy equation of state parameter, w. The CfA3 sample is added to
Probing cosmic acceleration by using the SNLS3 SNIa dataset
• Physics
• 2011
We probe the cosmic acceleration by using the recently released SNLS3 sample of 472 type Ia supernovae. Combining this type Ia supernovae dataset with the cosmic microwave background anisotropy data
Constraints on holographic dark energy from the latest supernovae, galaxy clustering, and cosmic microwave background anisotropy observations
• Physics
• 2007
The holographic dark energy model is proposed by Li as an attempt for probing the nature of dark energy within the framework of quantum gravity. The main characteristic of holographic dark energy is
The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations
• Physics
• 2011
We present measurements of the baryon acoustic peak at redshifts z = 0.44, 0.6 and 0.73 in the galaxy correlation function of the final dataset of the WiggleZ Dark Energy Survey. We combine our
The Supernova Legacy Survey 3-year sample: Type Ia supernovae photometric distances and cosmological constraints ,
• Physics
• 2010
Aims. We present photometric properties and distance measurements of 252 high redshift Type Ia supernovae (0.15 < z < 1.1) discovered during the first three years of the Supernova Legacy Survey