Constraints on Dark Energy from New Observations including Pan-STARRS
Wei Zheng, Si-Yu Li, Hong Li, Jun-Qing Xia, Mingzhe Li, Tan Lu

TL;DR
This study uses new observational data from Planck, Pan-STARRS, and BAO to constrain dark energy's equation of state, finding results mostly consistent with the cosmological constant but hinting at possible evolution.
Contribution
It provides updated constraints on dark energy parameters using combined datasets and explores a parametrization-independent approach via principal component analysis.
Findings
Constant EoS parameter w=-1.141±0.075 consistent with ΛCDM
Time evolving w(a) model compatible with ΛCDM within 1σ
Weak evidence of deviation from ΛCDM in some redshift bins
Abstract
In this paper, we set the new limits on the equation of state parameter (EoS) of dark energy with the observations of cosmic microwave background radiation (CMB) from Planck satellite, the type Ia supernovae from Pan-STARRS and the baryon acoustic oscillation (BAO). We consider two parametrization forms of EoS: a constant and time evolving . The results show that with a constant EoS, (), which is consistent with CDM at about confidence level. For a time evolving model, we get (), (), and in this case CDM can be comparable with our observational data at confidence level. In order to do the parametrization independent analysis, additionally we adopt the so called principal component analysis (PCA) method, in…
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