Cosmology using long gamma-ray bursts: statistical analysis of errors in calibrated data
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摘要:
We investigate direction dependence and non-Gaussian features in high-z cosmological data using △x2 and △x statistics and the Kolmogorov-Smirnov test.These techniques are applied on a set of calibrated long gamma-ray bursts (GRBs) and its combination with recent Type Ia supernovae data (Union2).Our statistical analysis shows a weak but consistent direction dependence in both the data sets.The analysis also indicates a non-Gaussian nature of errors in both data sets.