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Dependence of the GRB Lag Luminosity Relation on Redshift in the Source Frame

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Figure

Table 2. The best-fit values for the normalization, A, and the slope, B, along with their 1  errors, obtained when a weighted least-squares fit was used
Figure 1. the normalized time-lag in the burst’s source frame. The best- fit lines for a weighted least-squares fit are shown for the three redshift bins used, where bin 1 represents the lowest redshift range

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