| Abstract: | The correlation between distant Gamma-Ray Bursts (GRBs) and foreground galaxy clusters is re-examined by using the well localized (with an accuracy down to a few arcsec) Swift/XRT GRBs.The galaxy clusters are compiled from both the X-ray selected ROSAT brightest cluster sample (BCS) and the BCS extension by requiring δ≧ 0° and b ≧ 20°.The Swift/XRT GRBs fulfilling the above selection criteria are cross-correlated with the clusters.Both Nearest-Neighbor analysis and the angular two-point cross-correlation function show that there is not enough evidence supporting the correlation between the GRBs and foreground clusters.We suggest that the non-correlation is probably related to the GRB number-flux relation slope. |
