Image Details
Caption: Figure 2.
Cross correlations obtained for each night listed in Table 1. In each case, the mean number of correlations per timing bin has been subtracted so that the HBT peak is more visible, and the green dotted lines mark the expected locations of the peaks. Except where otherwise noted, the three-telescope arrangement discussed in the text was used.
© 2026. The Author(s). Published by the American Astronomical Society.