Image Details
Caption: Figure 6.
The number of GRBs pc−2 populated in Model 2 in 0.5 kpc bins for (a) the entire history of the Milky Way, or t > 0 Gya, (b) excluding the last 5 Gyr, or t > 5 Gya, (c) within the last 5 Gyr, t < 5 Gya, and (d) within the last 1 Gyr, t < 1 Gya.
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