Review Article
A New Era of Submillimeter GRB Afterglow Follow-Ups with the Greenland Telescope
Figure 8
Expected RS (dashed-dot) and FS (dashed) light curves in the 230 GHz band at , 0.5, and 0.7 with erg, cm−3, , , and . Solid lines indicate the total of RS and FS. GLT has also enough sensitivity to characterize the FS components for nearby () GRBs. The expected GLT 3- limits with 1 h and 3 h exposure are indicated with dotted lines.