| KEY |
| AG = GRB afterglow |
| NO OBS. = no observations are to be done |
| low reddening = E(B-V) < 0.7 high reddening = E(B-V) > 0.7 |
| The time criteria ( < 10 hrs or 10-24 hrs) = approximately how long after the GRB occurred are observations going to take place? |
| bright = mag.<19 intermediate = 19< mag. <21 dim = mag.>21 |
| S1 = GRB_triggered.pro (info), observe 2x S2 = GRB_triggered.pro (info), observe 1x S3 = GRBred_IJ3.pro (info), observe 2x S4 = GRBred_IJ3.pro (info), observe 1x S5 = GRB_triggered.pro (info), observe 2-3x S6 = GRBred_IJ6.pro (info), observe 2x S7 = GRB_triggered.pro (info), observe 2-3x S8 = GRBred_IJ6.pro (info), observe 2x *multiple observations should be spread in time to allow for significant afterglow decay |
| If no afterglow has been reported by other observers through the GCN but initial SMARTS observations reveal an AG candidate, then switch from the "no optical/IR reported or observed" track to the "optical/IR reported or observed" [but first allow any active telescope scripts to finish running]. Remember to periodically refresh the GCN page! |