Open Access
Table B.2.
Selection of one observation per telescope.
Telescope | Source | δt(h) | Limiting magnitude | Filter |
---|---|---|---|---|
BJP/ALi-50 | GRB220403B | 0.14 | 20.1 | Clear |
SNOVA | GRB220430A | 17.74 | 19.3 | Clear |
NOWT | GRB220325A | 4.72 | 20.9 | R |
KAO | GRB220325A | 8.11 | 21.5 | R |
C2PU-Omicron | GRB220325A | 10.16 | 21.6 | r′ |
UBAI/AZT-22 | GRB220412A | 33.9 | 21.7 | R |
TRT-SRO | GRB220408A | 1.82 | 19.3 | R |
Xinglong-TNT | GRB220408A | 4.95 | 20.6 | R |
MOSS | GRB220430A | 6.59 | 20.3 | Clear |
GMG-2.4 | GRB220412A | 6.06 | 20.5 | r′ |
VIRT | GRB220412A | 17.59 | 20.3 | R |
Les Makes/T60 | GRB220427A | 1.13 | 20.4 | Clear |
TAROT/TRE | GRB220427A | 0.06 | 16.4 | Clear |
Abatsumani/T70 | GRB220430A | 3.22 | 18.7 | R |
OWL | GRB220514A | 1.82 | 18.4 | Clear |
FRAM-CTA-N | GRB220514A | 2.28 | 18.3 | Clear |
2.2mCAHA | GRB220514A | 9.61 | 22.0 | i′ |
Note: The images were provided during the campaign and allowed us to provide an upper limit. Here, we present 17 telescopes that provide good-quality images, resulting in upper limits.
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