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Table 10.

Main features for the four studied GRB afterglows.

GRB X-ray GROND Sub-mm Radio Notes
100418A Steep decay 8 epochs SMA: 3 det. VLA: 7 det. Non-spreading JB
Plateau phase Plateau phase PdBI: 7 det. ATCA: 6 det. Fast/slow cooling
EI, JB No SED evol. Evol. of α ISS Wind
No SED evol. EI, JB

110715A 2 breaks 6 epochs APEX: 1 det. ATCA: 22 det, 1 UL EI
Plateau phase ALMA: 1 det. ISS Non-spreading JB
EI Wind
Early IC

121024A Plateau phase. 6 epochs. APEX: 2 UL EVLA: 1 det 1 <  p <  2
EI Plateau phase. CARMA: 1 det EI before tb, p>2
Achromatic break. EI Jet break, 1 <  p <  2
No SED evol. Achromatic break EI after tb, p >  2
JB No SED evol. Polarisation det.
Jet break Wind

130418A < 104 ks 7 epoch SMA: 1 UL. CARMA: 1 det. No SED evol.
Jet break 2 breaks, jet APEX: 2 det, 1 UL. WSRT: 1 UL Early IC
α too steep for EI EI EI
β too flat vs β opt. Achromatic break Jet break
JB Wind

Notes. The number of epochs corresponds to the number of time slices used in the SED analysis. EI: Energy injection. ISS: Interstellar scintillation. JB: Jet break. UL: Upper limit. Det: detection.

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