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Table A.3

Total- and MM1-burst fluxes: similar to Table A.2 but for the burst epoch.

Wavelength Total flux Ref. MM1 flux
[μm] [erg cm−2 s−1] [erg cm−2 s−1]
  2.15 (*) 9.20 ± 0.92 × 10−13 1
 3.4  (*) 8.82 ± 0.89 × 10−11 1
 4.6  (*) 2.93 ± 0.30 × 10−10 1
52.0 5.51 ± 0.56 × 10−9 1 4.85 ± 0.49 × 10−9
54.8 6.94 ± 0.70 × 10−9 1 6.12 ± 0.62 × 10−9
60.7 6.20 ± 0.62 × 10−9 1 5.04 ± 0.51 × 10−9
87.2 7.48 ± 0.75 × 10−9 1 5.35 ± 0.54 × 10−9
118.6  6.45 ± 0.65 × 10−9 1 4.59 ± 0.46 × 10−9
124.2  8.97 ± 0.90 × 10−9 1 7.22 ± 0.72 × 10−9
142.2  5.26 ± 0.53 × 10−9 1 5.25 ± 0.53 × 10−9
153.3  5.29 ± 0.53 × 10−9 1 4.08 ± 0.41 × 10−9
162.8  5.47 ± 0.55 × 10−9 1 4.41 ± 0.45 × 10−9
186.4  4.58 ± 0.46 × 10−9 1 3.82 ± 0.39 × 10−9
889   3.81 ± 0.11 × 10−12 2 1.72 ± 0.07 × 10−12
1282   4.21 ± 0.03 × 10−13 2
1420   2.74 ± 0.28 × 10−13 2
1532   1.88 ± 0.01 × 10−13 2

Notes. We assume that during the burst only the luminosity of MM1 increased while all other sources remained constant. We note that we do not provide MM1 fluxes for λ > 890 μm, since the data points at these wavelengths are discarded for the burst SED fit as discussed in Sect. 9.1. Facilities and instruments are given behind corresponding references. (*) Upper limit.

References. (1) Present paper (2.2-m MPG/ESO telescope/GROND, NEOWISE, SOFIA/FIFI-LS); (2) Brogan et al. (2019) (ALMA, SMA).

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