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Table B.1

Observing log.

t − t0 Exp. Instrument/ Band AB mag. Flux density
(days) (s) Telescope (Jy)

1.02 10 × 60 HAWKI/VLT K S 20.48 ± 0.12 (2.33 ± 0.26) × 10-5
2.05 10 × 60 HAWKI/VLT K S 20.64 ± 0.13 (2.01 ± 0.24) × 10-5
4.84 15 × 15 OSIRIS/GTC r >23.3 <1.7 × 10-6
19.0 10 × 60 HAWKI/VLT K S 21.14 ± 0.29 (1.27 ± 0.33) × 10-5

277 5 × 700 LT u >23.0 <2.3 × 10-6
194 11 × 200 OSIRIS/GTC g 24.80 ± 0.15 (4.36 ± 0.60) × 10-7
194 16 × 80 OSIRIS/GTC r 24.17 ± 0.14 (7.80 ± 1.01) × 10-7
194 6 × 100 OSIRIS/GTC i 24.15 ± 0.16 (7.94 ± 1.17) × 10-7
194 18 × 90 OSIRIS/GTC z 23.89 ± 0.17 (1.01 ± 1.58) × 10-6
252 93 × 60 OMEGA2000/3.5mCAHA Y >23.4 <1.6 × 10-6
203 20 × 60 HAWKI/VLT J 22.78 ± 0.15 (2.81 ± 0.39) × 10-6
203 17 × 60 HAWKI/VLT H 22.24 ± 0.24 (4.61 ± 1.02) × 10-6
203 17 × 60 HAWKI/VLT K S 21.39 ± 0.22 (1.01 ± 0.20) × 10-5

1.34 9000 SMA 358 GHz <3.3 × 10-2
4.34 8172 SMA 230 GHz <2.1 × 10-3

Notes. Optical and NIR magnitudes and fluxes have not been corrected for Galactic extinction (E(B − V) = 0.049; Schlafly & Finkbeiner 2011). Optical data have been calibrated using SDSS as reference and for NIR we have used UKIDSS.

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