Open Access

Table A.1.

Photometry used in the SED fitting analysis

Filter units GN20 GN20.2a GN20.2b BD29079

z 4.0553 ± 0.0002 4.0508 ± 0.0013 4.0563 ± 0.0003 4.058††
ACS/F435W μJy < 0.092 < 0.086 < 0.081 < 0.061
ACS/F606W μJy 0.348 ± 0.027 0.290 ± 0.025 0.152 ± 0.023 0.306 ± 0.017
ACS/F775W μJy 0.710 ± 0.041 0.657 ± 0.039 0.308 ± 0.036 0.875 ± 0.027
ACS/F814W μJy 0.758 ± 0.050 0.573 ± 0.047 0.225 ± 0.043 1.047 ± 0.035
ACS/F850LP μJy 0.822 ± 0.038 0.628 ± 0.037 0.281 ± 0.034 1.159 ± 0.025
WFC3/F105W μJy 0.905 ± 0.062 0.608 ± 0.060 0.360 ± 0.054 1.202 ± 0.040
WFC3/F125W μJy 1.060 ± 0.083 0.531 ± 0.082 0.456 ± 0.073 1.373 ± 0.040
WFC3/F140W μJy 1.21 ± 0.11 - 0.455 ± 0.094 1.333 ± 0.067
WFC3/F160W μJy 1.148 ± 0.083 0.760 ± 0.076 0.603 ± 0.068 1.470 ± 0.039
MIRIM/F560W μJy 10.76 ± 0.23 3.32 ± 0.23 8.17 ± 0.25 2.47 ± 0.15
MIRIM/F770W μJy 17.85 ± 0.30 6.07 ± 0.28 12.54 ± 0.32 2.86 ± 0.18
MIRIM/F1280W μJy 23.48 ± 0.73 9.01 ± 0.72 10.97 ± 0.79 6.97 ± 0.47
MIRIM/F1800W μJy 35.8 ± 3.6 13.9 ± 3.4 14.3 ± 3.7 16.2 ± 2.4
IRAC/3.6μm μJy 5.949 ± 0.090 2.48 ± 0.10 4.50 ± 0.12 4.29 ± 0.04
IRAC/4.5μm μJy 8.249 ± 0.077 2.637 ± 0.085 6.42 ± 0.09 3.08 ± 0.07
IRAC/5.7μm μJy 14.29 ± 0.69 4.09 ± 0.76 9.03 ± 0.84 3.35 ± 0.50
IRAC/7.8μm μJy 22.57 ± 0.55 6.80 ± 0.60 13.37 ± 0.70 4.69 ± 0.52
MIPS/24μm μJy 65.5 ± 3.5 30.2 ± 5.6 12.0 ± 4.3 47.3 ± 5.4
PACS/100μm mJy 0.70 ± 0.42 0.12 ± 0.44 0.61 ± 0.46 0.54 ± 0.33
PACS/160μm mJy 5.5 ± 1.0 1.2 ± 1.4 2.3 ± 1.4 1.72 ± 0.65
SPIRE/250μm mJy 18.6 ± 2.7 - - < 5.4
SPIRE/350μm mJy 41.3 ± 5.2 - - -
SPIRE/500μm mJy 39.7 ± 6.1 - - < 6.6
SCUBA/850μm mJy 20.3 ± 2.1 9.9 ± 2.3 9.9 ± 2.0 -
PdBI/1.2mm mJy 8.47 ± 0.79 3.83 ± 0.48 3.25 ± 0.52 -
PdBI/2.2mm mJy 0.95 ± 0.14 0.52 ± 0.23 < 0.80 -
PdBI/3.3mm mJy 0.229 ± 0.036 0.177 ± 0.071 0.114 ± 0.035 -

Notes. HST and MIRI fluxes measured through aperture photometry (see Sect. 3.2). Photometric values beyond 2 μm correspond to the GOODS-N catalogue presented in Liu et al. (2018). Upper limits are set as 3σ values in those filters where the uncertainty is larger than the flux measurement. Hyphens represent the non-coverage of the object by the corresponding filter. Redshift assumed during the SED fitting, computed in Tan et al. (2014). †† Redshift derived in Daddi et al. (2009).

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