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Table C.2.

Upper limits on the [CII] fluxes and luminosities of target sources assuming that [CII] line is in the frequency range probed by the ALPINE observations.

Name 3-σ upper limit on I[CII]
 3-σ upper limit on L[CII]
aggr. norm. sec. aggr. norm. sec.
(Jy km s−1) (log10(L/L⊙))
CANDELS_GOODSS_19 < 0.142 < 0.157 < 0.213 < 7.94 < 7.98 < 8.11
CANDELS_GOODSS_37 < 0.138 < 0.151 < 0.211 < 7.93 < 7.97 < 8.11
CANDELS_GOODSS_57 < 0.106 < 0.116 < 0.143 < 7.95 < 7.99 < 8.08
CANDELS_GOODSS_8 < 0.099 < 0.108 < 0.133 < 7.92 < 7.95 < 8.04
DEIMOS_COSMOS_206253 < 0.172 < 0.189 < 0.272 < 8.02 < 8.06 < 8.22
DEIMOS_COSMOS_224751 < 0.085 < 0.094 < 0.119 < 7.87 < 7.91 < 8.02
DEIMOS_COSMOS_298678 < 0.131 < 0.141 < 0.175 < 8.05 < 8.09 < 8.18
DEIMOS_COSMOS_328419 < 0.168 < 0.180 < 0.229 < 8.17 < 8.20 < 8.30
DEIMOS_COSMOS_336830 < 0.100 < 0.108 < 0.148 < 7.94 < 7.98 < 8.11
DEIMOS_COSMOS_406956 < 0.134 < 0.146 < 0.177 < 8.06 < 8.10 < 8.19
DEIMOS_COSMOS_412589 < 0.173 < 0.186 < 0.269 < 8.01 < 8.05 < 8.21
DEIMOS_COSMOS_420065 < 0.092 < 0.101 < 0.143 < 7.91 < 7.95 < 8.10
DEIMOS_COSMOS_421062 < 0.097 < 0.104 < 0.134 < 7.91 < 7.94 < 8.05
DEIMOS_COSMOS_431067 < 0.192 < 0.210 < 0.298 < 8.06 < 8.10 < 8.25
DEIMOS_COSMOS_442844 < 0.166 < 0.179 < 0.253 < 8.00 < 8.04 < 8.19
DEIMOS_COSMOS_460378 < 0.139 < 0.148 < 0.188 < 8.05 < 8.08 < 8.18
DEIMOS_COSMOS_470116 < 0.087 < 0.098 < 0.136 < 7.88 < 7.93 < 8.07
DEIMOS_COSMOS_471063 < 0.148 < 0.161 < 0.206 < 8.11 < 8.15 < 8.26
DEIMOS_COSMOS_472215 < 0.144 < 0.154 < 0.190 < 8.09 < 8.12 < 8.21
DEIMOS_COSMOS_503575 < 0.087 < 0.098 < 0.127 < 7.87 < 7.92 < 8.04
DEIMOS_COSMOS_549131 < 0.140 < 0.153 < 0.201 < 8.07 < 8.11 < 8.23
DEIMOS_COSMOS_550156 < 0.171 < 0.191 < 0.271 < 8.01 < 8.05 < 8.21
DEIMOS_COSMOS_567070 < 0.215 < 0.235 < 0.322 < 8.13 < 8.17 < 8.30
DEIMOS_COSMOS_576372 < 0.117 < 0.126 < 0.151 < 8.01 < 8.04 < 8.12
DEIMOS_COSMOS_586681 < 0.204 < 0.220 < 0.271 < 8.27 < 8.30 < 8.39
DEIMOS_COSMOS_592644 < 0.177 < 0.194 < 0.284 < 8.04 < 8.08 < 8.24
DEIMOS_COSMOS_628137 < 0.100 < 0.106 < 0.142 < 7.94 < 7.97 < 8.09
DEIMOS_COSMOS_629750 < 0.134 < 0.148 < 0.186 < 8.00 < 8.04 < 8.14
DEIMOS_COSMOS_743730 < 0.147 < 0.158 < 0.219 < 7.95 < 7.99 < 8.13
DEIMOS_COSMOS_761315 < 0.139 < 0.152 < 0.215 < 7.94 < 7.98 < 8.13
DEIMOS_COSMOS_787780 < 0.192 < 0.210 < 0.282 < 8.07 < 8.11 < 8.24
DEIMOS_COSMOS_790930 < 0.088 < 0.096 < 0.136 < 7.88 < 7.92 < 8.07
DEIMOS_COSMOS_838532 < 0.177 < 0.191 < 0.268 < 8.04 < 8.07 < 8.22
DEIMOS_COSMOS_869970 < 0.097 < 0.105 < 0.146 < 7.87 < 7.90 < 8.04
DEIMOS_COSMOS_910650 < 0.095 < 0.102 < 0.141 < 7.91 < 7.95 < 8.08
DEIMOS_COSMOS_920848 < 0.187 < 0.202 < 0.287 < 8.07 < 8.10 < 8.25
DEIMOS_COSMOS_926434 < 0.181 < 0.200 < 0.267 < 8.04 < 8.08 < 8.20
DEIMOS_COSMOS_933876 < 0.183 < 0.200 < 0.282 < 8.04 < 8.07 < 8.22
vuds_cosmos_5101013812 < 0.185 < 0.203 < 0.288 < 8.04 < 8.08 < 8.23
vuds_cosmos_510148750 < 0.132 < 0.143 < 0.190 < 7.91 < 7.94 < 8.07
vuds_cosmos_510327576 < 0.209 < 0.224 < 0.308 < 8.11 < 8.14 < 8.28
vuds_cosmos_510581738 < 0.163 < 0.178 < 0.260 < 8.00 < 8.04 < 8.20
vuds_cosmos_5131465996 < 0.162 < 0.174 < 0.251 < 7.99 < 8.02 < 8.18

Notes. The three methods used to compute them (aggressive, normal, and secure) are the same as in Table B.2 (method described in Sect. 3.3), but applied to the moment-0 maps. In the absence of any external information, we recommend to use the secure upper limits. If the source is known to be point-like, the normal upper limits can be used.

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