Table 5.
Sub-sample of ten galaxies in the catalogue with their properties.
OBJ_ID | RA | Dec | Pointing | Z_SPEC | Q_flag | ||
---|---|---|---|---|---|---|---|
373952 | 150.36320 | 2.46340 | P100_COSMOS_HaHP1 | 1.7195 | 4.0 | ||
399202 | 150.37578 | 2.51607 | P100_COSMOS_HaHP1 | 1.5130 | 4.0 | ||
399761 | 150.34360 | 2.51690 | P100_COSMOS_HaHP1 | 1.3991 | 4.0 | ||
388984 | 34.74180 | −4.86346 | P100_SXDF_HaKP2 | 2.3486 | 3.0 | ||
105609 | 34.59267 | −5.35292 | P100_SXDF_haHP1_v2 | 1.6199 | 3.0 | ||
111251 | 34.61345 | −5.34167 | P100_SXDF_haHP1_v2 | 1.5970 | 4.0 | ||
122473 | 34.61895 | −5.31527 | P100_SXDF_haHP1_v2 | 1.6256 | 3.0 | ||
274911 | 36.720165 | −4.46552 | P100_VVDS_HaHP2 | 1.6092 | 4.0 | ||
394673 | 36.31682 | −4.244806 | P102_VVDS_HaHP2 | 1.5689 | 4.0 | ||
247070 | 36.87232 | −4.51824 | P101_VVDS_HaHP2 | 1.5130 | 4.0 | ||
390870 | 36.33725 | −4.25240 | P99_VVDS_HaHP2_v2 | 1.4341 | 3.5 | ||
OBJ_ID | PHOTO-Z | Priority (M17) | EBV_BEST | ||||
373952 | 1.5269 | 500 | 0.1 | ||||
377914 | 1.6315 | 250 | 0.1 | ||||
399202 | 1.4793 | 500 | 0.3 | ||||
399761 | 1.3806 | 400 | 0.3 | ||||
400978 | 1.5295 | 1000 | 0.3 | ||||
405462 | 1.5557 | 200 | 0.3 | ||||
405597 | 1.4334 | 250 | 0.3 | ||||
405666 | 1.4477 | 200 | 0.2 | ||||
405763 | 1.4553 | 1000 | 0.5 | ||||
OBJ_ID | MASS_INF | MASS_MED | MASS_SUP | SFR_INF | SFR_MED | SFR_SUP | FHα, 1.2 |
log10(M⋆/M⊙) | log10(M⋆/M⊙) | log10(M⋆/M⊙) | log10(M⊙ yr−1) | log10(M⊙ yr−1) | log10(M⊙ yr−1) | 10−17 erg cm−2 s−1 | |
373952 | 8.93 | 9.15 | 9.25 | 0.89 | 1.04 | 1.43 | 4.44 |
377914 | 9.10 | 9.35 | 9.49 | 0.83 | 0.98 | 1.33 | 4.45 |
399202 | 10.01 | 10.11 | 10.18 | 0.95 | 1.15 | 1.38 | 7.87 |
399761 | 9.80 | 10.06 | 10.14 | 1.11 | 1.24 | 1.57 | 6.98 |
400978 | 9.23 | 9.53 | 9.68 | 1.06 | 1.36 | 1.50 | 5.13 |
405462 | 9.95 | 10.00 | 10.05 | 1.33 | 1.44 | 1.55 | 8.10 |
405597 | 10.37 | 10.41 | 10.44 | 1.72 | 1.80 | 1.88 | 12.91 |
405666 | 9.66 | 9.73 | 9.80 | 1.01 | 1.11 | 1.19 | 10.22 |
405763 | 10.18 | 10.36 | 10.46 | 1.47 | 1.68 | 1.93 | 3.24 |
Notes. The full table can be found at CDS. The explanation of the different columns is given in Sect. 8. The column “ID” is repeated at the beginning of each part of the table for the sake of clarity. We estimated that, due to the uncertainties in the spectrophotometric calibrations, the precision on the Hα flux measurement is not better than 10%.
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