Table 1
New galaxies in the COSMOS, EGS, and CANDELS/GOODS-North fields used to derive the LyC relative escape fraction.
| ID | Field | RAD | Dec | z spec | Rmag | Umag | M 1500 |
|
Cont |
| (deg) | (deg) | (AB) | (AB) | ||||||
|
|
|||||||||
| 53167 | COSMOS | 149.852446 | +2.397032 | 3.359 | 22.95 | ≥29.38 | –22.75 | ≤0.029 | No |
| 218783 | COSMOS | 149.920820 | +2.387060 | 3.297 | 24.49 | ≥29.39 | –21.21 | ≤0.118 | No |
| 223954 | COSMOS | 149.831880 | +2.404150 | 3.371 | 24.77 | ≥29.58 | –20.93 | ≤0.128 | No |
| 219315 | COSMOS | 149.839520 | +2.388460 | 3.363 | 25.21 | ≥29.70 | –20.49 | ≤0.171 | No |
| 215511 | COSMOS | 149.848260 | +2.376170 | 3.363 | 25.24 | ≥29.70 | –20.46 | ≤0.176 | No |
| 220771 | COSMOS | 149.836280 | +2.393190 | 3.359 | 24.84 | ≥29.22 | –20.86 | ≤0.188 | No |
| 217597 | COSMOS | 149.865340 | +2.382770 | 3.284 | 25.73 | ≥29.88 | –19.97 | ≤0.233 | No |
| 211934 | COSMOS | 149.847250 | +2.364040 | 3.355 | 26.86 | ≥29.64 | –18.84 | ≤0.827 | No |
|
|
|||||||||
| 59330a | COSMOS | 150.077045 | +2.360797 | 3.417 | 24.15 | ≥28.93 | –17.40 | ≤0.232 | No |
|
|
|||||||||
| 6328 | EGS | 214.586647 | +52.512559 | 3.357 | 24.26 | ≥29.89 | –21.44 | ≤0.060 | No |
| 9524 | EGS | 214.500676 | +52.477565 | 3.295 | 24.06 | ≥29.54 | –21.64 | ≤0.069 | No |
| 6439 | EGS | 214.552783 | +52.511284 | 3.392 | 24.15 | ≥29.56 | –21.55 | ≤0.073 | No |
| 724 | EGS | 214.501128 | +52.570535 | 3.353 | 24.76 | ≥30.06 | –20.94 | ≤0.081 | No |
| 6922 | EGS | 214.461916 | +52.505537 | 3.351 | 24.71 | ≥29.95 | –20.99 | ≤0.086 | No |
| 4580 | EGS | 214.508258 | +52.531509 | 3.279 | 24.79 | ≥29.90 | –20.91 | ≤0.096 | No |
| 8642 | EGS | 214.460301 | +52.487802 | 3.285 | 24.50 | ≥29.60 | –21.20 | ≤0.098 | No |
| 5197 | EGS | 214.283603 | +52.524388 | 3.271 | 24.52 | ≥29.15 | –21.18 | ≤0.150 | No |
| 6612 | EGS | 214.500033 | +52.509127 | 3.340 | 25.89 | ≥30.45 | –19.81 | ≤0.162 | No |
| 2783 | EGS | 214.554012 | +52.549350 | 3.272 | 25.70 | ≥30.02 | –20.00 | ≤0.200 | No |
| 12335 | EGS | 214.455464 | +52.446348 | 3.287 | 25.32 | ≥29.61 | –20.38 | ≤0.205 | No |
| 13346 | EGS | 214.413697 | +52.433529 | 3.307 | 24.73 | ≥28.87 | –20.97 | ≤0.237 | No |
| 7690 | EGS | 214.249912 | +52.497386 | 3.272 | 25.18 | ≥28.77 | –20.52 | ≤0.392 | No |
| 11372 | EGS | 214.407226 | +52.458201 | 3.294 | 25.36 | 28.48 | –20.34 | 0.603 | No |
| 14043 | EGS | 214.376422 | +52.424380 | 3.344 | 25.18 | ≥28.29 | –20.52 | ≤0.610 | No |
|
|
|||||||||
| 16428 | GDN | 189.216181 | +62.254036 | 3.333 | 23.91 | ≥29.82 | –21.79 | ≤0.048 | No |
| 19977 | GDN | 189.179397 | +62.276656 | 3.363 | 24.38 | ≥30.03 | –21.32 | ≤0.061 | No |
| 12305 | GDN | 189.219779 | +62.227532 | 3.369 | 25.09 | ≥30.35 | –20.61 | ≤0.087 | No |
| 4341 | GDN | 189.290579 | +62.171244 | 3.384 | 24.68 | ≥29.81 | –21.02 | ≤0.094 | No |
| 14132 | GDN | 189.206264 | +62.239252 | 3.367 | 25.44 | ≥30.23 | –20.26 | ≤0.135 | No |
| 91200 | GDN | 189.311200 | +62.311020 | 3.390 | 25.76 | ≥30.21 | –19.94 | ≤0.184 | No |
| 16169 | GDN | 189.215365 | +62.252800 | 3.364 | 25.42 | ≥29.67 | –20.28 | ≤0.214 | No |
| 18979 | GDN | 189.296340 | +62.270650 | 3.350 | 25.80 | ≥29.90 | –19.90 | ≤0.246 | No |
| 91000 | GDN | 188.999330 | +62.202417 | 3.300 | 26.53 | ≥30.21 | –19.17 | ≤0.377 | No |
| 16479 | GDN | 189.194532 | +62.254757 | 3.371 | 25.00 | 27.79 | –20.70 | 0.821 | Yes |
Notes. The galaxies are sorted in ascending order of relative escape fraction in each field (COSMOS, EGS, GDN = CANDELS/GOODS-North). The identification number, ID, is the LBC number for the COSMOS and EGS fields, while it is the CANDELS official identifier for the GOODS-North field. Two sources, indicated by ID > 90 000, are outside the CANDELS/GOODS-North area. The non-detections (i.e., S/N< 1) in the LBC U-band, for which an upper limit (at 1σ) to the relative escape fraction is provided, are indicated by the Umag ≥ and 
symbols, respectively. The last column, Cont, indicates whether a galaxy is possibly contaminated by foreground objects. Notes on individual objects: (a): object ID = 59330 in COSMOS is the lensed galaxy studied by van der Wel et al. (2013) and by Amorin et al. (2014). The U- and R-band magnitudes are the observed photometry for ID = 59330, while the absolute magnitude provides the intrinsic luminosity after the correction by a magnification factor of 40 ± 1.
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