Table 3.
First five rows of the table containing the candidate properties of the U + E sample.
| ID | RA | Dec | zphot | χ2 | zphot, sec | χsec2 | UCD | χUCD2 | EWLyα | MUV |
|---|---|---|---|---|---|---|---|---|---|---|
| [deg] | [deg] | Model | [Å] | |||||||
| EUCL J100054.15+015048.3 | 150.226 | 1.846 | ![]() |
8.4 | 1.45 | 13.4 | M6 | 12.2 | 0.0 | ![]() |
| EUCL J100105.05+015227.0 | 150.271 | 1.874 | ![]() |
6.5 | 1.50 | 27.6 | M6 | 21.4 | 0.0 | ![]() |
| EUCL J100048.32+015330.8 | 150.201 | 1.892 | ![]() |
10.3 | 1.45 | 38.0 | T3 | 22.1 | 0.0 | ![]() |
| EUCL J100028.55+015503.9 | 150.119 | 1.918 | ![]() |
14.1 | 1.55 | 42.4 | T8 | 21.2 | 0.0 | ![]() |
| EUCL J100120.73+015542.5 | 150.336 | 1.928 | ![]() |
7.1 | 1.55 | 31.1 | T3 | 21.7 | 0.0 | ![]() |
| ⋮ |
Notes. The fluxes within
diameter circular apertures, along with uncertainties, are also provided in the full version available at the CDS. We also provide the same table for the U-only sample. The first three columns show the ID, RA, and Dec of the source. The next six columns show photometric redshift and χ2 value of the LBG solution, as well as the low-redshift dusty galaxy solution, and the stellar type and χ2 of the UCD solution. The final two columns show the equivalent width of the Lyman-α emission line if a template with the emission line is preferred, and the absolute rest-frame UV magnitude MUV.
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