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Table 1

List of ELGs identified in SHARDS and its main properties.

ID RA Dec zphot zspec zlines pEWH α sEWH α FH α pEW[OIII] sEW[OIII] FOIII LHα F850LP N2
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15)
20002280 189.3239 62.19090 0.21 0.213 0.22 65 ± 14 88 ± 12 72 ± 11 34 ± 17 44 ± 4 60 ± 25 153 ± 23 22.661 ± 0.019 0.14
10000098 189.3262 62.19741 0.11 0.105 0.11 19 ± 13 9.2 ± 0.4 169 ± 97 18 ± 12 3.4 ± 0.2 124 ± 71 53 ± 31 21.046 ± 0.002 0.38 ± 0.04
10000145 189.3580 62.20181 0.09 0.089 0.09 45 ± 8 55 ± 1 182 ± 26 26 ± 10 29 ± 1 154 ± 48 57 ± 8 21.313 ± 0.006 0.05
10000515 189.3600 62.22278 0.30 0.299 0.29 43 ± 28 21 ± 2 26 ± 13 16 ± 8 11 ± 2 17 ± 8 181 ± 89 23.257 ± 0.022 0.48
10000777 189.3220 62.23236 0.33 0.336 0.33 32 ± 17 41 ± 2 194 ± 89 20 ± 8 21 ± 1 177 ± 57 1078 ± 492 20.971 ± 0.002 0.13
.....

Notes. EWs and Hα luminosity are corrected by extinction. The complete table is available at the CDS; only the first rows are shown here as guidance. Columns: (1) SHARDS ID. (2) Right ascension from SHARDS catalog. (3) Declination from SHARDS catalog. (4) Photometric redshift from SHARDS catalog. (5) Spectroscopic redshift from Barger et al. (2008). (6) Photometric redshift derived in this study using Hα and [OIII]5007 lines. (7) Photometrically derived Hα EW, in Ångstroms. (8) Spectroscopically derived Hα EW, in Ångstroms. (9) Photometrically derived Hα flux, in 10−18 erg s−1 cm−2. (10) Photometrically derived [OIII]5007 EW, in Ångstroms. (11) Spectroscopically derived [OIII]5007 EW, in Ångstroms. (12) Photometrically derived [OIII]5007 flux, in 10−18 erg s−1 cm−2. (13) Photometrically derived Hα luminosity, in 1038 erg s−1. (14) Magnitude of the galaxy in F850LP band, from HST (Skelton et al. 2014). (15) [NII6583]/Hα ratio derived from spectroscopy. If no uncertainty is shown, the value is an upper limit.

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