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Table E.1

Properties of the best-fit SEDs from SED fitting and values for EWobs from the TPV.

SED Fitting TPV
IDa RA (J200) Dec (J2000) Massb ES(B − V) c Age d τ e SFR f g Z h f cov i E W obs j
7 +10:01:54.356 +01:53:18.36
14 +10:01:57.962 +01:53:57.58
33 +10:01:45.444 +01:55:22.99
94 +10:01:37.653 +02:10:33.39
96 +10:02:12.744 +02:10:47.98
97 +10:02:16.988 +02:10:55.96
99 +10:02:15.195 +02:10:54.36
104 +10:02:15.978 +02:11:18.89
105 +10:02:07.660 +02:11:20.09
111 +10:02:16.354 +02:12:00.30
113 +10:01:41.651 +02:12:02.75
114 +10:02:09.637 +02:12:02.47
117 +10:02:17.543 +02:12:12.54
121 +10:02:03.952 +02:12:39.54
122 +10:02:01.838 +02:12:38.81
124 +10:02:16.714 +02:12:55.00
125 +10:02:18.112 +02:13:02.53
126 +10:01:47.095 +02:13:26.64
128 +10:01:46.900 +02:13:30.85
131 +10:02:06.263 +02:13:40.26
135 +10:01:52.737 +02:13:53.75
138 +10:02:17.661 +02:14:02.29
147 +10:01:46.836 +02:14:24.08
150 +10:02:12.970 +02:14:28.42
153 +10:02:18.594 +02:14:41.36
161 +10:01:54.279 +02:15:26.80
164 +10:02:04.380 +02:15:30.63
167 +10:01:53.203 +02:15:49.45
170 +10:02:15.102 +02:15:59.41
172 +10:00:46.944 +02:26:10.89
186 +10:00:12.440 +02:27:46.31
204 +10:00:41.641 +02:29:02.47
205 +10:00:41.331 +02:29:04.57
226 +10:00:36.526 +02:31:07.13
235 +10:00:44.244 +02:32:18.36

Notes. This table extends Table 4.

(a)

NBES

(b)

log 10(M [ M⊙ ]); mass in stars at time of observation.

(c)

Stellar extinction assuming Calzetti et al. (2000) extinction law.

(d)

log 10(Age [ yr ])

(e)

log 10(τ [ yr ])

(f)

[ M⊙yr-1 ]; instantaneous SFR at time of observation.

(g)

[ M⊙yr-1 ]; SFR averaged over 100Myr before time of observation.

(h)

Metallicity in [ Z⊙ ].

(i)

Covering fraction of the gas; related to the escape of ionizing radiation through fesc;ion = 1 − fcov

(j)

[ nm ].

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