Table 1.
Properties of the targets.
cluster ID | galaxy ID | zspec | Log(M⋆/M⊙) | SFR(Hα) (M⊙/yr) | sSFR(Hα) (Gyr−1) | τdep(Hα) (108 yr) | Re (kpc) | |
---|---|---|---|---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
ISCSJ1426.5+3339 | J142626.1+333827 | 1.17±0.01 | 10.8 ± 0.5 | 79.1±5.3 | 3.0 | |||
J142626.1+333826 | 1.17±0.01 | 10.8 ± 0.5 | 83.7±4.8 | 3.9 |
Notes. (1) cluster and (2) galaxy name; (3) spectroscopic (HST WFC3) redshift of the galaxy; (4) galaxy stellar mass; (5) Hα +[NII] line flux; (6) SFR(Hα) estimated following Zeimann et al. (2013); (7) sSFR(Hα) = SFR(Hα)/M⋆; (8) τdep(Hα) = M(H2)/SFR(Hα) estimated assuming that the two sources equally contribute to the observed CO(2−1) flux, i.e., f = 1/2; (9) effective radius estimated using SExtractor and the HST WFC3 image. Columns (3)–(5) are from Zeimann et al. (2013).
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