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Table 3.

Properties of MUSE members of the overdensity.

ID M2800 β SFR log(M*) log(sSFR)
(AB) (M yr−1) (M) (Gyr−1)
(1) (2) (3) (4) (5) (6)
m1 −19.52 −1.33 20.2 ± 3.4 9.36 0.94 ± 0.55
m2 −19.53 −1.45 18.1 ± 3.4 9.69 0.57 ± 0.11
m3 −21.25 −1.88 57.1 ± 6.2 10.09 0.67 ± 0.08
m4 −20.08 −2.22 13.8 ± 1.1 9.33 0.81 ± 0.23
m5 −19.96 −2.70 7.6 ± 1.1 9.54 0.34 ± 0.28
m6 −19.94 −0.35 13.1 ± 1.0 (a) 10.48 −0.37 ± 0.04

Notes. Columns: (1) source identifier; (2) absolute magnitude at 2800Å rest-frame (not corrected for extinction); (3) slope of the optical spectrum (fλ ∝ λβ); (4) extinction-corrected star formation rate based on the UV spectrum; (5) stellar mass; and (6) specific star formation rate.

(a)

Based on the SED fitting because it provides a more reliable estimate for this source (see text for details).

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