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Table 1.

Compiled data for our sample of SF galaxies.

(1) (2) (3) (4) (5) (6)
SpecObjID log(M) log(SFR) 12 + log(O/H) Dn(4000) Catalogue
[M] [M yr−1]
995351907448940544 9.95 ± 0.10 0.41 ± 0.03 8.49 ± 0.01 1.20 ± 0.01 SIG
891794679312443392 10.50 ± 0.10 0.33 ± 0.09 8.60 ± 0.02 1.58 ± 0.03 SIG
464046166120622080 9.68 ± 0.10 0.42 ± 0.02 8.33 ± 0.00 1.10 ± 0.01 SIG
2052605755323869184 10.56 ± 0.10 0.69 ± 0.04 8.59 ± 0.01 1.34 ± 0.02 SIG
2848665917645154304 10.53 ± 0.10 −0.05 ± 0.07 8.60 ± 0.02 1.46 ± 0.01 SIG
2568209360727599104 10.61 ± 0.10 0.76 ± 0.03 8.61 ± 0.01 1.28 ± 0.01 SIG
1148505361804716032 7.75 ± 0.10 −1.52 ± 0.03 8.00 ± 0.03 1.06 ± 0.04 SIP
2046971318942853120 7.84 ± 0.10 −2.05 ± 0.01 8.01 ± 0.06 1.25 ± 0.06 SIP
369358979404425216 10.03 ± 0.10 −0.40 ± 0.10 8.59 ± 0.02 1.27 ± 0.02 SIP
498809974038751232 9.79 ± 0.10 −0.43 ± 0.02 8.63 ± 0.00 1.37 ± 0.01 SIT

Notes. The list of galaxies for each sample is randomly sorted. The full table is available in electronic format at the CDS. The columns correspond to: (1) SDSS spectroscopic name; (2) log(M), stellar mass from Argudo-Fernández et al. (2015) in M; (3) log(SFR), aperture corrected star formation rate as described in Sect. 3.1, in M yr−1; (4) 12 + log(O/H), oxygen abundance as described in Sect. 3.2; (5) Dn(4000), narrow definition of the 4000 Å break strength in Balogh et al. (1999) from the MPA-JHU catalogue; and (6) indicates if the galaxy is coming from the SIG, SIP, or SIT catalogues.

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