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Table 1
Fundamental parameters of the MASSIV sample.
| VVDS ID | Redshift | Flux(Hα) | [N ii]/Hα | SFR | SFR c | Z PMC09 | Z T04 | log (M∗) |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
|
|
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| 020106882 | 1.3980 | 14.4 ± 2.4 | 0.23 ± 0.07 | 13.3 ± 0.8 | 38.10 ± 2.24 | 8.56 ± 0.11 | 8.80 ± 0.11 | 9.99 ± 0.22 |
| 020116027 | 1.5259 | 15.6 ± 1.5 | 0.13 ± 0.06 | 14.7 ± 3.6 | 42.20 ± 1.62 | 8.37 ± 0.15 | 8.55 ± 0.15 | 10.09 ± 0.23 |
| 020147106 | 1.5174 | 39.5 ± 4.0 | 0.08 ± 0.03 | 54.3 ± 6.8 | 92.10 ± 1.62 | 8.22 ± 0.11 | 8.38 ± 0.11 | 10.10 ± 0.38 |
| 020164388 | 1.3532 | 24.4 ± 2.5 | 0.11 ± 0.03 | 21.1 ± 1.1 | 46.50 ± 1.86 | 8.31 ± 0.10 | 8.48 ± 0.10 | 10.13 ± 0.31 |
| 020193070 | 1.0273 | 6.8 ± 1.5 | 0.20 ± 0.10 | 3.0 ± 0.4 | 14.40 ± 1.58 | 8.51 ± 0.17 | 8.73 ± 0.17 | 10.15 ± 0.20 |
| 020214655 | 1.0369 | 24.2 ± 7.4 | 0.20 ± 0.04 | 10.6 ± 0.5 | 51.70 ± 2.51 | 8.53 ± 0.07 | 8.76 ± 0.07 | 10.02 ± 0.16 |
| 020218856 | 1.3096 | 8.1 ± 0.9 | 0.10 ± 0.04 | 6.3 ± 0.6 | 29.65 ± 0.57 | 8.27 ± 0.14 | 8.43 ± 0.14 | 9.70 ± 0.26 |
| 020255799 | 1.0352 | 5.4 ± 1.5 | 0.21 ± 0.15 | 2.6 ± 0.3 | 12.80 ± 2.34 | 8.54 ± 0.25 | 8.77 ± 0.25 | 9.87 ± 0.16 |
| 020261328 | 1.5291 | 9.0 ± 2.7 | 0.12 ± 0.11 | 11.2 ± 1.0 | 19.00 ± 3.71 | 8.34 ± 0.30 | 8.52 ± 0.30 | 10.01 ± 0.20 |
| 020283083 | 1.2809 | 13.5 ± 2.5 | 0.19 ± 0.06 | 10.3 ± 0.8 | 17.40 ± 2.34 | 8.50 ± 0.11 | 8.72 ± 0.11 | 10.05 ± 0.21 |
| 020283830 | 1.3949 | 11.1 ± 1.8 | 0.15 ± 0.07 | 10.3 ± 1.0 | 50.40 ± 1.62 | 8.42 ± 0.16 | 8.62 ± 0.16 | 10.37 ± 0.17 |
| 020363717 | 1.3335 | 38.5 ± 4.2 | 0.13 ± 0.03 | 31.5 ± 3.6 | 53.40 ± 2.04 | 8.38 ± 0.08 | 8.57 ± 0.08 | 9.68 ± 0.20 |
| 020370467 | 1.3330 | 15.9 ± 2.5 | 0.25 ± 0.06 | 14.6 ± 2.5 | 71.20 ± 1.38 | 8.59 ± 0.08 | 8.84 ± 0.08 | 10.57 ± 0.14 |
| 020386743 | 1.0465 | 18.6 ± 2.2 | 0.10 ± 0.03 | 8.1 ± 0.8 | 39.40 ± 3.24 | 8.29 ± 0.09 | 8.46 ± 0.09 | 9.88 ± 0.21 |
| 020461235 | 1.0351 | 8.7 ± 0.9 | 0.18 ± 0.04 | 3.3 ± 0.9 | 9.60 ± 1.99 | 8.47 ± 0.09 | 8.68 ± 0.09 | 10.36 ± 0.14 |
| 140083410 | 0.9426 | 45.5 ± 4.3 | 0.13 ± 0.02 | 16.8 ± 1.2 | 37.10 ± 4.17 | 8.37 ± 0.09 | 8.55 ± 0.09 | 10.07 ± 0.18 |
| 140123568 | 1.0016 | 6.6 ± 0.8 | 0.24 ± 0.06 | 2.4 ± 0.5 | 11.80 ± 2.34 | 8.58 ± 0.09 | 8.83 ± 0.09 | 9.73 ± 0.40 |
| 140137235 | 1.0444 | 9.2 ± 1.6 | 0.11 ± 0.20 | 4.4 ± 1.1 | 21.60 ± 3.71 | 8.30 ± 0.25 | 8.47 ± 0.25 | 10.07 ± 0.29 |
| 140217425 | 0.9758 | 118.1 ± 4.4 | 0.36 ± 0.03 | 41.0 ± 1.9 | 200.00 ± 1.51 | 8.72 ± 0.02 | 9.01 ± 0.02 | 10.84 ± 0.17 |
| 140258511 | 1.2421 | 49.2 ± 2.2 | 0.26 ± 0.05 | 30.0 ± 1.9 | 146.40 ± 3.02 | 8.61 ± 0.06 | 8.87 ± 0.06 | 10.80 ± 0.48 |
| 140262766 | 1.2813 | 10.6 ± 2.6 | 0.19 ± 0.15 | 10.0 ± 3.8 | 10.00 ± 4.79 | 8.50 ± 0.26 | 8.72 ± 0.26 | 9.84 ± 0.43 |
| 140545062 | 1.0401 | 27.5 ± 3.4 | 0.17 ± 0.03 | 13.4 ± 1.5 | 22.70 ± 1.44 | 8.47 ± 0.05 | 8.68 ± 0.05 | 10.60 ± 0.18 |
| 220014252 | 1.3097 | 51.9 ± 6.9 | 0.19 ± 0.05 | 40.5 ± 2.5 | 197.50 ± 2.63 | 8.50 ± 0.08 | 8.72 ± 0.08 | 10.78 ± 0.21 |
| 220015726 | 1.3091 | 54.4 ± 1.8 | 0.21 ± 0.02 | 37.0 ± 5.2 | 106.40 ± 1.44 | 8.53 ± 0.03 | 8.76 ± 0.03 | 10.77 ± 0.27 |
| 220376206 | 1.2440 | 73.5 ± 8.0 | 0.09 ± 0.03 | 51.2 ± 3.9 | 249.70 ± 2.45 | 8.26 ± 0.09 | 8.42 ± 0.09 | 10.67 ± 0.27 |
| 220386469 | 1.0240 | 16.5 ± 6.3 | 0.11 ± 0.04 | 7.5 ± 1.1 | 36.50 ± 1.41 | 8.31 ± 0.13 | 8.48 ± 0.13 | 10.80 ± 0.16 |
| 220397579 | 1.0367 | 71.9 ± 9.4 | 0.13 ± 0.03 | 29.4 ± 4.0 | 143.20 ± 3.24 | 8.38 ± 0.09 | 8.57 ± 0.09 | 10.23 ± 0.17 |
| 220544103 | 1.3970 | 50.8 ± 7.4 | 0.23 ± 0.05 | 52.2 ± 1.4 | 117.50 ± 2.57 | 8.57 ± 0.07 | 8.81 ± 0.07 | 10.71 ± 0.27 |
| 220544394 | 1.0077 | 29.8 ± 3.8 | 0.14 ± 0.03 | 10.3 ± 0.7 | 50.10 ± 2.40 | 8.39 ± 0.07 | 8.58 ± 0.07 | 10.34 ± 0.23 |
| 220576226 | 1.0217 | 30.2 ± 3.1 | 0.18 ± 0.01 | 13.6 ± 0.7 | 66.30 ± 2.75 | 8.48 ± 0.03 | 8.69 ± 0.03 | 10.31 ± 0.23 |
| 220578040 | 1.0461 | 20.2 ± 1.6 | 0.18 ± 0.02 | 9.4 ± 0.9 | 20.80 ± 1.62 | 8.48 ± 0.05 | 8.69 ± 0.05 | 10.72 ± 0.16 |
| 220584167 | 1.4637 | 64.6 ± 2.9 | 0.13 ± 0.02 | 68.6 ± 3.4 | 202.60 ± 1.78 | 8.37 ± 0.06 | 8.55 ± 0.06 | 11.21 ± 0.25 |
| 910163602 | 1.3263 | 15.9 ± 3.1 | 0.37 ± 0.05 | 11.9 ± 2.0 | 54.35 ± 2.04 | 8.73 ± 0.05 | 9.03 ± 0.05 | 10.83 ± 0.12 |
| 910186191 | 1.5399 | 35.4 ± 6.0 | 0.12 ± 0.02 | 39.1 ± 6.1 | 31.43 ± 6.10 | 8.35 ± 0.06 | 8.53 ± 0.06 | 11.27 ± 0.45 |
| 910193711 | 1.5523 | 33.0 ± 6.9 | 0.18 ± 0.04 | 40.6 ± 22.7 | 197.70 ± 2.04 | 8.48 ± 0.08 | 8.69 ± 0.08 | 9.99 ± 0.18 |
| 910207502 | 1.4656 | 9.3 ± 1.2 | 0.26 ± 0.04 | 10.3 ± 1.0 | 50.22 ± 1.03 | 8.61 ± 0.05 | 8.87 ± 0.05 | 10.31 ± 0.33 |
| 910224801 | 1.3201 | 10.7 ± 3.1 | 0.37 ± 0.05 | 8.8 ± 1.8 | 18.12 ± 1.77 | 8.73 ± 0.04 | 9.03 ± 0.04 | 9.96 ± 0.20 |
| 910238285 | 1.5405 | 7.7 ± 3.0 | 0.16 ± 0.03 | 14.6 ± 2.6 | 41.89 ± 2.63 | 8.44 ± 0.07 | 8.64 ± 0.07 | 10.92 ± 0.13 |
| 910250031 | 1.6609 | 28.4 ± 1.4 | 0.03 ± 0.02 | 48.6 ± 5.6 | 139.84 ± 5.58 | 7.92 ± 0.19 | 8.09 ± 0.19 | 10.15 ± 0.20 |
| 910259245 | 1.5174 | 4.9 ± 1.8 | 0.27 ± 0.15 | 5.6 ± 1.0 | 27.08 ± 0.98 | 8.62 ± 0.20 | 8.88 ± 0.20 | 10.79 ± 0.12 |
| 910261247 | 1.4262 | 18.8 ± 3.3 | 0.21 ± 0.02 | 19.8 ± 1.1 | 96.78 ± 1.14 | 8.54 ± 0.03 | 8.77 ± 0.03 | 10.57 ± 0.14 |
| 910266034 | 1.5642 | 15.8 ± 4.0 | 0.08 ± 0.03 | 20.4 ± 3.0 | 76.25 ± 2.95 | 8.19 ± 0.14 | 8.34 ± 0.14 | 10.07 ± 0.20 |
| 910276733 | 1.3390 | 3.8 ± 0.9 | 0.16 ± 0.06 | 11.0 ± 2.1 | 53.67 ± 2.11 | 8.44 ± 0.12 | 8.64 ± 0.12 | 10.14 ± 0.19 |
| 910279515 | 1.3983 | 14.2 ± 1.5 | 0.24 ± 0.11 | 14.2 ± 2.0 | 69.00 ± 4.68 | 8.58 ± 0.15 | 8.83 ± 0.15 | 10.79 ± 0.14 |
| 910279755 | 1.3127 | 23.5 ± 1.4 | 0.15 ± 0.05 | 16.3 ± 1.3 | 27.71 ± 1.29 | 8.42 ± 0.10 | 8.62 ± 0.10 | 9.96 ± 0.24 |
| 910337228 | 1.3972 | 15.8 ± 1.2 | 0.09 ± 0.08 | 39.1 ± 16.6 | 44.97 ± 16.57 | 8.23 ± 0.30 | 8.39 ± 0.30 | 9.96 ± 0.20 |
| 910340496 | 1.3981 | 4.5 ± 0.6 | 0.26 ± 0.13 | 3.7 ± 0.5 | 17.95 ± 0.50 | 8.60 ± 0.18 | 8.85 ± 0.18 | 10.03 ± 0.25 |
| 910370574 | 1.6632 | 12.6 ± 1.5 | 0.10 ± 0.02 | 16.8 ± 3.6 | 82.00 ± 3.65 | 8.28 ± 0.08 | 8.44 ± 0.08 | 10.09 ± 0.24 |
Notes. Column 1 lists the VVDS identification number. Column 2 gives the redshift. Columns 3 and 4 list the Hα flux (in erg s-1 cm-2) and the flux ratio [N ii]/Hα respectively. The star formation rate (in M⊙ yr-1) is given in Cols. 5 (not corrected for extinction) and 6 (dereddened value). Columns 7 and 8 list the metallicity computed with the Pérez-Montero & Contini (2009) and Tremonti et al. (2004) calibrations respectively. Stellar mass (in log of M⊙) is given in Col. 9 (from Contini et al. 2012).
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