Table B.2
Emission line fluxes and EWs of selected galaxies in VUDS.
| VUDS ID | [O ii] | W([O ii]) | [Ne iii] | Hγ | [O iii] | Hβ | W([Hβ]) | [O iii] | [O iii] | W([O iii]) | Hα | W(Hα) | [N ii] | [S ii] | [S ii] | c(Hβ) |
| λ3727 | λ3868 | λ4363 | λ4959 | λ5007 | λ6583 | λ6716 | λ6731 | |||||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) | (15) | (16) | (17) |
|
|
||||||||||||||||
| 510086862 | 13.7 ± 1.5 | 80.3 ± 4 | 3.4 ± 0.9 | – | – | 5.5 ± 0.8 | 31.5 ± 3 | 3.3 ± 1.0 | 10.1 ± 1.0 | 52.0 ± 7.0 | 12.5 ± 2 | 80 ± 15 | 1.5 ± 0.4 | – | – | 0.078c |
| 510146174 | 9.8 ± 1 | 158 ± 60 | 2.1 ± 0.4 | 3 ± 0.5 | – | 7.4 ± 1.5 | 106 ± 37 | 11.9 ± 1.6 | 39.6 ± 0.8 | 560.0 ± 150.0 | – | – | – | – | – | 0.627c |
| 510165275 | 20.8 ± 1.5 | 75 ± 13 | 9.4 ± 0.6 | 12 ± 1.5 | 3.2 ± 0.5 | 23.5 ± 0.7 | 150 ± 15 | 35.5 ± 1.5 | 102.4 ± 1.3 | 661.0 ± 170.0 | – | – | – | – | – | 0.229b |
| 510175664 | 12.1 ± 1.4 | 92 ± 30 | 4.7 ± 1 | – | – | 14.7 ± 1.2 | 135 ± 70 | 17.1 ± 0.9 | 48.9 ± 1.2 | 648.0 ± 250.0 | – | – | – | – | – | 0.157c |
| 510229076 | 6.4 ± 0.8 | 49 ± 17 | 2 ± 0.2 | 3.3 ± 0.6 | – | 5.8 ± 1.6 | 44.5 ± 15 | 5.4 ± 0.5 | 17.4 ± 1.4 | 109.0 ± 36.0 | 25.1 ± 1.6 | 116 ± 36 | – | 4.9 ± 1 | 0.6 ± 0.4 | 0.594a |
| 510329403 | 6.8 ± 1.3 | 59 ± 12 | 2.5 ± 0.9 | – | – | 3.6 ± 0.8 | 12.7 ± 2.7 | 4.1 ± 0.9 | 11.4 ± 1.0 | 37.0 ± 7.0 | 12 ± 1.5 | 50 ± 11 | – | – | – | 0.232a |
| 510330378 | 15 ± 2 | 130 ± 60 | – | 3 ± 0.6 | – | 13.5 ± 1.1 | 66 ± 13 | 23.3 ± 1.5 | 67.5 ± 1.5 | 274.0 ± 44.0 | 42 ± 4 | 260 ± 120 | 3.7 ± 1.1 | – | – | 0.136a |
| 510352169 | 26.4 ± 2.6 | 50 ± 11 | 29.7 ± 3.4 | – | – | 50.8 ± 4.0 | 195 ± 34 | 94.2 ± 5.0 | 247.0 ± 3.0 | 670.0 ± 190.0 | – | – | – | – | – | 0.47c |
| 510353245 | 12 ± 2 | 24.3 ± 5 | – | – | – | 9.0 ± 1.6 | 25 ± 6 | 13.0 ± 2.5 | 39.5 ± 2.5 | 122.0 ± 24.0 | 17.1 ± 2 | 116 ± 46 | – | – | – | 0.392c |
| 510376669 | 9.9 ± 0.7 | 44 ± 11 | 6.6 ± 0.7 | 7.2 ± 1 | 3.1 ± 0.4 | 24.0 ± 1.6 | 184 ± 60 | 55.6 ± 1.5 | 116.0 ± 2.0 | 950.0 ± 300.0 | – | – | – | – | – | 0.235c |
Notes. Columns: (1) VUDS identification number; (2) to (16) Fluxes and EWs of the emission lines measured with the task splot of IRAF. The fluxes are given in 10-18 erg cm-2 s-1, while the equivalent widths (W) are in Å. No extinction correction has been applied to these fluxes. (17) Reddening constant derived from (a) Hα/Hβ or (b) Hγ/Hβ ratios, whenever possible, or (c) the SED best-fitting for those galaxies where (a) and (b) cannot be measured or where they produce a negative extinction (i.e., Hα/Hβ< 2.82 or Hγ/Hβ< 0.47, assuming Case B recombination with Te= 2 × 104 K, ne= 100 cm-3). The entire version of this table for the full sample of ELGs is available at the CDS.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.