Table 3
Hα flux emission and derived quantities for the (U)LIRGs in the VIMOS sample.
| IRAS | Flux Hα | fslit | E(B − V) | Fluxcorr Hα | SFRHα | SFRLIR | |
| name | 10-13 erg cm-2 s-1 | PA 0°/90° | 10-13 erg cm-2 s-1 | M⊙ yr-1 | M⊙ yr-1 | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | |
|
|
|||||||
| F01159−4443c | 3.88 | 0.47/0.55 | 1.41(N),0.91(S) | 31.30 ± 8.44 | 30.14 ± 8.13 | 51.98 | |
| F01341−3735N | 5.97 | 0.30/0.24 | 0.45 | 9.14 ± 1.65 | 4.96 ± 0.89 | 6.27 | |
| F01341−3735S | 1.98 | 0.60/0.67 | 0.24 | 2.94 ± 0.67 | 1.60 ± 0.36 | 19.78 | |
| F04315−0840 | 14.75 | 0.46/0.50 | 1.36 | 168.7 ± 45.90 | 77.07 ± 21.04 | 84.31 | |
| F05189−2524 | 0.15 | 0.67/0.47 | 1.83 | 6.40 ± 1.81 | – | – | |
| F06035−7102ac | 1.40 | 0.18/0.26 | 1.40(W),0.99(E) | 6.43 ± 1.55 | 85.36 ± 20.63 | 313.26 | |
| F06076−2139 | 0.63 | 0.36/0.33 | – | – | – | – | |
| F06206−6315 | 0.16 | 0.44/0.31 | 1.87 | 4.96 ± 1.39 | 91.79 ± 25.73 | 320.55 | |
| F06259−4708Cb | 2.82 | 0.54/0.36 | 0.93 | 13.82 ± 3.58 | 39.73 ± 10.3 | 139.93 | |
| F06259−4708N | 2.28 | 0.53/0.66 | 0.13 | 2.80 ± 0.60 | 8.04 ± 1.72 | – | |
| F06259−4708S | 0.75 | 0.58/0.26 | – | – | – | – | |
| F06295−1735 | 3.81 | 0.58/0.65 | 0.36 | 5.06 ± 0.85 | 4.20 ± 0.71 | 32.05 | |
| F06592−6313 | 0.52 | 0.26/0.14 | 1.28 | 6.33 ± 1.75 | 6.12 ± 1.7 | 28.57 | |
| F07027−6011Nb | 1.86 | 0.30/0.33 | 1.30 | 12.92 ± 3.34 | 23.78 ± 6.15 | 75.14 | |
| F07027−6011S | 2.87 | 0.55/0.58 | – | – | – | – | |
| F07160−6215 | 5.95 | 0.39/0.21 | – | – | – | 24.97 | |
| 08355−4944 | 25.72 | 0.53/0.58 | – | – | – | 68.77 | |
| 08424−3130N | 0.71 | 0.59/0.83 | – | – | – | 18.94 | |
| 08424−3130S | 1.36 | 0.44/0.44 | – | – | – | – | |
| F08520−6850 | 2.00 | 0.30/0.53 | – | – | – | 116.79 | |
| 09022−3615 | 5.59 | 0.52/0.57 | – | – | – | 360.93 | |
| F09437 + 0317Na | 4.39 | 0.10/0.11 | – | – | – | 28.01 | |
| F09437 + 0317S | 3.50 | 0.10/0.14 | – | – | – | – | |
| F10015−0614 | 8.18 | 0.15/0.15 | 0.74 | 13.51 ± 2.33 | 6.94 ± 1.20 | 35.14 | |
| F10038−3338a | 0.50 | 0.50/0.60 | – | – | – | 101.72 | |
| F10257−4339 | 80.06 | 0.13/0.19 | – | – | – | 84.61 | |
| F10409−4556 | 3.72 | 0.11/0.19 | 0.47 | 5.06 ± 0.85 | 4.08 ± 0.68 | 31.32 | |
| F10567−4310 | 2.90 | 0.21/0.24 | 1.03 | 9.38 ± 2.10 | 5.02 ± 1.12 | 20.22 | |
| F11255−4120 | 1.34 | 0.27/0.24 | 0.86 | 3.52 ± 0.75 | 2.00 ± 0.36 | 18.88 | |
| F11506−3851 | 12.90 | 0.21/0.26 | 1.16 | 56.00 ± 13.4 | 11.62 ± 2.78 | 34.35 | |
| F12043−3140Sb | 0.81 | 0.20/0.22 | 0.93 | 1.54 ± 0.33 | 1.60 ± 0.33 | 40.35 | |
| F12043−3140N | 1.54 | 0.62/0.73 | 0.00 | 2.10 ± 0.44 | 2.07 ± 0.43 | – | |
| F12115−4656 | 3.91 | 0.23/0.26 | 0.55 | 6.43 ± 1.16 | 4.00 ± 0.72 | 22.17 | |
| 12116−5615 | 1.55 | 0.63/0.70 | – | – | – | 70.37 | |
| F12596−1529c | 3.11 | 0.38/0.38 | 1.07(W),0.70(E) | 10.61 ± 2.51 | 4.85 ± 1.15 | 20.22 | |
| F13001−2339 | 0.66 | 0.33/0.48 | 0.78 | 2.20 ± 0.53 | 2.00 ± 0.46 | 51.98 | |
| F13229−2934 | 4.30 | 0.37/0.39 | 0.46 | 7.38 ± 1.46 | 2.50 ± 0.49 | 33.56 | |
| F14544−4255Wb | 2.75 | 0.45/0.32 | 0.31 | 4.01 ± 0.77 | 1.80 ± 0.35 | 22.17 | |
| F14544−4255E | 0.56 | 0.04/0.14 | – | – | – | – | |
| F17138−1017 | 2.12 | 0.50/0.14 | - | – | – | 44.25 | |
| F18093−5744Nb | 15.60 | 0.21/0.19 | 0.47 | 21.83 ± 3.67 | 12.00 ± 2.00 | 63.96 | |
| F18093−5744C | 4.43 | 0.54/0.57 | 0.82 | 18.09 ± 4.64 | 9.86 ± 2.53 | – | |
| F18093−5744S | 2.73 | 0.29/0.29 | – | – | – | – | |
| F21130−4446 | 0.83 | 0.44/0.18 | 0.44 | 1.45 ± 0.30 | 27.00 ± 5.52 | 212.53 | |
| F21453−3511 | 9.48 | 0.31/0.24 | 0.62 | 18.52 ± 3.66 | 8.71 ± 1.72 | 44.25 | |
| F22132−3705 | 11.36 | 0.10/0.10 | 1.05 | 22.49 ± 4.05 | 5.23 ± 0.94 | 28.57 | |
| F22491−1808 | 0.45 | 0.37/0.59 | 0.74 | 1.60 ± 0.41 | 20.31 ± 5.15 | 254.62 | |
| F23128−5919c | 2.29 | 0.46/0.26 | 1.08(N),0.81(S) | 10.10 ± 2.54 | 38.90 ± 9.79 | 197.65 | |
Notes. Column (1): IRAS name. Column (2): Hα fluxes without reddening correction. An error of 20% is assumed for these values. Column (3): fraction of the observed Hα emission within a slit of width 2 arsec at PAs 0 and 90° (see text for details). Column (4): E(B − V) for those objects with nuclear Hα/Hβ measurements in the literature. The references for the nuclear data are those shown in Col. (12) in Table 1. For those objects with multiple references we have used the more recent one. Assuming a typical 10% for the Hα/Hβ ratio (e.g. Veilleux et al. 1999) we find that the formal error for the E(B − V) values in the table is 0.09. Column (5): the Hα flux values corrected from reddening effects. These values have been calculated using the E(B − V) values in Col. (4) to deredden the fraction of the flux within the slit and assuming no reddening outside the slit. The slit PA including the larger fraction of the Hα emission was used during the process (see text for details). Columns (6) and (7): the SFRs derived using the Hα luminosity (LHα) corrected from reddening effects, and the IR luminosity (LIR).
The SFRIR values in the table refer to the whole system with the exception of IRAS F18093-5744, for which the SFRIR refer to the northern pair (IC 4687/IC 4686). In addition, there are no Hα/Hβ nuclear measurements available for the southern galaxies of IRAS F06295-1735, IRAS F07027-6011 and IRAS F18093-5744, and the eastern galaxy in IRAS F14544-4255. These galaxies were not used when calculating SFRHα.
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.