Table 3.
Fluxes and velocities for the Hα, Hβ and [O III] λλ4959, 5007 galaxy line components, from the integrated spectra over the regions shown in Figs. 5 and 7 for DELS J0411–0907 (upper panels) and VDES J0020–3653 (lower panels).
| FHβ | F[O III]λ4959 | F[O III]λ5007 | FHα | F[N II]λ6584 | Vr | Vσ | |
|---|---|---|---|---|---|---|---|
| (10−18 erg s−1 cm−2) [S/N] | (km s−1) | (km s−1) | |||||
| DELS J0411–0907 | |||||||
| N&B quasar subtraction | |||||||
| Region 1, GN | 3.8±0.2 [23] | 5.6±0.2 [34] | 16.8±0.2 [92.4] | 9.0±0.4 [21] | < 1.0 | 65±51 | 135±51 |
| Region 2, GN | 5.2±1.1 [4.8] | 6.8±0.9 [7.2] | 20.5±1.1 [19] | 11.0±2.3 [4.7] | < 5.1 | 163±51 | 314±51 |
| Region 2, GB | < 5.5 | 3.8±1.6 [2.5] | 11.6±1.7 [6.8] | < 8.6 | < 8.5 | −783±51 | 526±51 |
| Region 3, GN | < 0.4 | 0.8±0.1 [6.7] | 2.5±0.1 [18] | < 0.8 | < 0.8 | 396±51 | 161±51 |
| Region 3, GB | < 1.9 | 1.5±0.6 [2.4] | 4.4±0.6 [6.8] | < 3.5 | < 3.5 | 38±51 | 764±51 |
| BLR quasar subtraction | |||||||
| Region 1, GN | 3.4±0.2 [20] | 5.6±0.2 [34] | 16.9±0.2 [92.9] | 9.4±0.4 [22] | < 1.0 | 64±51 | 135±51 |
| Region 2, GN | 4.2±1.0 [4.1] | 9.8±0.9 [11] | 29.6±1.0 [28.7] | 30.1±2.3 [13] | < 4.9 | 22±51 | 303±51 |
| Region 2, GB | < 8.2 | 20.9±2.4 [8.8] | 62.8±2.5 [25] | < 12.6 | < 12.6 | −374±51 | 807±51 |
| Region 3, GN | < 0.4 | 0.8±0.1 [6.6] | 2.5±0.1 [18] | < 0.8 | < 0.8 | 392±51 | 162±51 |
| Region 3, GB | < 1.9 | 1.6±0.6 [2.7] | 5.0±0.6 [7.6] | < 3.5 | < 3.5 | 7±51 | 764±51 |
| VDES J0020–3653 | |||||||
| N&B quasar subtraction | |||||||
| Region 1, GN | 2.1±0.2 [11] | 5.4±0.2 [27] | 16.2±0.3 [82] | 7.9±0.6 [22] | < 1.4 | −30±51 | 319±51 |
| Region 2, GN | 2.3±1.2 [2.6] | 4.8±1.0 [5.3] | 14.4±1.0 [16] | 17.4±2.8 [11] | < 5.9 | 149±51 | 369±51 |
| Region 2, GB | < 6.7 | 2.4±1.9 [1.4] | 7.4±1.9 [4.3] | < 11.5 | < 11.2 | −877±51 | 698±51 |
| Region 3, GN | 1.2±0.2 [8.9] | 1.5±0.2 [11] | 4.6±0.2 [33] | 5.7±0.5 [19] | < 1.1 | 232±51 | 250±51 |
| Region 4, GN | 1.4±0.2 [13] | 2.1±0.2 [19] | 6.2±0.2 [56] | 5.6±0.4 [21] | < 0.9 | 367±51 | 189±51 |
| BLR quasar subtraction | |||||||
| Region 1, GN | 2.9±0.3 [11] | 5.8±0.3 [23] | 17.3±0.3 [63] | 8.3±0.7 [12] | < 1.4 | −40±51 | 332±51 |
| Region 2, GN | 4.5±0.9 [5.2] | 4.6±0.7 [6.5] | 13.7±0.7 [19] | 17.9±2.1 [8.5] | < 4.0 | 15±51 | 263±51 |
| Region 2, GB | 16.0±2.9 [5.6] | 14.3±2.6 [5.6] | 43.1±2.6 [17] | < 14.8 | < 14.6 | −460±51 | 942±51 |
| Region 3, GN | 1.3±0.2 [6.1] | 1.5±0.2 [7.8] | 4.6±0.2 [23] | 5.7±0.5 [12] | < 1.1 | 227±51 | 252±51 |
| Region 4, GN | 1.4±0.2 [8.6] | 2.1±0.2 [12] | 6.2±0.2 [34] | 5.6±0.4 [14] | < 0.9 | 367±51 | 189±51 |
Notes. The values in braces give the integrated S/N of each line. We present the results from both the N&B quasar subtraction and the BLR quasar subtraction. We fit the narrow line spectra with two components, a true narrow line (GN) as well as a galaxy ‘broad’ wing (GB) component likely associated with outflows; we note that this ‘broad’ component is not from the quasar BLR, which has been subtracted from these spectra. In regions where no broader GB line component is detected, we fit only a single GN component. Upper limits for undetected lines are 3σ limits on the line flux, taken from the ERR array. Uncertainties on the velocity and velocity dispersion assume an uncertainty of ±1 wavelength element, ±6.65 Å or 51 km s−1. The velocity dispersions have been corrected for an instrumental broadening of FWHMinst = 115 km s−1.
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.