Table 1.
Absorption lines identified in the VLT spectrum of SDSS J0932+0840 and their measured column densities.
Ion | λ (a) | log(f) (b) | Elow(c) | Nion(d) |
---|---|---|---|---|
(Å) | (cm−1) | (log(cm−2)) | ||
H I | 1215.67 | −0.38 | 0 | > 14.57−0.23 |
He I* | 2829.91 | −2.22 | 159856 | ![]() |
C II | 1334.53 | −0.89 | 0 | > 15.20−0.18 |
C II* | 1335.71 | −0.94 | 63 | > 15.24−0.32 |
N V | 1238.82, 1242.80 | −0.80, −1.10 | 0 | > 15.31−0.33 |
Mg II | 2796.35, 2803.53 | −0.22, −0.52 | 0 | > 14.52−0.29 |
Al III | 1854.72, 1862.79 | −0.25, −0.55 | 0 | > 14.70−0.16 |
Si II | 1808.01 | −2.60 | 0 | ![]() |
Si II* | 1816.93 | −2.71 | 287 | ![]() |
Si IV | 1393.75, 1402.77 | −0.29, −0.59 | 0 | > 14.84−0.32 |
S II | 1250.58, 1253.81 | −0.22, −1.92 | 0 | > 16.44−0.31 |
Cr II | 2056.25, 2062.24, 2066.16 | −0.99, −1.12, −1.29 | 0 | > 15.08−0.10 |
Cr II* | 2161.38 | −1.84* | 42898 | ![]() |
Mn II | 2576.88 | −0.45 | 0 | > 14.04−0.11 |
Fe II | 1901.78 | ![]() |
0 (0) | ![]() |
Fe II* | 1267.42, 2253.82 | −1.85, −2.47 | 385 (1) | ![]() |
Fe II* | 1271.98, 1272.61 | −1.85, −2.36 | 668 (2) | ![]() |
Fe II* | 1275.14, 1275.78 | −2.15, −2.00 | 863 (3) | ![]() |
Fe II* | 1277.66 | −1.85 | 977 (4) | ![]() |
Fe II* | 1405.60, 1412.83, 1418.85 | −2.92, −2.47, −3.04* | 1873 (5) | ![]() |
Fe II* | 2371.22 | −1.84 | 3117 (8) | > 15.33−0.11 |
Fe II* | 2749.99 | −0.86 | 8680 (11) | > 14.32−0.10 |
Fe III* | 1895.48, 1914.07, 1926.32 | −0.33, −0.49, −0.60 | 30089 | ![]() |
Co II | 1941.28, 2012.17 | −1.47, −1.43 | 0 | ![]() |
Co II* | 2286.86 | −0.51 | 3350 | ![]() |
Ni II | 1751.91 | −1.54 | 0 | > 15.35−0.21 |
Ni II* | 2131.93 | −2.58* | 8394 | ![]() |
Ni II* | 2207.41, 2265.16 | −0.79, −0.83 | 10115 | ![]() |
Zn II | 2026.14 | −0.30 | 0 | ![]() |
Notes.
Rest wavelength of the transition in vacuum. Multiple values, wherever mentioned, correspond to detection of multiple troughs for the given energy level of the ionic species.
Logarithm of the oscillator strength of the transition. These were taken from the National Institute of Standards and Technology (NIST) Atomic Spectra Database vers. 5.11, unless marked otherwise. The values marked with an asterisk were obtained from Kurucz & Bell (1995), and the value for the Fe II 1902 transition was determined from our calculations described in Sect. 3.3.
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