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Table 9.

Emission line fluxes, luminosities, and widths of four sources in the HLS field.

Source Line Fobs Sline Lline FWHM
[GHz] [mJy km s−1] [109 K km s−1 pc2] [107 L] [km s−1]
HLS-2-1 CO(4–3) 73.852 < 240 < 15.0 < 4.7 254
CO(5–4) 92.309 246 ± 65 9.8 ± 2.6 6.0 ± 1.6
CO(8–7) 147.658 193 ± 44 3.0 ± 0.7 7.6 ± 1.7
HLS-2-2 CO(4–3) 75.226 309 ± 96 18.6 ± 5.8 5.8 ± 1.8 487
CO(5–4) 94.027 < 513 (1) < 11.2 (1) < 6.9 (1)
CO(7–6) 131.618 < 164 (1) < 3.2 (1) < 5.4 (1)
[CI](2–1) 132.057 196 ± 50 3.8 ± 1.0 6.5 ± 1.7
CO(8–7) 150.406 < 151 (1) < 2.3 (1) < 5.7 (1)
HLS-3 CO(3–2) (2) 83.856 < 665 (1) < 32.8 (1) < 4.3 (1) 752
CO(5–4) (2) 139.746 1347 ± 164 23.9 ± 2.9 14.7 ± 1.8
CO(4–3) (3) 139.746 1347 ± 164 22.3 ± 2.8 7.0 ± 0.9
HLS-22 CO(3–2) 85.691 521 ± 82 24.5 ± 3.8 3.2 ± 0.5 508
CO(4–3) 114.250 719 ± 170 19.0 ± 4.5 6.0 ± 1.4

Notes. (1)Upper limits are given at 3σ. (2)Considering z = 3.123. (3)Considering z = 2.299. Given the line detected at 139.746 GHz, no other CO or [CI] line is expected to fall within the spectral coverage.

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