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Table 3.

CO line identification towards the five sources shown in Figures 5 and 6.

SDSS ID zSDSS CO νobs Δvel σpeak FWHMCO SCO fit
transition [GHz] [km s−1] [km s−1] [Jy.km s−1]
J010249.02–010544.8 1.037 6–5 339.98 440 17.2 84.7 ± 4.7 2.935 ± 0.150
J011922.85–004419.7 1.057 6–5 336.43 270 4.9 166.8 ± 23.2 1.934 ± 0.243
J011032.18–010320.4 1.314 7–6 348.71 85 3.3 101.6 ± 30.0 0.604 ± 0.156
J013523.49+001046.3 1.381 7–6 339.18 350 5.5 165.6 ± 31.1 1.115 ± 0.184
J013150.85–002701.8 1.404 7–6 335.58 –90 5.3 97.6 ± 27.6 1.034 ± 0.195

Notes. The observed frequency (νobs), velocity offset of the CO line with respect to zSDSSvel), significance of the detection peak (σpeak), FWHM of the Gaussian fit (FWHMCO), and integrated line flux from the Gaussian fit (SCO fit) are reported.

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