Table 2.
Open in new tab

Summary of CO(1–0) VEGAS measurements.

IDνobszCO(1–0)ΔVSΔVaSν|$\mu L^{\prime }_{{\rm CO}}$|
(GHz)(km s−1)(Jy km s−1)Peak (mJy)(1010 K km s−1 pc2)
PJ105353.028.77123.0053 ± 0.00016738 ± 384.3 ± 1.36.2 ± 1.9170 ± 60
PJ112714.535.62482.2352 ± 0.00006736 ± 207.4 ± 2.29.3 ± 2.8178 ± 63
PJ120207.633.49702.442 ± 0.00007602 ± 215.5 ± 1.78.9 ± 2.7154 ± 55
PJ132302.933.73502.4165 ± 0.00006540 ± 174.7 ± 1.48.4 ± 2.5129 ± 46
PJ142823.949.57661.3254 ± 0.00005436 ± 251.2 ± 0.42.9 ± 0.911 ± 4
PJ160722.646.41151.4838 ± 0.00006374 ± 271.0 ± 0.32.4 ± 0.712 ± 4
PJ160917.827.09113.2567 ± 0.00014705 ± 317.6 ± 2.39.8 ± 2.9343 ± 121
IDνobszCO(1–0)ΔVSΔVaSν|$\mu L^{\prime }_{{\rm CO}}$|
(GHz)(km s−1)(Jy km s−1)Peak (mJy)(1010 K km s−1 pc2)
PJ105353.028.77123.0053 ± 0.00016738 ± 384.3 ± 1.36.2 ± 1.9170 ± 60
PJ112714.535.62482.2352 ± 0.00006736 ± 207.4 ± 2.29.3 ± 2.8178 ± 63
PJ120207.633.49702.442 ± 0.00007602 ± 215.5 ± 1.78.9 ± 2.7154 ± 55
PJ132302.933.73502.4165 ± 0.00006540 ± 174.7 ± 1.48.4 ± 2.5129 ± 46
PJ142823.949.57661.3254 ± 0.00005436 ± 251.2 ± 0.42.9 ± 0.911 ± 4
PJ160722.646.41151.4838 ± 0.00006374 ± 271.0 ± 0.32.4 ± 0.712 ± 4
PJ160917.827.09113.2567 ± 0.00014705 ± 317.6 ± 2.39.8 ± 2.9343 ± 121

Notes. |$T_{\rm A}^{*}$| to flux density using the GBT: Q-band is 1 K/1.7 Jy, Ka band is 1 K/1.6 Jy. The reported redshifts correspond to the values obtained after velocity offset corrections. The line widths reported indicate the FWHM values after correcting for the instrumental resolution. This correction was on average less than 1 per cent due to large observed line widths.

aThe integrated value obtained within the interval of ±1500 km s−1from the centre.

Table 2.
Open in new tab

Summary of CO(1–0) VEGAS measurements.

IDνobszCO(1–0)ΔVSΔVaSν|$\mu L^{\prime }_{{\rm CO}}$|
(GHz)(km s−1)(Jy km s−1)Peak (mJy)(1010 K km s−1 pc2)
PJ105353.028.77123.0053 ± 0.00016738 ± 384.3 ± 1.36.2 ± 1.9170 ± 60
PJ112714.535.62482.2352 ± 0.00006736 ± 207.4 ± 2.29.3 ± 2.8178 ± 63
PJ120207.633.49702.442 ± 0.00007602 ± 215.5 ± 1.78.9 ± 2.7154 ± 55
PJ132302.933.73502.4165 ± 0.00006540 ± 174.7 ± 1.48.4 ± 2.5129 ± 46
PJ142823.949.57661.3254 ± 0.00005436 ± 251.2 ± 0.42.9 ± 0.911 ± 4
PJ160722.646.41151.4838 ± 0.00006374 ± 271.0 ± 0.32.4 ± 0.712 ± 4
PJ160917.827.09113.2567 ± 0.00014705 ± 317.6 ± 2.39.8 ± 2.9343 ± 121
IDνobszCO(1–0)ΔVSΔVaSν|$\mu L^{\prime }_{{\rm CO}}$|
(GHz)(km s−1)(Jy km s−1)Peak (mJy)(1010 K km s−1 pc2)
PJ105353.028.77123.0053 ± 0.00016738 ± 384.3 ± 1.36.2 ± 1.9170 ± 60
PJ112714.535.62482.2352 ± 0.00006736 ± 207.4 ± 2.29.3 ± 2.8178 ± 63
PJ120207.633.49702.442 ± 0.00007602 ± 215.5 ± 1.78.9 ± 2.7154 ± 55
PJ132302.933.73502.4165 ± 0.00006540 ± 174.7 ± 1.48.4 ± 2.5129 ± 46
PJ142823.949.57661.3254 ± 0.00005436 ± 251.2 ± 0.42.9 ± 0.911 ± 4
PJ160722.646.41151.4838 ± 0.00006374 ± 271.0 ± 0.32.4 ± 0.712 ± 4
PJ160917.827.09113.2567 ± 0.00014705 ± 317.6 ± 2.39.8 ± 2.9343 ± 121

Notes. |$T_{\rm A}^{*}$| to flux density using the GBT: Q-band is 1 K/1.7 Jy, Ka band is 1 K/1.6 Jy. The reported redshifts correspond to the values obtained after velocity offset corrections. The line widths reported indicate the FWHM values after correcting for the instrumental resolution. This correction was on average less than 1 per cent due to large observed line widths.

aThe integrated value obtained within the interval of ±1500 km s−1from the centre.

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