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Table 2

Observed line parameters.

Galaxy Line νobs S(CO)a Vb ΔVFWHM /1010 S60 S100c log LFIR F(1.4 GHz)d
[GHz] [Jy  km s-1] [km s-1] [km s-1] [K  km s-1  pc2] [Jy] [Jy] [L⊙] [mJy]
G1 CO(1–0) 88.534 7.5  ±  1.4 –29.  ±  33. 398.  ±  98. 3.58 0.68 0.77 12.54
G1 CO(3–2) 265.588 6.2  ±  2.0 –38.  ±  21. 148.  ±  62. 0.33 0.68 0.77 12.54
G2 CO(1–0) 83.228  < 1.2  < 0.9 0.67 1.13 12.84 4.09
G2 CO(3–2) 249.672  < 3.2  < 0.3 0.67 1.13 12.84 4.09
G3 CO(1–0) 92.513 2.3  ±  0.5 –168.  ±  41. 314.  ±  66. 0.73 1.18 1.55 12.59 2.16
G3 CO(3–2) 277.525 9.6  ±  0.9 –185.  ±  37. 498.  ±  47. 0.33 1.18 1.55 12.59 2.16
G4 CO(1–0) 94.253 6.5  ±  0.7 248.  ±  24. 434.  ±  52. 1.67 1.23 1.52 12.50 3.09
G5 CO(1–0) 94.718 3.4  ±  0.6 178.  ±  20. 240.  ±  44. 0.83 1.36 1.54 12.51 25.5
G6 CO(1–0) 90.409  < 1.7  < 0.7 0.72 0.69 12.44 3.0
G7 CO(1–0) 84.758  < 1.7  < 1.2 1.18 1.20 12.94
G7 CO(3–2) 254.262  < 4.5  < 0.3 1.18 1.20 12.94
G8 CO(1–0) 93.186 3.4  ±  0.7 –135.  ±  32. 301.  ±  82. 1.0 0.99 1.43 12.49 5.96
G9 CO(1–0) 92.439 2.1  ±  0.5 469.  ±  30. 290.  ±  72. 0.67 0.94 1.10 12.48 3.85
G10 CO(1–0) 91.850  < 1.7  < 0.6 0.82 1.04 12.46 7.44
G11 CO(1–0) 89.985 4.5  ±  0.6 85.  ±  30. 428.  ±  66. 1.86 0.84 1.15 12.58 2.77
G12 CO(1–0) 92.811 7.7  ±  0.8 –5.  ±  21. 430.  ±  44. 2.33 1.48 1.99 12.68 5.67
G13 CO(1–0) 88.875  < 1.7  < 0.8 1.24 2.13 12.84 95.
G14 CO(1–0) 92.811 2.4  ±  0.7 –10.  ±  70. 420.  ±  140. 0.73 1.06 1.43 12.53
G15 CO(1–0) 88.330 6.9  ±  1.1 200.  ±  34. 433.  ±  73. 3.38 1.22 1.27 12.79
G16 CO(1–0) 86.932  < 1.2  < 0.7 0.58 1.14 12.63 40.3
G17 CO(1–0) 82.337 8.3  ±  0.9 478.  ±  19. 363.  ±  46. 7.14 0.32 0.64 12.59
G17 CO(3–2) 246.997 12.9  ±  2.0 500.  ±  22. 303.  ±  56. 1.24 0.32 0.64 12.59
G18 CO(1–0) 85.008 7.6  ±  0.7 253.  ±  32. 651.  ±  64. 5.18 0.61 1.22 12.75 2.3
G18 CO(3–2) 255.012  < 4.5  < 0.3 0.61 1.22 12.75 2.3
G19 CO(2–1) 159.874 1.5  ±  0.4 –28.  ±  30. 225.  ±  63. 0.40 0.53  < 0.44 12.78 6.87
G20 CO(2–1) 154.723  < 1.4  < 0.5 0.23 0.57 12.70 8.82
G21 CO(1–0) 88.670  < 1.7  < 0.8 0.71 0.76 12.54 7.78
G21 CO(3–2) 265.997  < 4.5  < 0.2 0.71 0.76 12.54 7.78
G22 CO(1–0) 87.129 1.5  ±  0.3 –41.  ±  26. 196.  ±  44. 0.82 0.62 0.99 12.62 1.59
G22 CO(3–2) 261.373  < 2.3  < 0.1 0.62 0.99 12.62 1.59
G23 CO(2–1) 159.763 4.7  ±  0.7 91.  ±  25. 370.  ±  60. 1.27 0.23 0.62 12.61 1.76
G24 CO(1–0) 85.134  < 0.8  < 0.6 0.52 1.83 12.80
G24 CO(3–2) 255.388  < 4.5  < 0.3 0.52 1.83 12.80
G25 CO(1–0) 87.859  < 1.2  < 0.6 0.40 1.06 12.49
G25 CO(3–2) 263.564  < 9.0  < 0.5 0.40 1.06 12.49
G26 CO(1–0) 86.410  < 1.2  < 0.7 0.46 0.83 12.54 1.36
G26 CO(3–2) 259.217  < 4.5  < 0.3 0.46 0.83 12.54 1.36
G27 CO(2–1) 146.373 2.1  ±  0.6 –126.  ±  34. 231.  ±  90. 0.95 0.43  < 0.94 13.11 2.7
G28 CO(2–1) 144.719  < 1.9  < 0.9 0.60 1.26 13.28 7000
G29e CO(1–0) 84.170 1.9  ±  0.3 –6.  ±  10. 270.  ±  20. 1.42 0.74 0.83 12.78 16000
G30f CO(1–0) 91.123 3.8  ±  0.4 185.  ±  20. 270.  ±  30. 1.40 1.45 1.82 12.75 5.49

Notes. Quoted errors are statistical errors from Gaussian fits. The systematic calibration uncertainty is 10%.

(a)

The upper limits are at 3σ with an assumed ΔV = 300  km s-1.

(b)

The velocity is relative to the optical redshift given in Table 1.

(c)

The 60 and 100 μm   fluxes are from NED (http://nedwww.ipac.caltech.edu/).

(d)

From the FIRST catalog (http://sundog.stsci.edu/). Errors are typically 0.14 mJy.

(e)

From Wink et al. (1997).

(f)

From Solomon et al. (1997).

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