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Table 2

SPIRE/FTS line fluxes.

Transition νrest Fluxes (10-15 erg cm-2 s-1)

(GHz) NGC 34 IRASF 05189–2524 UGC 05101 NGC 5135 NGC 7130 NGC 7469

12CO J = 4–3 461.041 <10.6 ···a ···a 33.2 ± 3.7 33.0 ± 3.8 28.8 ± 3.3
12CO J = 5–4 576.268 14.3 ± 1.9 5.7 ± 1.3 11.6 ± 3.3 35.9 ± 3.9 34.2 ± 3.8 38.6 ± 4.2
12CO J = 6–5 691.473 17.7 ± 2.1 9.1 ± 1.3 14.0 ± 2.0 36.1 ± 3.7 25.6 ± 2.9 37.5 ± 3.9
12CO J = 7–6 806.652 21.3 ± 2.4 7.9 ± 1.1 10.5 ± 1.6 29.3 ± 3.1 25.5 ± 2.8 31.1 ± 3.3
12CO J = 8–7 921.800 18.2 ± 2.3 10.5 ± 1.6 10.6 ± 2.3 23.4 ± 2.7 20.8 ± 2.5 26.9 ± 3.1
12CO J = 9–8 1036.912 22.6 ± 2.6 8.9 ± 1.4 <10.1 17.5 ± 2.1 24.2 ± 2.8 21.4 ± 2.4
12CO J = 10–9 1151.985 18.3 ± 2.2 11.2 ± 1.5 12.1 ± 2.2 12.2 ± 1.8 16.9 ± 2.6 15.4 ± 2.1
12CO J = 11–10 1267.014 17.1 ± 2.1 9.3 ± 1.4 <10.0 7.1 ± 1.6 12.8 ± 2.1 13.0 ± 1.9
12CO J = 12–11 1381.995 12.5 ± 1.8 8.0 ± 1.2 <8.2 8.5 ± 1.4 10.5 ± 1.9 9.9 ± 1.7
12CO J = 13–12 1496.923 9.3 ± 1.7 8.0 ± 1.3 <10.5 <11.6 <12.1 9.1 ± 1.9
o-H2O 110–101 556.936 <6.2 <5.3 <12.9 <7.6 <14.7 <12.7
p-H2O 211–202 752.033 3.6 ± 1.0 4.5 ± 1.0 7.0 ± 1.6 5.4 ± 1.3 5.9 ± 1.6 5.4 ± 1.4
p-H2O 202–111 987.927 9.6 ± 1.7 <6.5 <10.1 11.2 ± 2.5 18.8 ± 3.0 <8.5
o-H2O 312–303 1097.365 <5.3 5.5 ± 1.3 <9.1 6.3 ± 1.8 10.5 ± 2.3 <6.0
p-H2O 111–000 1113.343 <7.4 <5.7 <9.1 8.9 ± 1.9 <10.0 12.0 ± 1.6
o-H2O 321–312 1162.912 7.7 ± 1.7 9.1 ± 1.2 9.0 ± 2.1 <6.4 <12.4 6.8 ± 2.0
p-H2O 422-413 1207.639 <5.6 4.6 ± 1.4 <9.8 <8.0 <11.3 <7.6
p-H2O 220–211 1228.789 4.1 ± 1.1 4.0 ± 1.0 <9.6 8.9 ± 1.5 12.8 ± 2.1 6.8 ± 1.7

[C i]3P13P0 492.161 7.7 ± 2.1 <6.0 <12.6 28.6 ± 2.4 16.4 ± 3.5 19.9 ± 2.7
[C i]3P23P1 809.342 9.9 ± 1.2 5.5 ± 0.7 12.8 ± 1.6 59.5 ± 1.0 26.7 ± 1.3 37.7 ± 1.3
[N ii]3P13P0 1461.132 20.7 ± 2.5 11.0 ± 1.4 31.3 ± 3.8 147.0 ± 3.3 118.3 ± 3.0 99.6 ± 3.7

Notes. Measured line fluxes and 1 σ statistical uncertainties. For non detections, we state the 3σ upper limits. The molecular transitions frequencies are from the Jet Propulsion Laboratory and the Cologne databases for molecular spectroscopy (Pickett et al. 1998; Müller et al. 2005).

(a)

Because of the higher redshift of IRASF 05189–2524 and UGC 05101, the CO J = 4 − 3 transition does not lie in the SPIRE/FTS spectral range.

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