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Table 3

Herschel/PACS [C ii] 157μm line observations and fluxes.

Galaxy Program Line OD(a) OBSID Map area V ΔV(b) Total flux Flux in CO(1–0) area(c)

Haro 11 DGS [C ii] 409 1342199236 51′′ × 51′′ 6193 160 6.48 ± 0.02 5.28 ± 0.01
[O i] 409 1342199237 51′′ × 51′′ 6184 140 6.45 ± 0.10 5.34 ± 0.02
Mrk 1089 DGS [C ii] 690 1342217859 51′′ × 51′′ 4020 8.84 ± 0.14 4.08 ± 0.01
[O i] 690 1342217861 53′′ × 53′′ 4022 80 2.83 ± 0.06 1.48 ± 0.01
Mrk 930 DGS [C ii] 607 1342212520 51′′ × 51′′ 5486 100 2.31 ± 0.55 1.40 ± 0.01
[O i] 607 1342212518 47′′ × 47′′ 5488 120 1.58 ± 0.10 0.89 ± 0.01
NGC 4861 SHINING [C ii] 549 1342208902 1.4′ × 3.6′ 801 6.96 ± 0.26 1.39 ± 0.01
[O i] 745 1342221887 47′′ × 47′′ 799 40 1.95 ± 0.07 1.23 ± 0.01
NGC 625 SHINING [C ii] 754 1342222218 1.4′ × 1.4′ 383 16.9 ± 0.15 4.07 ± 0.01
[O i] 754 1342222217 47′′ × 47′′ 388 100 4.85 ± 0.07 1.25 ± 0.10
UM 311 DGS [C ii] 621 1342213288 1.2′ × 1.2′ 1698 9.98 ± 0.17 2.23 ± 0.05
[O i] 621 1342213291 1.0′ × 1.0′ 1683 75 3.28 ± 0.14 1.28 ± 0.28

Notes. Fluxes are given in 10-16 W m-2 and velocities in km s-1 in the LSR reference frame. The uncertainties on the flux quoted here are those associated with the line fitting and do not take into account the 30% calibration errors. (a) Observation Day of the Herschel mission. (b) Intrinsic broadening of the line in km s-1. (c) The aperture over which the fluxes are integrated are shown in Fig. 5.

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