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Table 3

[O i] and [C ii] line fluxes.

Star [O i] 63 μm [O i] 145 μm [C ii]a

AB Aur 94.6 ± 5.2 3.7 ± 0.7 2.0
HD 35187 4.8 ± 2.0
HD 36112 5.6 ± 0.7 <1.1 <1.2
HD 38120 7.6 ± 0.8 0.7 ± 0.1 3.3
HD 50138 240 ± 10 6.6 ± 0.2 7.8
HD 97048 136 ± 5 5.3 ± 0.5 6.3
HD 98922 23.1 ± 1.2
HD 100453 10.2 ± 0.7 <1.2 <1.3
HD 100546 596 ± 6 21.1 ± 1.1 17.6
HD 104237 7.4 ± 0.7 <1.5 <1.5
HD 135344 B 3.6 ± 0.5 <1.2 <1.4
HD 139614 3.1 ± 0.4 <1.2 <1.3
HD 141569 A 25.3 ± 1.5
HD 142666 <50
HD 142527 3.6 ± 0.8 <2.9 <2.8
HD 144432 <5.6
HD 144668 13.3 ± 1.0 <0.9 <1.1
Oph IRS 48 30.8 ± 1.5 2.9 ± 0.6 1.2
HD 150193 3.2 ± 0.7
HD 163296 18.2 ± 0.9 <1.3 <1.3
HD 169142 8.9 ± 2.0 <2.2 <2.5
HD 179218 17.9 ± 0.9 0.95 ± 0.1 0.4b

DG Tau 153 ± 2.0 8.3 ± 0.4 7.4
HT Lup 4.0 ± 0.8
RU Lup 18.9 ± 1.2
RY Lup 5.0 ± 2.0
AS 205 21.5 ± 1.4 1.6 ± 0.4 <1.5
EM* SR 21 <5.4 <1.3 0.13
RNO 90 12.5 ± 1.0
S Cra 43.6 ± 1.3 1.8 ± 0.5 <1.7

Notes. Flux unit 10-17 W m-2. Flux uncertainties refer to 1σ error. For non detection the 3σ upper limit is given.

(a)

After subtraction of the extended emission.

(b)

[C ii] emission is only detected in the central spaxel.

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