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Table A.2

Line fluxes of Class 0 and I sources in 10-20 W cm-2.

Species Trans. λlab (μm) Full array flux (10-20 W cm-2)
IRAS2A IRAS4A L1527 CedIRS4 BHR71 IRAS 15398 L483 SerSMM4
CO 14–13 185.999 1.65 ± 0.28 9.42 ± 0.08 0.52 ± 0.14 0.14 ± 0.01 7.79 ± 0.15 4.19 ± 0.10 1.31 ± 0.02 5.75 ± 0.10
CO 16–15 162.812 2.11 ± 0.38 8.00 ± 0.09 0.57 ± 0.07 0.16 ± 0.01 ... 4.24 ± 0.12 1.10 ± 0.02 ...
CO 18–17 144.784a 2.76 ± 0.29 6.74 ± 0.09 0.51 ± 0.08 0.24 ± 0.02 8.54 ± 0.16 3.11 ± 0.09 1.16 ± 0.05 3.68 ± 0.12
CO 22–21 118.581 ... 3.12 ± 0.27 0.31 ± 0.11 <0.20 ... 2.21 ± 0.20 0.61 ± 0.02 ...
CO 23–22 113.458b 3.16 ± 0.37 ... 0.95 ± 0.12 0.59 ± 0.02 ... 3.56 ± 0.14 2.55 ± 0.07 ...
CO 24–23 108.763 ... 3.92 ± 0.28 <0.26 0.20 ± 0.03 5.65 ± 0.33 1.13 ± 0.11 0.97 ± 0.04 1.17 ± 0.18
CO 29–28 90.163c <0.30 ... 0.10 ± 0.02 ... ... 0.42 ± 0.04 0.59 ± 0.04 ...
CO 30–29 87.190 <0.67 0.97 ± 0.12 <0.33 <0.35 ... 0.36 ± 0.03 0.41 ± 0.05 ...
CO 32–31 81.806 <0.37 0.45 ± 0.05 <0.21 0.16 ± 0.04 ... 0.26 ± 0.04 0.43 ± 0.05 ...
CO 33–32 79.360 <0.54 0.47 ± 0.09 0.13 ± 0.03 0.14 ± 0.05 ... 0.40 ± 0.05 0.60 ± 0.07 ...
CO 36–35 72.843d <0.42 <0.09 <0.36 <0.08 0.89 ± 0.08 <0.16 0.19 ± 0.04 0.40 ± 0.09
o-H2O 221–212 180.488d 2.72 ± 0.32 ... 0.11 ± 0.04 ... ... ... 0.50 ± 0.02 ...
o-H2O 212–101 179.527 3.13 ± 0.34 13.03 ± 0.08 0.77 ± 0.06 <0.13 ... 2.18 ± 0.06 1.45 ± 0.02 ...
o-H2O 303–212 174.626 4.88 ± 0.47 10.54 ± 0.11 0.61 ± 0.07 0.24 ± 0.01 ... 1.93 ± 0.09 1.30 ± 0.02 ...
p-H2O 313–202 138.528 2.60 ± 0.33 6.91 ± 0.08 0.39 ± 0.07 0.12 ± 0.02 ... 1.10 ± 0.08 1.00 ± 0.02 ...
p-H2O 404–313 125.354d <0.31 ... 0.17 ± 0.06 ... ... ... 0.59 ± 0.03 ...
o-H2O 221–110 108.073 3.84 ± 0.51 10.23 ± 0.21 0.78 ± 0.17 0.26 ± 0.04 4.88 ± 0.22 1.82 ± 0.19 1.33 ± 0.05 2.16 ± 0.17
p-H2O 322–211 89.988 <0.30 2.37 ± 0.12 0.10 ± 0.03 0.13 ± 0.04 ... 0.30 ± 0.02 0.61 ± 0.04 ...
o-H2O 716–707 84.767 <0.44 <0.14 <0.36 <0.28 ... <0.10 0.14 ± 0.05 ...
p-H2O 615–524 78.928 <0.65 <0.30 <0.41 <0.48 ... <0.13 <0.54 ...
o-H2O 423–312 78.742c <0.65 2.03 ± 0.19 0.33 ± 0.03 0.24 ± 0.06 ... ... 1.34 ± 0.08 ...
o-H2O 707–616 71.947e <0.62 0.78 ± 0.08 <0.26 ... 0.32 ± 0.04 ... 0.60 ± 0.05 <0.26
o-H2O 818–707 63.324 <0.77 <0.16 <0.47 <0.57 0.50 ± 0.11 <0.19 0.41 ± 0.05 <0.44
O i 145.525 <0.2 0.42 ± 0.10 1.07 ± 0.10 0.87 ± 0.10 1.33 ± 0.12 1.13 ± 0.11 0.78 ± 0.10 2.36 ± 0.06
O i 63.184 9.01 ± 1.83 2.33 ± 0.28 11.29 ± 0.30 8.92 ± 0.46 20.91 ± 0.53 19.07 ± 0.47 8.16 ± 0.62 23.21 ± 0.41

Notes.NGC 1333-IRAS4B and Serpens SMM1 fluxes are published separately in Herczeg et al. (2012) and Goicoechea et al. (2012), respectively. CO 31–30 and OH 84.6 μm fluxes are presented in Wampfler et al. (2013). NGC 1333-IRAS2A and NGC 1333-IRAS4A full PACS range fluxes will appear in Karska et al. (in prep.), but IRAS2A central spaxel only fluxes were listed in Visser et al. (2012). Non-observed lines are marked with ellipsis dots (...). The uncertainties are 1σ measured in the continuum on both sides of each line; calibration uncertainty of 30% of the flux should be included for comparisons with other modes of observations or instruments. 1σ upper limits calculated using wavelength dependent values of full-width high maximum for a point source observed with PACS are listed for non-detections.

(a)

The baseline from one side is affected by p-H2O 413–322 line at 144.518 μm, which falls in the edge of the scan.

(b)

A blend with the o-H2O 414–303 line at 113.537 μm.

(c)

Lines at the edges of the scans, for many cases not possible to measure. Selected objects were observed in dedicated scan for the CO 29–28 line.

(d)

Lines observed in dedicated scans only for selected objects.

(e)

The line falls in the leakage region of PACS and therefore the flux is less reliable.

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