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Table 2

Survey positions and fit results.

PACS(1) HIFI(2) PACS-HIFI(3)
Position Offset(4) I[1670 GHz]peak Diam. I[557 GHz] VLSR ΔV log[N(H2O)] log(nT)
(′′,′′) (K km s-1) (′′) (K km s-1) (km s-1) (km s-1) (cm-2) (cm-3 K)

N1333I2-B (−103, +23) 3.5 (0.6) 30 (4.8) 6.34 (0.04) −0.14 (0.04) 11.3 (0.08) 13.4 (0.2) 9.2 (0.1)
N1333I2-R (+67, −17) 5.5 (0.8) 22 (2.3) 7.15 (0.06) 14.0 (0.07) 14.2 (0.1) 13.3 (0.2) 9.4 (0.1)
N1333I3-B2 (+20, −50) 1.7 (0.2) 27 (3.1) 2.65 (0.07) 2.0 (0.3) 20.5 (0.6) 12.8 (0.2) 9.4 (0.1)
N1333I3-B1 (+20, −20) 5.9 (1.4) 18 (2.9) 5.35 (0.08) −4.6 (0.2) 25.4 (0.4) 13.1 (0.1) 9.7 (0.1)
N1333I4A-B (−6, −19) 14.0 (2.9) 34 (6.8) 15.0 (0.1) 1.3 (0.06) 17.4 (0.1) 13.5 (0.1) 9.1 (0.1)
N1333I4A-R (+13, +25) 9.3 (1.2) 28 (3.5) 7.76 (0.07) 13.3 (0.09) 19.3 (0.2) 13.4 (0.1) 9.7 (0.1)
HH211-R (−37, +15) 2.8 (0.6) 28 (5.8) No data
HH211-C (0,0) 11.7 (1.6) 17 (1.7) 6.53 (0.02) 11.5 (0.07) 41.4 (0.1) 13.2 (0.1) 9.8 (0.1)
HH211-B (+37, −15) 7.7 (1.0) 14 (1.3) 2.33 (0.06) 6.2 (0.3) 20.0 (0.7) 12.8 (0.1) 10.1 (0.1)
IRAS04166-R (−20, −35) No data No data 0.27 (0.05) 13.0 (0.7) 9.1 (2.4)
IRAS04166-B (+20, +35) Bad fit Bad fit 0.53 (0.04) 0.0 (0.4) 10.0 (1.1) 12.4 (0.3) 9.2 (0.1)
L1551-B (−255, −255) Bad fit Bad fit 0.36 (0.03) −3.2 (0.2) 5.9 (0.5) 12.3 (0.2) 9.2 (0.1)
L1551-R (+150, +20) 1.3 (0.2) 13 (1.4) 0.58 (0.04) 7.8 (0.3) 5.7 (0.6) 12.4 (0.1) 9.7 (0.1)
L1527-B (+40, +10) No data No data 0.93 (0.07) 9.3 (0.8) 20.3 (2.1)
HH1 (−30, +55) 2.9 (0.3) 13 (1.0) No data
HH2 (+60, −80) 3.5 (0.5) 30 (4.4) 2.4 (0.05) 9.8 (0.2) 17.7 (0.4) 12.9 (0.1) 9.7 (0.1)
HH212-B (−15, −35) 0.4 (0.1) 37 (13) 0.76 (0.04) 1.1 (0.2) 8.4 (0.5) 12.3 (0.1) 9.5 (0.1)
HH212-C (0,0) 2.5 (0.4) 18 (1.9) 2.3 (0.07) 2.6 (0.4) 23.2 (0.8) 12.6 (0.1) 9.8 (0.1)
HH25-C (0,0) 12.5 (0.9) 14 (0.7) 5.2 (0.06) 12.4 (0.09) 16.6 (0.3) 13.1 (0.1) 9.9 (0.1)
HH25-R (+36, −57) 3.2 (0.4) 36 (4.4) 4.9 (0.07) 11.2 (0.04) 6.9 (0.09) 13.1 (0.2) 9.5 (0.1)
HH111-B (−170, +21) 0.3 (0.1) 34 (11) Bad fit
HH111-C (0,0) 2.0 (0.3) 12 (1.3) 0.54 (0.05) 9.3 (0.6) 14.6 (1.6) 12.4 (0.1) 9.9 (0.1)
HH46-R (−40, −20) 0.8 (0.2) 35 (7.3) No data
HH46-B (−10,0) No data No data 1.54 (0.06) 10.8 (0.4) 20.0 (1.0)
BHR71-R (−39, +140) 1.9 (0.2) 46 (5.5) 7.0 (0.08) 3.0 (0.1) 16.1 (0.2) 13.4 (0.5) 8.8 (0.4)
BHR71-B (+42, −100) 2.7 (0.3) 32 (3.4) 3.4 (0.06) −6.4 (0.07) 7.5 (0.2) 13.6 (0.7) 8.9 (0.6)
HH54B(5) (2,4) 8.8 (0.4) 22 (0.8) 10.6 (0.07) −6.6 (0.05) 14.5 (0.1) 13.3 (0.1) 9.6 (0.1)
IRAS16293-B (+72, −56) 0.1 (0.2) 13 (16) 1.6 (0.05) 1.7 (0.06) 3.6 (0.1)
IRAS16293-R (+72, +49) 0.8 (0.1) 38 (6.2) 6.2 (0.04) 8.2 (0.03) 9.7 (0.07) 14.1 (0.2) 7.8 (0.2)
L483-B (−60, +30) 0.4 (0.2) 21 (6.3) 0.70 (0.05) 1.4 (0.5) 12.7 (1.0) 13.6 (0.6) 8.0 (0.5)
S68N-B (−12, +24) 6.9 (0.5) 23 (1.6) 4.5 (0.07) 6.1 (0.1) 15.5 (0.4) 13.2 (0.1) 9.6 (0.1)
S68N-C (0,0) 8.9 (1.2) 31 (3.6) 10.9 (0.07) 9.1 (0.05) 17.6 (0.2) 13.2 (0.1) 9.8 (0.1)
SERSMM1-B (−18, +30) 8.8 (0.8) 21 (1.9) 4.5 (0.09) 10.0 (0.2) 22.6 (0.9) 13.2 (0.1) 9.7 (0.1)
SERSMM4-B (−60, +30) 0.4 (0.2) 18 (10) 1.9 (0.03) 5.0 (0.04) 5.7 (0.1) 13.9 (0.2) 7.6 (0.4)
SERSMM4-R(6) (+30, −60) 0.4 (0.1) 44 (21) 1.9 (0.05) 11.6 (0.2) 13.2 (0.6) 13.1 (0.6) 8.6 (0.5)
B335-B (+30,0) No data No data Bad fit
N7129FIR2-R (+50, −50) 0.3 (0.2) 19 (7.1) Bad fit
CEPE-B (−12, −20) 71.2 (7.7) 15 (1.1) 26.2 (0.2) −27.4 (0.2) 44.6 (0.4) 13.9 (0.1) 10.0 (0.1)
CEPE-R (+8, +20) 27.7 (3.4) 22 (2.1) No data

Notes.(1) PACS results from Gaussian fits to the radial profiles of integrated intensity with rms uncertainty values in parenthesis. The origin of the profile is the emission centroid and the diameter is the FWHM of the fitted Gaussian (without correction for the 13′′ telescope beam); (2) HIFI results from Gaussian fits to the spectra with rms uncertainty values in parenthesis. ΔV represents the FWHM of the emission; (3) results from the analysis of the combined PACS and HIFI data toward the emission peak and with a resolution of 13′′, see Sect. 7.2; (4) offsets are given with respect to the central position in Table 1; (5) data previously published by Bjerkeli et al. (2011); (6) position excluded from sample analysis due to dubious outflow origin.

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