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Table 3

CO and H2O rotational excitation and number of emitting molecules based on the full array data.

Source Warm CO Hot CO H2O /
Trot (K) Trot (K) Trot (K)

NGC 1333-IRAS2A 310 49.1 ... ... (210) ...
NGC 1333-IRAS4A 300 49.7 (390) (49.4) 90 (0.5)
NGC 1333-IRAS4B 340 49.6 820 48.7 200 0.1
L1527 (297) (48.0) (600) (47.2) 70 (0.2)
Ced110-IRS4 (490) (47.2) (800) (46.9) 90 (0.4)
BHR71 (370) (49.4) (550) (49.0) (140) (0.4)
IRAS 15398 280 48.9 (530) (47.8) 50 (0.1)
L483 360 48.6 620 48.1 150 0.3
Serpens SMM1 350 49.9 690 49.0 150 0.1
Serpens SMM4 (260) (49.5) (690) (48.3) ... (0.1)
Serpens SMM3 290 49.6 660 48.6 130 0.1
L723 431 48.5 ... ... 130 (0.4)

L1489 471 48.1 ... ... 170 (0.8)
TMR1 470 48.3 ... ... 170 (0.4)
TMC1A 420 47.9 ... ... ... ...
TMC1 350 48.1 510 47.7 160 0.4
HH46 310 49.2 (630) (48.3) 50 (0.1)
RNO91 (250) (47.8) ... ... (100) ...

Notes.Rotational temperatures and corresponding numbers of emitting molecules measured using less than 5 points are written in brackets (see Figs. F.1 and F.2). Non-detections are marked with ellipsis dots (...). In case of L723, L1489, TMR1, and TMC1A one component fit is used.

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