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Table 1

The WILL survey source sample.

Name   RA (J2000) Dec (J2000) d νLSR a L bol b b T bol b α IR b M env b Classc Other namesd
  (h m s) (°′′′) (pc) (km s-1) (L⊙) (%) (K) (M⊙)
AQU 01e   18:29:03.82 −01:39:01.5 436 +7.4 2.6 11.8 24 − 3.15 0 Aqu-MM2
AQU 02e   18:29:08.60 −01:30:42.8 436 +7.5 9.0 7.8 33 − 2.17 0 Aqu-MM4, IRAS 18265-0132
AQU 03e   18:30:25.10 −01:54:13.4 436 +7.1 3.5 5.3 246 0.7 0.79 II Aqu-MM6, IRAS 18278-0156
AQU 04e   18:30:28.63 −01:56:47.7 436 +7.6 6.5 4.5 320 0.5 1.21 I Aqu-MM7, IRAS 18278-0158
AQU 05   18:30:29.03 −01:56:05.4 436 +7.3 2.4 9.2 37 1.4 0.68 0 Aqu-MM10
AQU 06   18:30:49.94 −01:56:06.1 436 +8.3 1.3 8.2 40 1.9 0.59 0 Aqu-MM14
CHA 01   11:09:28.51 −76:33:28.4 150 +4.9 1.6 − 189 1.6 − II GM Cha, ISO-ChaI 192, CaINa2
CHA 02   12:59:06.58 −77:07:39.9 178 +3.0 1.8 0.6 236 1.3 − I ISO-ChaII 28, IRAS 12553-7651
CRA 01   19:02:58.67 −37:07:35.9 130 +5.6 2.4 2.2 55 1.7 0.49 0 ISO-CrA 182, IRAS 18595-3712
OPH 01   16:26:59.10 −24:35:03.3 125 +3.8 4.3 − 69 2.0 0.17 II+PDR? ISO-Oph 90, WL 22
OPH 02   16:32:00.99 −24:56:42.6 125 +4.2 8.6 0.1 80 1.8 0.09 I ISO-Oph 209, Oph-emb 10
PER 01   03:25:22.32 +30:45:13.9 235 +4.1 4.5 2.7 44 2.3 0.89 0 L1448 IRS2, Per-emb 22
PER 02   03:25:36.49 +30:45:22.2 235 +4.5 9.2 1.7 54 2.6 3.48 0 L1448 N(A), L1448 IRS3, Per-emb 33
PER 04   03:26:37.47 +30:15:28.1 235 +5.2 1.2 4.2 60 1.2 0.29 0 IRAS 03235+3004, Per-emb 25
PER 05   03:28:37.09 +31:13:30.8 235 +7.3 11.1 0.6 84 2.2 0.36 I NGC 1333 IRAS1, Per-emb 35
PER 06   03:28:57.36 +31:14:15.9 235 +7.3 7.1 − 82 1.5 0.34 I NGC 1333 IRAS2B, Per-emb 36
PER 07   03:29:00.55 +31:12:00.8 235 +7.4 0.7 3.9 37 2.1 0.32 0 Per-emb 3
PER 08   03:29:01.56 +31:20:20.6 235 +7.7 16.9 1.3 129 2.5 0.83 I Per-emb 54, NGC 1333 IRAS6
PER 09   03:29:07.78 +31:21:57.3 235 +7.5 22.7 − 129 2.6 0.26 I IRAS 03260+3111(W), Per-emb 50
PER 10   03:29:10.68 +31:18:20.6 235 +8.7 6.0 2.2 47 1.9 1.10 0 NGC 1333 IRAS7, Per-emb 21
PER 12   03:29:13.54 +31:13:58.2 235 +7.8 1.1 8.7 31 2.4 1.20 0 NGC 1333 IRAS4C, Per-emb 14
PER 13   03:29:51.82 +31:39:06.0 235 +8.0 0.7 5.0 40 3.5 0.49 0 IRAS 03267+3128, Per-emb 9
PER 14   03:30:15.14 +30:23:49.4 235 +6.2 1.8 1.6 88 1.8 0.15 I IRAS 03271+3013, Per-emb 34
PER 15   03:31:20.98 +30:45:30.1 235 +6.9 1.6 5.8 36 1.2 1.16 0 IRAS 03282+3035, Per-emb 5
PER 16   03:32:17.96 +30:49:47.5 235 +7.0 1.1 13.3 29 1.0 2.88 0 IRAS 03292+3039, Per-emb 2
PER 17   03:33:14.38 +31:07:10.9 235 +6.6 0.2 − 71 2.4 1.94 I B1 SMM3, Per-emb 6
PER 18   03:33:16.44 +31:06:52.5 235 +6.6 0.5 − 38 1.6 1.59 0 B1d, Per-emb 10
PER 19   03:33:27.29 +31:07:10.2 235 +6.8 1.1 1.7 93 1.9 0.29 I B1 SMM11, Per-emb 30
PER 20   03:43:56.52 +32:00:52.8 235 +8.9 2.2 6.3 27 0.7 1.93 0 IRAS 03407+3152, HH 211, Per-emb 1
PER 21   03:43:56.84 +32:03:04.7 235 +8.8 1.9 3.8 35 1.5 1.54 0 IC348 MMS, Per-emb 11
PER 22   03:44:43.96 +32:01:36.2 235 +9.8 2.4 3.4 45 0.9 0.70 0 IRAS 03415+3152, Per-emb 8
SCO 01   16:46:58.27 −09:35:19.8 125 +3.6f 0.5 0.6 201 0.9 0.10 II IRAS 16442-0930, L260 SMM1
SERS 01   18:29:37.70 −01:50:57.8 436 +8.2 17.4 3.9 46 1.3 1.10 0 IRAS 18270-0153, SerpS-MM1
SERS 02   18:30:04.13 −02:03:02.1 436 +7.8 73.2 4.6 34 2.5 8.44 0 SerpS-MM18
TAU 01   04:19:58.40 +27:09:57.0 140 +6.8 1.5 3.3 136 1.4 0.27 I IRAS 04169+2702
TAU 02   04:21:11.40 +27:01:09.0 140 +6.6 0.5 0.8 282 0.5 − I IRAS 04181+2654A
TAU 03   04:22:00.60 +26:57:32.0 140 +7.4f 0.4 0.2 196 1.0 − II IRAS 04189+2650(W)
TAU 04   04:27:02.60 +26:05:30.0 140 +6.3 1.4 1.5 161 0.8 0.64 I DG TAU B
TAU 06   04:27:57.30 +26:19:18.0 140 +7.2 0.6 2.7 80 0.8 0.09 I HH31 IRS 2, IRAS 04248+2612
TAU 07   04:29:30.00 +24:39:55.0 140 +6.3f 0.6 0.2 169 0.9 − II HH 414, IRAS 04264+2433
TAU 08   04:32:32.00 +22:57:26.0 140 +5.5g 0.5 1.2 300 0.5 0.18 II L1536 IRS, IRAS 04295+2251
TAU 09   04:35:35.30 +24:08:19.0 140 +5.5 1.0 1.7 82 1.4 0.06 II L1535 IRS, IRAS 04325+2402
W40 01   18:31:09.42 −02:06:24.5 436 +4.9 13.3 7.4 40 2.3 1.97 0+PDR W40-MM3
W40 02   18:31:10.36 −02:03:50.4 436 +4.8 32.6 3.7 46 4.6 2.25 0 W40-MM5
W40 03   18:31:46.54 −02:04:22.5 436 +6.4 8.3 20.6 15 − 3.37 PS?+PDR W40-MM26
W40 04   18:31:46.78 −02:02:19.9 436 +6.7 6.1 9.4 16 − 1.69 PS?+PDR W40-MM27
W40 05   18:31:47.90 −02:01:37.2 436 +6.5 5.9 27.3 14 − 1.97 PS?+PDR W40-MM28
W40 06   18:31:57.24 −02:00:27.7 436 +6.6 4.1 2.2 33 − 0.31 PS?+PDR W40-MM34
W40 07   18:32:13.36 −01:57:29.6 436 +7.4 3.6 3.3 36 0.9 0.25 0 W40-MM36

Notes.

(a)

From Gaussian fits to the C18O J = 3−2 observations (see Table A.9).

(b)

Calculated as discussed in Sect. A.7.

(c)

Evolutionary classification, see Sect. A.7 for details of the determination. PS = pre-stellar, PDR = narrow, bright 12CO J = 10−9 emission consistent with a photon-dominated region.

(d)

First additional names for Aquila, Serpens South and W40 are from Maury et al. (2011), “-emb” names from Enoch et al. (2009).

(e)

Sources off-centre in beam. Peak coordinates in PACS maps used for extraction of ground-based data: AQU 01 18:29:03.61 −01:39:05.6; AQU 02 18:29:08.20 −01:30:46.6; AQU 03 18:30:24.69 −01:54:11.0; AQU 04 18:30:29.32 −01:56:42.4.

(f)

From Gaussian fits to the 13CO (J = 3−2) observations as C18O is not detected.

(g)

Taken from Caselli et al. (2002).

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