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Table 2:

The sample of sources observed with CHAMP+.
Source RA Dec D $L_{\rm {bol}}$ $T_{\rm {bol}}$ Class
  (J2000) (J2000) (pc) ( $L_{\rm {\odot}}$) (K)  
NGC 1333 IRAS 2 03:28:55.2 +31:14:35 250 12.7 62 0
L1551 IRS 5 04:31:34.1 +18:08:05.0 160 20 75 1
TMR 1 04:39:13.7 +25:53:21 140 3.1 133 1
HH 46 08:25:43.8 -51:00:35.6 450 16 102 1
Ced 110 IRS 4 11:06:47.0 -77:22:32.4 130 0.8 55 1
BHR 71 12:01:36.3 -65:08:44 200 11 60 0
IRAS 12496-7650 12:53:17.2 -77:07:10.6 250 24 326b 1
RCrA IRS 7Ac 19:01:55.2 -36:57:21.0 170 - - 0
Sett.a Ref. Cont. Ref. CO
NGC 1333 IRAS 2 A 1, 2, 3, 4, 5, 6, 7 vii    
L1551 IRS 5 A 2, 8, 9, 10, 11, 12 i    
TMR 1 AB 13, 14, 15, 16 i    
HH 46 ABC 1, 17, 18 ii, iii    
Ced 110 IRS 4 AB 7,19,20,21,22 iii, iv    
BHR 71 AB 17, 23, 24, 25 v    
IRAS 12496-7650 AB 26, this work iii, viii    
RCrA IRS 7Ac A 1, 7, 27, 28 iii, viii    

a Observed settings with CHAMP+. See Table 1.
b IRAS 12496-7650 is likely to be viewed face-on and thus has strong IR emission and a high $T_{\rm {bol}}$. See van Kempen et al. (2009, submitted).
c RCrA IRS 7 is a binary. Pointing was chosen to be on RCrA IRS 7A, believed to be the main embedded source, following results from van Kempen et al. (2009, submitted) and Groppi et al. (2007). RCrA IRS 7B is located 15 $^{\prime \prime }$to the east. At mid- and far-IR wavelengths, the source is heavily confused with RCrA. Therefore, no reliable $T_{\rm {bol}}$ and $L_{\rm {bol}}$ could be derived.
Continuum References: 1: Di Francesco et al. (2008) 2: Motte & André (2001) 3: Gutermuth et al. (2008) 4: Enoch et al. (2006) 5: Hatchell et al. (2007) 6: Sandell & Knee (2001) 7: Froebrich (2005) 8: Chandler & Richer (2000) 9: Reipurth et al. (2002) 10: Osorio et al. (2003) 11: Liu et al. (1996) 12: Butner et al. (1991) 13: Kenyon et al. (1994) 14: Hogerheijde et al. (1999) 15: Furlan et al. (2008) 16: Terebey et al. (1993) 17: Henning & Launhardt (1998) 18: van Kempen et al. (2009) 19: Reipurth et al. (1993) 20: Luhman et al. (2008) 21: Lehtinen et al. (2001) 22: Lehtinen et al. (2003) 23: Evans et al. (2007) 24: Bourke et al. (1997) 25: Bourke (2001) 26: Henning et al. (1993) 27: Nutter et al. (2005) 28: Groppi et al. (2007)
CO references: i: Hogerheijde et al. (1998), ii: van Kempen et al. (2009, submitted), iii: Paper I, iv: Hiramatsu et al. (2007), v: Parise et al. (2006), vi: Knee & Sandell (2000), vii: Giannini et al. (2001), viii: Giannini et al. (1999).


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