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Table 3:

Outflow status of VeLLos and other low-luminosity embedded objects from Dunham et al. (2008).

LLO1
Spitzer ID1 Submm2 Instrument Outflow? SHARC-II3 Other names/location
(1) (2) (3) (4) (5) (6) (7)
VeLLos
65 J032900.55+311200.7 HRF71 HARP y?cLL068 y southwest of NGC1333
73 J032912.07+311301.6 HRF42 B y - NGC1333 IRAS4B
108 J034402.64+320159.5 HRF16 HARP n n in IC348 horseshoe by 107
Low luminosity objects ( Dunham et al. 2008 groups 1-4, probably embedded)
55 J032536.22+304515.8 HRF28 B y - L1448NW
56 J032539.12+304358.1 HRF29 B y - L1448C
60 J032637.46+301528.1 HRF80 HARP y y IRAS 03235+3004
63 J032738.26+301358.8 HRF39 B y - L1455 FIR1/2
64 J032832.57+311105.3 HRF74 HARP y y  
68 J032845.29+310542.0 HRF75 HARP y y 30'' southeast of the submm peak
71 J032900.55+311200.7 HRF65 HARP y y  
74 J032913.54+311358.1 HRF48 B y?a cHRF42 - NGC1333 IRAS4C
75 J032917.16+312746.4 HRF61 HARP n y N of NGC1333
78 J032923.47+313329.5 HRF58 HARP yb y N of NGC1333
80 J032951.82+313906.1 - - - - Far north of NGC1333, outside SCUBA map.
81 J033032.69+302626.5 Bolo62 HARP y?$^{\it b}$cHRF81 y NE of IRAS03271+3013 (HRF81)
84 J033120.98+304530.2 HRF77 B y - IRAS03282+3035
88 J033217.95+304947.6 HRF76 B y - IRAS03292+3039
90 J033229.18+310240.9 - HARP y y W of B1. Weak 850  $\mu {\rm m}$ emission peaks 10'' SSW.
92 J033314.38+310710.9 HRF4 B y - NW of the submm peak
93 J033316.44+310652.6 HRF4 B y - Coincident with submm peak
104 J034351.02+320307.9 HRF15 B/HARP y y IC348-SMM3c
105 J034356.52+320052.9 HRF12 B y - HH211
106 J034356.83+320304.7 HRF14 B y - IC348 mms
107 J034402.40+320204.9 HRF16 HARP n n in IC348 horseshoe by 108
109 J034421.36+315932.6 Bolo113 - -    
Low Luminosity objects observed by HARP (groups 5-6, likely not embedded)
66 J032843.58+311736.2 HRF55 HARP y?c45 n W of NGC1333
76 J032919.75+311256.9 - HARP y?c46,LL077 n SW of NGC1333 IRAS4B
77 J032920.35+311250.4 - HARP y?c46,LL076 n SW of NGC1333 IRAS4B
a The NGC1333 IRAS4C outflow status is uncertain from the R$\times $B maps (Paper III). b Flows detected by the lower linewing criterion (Sect. 3.1.2). c There is an additional Spitzer source to the north (``LL104N'') which is not classified as a LLO but appears to be the outflow driving source.

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