The structured environments of embedded star-forming cores - PACS and SPIRE mapping of the enigmatic outflow source UYSO 1

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Table 2:

Point source fluxes (without colour correction). The overall uncertainties are 20% for all wavelengths except for 160 $\mu$ m (25%).
ID	$F_\nu$ [ Jy]	$F_\nu$ [ Jy]	$F_\nu$ [ Jy]	$F_\nu$ [ Jy]
	(24 $\mu$ m)	(70 $\mu$ m)	(100 $\mu$ m)	(160 $\mu$ m)
UYSO 1^a	-	168	239	193
LDN 1657A-1	0.07	0.6	0.8	1.5
LDN 1657A-2	0.10	0.2	0.2	<0.2
LDN 1657A-3	0.09	0.5	0.9	1.3
LDN 1657A-4	<0.002	0.3	1.1	2.6
LDN 1657A-5	0.04	0.4	0.5	0.7

Notes. ^(a) Photometry obtained with large aperture (see Sect. 3.1). The corresponding SPIRE fluxes used for Fig. 3 are: (91.1 $\pm$ 13.7) Jy (250 $\mu$ m), (32.5 $\pm$ 4.9) Jy (350 $\mu$ m), and (11.2 $\pm$ 1.7) Jy (500 $\mu$ m).

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