Multi-wavelength observations of the young binary system Haro 6-10: The case of misaligned discs

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Table A.1

SED with photometry from the literature (references in the last column) of Haro 6-10 N and Haro 6-10 S.

λ	Flux (N+S)	Flux (S)	Flux (N)	Instrument	Beam size	Date	Reference
[μm]	[mJy]	[mJy]	[mJy]		[″]

0.593	0.438 ± 0.001	0.437 ± 0.001	0.001 ± 0.000	HST	0.5	Nov. 1998	this work
0.792	2.374 ± 0.004	2.365 ± 0.004	0.009 ± 0.000	HST	0.5	Nov. 1998	this work
1.650	39.2 ± 3.4	37.0 ± 3.4	2.1 ± 0.2	NACO	0.2	Dec. 2003	this work
2.160	166.3 ± 12.6	132.9 ± 12.2	33.4 ± 3.1	NACO	0.2	Dec. 2003	this work
12	16 600 ± 2200	–	–	IRAS			Chandler et al. (1998)
25	37 600 ± 3200	–	–	IRAS			Chandler et al. (1998)
60	58 400 ± 9700	–	–	IRAS			Chandler et al. (1998)
100	47 000 ± 11 000	–	–	IRAS			Chandler et al. (1998)
350	3420 ± 250	–	–	JCMT/UKT14	19		Dent et al. (1998)
443	2370 ± 500	–	–	JCMT/UKT14	19	Sep. 1991	Chandler et al. (1998)
790	571 ± 44	–	–	JCMT/UKT14	16	Sep. 1991	Chandler et al. (1998)
1104	179 ± 17	–	–	JCMT/UKT14	19	Sep. 1991	Chandler et al. (1998)
1260	99 ± 30	–	–	JCMT/UKT14	21	Sep. 1991	Chandler et al. (1998)
1300	90.5 ± 4.5	46.7 ± 3.2	43.8 ± 3.1	PdBI	0.9 × 0.6		Guilloteau et al. (2011)
2700	19.6 ± 1.0	9.1 ± 0.7	10.5 ± 0.7	PdBI			Guilloteau et al. (2011)
3400	11.9 ± 1.7	–	–	OVRO	6	1993/1994	Hogerheijde et al. (1997)
36 000	–	1.10	0.10	VLA	0.29 × 0.26	March 2002	Reipurth et al. (2004)

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