Revisiting G29.862–0.0044: A jet cavity disrupted by an outflow in a likely young stellar object wide binary system

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Table C.1

Mid-IR, submillimetre and millimetre fluxes ƒ_λ in the direction of YSO-G29.

Source	Band	ƒ_λ ± ∆ƒ_λ
	[µm]	[Jy]
BGPS G029.863–00.048	1100	1.90 ± 0.2
AGAL 029.862–00.044	870	13.1 ± 2.2
HIGALPL029.8647–0.0450	500	49.1 ± 2.0
HIGALPM029.8643–0.0447	350	117.4 ± 2.1
HIGALPS029.8636–0.0451	250	270.0 ± 1.4
HIGALPR029.8632–0.0437	160	292.7 ± 1.2
HIGALPB029.8624–0.0437	70	382.2 ± 0.7
allWISE J184559.51–024506.1	22	40.0 ± 0.1

Notes. The WISE 22 µm flux (ƒ₂₂) was calculated from the magnitude m₂₂ = −1.70 ± 0.03 of the allWISE Catalog, using the formula $f_{22} = f_{0} 10^{- 2.5 / m_{22}}$ ${f_{22}} = {f_0}{10^{ - 2.5/{m_{22}}}}$ , with the zero point ƒ₀ = 8.36 Jy reported in the VOSA SED Analyzer (Bayo et al. 2008).

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