Survey of (sub)millimeter water masers in low-mass star-forming regions

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Volume 701 (September 2025)

A&A, 701 (2025) A167

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Table B.2.

GalaPy’s SED-fitting results for each source.

Source	T_MC	T_DD	Cont. peak
	[K]	[K]	[Å]
IRAS 16293	39.60 $_{- 1.61}^{+ 1.78}$ $_{-1.61}^{+1.78}$	16.92 $_{- 4.70}^{+ 10.20}$ $_{-4.70}^{+10.20}$	1.30
CARMA 7	23.82 $_{- 2.454}^{+ 3.785}$ $_{-2.454}^{+3.785}$	29.56 $_{- 2.50}^{+ 2.89}$ $_{-2.50}^{+2.89}$	1.74
YLW16A	24.62 $_{- 8.72}^{+ 12.54}$ $_{-8.72}^{+12.54}$	37.93 $_{- 11.14}^{+ 28.00}$ $_{-11.14}^{+28.00}$	1.58
Serpens FIRS	34.89 $_{- 7.01}^{+ 7.72}$ $_{-7.01}^{+7.72}$	42.07 $_{- 17.61}^{+ 15.42}$ $_{-17.61}^{+15.42}$	1.47
L1641N	51.87 $_{- 15.69}^{+ 4.95}$ $_{-15.69}^{+4.95}$	48.493 $_{- 11.54}^{+ 6.18}$ $_{-11.54}^{+6.18}$	1.00
NGC 2024	65.85 $_{- 23.18}^{+ 24.38}$ $_{-23.18}^{+24.38}$	94.04 $_{- 44.80}^{+ 62.58}$ $_{-44.80}^{+62.58}$	1.04

Notes. T_MC is the molecular cloud temperature, T_DD is the diffuse dust temperature. Both temperatures come from different gray body fits (see blue and yellow fitting lines inside the SEDs in Fig. B.1, respectively). The continuum peak (Cont. peak) is the wavelength at which the SED model peaks. Other parameters, such as stellar mass or bolometric luminosity are not taking into account as they can be strongly affected by the chosen apertures or source’s variability and are also not required for our analysis.

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