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Table A.1

Positions for spectral extraction and source properties.

Source R.A. [hh:mm:ss] Decl. [dd:mm:ss] Optical depth rms Lbol [L] d [pc] References
IRAS 16253 16:28:21.71 −24:36:23.06 0.0045 0.16 140 Ortiz-León et al. (2018); Aso et al. (2023)
B335 19:37:01.03 07:34:07.70 0.014 1.4 165 Watson (2020); Evans et al. (2023)
HOPS 153 05:37:57.11 −07:06:57.30 0.0076 3.8 390 Tobin et al. (2020)
HOPS 370 05:35:27.50 −05:09:32.65 0.0009 315.7 390 Tobin et al. (2020)
IRAS 20126 20:14:26.10 41:13:29.46 0.0026 104 1550 Johnston et al. (2011); Reid et al. (2019)

Notes. Second and third columns give the right ascension and declination of the center of the aperture used to extract the spectrum (see Fig. A.1). The references of bolometric luminosities and distances of the central sources are given in the right-most column.

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