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Table B.1.

Flux density in Janskys (Jy) at different wavelengths with associated uncertainties. The SED is displayed in Fig. 1 complemented with ALMA observations. I19: Neugebauer et al. (2019), S04: Smith et al. (2004), F07: Fouqué et al. (2007), K09: Kervella et al. (2009), M24: Marton et al. (2024), H24: Herschel Team (2024).

Inst. λeff Flux density References
System (μm) (Jy)
Johnson 0.44 72.6 ± 2.0 F07
Johnson 0.55 181 ± 5.1 F07
Cousins 0.75 274 ± 7.7 F07
2MASS 1.22 382 ± 18 F07
2MASS 1.65 342 ± 16 F07
2MASS 2.16 269 ± 13 F07
COBE 3.50 127 ± 17 S04
IRAC 3.55 117 ± 4 K09
IRAC 4.49 68 ± 2 K09
COBE 4.90 60 ± 10 S04
IRAC 5.73 46.3 ± 1.4 K09
IRAC 7.87 29.1 ± 0.9 K09
VISIR 8.60 24.6 ± 0.9 K09
VISIR 11.22 18.1 ± 0.7 K09
COBE 11.25 14.6 ± 0.5 S04
IRAS 11.79 13.9 ± 0.3 I19
IRAS 23.34 4.31 ± 0.26 I19
MIPS 23.68 3.73 ± 0.15 K09
IRAS 59.32 0.896 ± 0.0801 I19
MIPS 71.42 0.45 ± 0.02 K09
PACS 160 0.106 ± 0.013 M24
SPIRE 250 0.0488 ± 0.0021 H24
SPIRE 363 0.0288 ± 0.0023 H24

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