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Table D.1

Flux densities used in the SED fits in Sect. 4.1.

Name Wavelength Flux density Reference
Telescope [μm] [Jy]

IRS7A
Spitzer 3.6 0.0509 Peterson et al. (2011)
4.5 0.239
5.8 0.546
8.0 1.05
SMM 1C
JCMT SCUBAa 450 45 Nutter et al. (2005)
850 5.6
IRS7B
Spitzer 3.6 0.0367 Peterson et al. (2011)
4.5 0.257
5.8 0.697
8.0 0.957
JCMT SCUBAa 450 50 Nutter et al. (2005)
850 5.4
R CrA
SAAO 0.36 0.0141 Koen et al. (2010)
0.45 0.0359
0.555 0.0647
0.67 0.116
0.87 0.180
2MASS 1.25 2.68 Skrutskie et al. (2006)
1.65 10.7
2.2 47.9
IRS5A
Spitzer 3.6 0.389 Peterson et al. (2011)
4.5 0.798
5.8 1.27
8.0 1.81
IRS5N
Spitzer 3.6 0.00856 Peterson et al. (2011)
4.5 0.0262
5.8 0.0528
8.0 0.0809
JCMT SCUBAa 450 12b Nutter et al. (2005)
850 1.8b

Notes.

(a)

The integrated flux density in apertures of 16″ × 16″ (SMM 1C), 18″ × 17″ (IRS7B), and 24″ × 24″ (IRS5N) are given.

(b)

This is the combined value for IRS5A and IRS5N, which are unresolved. For the SEDs, we assign half of the flux density to each source.

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