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Table 2.

SED for each component in VLA1623.

VLA 1623 A VLA 1623 B VLA 1623 W

RA 16:26:26.390 16:26:26.309 16:26:25.636
Dec −24:24:30.688 −24:24:30.588 −24:24:29.488

Wavelength Sint error Sint error Sint error Ref. Telescope
µm mJy mJy mJy mJy mJy mJy
3.6 0.74 0.12 1 Spitzer/IRAC1
4.5 2.35 0.19 1 Spitzer/IRAC2
5.8 3.26 0.33 1 Spitzer/IRAC3
8.0 2.60 0.26 1 Spitzer/IRAC4
24 40.4 ± 4.2a 164.26 4.54 2,1 Spitzer/MIPS1
70b 17424.5 ± 3.2a 5790.8 3.88 3 Herschel/PACS
100b 55092.3 ± 8.7a 10284.9c 8.6 3 Herschel/PACS
160b 81340.6 ± 10.3a 21457.2c 11.5 3 Herschel/PACS
450 3820.0 4.2 1723.0 5.7 3 ALMA/Band 9 Natural weighting
450 2910.0 6.4 1653.0 6.8 3 ALMA/Band 9 Briggs weighting
850 1139.5 3.4 373.0 4.6 69.0 7.0 3 ALMA/Band 7
1300 184.0 13.8 104.0 15.3 38.0 3.8 3 ALMA/Band 6 Cycle 0
1300 178.0 5.1 106.0 5.3 30.0 3.0 3 ALMA/Band 6 Cycle 2
1300 152.0 8.0 106.0 8.0 25.7 8.0 4 SMA
2700 25.5 6.3 25.8 3.5 3.1 1.5 5 BIMA
7000 1.2 0.2 2 0.2 6 VLA
36000 0.13 0.02 0.4 0.02 0.2 0.02 6,7 VLA
44000 <0.2 <0.2 6 MERLIN

Notes.

(a)

Unresolved fluxes.

(b)

Fluxes obtained with StarFinder PSF photometry using an aperture mask of 11.2″, 12.8″, and 19.2″ for 70, 100, and 160 µm, respectively. The aperture correction factors are 0.791, 0.795, and 0.789 for 70, 100, and 160 µm, respectively (Balog et al. 2014).

(c)

VLA 1623 W fluxes obtained using the deblend option in StarFinder, since no distinct peak for VLA 1623 W is observed.

References. (1) Gutermuth et al. (2009); (2) c2d catalog; (3) this work; (4) Murillo & Lai (2013); (5) Looney et al. (2000); (6) Ward-Thompson et al. (2011); (7) Bontemps & Andre (1997).

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