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Table 2

SED of DZ Cha.

Wavelength Flux Flux Dered. Error Ref.
(μm) (mJy) (mJy) (%)

0.15 2.20E-02 5.46E-02 30 1
0.23 8.50E-02 2.26E-01 30 1
0.44 7.90E+00 1.25E+01 15 2
0.48 1.38E+01 2.10E+01 15 2
0.55 2.85E+01 4.01E+01 10 2
0.62 5.09E+01 6.79E+01 10 2
0.76 1.17E+02 1.45E+02 10 2
1.24 2.62E+02 2.90E+02 5 3
1.65 3.41E+02 3.63E+02 5 3
2.16 2.72E+02 2.83E+02 5 3
3.35 1.66E+02 1.69E+02 5 4
3.55 1.65E+02 1.69E+02 5 5
4.49 1.73E+02 1.76E+02 5 5
4.60 1.54E+02 1.57E+02 5 4
5.73 1.90E+02 1.93E+02 5 5
7.87 3.66E+02 3.72E+02 5 5
11.56 4.42E+02 4.44E+02 5 4
22.09 1.54E+03 1.55E+03 5 4
23.67 1.24E+03 1.24E+03 10 5
70.00 1.73E+03 1.73E+03 5 6
160.00 1.09E+03 1.09E+03 5 6
250.00 3.48E+02 3.48E+02 5 6
363.00 1.59E+02 1.59E+02 5 6
517.00 7.41E+01 7.41E+01 15 6
870.00 <2.40E+01a <2.40E+01a ... 6

Notes. The columns list the effective wavelength of each filter, the observed flux, the de-reddened flux, and the associated errors. Extinction uncertainties dominate at wavelengths shorter than 1μm, while calibration uncertainties dominate at longer wavelengths. Photometry references: 1) Bianchi et al. (2011); 2) Henden et al. (2016); 3) Cutri et al. (2003); 4) Cutri et al. (2014); 5) Evans et al. (2009); 6) this work.

(a)

3σ upper limit.

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