Physical properties of z > 4 submillimeter galaxies in the COSMOS field | Astronomy & Astrophysics (A&A)

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Volume 576 (April 2015)

A&A, 576 (2015) A127

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Table 6

Physical properties derived from the IR SED of our z> 4 SMG sample.

Name

T _dust

M _dust

M _dust

L _IR

L _IR

SFR^a

[K]

[BB, 10⁸ M_⊙]

[DL07, 10⁸ M_⊙]

[BB, 10¹²L_⊙]

[DL07, 10¹²L_⊙]

[DL07, M_⊙ yr^-1]

AzTEC1

41.0 ± 5.0

AzTEC3

43.5 ± 11.5

AzTEC/C159

39.0 ± 2.0

J1000+0234^b

45.0 ± 17.5

Vd-17871

48.0 ± 5.0

AK03

41.0 ± 10.0

Notes.

^(a)

The SFRs were calculated using the L_IR values derived from the DL07 dust model.

^(b)

The large uncertainties in the derived values arise from the highly confused Herschel photometry for J1000+0234 (see Table 2).

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