On the frequency of star-forming galaxies in the vicinity of powerful AGNs: The case of SMM J04135+10277

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Table 2

Results of the SED modelling.

magphys model^a

log(M_∗/M_⊙)
SFR [ M_⊙/ yr]
log(M_dust/M_⊙)
log(L_dust/L_⊙)
T_dust/ K
A_V [mag]

Notes. The fitted parameters are corrected for gravitational lensing magnification (μ_L = 1.3; Knudsen et al. 2003).

^(a)

The lower and upper limits of the median values are given by the 16th and 84th percentile of the likelihood distribution.

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