Statistics for <i>Herschel</i> FIR counterparts of selected Lyα emitters at <i>z</i> ∼ 2.2 Fast evolution since <i>z</i> ∼ 3 or missed obscured AGNs?

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<i>Herschel</i> FIR counterparts of selected Lyα emitters at <i>z</i> ∼ 2.2 Fast evolution since <i>z</i> ∼ 3 or missed obscured AGNs? 0

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