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Published online by Cambridge University Press: 22 July 2013
Long gamma-ray bursts (GRBs) pinpoint star-forming galaxies as they are linked to thedeaths of massive stars. In most cases, these galaxies have been found to be blue,sub-luminous and of low-metallicity. However, our recent survey have demonstrated that asizeable fraction of GRBs reside in massive, dusty and star-forming extremely red objects(EROs, (R − K)AB > 3.5).The most remarkable case is the host of GRB 080207, one of the reddest galaxies everassociated with a GRB. This discovery suggests that at least a fraction of GRB afterglowstrace a subpopulation of massive starburst galaxies, which are markedly different from themost studied blue, sub-luminous and compact GRB host galaxies.