A dust-obscured massive maximum-starburst galaxy at a redshift of 6.34

  title={A dust-obscured massive maximum-starburst galaxy at a redshift of 6.34},
  author={Dominik A. Riechers and Charles Matt Bradford and David L. Clements and C. Darren Dowell and Ismael P{\'e}rez-Fournon and Robert J. Ivison and Carrie R. Bridge and Alex Conley and Hai Fu and Joaquin D. Vieira and Julie Wardlow and J. A. Calanog and Asantha Cooray and Peter D Hurley and Roberto Neri and Julia Kamenetzky and James E. Aguirre and Bruno Altieri and Vinodiran Arumugam and Dominic J. Benford and Matthieu B{\'e}thermin and James J. Bock and Denis Burgarella and Antonio Cabrera-Lavers and Scott C. Chapman and Pierre Cox and James S. Dunlop and Lieko Earle and Duncan Farrah and Patrizia Ferrero and Alberto Franceschini and Raphael Gavazzi and Jason Glenn and E. A. Gonz'alez Solares and Mark A. Gurwell and Mark Halpern and Evanthia Hatziminaoglou and Ashley K. Hyde and Edo Ibar and Attila Kov{\'a}cs and Melanie Krips and Roxana E. Lupu and Philip Richard Maloney and P. I. Martinez-Navajas and Hideo Matsuhara and Eric J. Murphy and Bret J. Naylor and H. T. Nguyen and S. J. Oliver and Alain Omont and M J Page and Glen Raymond Petitpas and Naseem Rangwala and Isaac Roseboom and Douglas Scott and A. J. Smith and Johannes G. Staguhn and A. Streblyanska and Alasdair P. Thomson and Ivan Valtchanov and Marco P. Viero and L. Wang and Michael Zemcov and Jonas Zmuidzinas},
Massive present-day early-type (elliptical and lenticular) galaxies probably gained the bulk of their stellar mass and heavy elements through intense, dust-enshrouded starbursts—that is, increased rates of star formation—in the most massive dark-matter haloes at early epochs. However, it remains unknown how soon after the Big Bang massive starburst progenitors exist. The measured redshift (z) distribution of dusty, massive starbursts has long been suspected to be biased low in z owing to… 

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