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Looking for molecular gas in a massive lyman break galaxy at z = 4.05

Published online by Cambridge University Press:  17 July 2013

Qinghua Tan ,
Emanuele Daddi ,
Mark Sargent ,
Jackie Hodge  and
Yu Gao
Qinghua Tan
Affiliation:
CEA, Laboratoire AIM, Irfu/SAp, F-91191 Gif-sur-Yvette, France email: edaddi@cea.fr Purple Mountain Observatory, CAS, 2 West Beijing Road, 210008 Nanjing, China
Emanuele Daddi
Affiliation:
CEA, Laboratoire AIM, Irfu/SAp, F-91191 Gif-sur-Yvette, France email: edaddi@cea.fr
Mark Sargent
Affiliation:
CEA, Laboratoire AIM, Irfu/SAp, F-91191 Gif-sur-Yvette, France email: edaddi@cea.fr
Jackie Hodge
Affiliation:
Max-Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany
Yu Gao
Affiliation:
Purple Mountain Observatory, CAS, 2 West Beijing Road, 210008 Nanjing, China
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Abstract

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We present a search for CO emission in a massive lyman break galaxy at z ~ 4.05.

Keywords

galaxies: high-redshiftgalaxies: star formationradio lines: galaxies

References

Magdis, G., Daddi, E., Elbaz, D., et al. 2011, ApJ, 740, 15Google Scholar
Magdis, G., Daddi, E., Sargent, M., et al. 2012a, ApJ, 758, 9CrossRefGoogle Scholar
Sargent, M., et al. 2012b, in preparationGoogle Scholar