Emission line galaxies at 9200 A, including a multi-component galaxy system at z =6.43
Simon Lilly, Kim-Vy Tran, Mark Brodwin, David Crampton, Stephanie Juneau, Henry McCracken
Abstract
This paper has been temporarily withdrawn by the authors. Subsequent observations with the VLT have shown that the high equivalent width line emission from the candidate z=6.4 galaxy most likely is associated with an unusually strong lined low redshift galaxy to the north west. The paper will be revised accordingly and resubmitted.
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