Emission line galaxies at 9200 A, including a multi-component galaxy system at z =6.43
classification
🌌 astro-ph
keywords
galaxyemissionlineaccordinglyassociatedauthorsbeencandidate
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This paper has been temporarily withdrawn by the authors.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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