Emission line galaxies at 9200 A, including a multi-component galaxy system at z =6.43

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dc.creatorLilly, Simon
dc.creatorTran, Kim-Vy
dc.creatorBrodwin, Mark
dc.creatorCrampton, David
dc.creatorJuneau, Stephanie
dc.creatorMcCracken, Henry
dc.date2003-04-22
dc.date2003-07-31
dc.date.accessioned2026-07-07T02:08:17Z
dc.date.available2026-07-07T02:08:17Z
dc.descriptionThis paper has been temporarily withdrawn by the authors.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.
dc.identifierhttps://arxiv.org/abs/astro-ph/0304376
dc.identifierhttp://arxiv.org/abs/astro-ph/0304376
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5988
dc.subjectAstrophysics
dc.titleEmission line galaxies at 9200 A, including a multi-component galaxy system at z =6.43
dc.typetext

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