Hot GRB-selected Submillimeter Galaxies

Simple item page
dc.creatorMichałowski, M. J.
dc.creatorHjorth, J.
dc.creatorCerón, J. M. Castro
dc.creatorWatson, D.
dc.date2007-08-29
dc.date.accessioned2026-07-07T08:26:35Z
dc.date.available2026-07-07T08:26:35Z
dc.descriptionUsing detailed spectral energy distribution fits we present evidence that submillimeter- and radio-bright gamma-ray burst host galaxies are hotter counterparts to submillimeter galaxies. This hypothesis makes them of special interest since hotter submm galaxies are difficult to find and are believed to contribute significantly to the star formation history of the Universe.
dc.description2 pages, 1 figure, In: Pathways through an eclectic Universe, J. H. Knapen, T. J. Mahoney, and A. Vazdekis (Eds.), ASP Conf. Ser., 2007, in press, for SED templates, see http://archive.dark-cosmology.dk/
dc.identifierhttps://arxiv.org/abs/0708.4017
dc.identifierhttp://arxiv.org/abs/0708.4017
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/136988
dc.subjectAstrophysics
dc.titleHot GRB-selected Submillimeter Galaxies
dc.typetext

Files

Collections

arXiv