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Near Infrared Observations of a Redshift 5.34 Galaxy: Further Evidence for Significant Dust Absorption in the Early Universe

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dc.contributor.author Armus, L. en_US
dc.contributor.author Matthews, K. en_US
dc.contributor.author Neugebauer, G. en_US
dc.contributor.author Soifer, B. T. en_US
dc.date.accessioned 2004-09-24T20:41:29Z
dc.date.available 2004-09-24T20:41:29Z
dc.date.issued 1998-04 en_US
dc.identifier.citation Astrophysical Journal Letters en_US
dc.identifier.citation USA en_US
dc.identifier.clearanceno 98-0646 en_US
dc.identifier.uri http://hdl.handle.net/2014/19323
dc.description.abstract In the last several years, the combination of new wavelength dropout discovery techniques coupled with the incredible power of deep imaging of the Hubble Space Telescope and the spectroscopic capabilities of a new generation of large ground-based telescopes, has lead to an astonishing blossoming of the study of galaxies at redshifts of z=2-4, when the Universe was less than 10-20% of its current age. en_US
dc.format.extent 889311 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other near infrared redshift 5.34 galaxy high redshift young en_US
dc.title Near Infrared Observations of a Redshift 5.34 Galaxy: Further Evidence for Significant Dust Absorption in the Early Universe en_US


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