Comments on the Redshift Distribution of 44,200 SDSS Quasars: Evidence for Predicted Preferred Redshifts?

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dc.creatorBell, M. B.
dc.date2004-03-03
dc.date.accessioned2026-07-07T02:12:29Z
dc.date.available2026-07-07T02:12:29Z
dc.descriptionA Sloan Digital Sky Survey (SDSS) source sample containing 44,200 quasar redshifts is examined. Although arguments have been put forth to explain some of the structure observed in the redshift distribution, it is argued here that this structure may just as easily be explained by the presence of previously predicted preferred redshifts.
dc.description6 pages, 3 figures. Submitted to ApJL
dc.identifierhttps://arxiv.org/abs/astro-ph/0403089
dc.identifierhttp://arxiv.org/abs/astro-ph/0403089
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7469
dc.subjectAstrophysics
dc.titleComments on the Redshift Distribution of 44,200 SDSS Quasars: Evidence for Predicted Preferred Redshifts?
dc.typetext

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