The environments of z<0.3 QSOs

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dc.creatorBoyle, B. J.
dc.creatorSmith, R. J.
dc.creatorMaddox, S. J.
dc.date1995-04-20
dc.date.accessioned2026-07-07T02:19:45Z
dc.date.available2026-07-07T02:19:45Z
dc.descriptionBased on a cross-correlation analysis of X-ray selected QSOs with faint (B<20.5) galaxies, we find a 5sigma galaxy excess around low-redshift (z<0.3) QSOs with an amplitude identical to that of the galaxy angular correlation function. The similarity between QSO-galaxy clustering and galaxy-galaxy clustering suggests that QSOs are unbiased with respect to galaxies and make useful tracers of large-scale structure in the Universe.
dc.descriptionuuencoded compressed postscript. The preprint is also available at http://www.ast.cam.ac.uk/preprint/PrePrint.html
dc.identifierhttps://arxiv.org/abs/astro-ph/9504067
dc.identifierhttp://arxiv.org/abs/astro-ph/9504067
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9987
dc.subjectAstrophysics
dc.titleThe environments of z<0.3 QSOs
dc.typetext

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