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dc.creatorBenítez, Narciso-
dc.creatorSanz, J. L.-
dc.creatorMartínez-González, Enrique-
dc.date2008-05-04T19:16:41Z-
dc.date2008-05-04T19:16:41Z-
dc.date2000-08-24-
dc.date.accessioned2017-01-31T01:09:26Z-
dc.date.available2017-01-31T01:09:26Z-
dc.identifierarXiv:astro-ph/0008394v1-
dc.identifierMon. Not. Roy. Astron. Soc. 320 (2001) 241-
dc.identifier0035-8711-
dc.identifierhttp://hdl.handle.net/10261/3980-
dc.identifier.urihttp://dspace.mediu.edu.my:8181/xmlui/handle/10261/3980-
dc.description9 pages, 6 figures.-- MNRAS accepted.-
dc.descriptionGravitational lensing predicts an enhancement of the density of bright, distant QSOs around foreground galaxies. We measure this QSO-galaxy correlation w_qg for two complete samples of radio-loud quasars, the southern 1Jy and Half-Jansky samples. The existence of a positive correlation between z~1 quasars and z~0.15 galaxies is confirmed at a p=99.0% significance level (>99.9%) if previous measurements on the northern hemisphere are included). A comparison with the results obtained for incomplete quasar catalogs (e.g. the Veron-Cetty and Veron compilation) suggests the existence of an `identification bias', which spuriously increases the estimated amplitude of the quasar-galaxy correlation for incomplete samples. This effect may explain many of the surprisingly strong quasar-galaxy associations found in the literature. Nevertheless, the value of w_qg that we measure in our complete catalogs is still considerably higher than the predictions from weak lensing. We consider two effects which could help to explain this discrepancy: galactic dust extinction and strong lensing.-
dc.descriptionPeer reviewed-
dc.format267551 bytes-
dc.formatapplication/pdf-
dc.languageeng-
dc.publisherBlackwell Publishing-
dc.relationPreprint-
dc.rightsopenAccess-
dc.subjectQuasar galaxy associations-
dc.subjectGravitational lensing-
dc.titleQuasar-galaxy associations revisited-
dc.typePre-print-
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