AGN and Galaxy Clustering at z = 0.3–3.0 Using the Japanese Virtual Observatory
AGN and Galaxy Clustering at z = 0.3–3.0 Using the Japanese Virtual Observatory
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Cambridge, UK: Cambridge University Press
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Language
English
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Publisher
Cambridge, UK: Cambridge University Press
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Contents
We present the results of a cross-correlation analysis of the projected positions of AGNs and galaxies at redshifts from 0.3 to 3.0. It is widely accepted that the origin of AGN activity is accretion of matter onto a massive black hole at the center of a galaxy (e.g., Lynden-Bell 1969). To explain the activity of AGNs, a large fraction of matter in...
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Full title
AGN and Galaxy Clustering at z = 0.3–3.0 Using the Japanese Virtual Observatory
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TN_cdi_proquest_miscellaneous_745939209
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_745939209
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ISSN
1743-9213
E-ISSN
1743-9221
DOI
10.1017/S1743921310006447
