{"paper":{"title":"The 2dF Galaxy Redshift Survey: The population of nearby radio galaxies at the 1 mJy level","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"B. A. Peterson, C.A. Jackson, C. Collins, C.S. Frenk, G. Dalton, G. Efstathiou, I. Lewis, J.A. Peacock, J. Bland-Hawthorn, K. Glazebrook, K. Taylor, M. Colless, M. Magliocchetti, O. Lahav, R. Cannon, R. De Propris, R.S. Ellis, S. Cole, S.J. Maddox, S. Lumsden, S.P. Driver, T. Bridges, W. Couch, W. Sutherland","submitted_at":"2001-06-23T14:49:14Z","abstract_excerpt":"We use redshift determinations and spectral analysis of galaxies in the 2dF Galaxy Redshift Survey to study the properties of local radio sources with $S\\ge 1$ mJy. 557 objects drawn from the FIRST survey, corresponding to 2.3 per cent of the total radio sample, are found in the 2dFGRS cataloge within the area $9^h 48^m \\simlt {\\rm RA}({\\rm 2000}) \\simlt 14^h 32^m$ and $-2.77^\\circ \\simlt {\\rm dec}({\\rm 2000}) \\simlt 2.25^\\circ$, down to a magnitude limit $b_J= 19.45$. The excellent quality of 2dF spectra allows us to divide these sources into classes, according to their optical spectra. Radio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0106430","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}