{"paper":{"title":"NIR Follow-Up of the VVDS 02hr Field","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. Bongiorno, A. Cappi, A. Iovino, A. Mazure, A. Pollo, A. Zanichelli, B. Garilli, B. Marano, B. Meneux, C. Adami, C. J. Walcher, C. Marinoni, D. Bottini, D. Maccagni, D. Vergani, E. Zucca, F. Lamareille, G. Vettolani, G. Zamorani, H. J. McCracken, I. Gavignaud, J. Brinchmann, J.-P. Picat, L. Guzzo, L. Pozzetti, L. Tresse, M. Bolzonella, M. Bondi, M. Radovich, M. Scodeggio, O. Cucciati, O. Ilbert, O. Le Fevre, P. Ciliegi, P. Franzetti, P. Merluzzi, R. Merighi, R. Pello, R. Scaramella, S. Arnouts, S. Bardelli, S. Charlot, S. de la Torre, S. Foucaud, S. Paltani, S. Temporin, T. Contini, V. Le Brun, Y. Mellier","submitted_at":"2006-11-03T11:36:38Z","abstract_excerpt":"We present a new K-band survey covering 623 arcmin$^2$ in the VVDS 0226-0430 deep field down to a limiting magnitude K$_{\\rm{Vega}}$ $\\leq$ 20.5. We use the spectroscopic sample extracted from this new K-band catalogue to assess the effectiveness of optical-near infrared color selections in identifying extreme classes of objects at high redshift."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0611108","kind":"arxiv","version":1},"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"}